[{"arxiv":1,"oa_version":"Preprint","month":"03","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","oa":1,"publication_status":"published","date_updated":"2022-08-18T11:27:43Z","publication_identifier":{"eissn":["1365-2966"],"issn":["0035-8711"]},"extern":"1","article_processing_charge":"No","citation":{"apa":"Santos, S., Sobral, D., Matthee, J. J., Calhau, J., da Cunha, E., Ribeiro, B., … Butterworth, J. (2020). The evolution of rest-frame UV properties, Ly α EWs, and the SFR–stellar mass relation at z ∼ 2–6 for SC4K LAEs. <i>Monthly Notices of the Royal Astronomical Society</i>. Oxford University Press. <a href=\"https://doi.org/10.1093/mnras/staa093\">https://doi.org/10.1093/mnras/staa093</a>","mla":"Santos, S., et al. “The Evolution of Rest-Frame UV Properties, Ly α EWs, and the SFR–Stellar Mass Relation at z ∼ 2–6 for SC4K LAEs.” <i>Monthly Notices of the Royal Astronomical Society</i>, vol. 493, no. 1, Oxford University Press, 2020, pp. 141–60, doi:<a href=\"https://doi.org/10.1093/mnras/staa093\">10.1093/mnras/staa093</a>.","ama":"Santos S, Sobral D, Matthee JJ, et al. The evolution of rest-frame UV properties, Ly α EWs, and the SFR–stellar mass relation at z ∼ 2–6 for SC4K LAEs. <i>Monthly Notices of the Royal Astronomical Society</i>. 2020;493(1):141-160. doi:<a href=\"https://doi.org/10.1093/mnras/staa093\">10.1093/mnras/staa093</a>","chicago":"Santos, S, D Sobral, Jorryt J Matthee, J Calhau, E da Cunha, B Ribeiro, A Paulino-Afonso, P Arrabal Haro, and J Butterworth. “The Evolution of Rest-Frame UV Properties, Ly α EWs, and the SFR–Stellar Mass Relation at z ∼ 2–6 for SC4K LAEs.” <i>Monthly Notices of the Royal Astronomical Society</i>. Oxford University Press, 2020. <a href=\"https://doi.org/10.1093/mnras/staa093\">https://doi.org/10.1093/mnras/staa093</a>.","short":"S. Santos, D. Sobral, J.J. Matthee, J. Calhau, E. da Cunha, B. Ribeiro, A. Paulino-Afonso, P. Arrabal Haro, J. Butterworth, Monthly Notices of the Royal Astronomical Society 493 (2020) 141–160.","ista":"Santos S, Sobral D, Matthee JJ, Calhau J, da Cunha E, Ribeiro B, Paulino-Afonso A, Arrabal Haro P, Butterworth J. 2020. The evolution of rest-frame UV properties, Ly α EWs, and the SFR–stellar mass relation at z ∼ 2–6 for SC4K LAEs. Monthly Notices of the Royal Astronomical Society. 493(1), 141–160.","ieee":"S. Santos <i>et al.</i>, “The evolution of rest-frame UV properties, Ly α EWs, and the SFR–stellar mass relation at z ∼ 2–6 for SC4K LAEs,” <i>Monthly Notices of the Royal Astronomical Society</i>, vol. 493, no. 1. Oxford University Press, pp. 141–160, 2020."},"title":"The evolution of rest-frame UV properties, Ly α EWs, and the SFR–stellar mass relation at z ∼ 2–6 for SC4K LAEs","status":"public","type":"journal_article","doi":"10.1093/mnras/staa093","external_id":{"arxiv":["1910.02959"]},"_id":"11533","page":"141-160","intvolume":"       493","acknowledgement":"We thank the anonymous referee for the valuable feedback that significantly improved the quality and clarity of this paper. SS and JC acknowledge studentships from Lancaster University. APA acknowledges support from Fundação para a Ciência e a Tecnologia through the project PTDC/FISAST/31546/2017. The authors would like to thank Ali Khostovan, Sara Perez Sanchez, Alex Bennett and Tom Rose for contributions and discussions in the early stages of this work. Based on data products from observations made with ESO Telescopes at the La Silla Paranal Observatory under ESO programme ID 179.A-2005 and on data products produced by CALET and the Cambridge Astronomy Survey Unit on behalf of the UltraVISTA consortium. Finally, the authors acknowledge the unique value of the publicly available analysis software TOPCAT (Taylor 2005) and publicly available programming language Python, including the numpy, pyfits, matplotlib, scipy and astropy (Astropy Collaboration et al. 2013) packages. This work is based on the public SC4K sample of LAEs (Sobral et al. 2018a) and we release the full catalogue with all the photometry and properties derived in this paper, in electronic format, along with the relevant tables.","quality_controlled":"1","issue":"1","author":[{"last_name":"Santos","first_name":"S","full_name":"Santos, S"},{"first_name":"D","last_name":"Sobral","full_name":"Sobral, D"},{"id":"7439a258-f3c0-11ec-9501-9df22fe06720","full_name":"Matthee, Jorryt J","last_name":"Matthee","first_name":"Jorryt J","orcid":"0000-0003-2871-127X"},{"first_name":"J","last_name":"Calhau","full_name":"Calhau, J"},{"full_name":"da Cunha, E","last_name":"da Cunha","first_name":"E"},{"first_name":"B","last_name":"Ribeiro","full_name":"Ribeiro, B"},{"last_name":"Paulino-Afonso","first_name":"A","full_name":"Paulino-Afonso, A"},{"first_name":"P","last_name":"Arrabal Haro","full_name":"Arrabal Haro, P"},{"full_name":"Butterworth, J","first_name":"J","last_name":"Butterworth"}],"volume":493,"abstract":[{"text":"We explore deep rest-frame UV to FIR data in the COSMOS field to measure the individual spectral energy distributions (SED) of the ∼4000 SC4K (Sobral et al.) Lyman α (Ly α) emitters (LAEs) at z ∼ 2–6. We find typical stellar masses of 109.3 ± 0.6 M⊙ and star formation rates (SFR) of SFRSED=4.4+10.5−2.4 M⊙ yr−1 and SFRLyα=5.9+6.3−2.6 M⊙ yr−1, combined with very blue UV slopes of β=−2.1+0.5−0.4⁠, but with significant variations within the population. MUV and β are correlated in a similar way to UV-selected sources, but LAEs are consistently bluer. This suggests that LAEs are the youngest and/or most dust-poor subset of the UV-selected population. We also study the Ly α rest-frame equivalent width (EW0) and find 45 ‘extreme’ LAEs with EW0 > 240 Å (3σ), implying a low number density of (7 ± 1) × 10−7 Mpc−3. Overall, we measure little to no evolution of the Ly α EW0 and scale length parameter (w0), which are consistently high (EW0=140+280−70 Å, w0=129+11−11 Å) from z ∼ 6 to z ∼ 2 and below. However, w0 is anticorrelated with MUV and stellar mass. Our results imply that sources selected as LAEs have a high Ly α escape fraction (fesc,Ly α) irrespective of cosmic time, but fesc,Ly α is still higher for UV-fainter and lower mass LAEs. The least massive LAEs (<109.5 M⊙) are typically located above the star formation ‘main sequence’ (MS), but the offset from the MS decreases towards z ∼ 6 and towards 1010 M⊙. Our results imply a lack of evolution in the properties of LAEs across time and reveals the increasing overlap in properties of LAEs and UV-continuum selected galaxies as typical star-forming galaxies at high redshift effectively become LAEs.","lang":"eng"}],"date_published":"2020-03-01T00:00:00Z","publication":"Monthly Notices of the Royal Astronomical Society","day":"01","year":"2020","language":[{"iso":"eng"}],"keyword":["Space and Planetary Science","Astronomy and Astrophysics","galaxies: evolution","galaxies: formation","galaxies: high-redshift","galaxies: star formation"],"publisher":"Oxford University Press","main_file_link":[{"open_access":"1","url":"https://arxiv.org/abs/1910.02959"}],"scopus_import":"1","date_created":"2022-07-07T12:05:23Z","article_type":"original"},{"author":[{"last_name":"Matthee","first_name":"Jorryt J","orcid":"0000-0003-2871-127X","full_name":"Matthee, Jorryt J","id":"7439a258-f3c0-11ec-9501-9df22fe06720"},{"first_name":"David","last_name":"Sobral","full_name":"Sobral, David"},{"last_name":"Gronke","first_name":"Max","full_name":"Gronke, Max"},{"full_name":"Pezzulli, Gabriele","first_name":"Gabriele","last_name":"Pezzulli"},{"last_name":"Cantalupo","first_name":"Sebastiano","full_name":"Cantalupo, Sebastiano"},{"full_name":"Röttgering, Huub","last_name":"Röttgering","first_name":"Huub"},{"full_name":"Darvish, Behnam","last_name":"Darvish","first_name":"Behnam"},{"first_name":"Sérgio","last_name":"Santos","full_name":"Santos, Sérgio"}],"volume":492,"abstract":[{"text":"The observed properties of the Lyman-α (Ly α) emission line are a powerful probe of neutral gas in and around galaxies. We present spatially resolved Ly α spectroscopy with VLT/MUSE targeting VR7, a UV-luminous galaxy at z = 6.532 with moderate Ly α equivalent width (EW0 ≈ 38 Å). These data are combined with deep resolved [CII]158μm spectroscopy obtained with ALMA and UV imaging from HST and we also detect UV continuum with MUSE. Ly α emission is clearly detected with S/N ≈ 40 and FWHM of 374 km s−1. Ly α and [C II] are similarly extended beyond the UV, with effective radius reff = 2.1 ± 0.2 kpc for a single exponential model or reff,Lyα,halo=3.45+1.08−0.87 kpc when measured jointly with the UV continuum. The Ly α profile is broader and redshifted with respect to the [C II] line (by 213 km s−1), but there are spatial variations that are qualitatively similar in both lines and coincide with resolved UV components. This suggests that the emission originates from two components with plausibly different H I column densities. We place VR7 in the context of other galaxies at similar and lower redshift. The Ly α halo scale length is similar at different redshifts and velocity shifts with respect to the systemic are typically smaller. Overall, we find little indications of a more neutral vicinity at higher redshift. This means that the local (∼10 kpc) neutral gas conditions that determine the observed Ly α properties in VR7 resemble the conditions in post-reionization galaxies.","lang":"eng"}],"date_published":"2020-02-01T00:00:00Z","issue":"2","keyword":["Space and Planetary Science","Astronomy and Astrophysics","galaxies: evolution","galaxies: high-redshift","dark ages","reionization","first stars","cosmology: observations"],"publication":"Monthly Notices of the Royal Astronomical Society","day":"01","language":[{"iso":"eng"}],"year":"2020","scopus_import":"1","publisher":"Oxford University Press","main_file_link":[{"url":"https://arxiv.org/abs/1909.06376","open_access":"1"}],"date_created":"2022-07-07T12:21:36Z","article_type":"original","arxiv":1,"oa":1,"publication_status":"published","date_updated":"2022-08-18T11:29:53Z","publication_identifier":{"eissn":["1365-2966"],"issn":["0035-8711"]},"month":"02","oa_version":"Preprint","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","title":"Resolved Lyman-α properties of a luminous Lyman-break galaxy in a large ionized bubble at z = 6.53 ","status":"public","type":"journal_article","citation":{"mla":"Matthee, Jorryt J., et al. “Resolved Lyman-α Properties of a Luminous Lyman-Break Galaxy in a Large Ionized Bubble at z = 6.53 .” <i>Monthly Notices of the Royal Astronomical Society</i>, vol. 492, no. 2, Oxford University Press, 2020, pp. 1778–90, doi:<a href=\"https://doi.org/10.1093/mnras/stz3554\">10.1093/mnras/stz3554</a>.","apa":"Matthee, J. J., Sobral, D., Gronke, M., Pezzulli, G., Cantalupo, S., Röttgering, H., … Santos, S. (2020). Resolved Lyman-α properties of a luminous Lyman-break galaxy in a large ionized bubble at z = 6.53 . <i>Monthly Notices of the Royal Astronomical Society</i>. Oxford University Press. <a href=\"https://doi.org/10.1093/mnras/stz3554\">https://doi.org/10.1093/mnras/stz3554</a>","short":"J.J. Matthee, D. Sobral, M. Gronke, G. Pezzulli, S. Cantalupo, H. Röttgering, B. Darvish, S. Santos, Monthly Notices of the Royal Astronomical Society 492 (2020) 1778–1790.","chicago":"Matthee, Jorryt J, David Sobral, Max Gronke, Gabriele Pezzulli, Sebastiano Cantalupo, Huub Röttgering, Behnam Darvish, and Sérgio Santos. “Resolved Lyman-α Properties of a Luminous Lyman-Break Galaxy in a Large Ionized Bubble at z = 6.53 .” <i>Monthly Notices of the Royal Astronomical Society</i>. Oxford University Press, 2020. <a href=\"https://doi.org/10.1093/mnras/stz3554\">https://doi.org/10.1093/mnras/stz3554</a>.","ama":"Matthee JJ, Sobral D, Gronke M, et al. Resolved Lyman-α properties of a luminous Lyman-break galaxy in a large ionized bubble at z = 6.53 . <i>Monthly Notices of the Royal Astronomical Society</i>. 2020;492(2):1778-1790. doi:<a href=\"https://doi.org/10.1093/mnras/stz3554\">10.1093/mnras/stz3554</a>","ista":"Matthee JJ, Sobral D, Gronke M, Pezzulli G, Cantalupo S, Röttgering H, Darvish B, Santos S. 2020. Resolved Lyman-α properties of a luminous Lyman-break galaxy in a large ionized bubble at z = 6.53 . Monthly Notices of the Royal Astronomical Society. 492(2), 1778–1790.","ieee":"J. J. Matthee <i>et al.</i>, “Resolved Lyman-α properties of a luminous Lyman-break galaxy in a large ionized bubble at z = 6.53 ,” <i>Monthly Notices of the Royal Astronomical Society</i>, vol. 492, no. 2. Oxford University Press, pp. 1778–1790, 2020."},"extern":"1","article_processing_charge":"No","acknowledgement":"We thank the referee for their suggestions and constructive comments that helped to improve the presentation of our results. Based on observations obtained with the Very Large Telescope, program 99.A-0462. Based on observations made with the NASA/ESA Hubble Space Telescope, obtained at the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5-26555. These observations are associated with program #14699. This paper makes use of the following ALMA data: ADS/JAO.ALMA#2017.1.01451.S. ALMA is a partnership of ESO (representing its member states), NSF (USA), and NINS (Japan), together with NRC (Canada) and NSC and ASIAA (Taiwan) and KASI (Republic of Korea), in cooperation with the Republic of Chile. The Joint ALMA Observatory is operated by ESO, AUI/NRAO, and NAOJ. MG acknowledges support from NASA grant NNX17AK58G. GP and SC gratefully acknowledge support from Swiss National Science Foundation grant PP00P2 163824. BD acknowledges financial support from the National Science Foundation, grant number 1716907. We have benefited greatly from the public available programming language PYTHON, including the NUMPY, MATPLOTLIB, SCIPY (Jones et al. 2001; Hunter 2007; van der Walt, Colbert & Varoquaux 2011) and ASTROPY (Astropy Collaboration 2013) packages, the astronomical imaging tools SEXTRACTOR, SWARP, and SCAMP (Bertin & Arnouts 1996; Bertin 2006, 2010) and the TOPCAT analysis tool (Taylor 2013).","quality_controlled":"1","doi":"10.1093/mnras/stz3554","external_id":{"arxiv":["1909.06376"]},"_id":"11534","page":"1778-1790","intvolume":"       492"},{"publication":"Monthly Notices of the Royal Astronomical Society","day":"01","year":"2020","language":[{"iso":"eng"}],"keyword":["Space and Planetary Science","Astronomy and Astrophysics","galaxies: active","galaxies: evolution","galaxies: high-redshift","quasars: supermassive black holes","galaxies: star formation","cosmology: observations","X-rays: galaxies"],"issue":"3","author":[{"full_name":"Calhau, João","last_name":"Calhau","first_name":"João"},{"first_name":"David","last_name":"Sobral","full_name":"Sobral, David"},{"first_name":"Sérgio","last_name":"Santos","full_name":"Santos, Sérgio"},{"full_name":"Matthee, Jorryt J","id":"7439a258-f3c0-11ec-9501-9df22fe06720","first_name":"Jorryt J","last_name":"Matthee","orcid":"0000-0003-2871-127X"},{"full_name":"Paulino-Afonso, Ana","last_name":"Paulino-Afonso","first_name":"Ana"},{"full_name":"Stroe, Andra","last_name":"Stroe","first_name":"Andra"},{"full_name":"Simmons, Brooke","last_name":"Simmons","first_name":"Brooke"},{"full_name":"Barlow-Hall, Cassandra","last_name":"Barlow-Hall","first_name":"Cassandra"},{"first_name":"Benjamin","last_name":"Adams","full_name":"Adams, Benjamin"}],"volume":493,"abstract":[{"lang":"eng","text":"Despite recent progress in understanding Ly α emitters (LAEs), relatively little is known regarding their typical black hole activity across cosmic time. Here, we study the X-ray and radio properties of ∼4000 LAEs at 2.2 < z < 6 from the SC4K survey in the COSMOS field. We detect 254 (⁠6.8per cent±0.4per cent⁠) LAEs individually in the X-rays (S/N > 3) with an average luminosity of 1044.31±0.01ergs−1 and average black hole accretion rate (BHAR) of 0.72±0.01 M⊙ yr−1, consistent with moderate to high accreting active galactic neuclei (AGNs). We detect 120 sources in deep radio data (radio AGN fraction of 3.2per cent±0.3per cent⁠). The global AGN fraction (⁠8.6per cent±0.4per cent⁠) rises with Ly α luminosity and declines with increasing redshift. For X-ray-detected LAEs, Ly α luminosities correlate with the BHARs, suggesting that Ly α luminosity becomes a BHAR indicator. Most LAEs (⁠93.1per cent±0.6per cent⁠) at 2 < z < 6 have no detectable X-ray emission (BHARs < 0.017 M⊙ yr−1). The median star formation rate (SFR) of star-forming LAEs from Ly α and radio luminosities is 7.6+6.6−2.8 M⊙ yr−1. The black hole to galaxy growth ratio (BHAR/SFR) for LAEs is <0.0022, consistent with typical star-forming galaxies and the local BHAR/SFR relation. We conclude that LAEs at 2 < z < 6 include two different populations: an AGN population, where Ly α luminosity traces BHAR, and another with low SFRs which remain undetected in even the deepest X-ray stacks but is detected in the radio stacks."}],"date_published":"2020-04-01T00:00:00Z","date_created":"2022-07-08T07:34:10Z","article_type":"original","publisher":"Oxford University Press","main_file_link":[{"url":"https://arxiv.org/abs/1909.11672","open_access":"1"}],"scopus_import":"1","oa_version":"Preprint","month":"04","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","publication_status":"published","oa":1,"date_updated":"2022-08-18T11:25:31Z","publication_identifier":{"issn":["0035-8711"],"eissn":["1365-2966"]},"arxiv":1,"doi":"10.1093/mnras/staa476","external_id":{"arxiv":["1909.11672"]},"page":"3341-3362","_id":"11539","intvolume":"       493","acknowledgement":"JM acknowledges the support of a Huygens PhD fellowship from Leiden University. We thank Camila Correa for help analysing snipshot merger trees. We thank the anonymous referee for constructive comments. We also thank Jarle Brinchmann, Rob Crain, Antonios Katsianis, Paola Popesso, and David Sobral for discussions and suggestions. We also thank the participants of the Lorentz Center workshop ‘A Decade of the Star-Forming Main Sequence’ held on 2017 September 4–8, for discussions and ideas. We have benefited from the public available programming language PYTHON, including the NUMPY, MATPLOTLIB, and SCIPY (Hunter 2007) packages and the TOPCAT analysis tool (Taylor 2013).","quality_controlled":"1","extern":"1","citation":{"ieee":"J. Calhau <i>et al.</i>, “The X-ray and radio activity of typical and luminous Ly α emitters from z ∼ 2 to z ∼ 6: Evidence for a diverse, evolving population,” <i>Monthly Notices of the Royal Astronomical Society</i>, vol. 493, no. 3. Oxford University Press, pp. 3341–3362, 2020.","ista":"Calhau J, Sobral D, Santos S, Matthee JJ, Paulino-Afonso A, Stroe A, Simmons B, Barlow-Hall C, Adams B. 2020. The X-ray and radio activity of typical and luminous Ly α emitters from z ∼ 2 to z ∼ 6: Evidence for a diverse, evolving population. Monthly Notices of the Royal Astronomical Society. 493(3), 3341–3362.","ama":"Calhau J, Sobral D, Santos S, et al. The X-ray and radio activity of typical and luminous Ly α emitters from z ∼ 2 to z ∼ 6: Evidence for a diverse, evolving population. <i>Monthly Notices of the Royal Astronomical Society</i>. 2020;493(3):3341-3362. doi:<a href=\"https://doi.org/10.1093/mnras/staa476\">10.1093/mnras/staa476</a>","chicago":"Calhau, João, David Sobral, Sérgio Santos, Jorryt J Matthee, Ana Paulino-Afonso, Andra Stroe, Brooke Simmons, Cassandra Barlow-Hall, and Benjamin Adams. “The X-Ray and Radio Activity of Typical and Luminous Ly α Emitters from z ∼ 2 to z ∼ 6: Evidence for a Diverse, Evolving Population.” <i>Monthly Notices of the Royal Astronomical Society</i>. Oxford University Press, 2020. <a href=\"https://doi.org/10.1093/mnras/staa476\">https://doi.org/10.1093/mnras/staa476</a>.","short":"J. Calhau, D. Sobral, S. Santos, J.J. Matthee, A. Paulino-Afonso, A. Stroe, B. Simmons, C. Barlow-Hall, B. Adams, Monthly Notices of the Royal Astronomical Society 493 (2020) 3341–3362.","apa":"Calhau, J., Sobral, D., Santos, S., Matthee, J. J., Paulino-Afonso, A., Stroe, A., … Adams, B. (2020). The X-ray and radio activity of typical and luminous Ly α emitters from z ∼ 2 to z ∼ 6: Evidence for a diverse, evolving population. <i>Monthly Notices of the Royal Astronomical Society</i>. Oxford University Press. <a href=\"https://doi.org/10.1093/mnras/staa476\">https://doi.org/10.1093/mnras/staa476</a>","mla":"Calhau, João, et al. “The X-Ray and Radio Activity of Typical and Luminous Ly α Emitters from z ∼ 2 to z ∼ 6: Evidence for a Diverse, Evolving Population.” <i>Monthly Notices of the Royal Astronomical Society</i>, vol. 493, no. 3, Oxford University Press, 2020, pp. 3341–62, doi:<a href=\"https://doi.org/10.1093/mnras/staa476\">10.1093/mnras/staa476</a>."},"article_processing_charge":"No","title":"The X-ray and radio activity of typical and luminous Ly α emitters from z ∼ 2 to z ∼ 6: Evidence for a diverse, evolving population","type":"journal_article","status":"public"},{"author":[{"orcid":"0000-0003-2871-127X","first_name":"Jorryt J","last_name":"Matthee","full_name":"Matthee, Jorryt J","id":"7439a258-f3c0-11ec-9501-9df22fe06720"},{"first_name":"David","last_name":"Sobral","full_name":"Sobral, David"}],"date_published":"2020-06-04T00:00:00Z","abstract":[{"lang":"eng","text":"Distant luminous Lyman-α emitters are excellent targets for detailed observations of galaxies in the epoch of reionisation. Spatially resolved observations of these galaxies allow us to simultaneously probe the emission from young stars, partially ionised gas in the interstellar medium and to constrain the properties of the surrounding hydrogen in the circumgalactic medium. We review recent results from (spectroscopic) follow-up studies of the rest-frame UV, Lyman-α and [CII] emission in luminous galaxies observed ∼500 Myr after the Big Bang with ALMA, HST/WFC3 and VLT/X-SHOOTER. These galaxies likely reside in early ionised bubbles and are complex systems, consisting of multiple well separated and resolved components where traces of metals are already present."}],"volume":15,"issue":"S352","keyword":["Astronomy and Astrophysics","Space and Planetary Science","galaxies: formation","galaxies: evolution","galaxies: high-redshift"],"publication":"Proceedings of the International Astronomical Union","language":[{"iso":"eng"}],"year":"2020","day":"04","scopus_import":"1","main_file_link":[{"open_access":"1","url":"https://arxiv.org/abs/1911.04774"}],"publisher":"Cambridge University Press","date_created":"2022-07-14T14:08:41Z","arxiv":1,"oa":1,"publication_status":"published","publication_identifier":{"eissn":["1743-9221"],"issn":["1743-9213"]},"date_updated":"2022-08-19T08:41:12Z","month":"06","oa_version":"Preprint","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","title":"Unveiling the most luminous Lyman-α emitters in the epoch of reionisation","status":"public","type":"conference","article_processing_charge":"No","extern":"1","citation":{"mla":"Matthee, Jorryt J., and David Sobral. “Unveiling the Most Luminous Lyman-α Emitters in the Epoch of Reionisation.” <i>Proceedings of the International Astronomical Union</i>, vol. 15, no. S352, Cambridge University Press, 2020, pp. 21–25, doi:<a href=\"https://doi.org/10.1017/s1743921319009451\">10.1017/s1743921319009451</a>.","apa":"Matthee, J. J., &#38; Sobral, D. (2020). Unveiling the most luminous Lyman-α emitters in the epoch of reionisation. In <i>Proceedings of the International Astronomical Union</i> (Vol. 15, pp. 21–25). Cambridge University Press. <a href=\"https://doi.org/10.1017/s1743921319009451\">https://doi.org/10.1017/s1743921319009451</a>","ama":"Matthee JJ, Sobral D. Unveiling the most luminous Lyman-α emitters in the epoch of reionisation. In: <i>Proceedings of the International Astronomical Union</i>. Vol 15. Cambridge University Press; 2020:21-25. doi:<a href=\"https://doi.org/10.1017/s1743921319009451\">10.1017/s1743921319009451</a>","chicago":"Matthee, Jorryt J, and David Sobral. “Unveiling the Most Luminous Lyman-α Emitters in the Epoch of Reionisation.” In <i>Proceedings of the International Astronomical Union</i>, 15:21–25. Cambridge University Press, 2020. <a href=\"https://doi.org/10.1017/s1743921319009451\">https://doi.org/10.1017/s1743921319009451</a>.","short":"J.J. Matthee, D. Sobral, in:, Proceedings of the International Astronomical Union, Cambridge University Press, 2020, pp. 21–25.","ieee":"J. J. Matthee and D. Sobral, “Unveiling the most luminous Lyman-α emitters in the epoch of reionisation,” in <i>Proceedings of the International Astronomical Union</i>, 2020, vol. 15, no. S352, pp. 21–25.","ista":"Matthee JJ, Sobral D. 2020. Unveiling the most luminous Lyman-α emitters in the epoch of reionisation. Proceedings of the International Astronomical Union. vol. 15, 21–25."},"quality_controlled":"1","external_id":{"arxiv":["1911.04774"]},"doi":"10.1017/s1743921319009451","intvolume":"        15","_id":"11586","page":"21-25"},{"intvolume":"       251","_id":"11610","external_id":{"arxiv":["2012.04051"]},"doi":"10.3847/1538-4365/abbee3","quality_controlled":"1","acknowledgement":"We thank the referee for comments that strengthened the manuscript. J. C. Z. and M. H. P. acknowledge support from NASA grants 80NSSC18K0391 and NNX17AJ40G. Y. E. and C. J. acknowledge the support of the UK Science and Technology Facilities Council (STFC). S. M. would like to acknowledge support from the Spanish Ministry with the Ramon y Cajal fellowship number RYC-2015-17697. R. A. G. acknowledges funding received from the PLATO CNES grant. R. S. acknowledges funding via a Royal Society University Research Fellowship. D.H. acknowledges support from the Alfred P. Sloan Foundation and the National Aeronautics and Space Administration (80NSSC19K0108). V.S.A. acknowledges support from the Independent Research Fund Denmark (Research grant 7027-00096B), and the Carlsberg foundation (grant agreement CF19-0649). This research was supported in part by the National Science Foundation under grant No. NSF PHY-1748958.\r\n\r\nFunding for the Stellar Astrophysics Centre (SAC) is provided by The Danish National Research Foundation (grant agreement No. DNRF106).\r\n\r\nThe K2 Galactic Archaeology Program is supported by the National Aeronautics and Space Administration under grant NNX16AJ17G issued through the K2 Guest Observer Program.\r\n\r\nThis publication makes use of data products from the Two Micron All Sky Survey, which is a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation.\r\n\r\nThis work has made use of data from the European Space Agency (ESA) mission Gaia (https://www.cosmos.esa.int/gaia), processed by the Gaia Data Processing and Analysis Consortium (DPAC, https://www.cosmos.esa.int/web/gaia/dpac/consortium). Funding for the DPAC has been provided by national institutions, in particular the institutions participating in the Gaia Multilateral Agreement.\r\n\r\nFunding for the Sloan Digital Sky Survey IV has been provided by the Alfred P. Sloan Foundation, the U.S. Department of Energy Office of Science, and the Participating Institutions. SDSS-IV acknowledges support and resources from the Center for High Performance Computing at the University of Utah. The SDSS website is www.sdss.org.\r\n\r\nSDSS-IV is managed by the Astrophysical Research Consortium for the Participating Institutions of the SDSS Collaboration, including the Brazilian Participation Group, the Carnegie Institution for Science, Carnegie Mellon University, the Chilean Participation Group, the French Participation Group, the Harvard–Smithsonian Center for Astrophysics, Instituto de Astrofísica de Canarias, The Johns Hopkins University, Kavli Institute for the Physics and Mathematics of the Universe (IPMU)/University of Tokyo, the Korean Participation Group, Lawrence Berkeley National Laboratory, Leibniz Institut für Astrophysik Potsdam (AIP), Max-Planck-Institut für Astronomie (MPIA Heidelberg), Max-Planck-Institut für Astrophysik (MPA Garching), Max-Planck-Institut für Extraterrestrische Physik (MPE), National Astronomical Observatories of China, New Mexico State University, New York University, University of Notre Dame, Observatário Nacional/MCTI, The Ohio State University, Pennsylvania State University, Shanghai Astronomical Observatory, United Kingdom Participation Group, Universidad Nacional Autónoma de México, University of Arizona, University of Colorado Boulder, University of Oxford, University of Portsmouth, University of Utah, University of Virginia, University of Washington, University of Wisconsin, Vanderbilt University, and Yale University.\r\n\r\nSoftware: asfgrid (Sharma & Stello 2016), emcee (Foreman-Mackey et al. 2013), NumPy (Walt 2011), pandas (McKinney 2010; Reback et al. 2020), Matplotlib (Hunter 2007), IPython (Pérez & Granger 2007), SciPy (Virtanen et al. 2020).","article_processing_charge":"No","extern":"1","citation":{"ieee":"J. C. Zinn <i>et al.</i>, “The K2 galactic archaeology program data release 2: Asteroseismic results from campaigns 4, 6, and 7,” <i>The Astrophysical Journal Supplement Series</i>, vol. 251, no. 2. IOP Publishing, 2020.","ista":"Zinn JC, Stello D, Elsworth Y, García RA, Kallinger T, Mathur S, Mosser B, Bugnet LA, Jones C, Hon M, Sharma S, Schönrich R, Warfield JT, Luger R, Pinsonneault MH, Johnson JA, Huber D, Aguirre VS, Chaplin WJ, Davies GR, Miglio A. 2020. The K2 galactic archaeology program data release 2: Asteroseismic results from campaigns 4, 6, and 7. The Astrophysical Journal Supplement Series. 251(2), 23.","apa":"Zinn, J. C., Stello, D., Elsworth, Y., García, R. A., Kallinger, T., Mathur, S., … Miglio, A. (2020). The K2 galactic archaeology program data release 2: Asteroseismic results from campaigns 4, 6, and 7. <i>The Astrophysical Journal Supplement Series</i>. IOP Publishing. <a href=\"https://doi.org/10.3847/1538-4365/abbee3\">https://doi.org/10.3847/1538-4365/abbee3</a>","mla":"Zinn, Joel C., et al. “The K2 Galactic Archaeology Program Data Release 2: Asteroseismic Results from Campaigns 4, 6, and 7.” <i>The Astrophysical Journal Supplement Series</i>, vol. 251, no. 2, 23, IOP Publishing, 2020, doi:<a href=\"https://doi.org/10.3847/1538-4365/abbee3\">10.3847/1538-4365/abbee3</a>.","short":"J.C. Zinn, D. Stello, Y. Elsworth, R.A. García, T. Kallinger, S. Mathur, B. Mosser, L.A. Bugnet, C. Jones, M. Hon, S. Sharma, R. Schönrich, J.T. Warfield, R. Luger, M.H. Pinsonneault, J.A. Johnson, D. Huber, V.S. Aguirre, W.J. Chaplin, G.R. Davies, A. Miglio, The Astrophysical Journal Supplement Series 251 (2020).","ama":"Zinn JC, Stello D, Elsworth Y, et al. The K2 galactic archaeology program data release 2: Asteroseismic results from campaigns 4, 6, and 7. <i>The Astrophysical Journal Supplement Series</i>. 2020;251(2). doi:<a href=\"https://doi.org/10.3847/1538-4365/abbee3\">10.3847/1538-4365/abbee3</a>","chicago":"Zinn, Joel C., Dennis Stello, Yvonne Elsworth, Rafael A. García, Thomas Kallinger, Savita Mathur, Benoît Mosser, et al. “The K2 Galactic Archaeology Program Data Release 2: Asteroseismic Results from Campaigns 4, 6, and 7.” <i>The Astrophysical Journal Supplement Series</i>. IOP Publishing, 2020. <a href=\"https://doi.org/10.3847/1538-4365/abbee3\">https://doi.org/10.3847/1538-4365/abbee3</a>."},"type":"journal_article","status":"public","title":"The K2 galactic archaeology program data release 2: Asteroseismic results from campaigns 4, 6, and 7","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","month":"12","oa_version":"Preprint","publication_identifier":{"issn":["0067-0049"],"eissn":["1538-4365"]},"date_updated":"2022-08-22T07:04:45Z","publication_status":"published","oa":1,"arxiv":1,"article_number":"23","date_created":"2022-07-18T13:27:26Z","article_type":"original","main_file_link":[{"url":"https://arxiv.org/abs/2012.04051","open_access":"1"}],"publisher":"IOP Publishing","scopus_import":"1","language":[{"iso":"eng"}],"year":"2020","day":"01","publication":"The Astrophysical Journal Supplement Series","keyword":["Space and Planetary Science","Astronomy and Astrophysics"],"issue":"2","date_published":"2020-12-01T00:00:00Z","abstract":[{"lang":"eng","text":"Studies of Galactic structure and evolution have benefited enormously from Gaia kinematic information, though additional, intrinsic stellar parameters like age are required to best constrain Galactic models. Asteroseismology is the most precise method of providing such information for field star populations en masse, but existing samples for the most part have been limited to a few narrow fields of view by the CoRoT and Kepler missions. In an effort to provide well-characterized stellar parameters across a wide range in Galactic position, we present the second data release of red giant asteroseismic parameters for the K2 Galactic Archaeology Program (GAP). We provide ${\\nu }_{\\max }$ and ${\\rm{\\Delta }}\\nu $ based on six independent pipeline analyses; first-ascent red giant branch (RGB) and red clump (RC) evolutionary state classifications from machine learning; and ready-to-use radius and mass coefficients, κR and κM, which, when appropriately multiplied by a solar-scaled effective temperature factor, yield physical stellar radii and masses. In total, we report 4395 radius and mass coefficients, with typical uncertainties of 3.3% (stat.) ± 1% (syst.) for κR and 7.7% (stat.) ± 2% (syst.) for κM among RGB stars, and 5.0% (stat.) ± 1% (syst.) for κR and 10.5% (stat.) ± 2% (syst.) for κM among RC stars. We verify that the sample is nearly complete—except for a dearth of stars with ${\\nu }_{\\max }\\lesssim 10\\mbox{--}20\\,\\mu \\mathrm{Hz}$—by comparing to Galactic models and visual inspection. Our asteroseismic radii agree with radii derived from Gaia Data Release 2 parallaxes to within 2.2% ± 0.3% for RGB stars and 2.0% ± 0.6% for RC stars."}],"volume":251,"author":[{"full_name":"Zinn, Joel C.","first_name":"Joel C.","last_name":"Zinn"},{"last_name":"Stello","first_name":"Dennis","full_name":"Stello, Dennis"},{"last_name":"Elsworth","first_name":"Yvonne","full_name":"Elsworth, Yvonne"},{"full_name":"García, Rafael A.","last_name":"García","first_name":"Rafael A."},{"last_name":"Kallinger","first_name":"Thomas","full_name":"Kallinger, Thomas"},{"first_name":"Savita","last_name":"Mathur","full_name":"Mathur, Savita"},{"full_name":"Mosser, Benoît","last_name":"Mosser","first_name":"Benoît"},{"orcid":"0000-0003-0142-4000","first_name":"Lisa Annabelle","last_name":"Bugnet","full_name":"Bugnet, Lisa Annabelle","id":"d9edb345-f866-11ec-9b37-d119b5234501"},{"last_name":"Jones","first_name":"Caitlin","full_name":"Jones, Caitlin"},{"first_name":"Marc","last_name":"Hon","full_name":"Hon, Marc"},{"full_name":"Sharma, Sanjib","last_name":"Sharma","first_name":"Sanjib"},{"full_name":"Schönrich, Ralph","first_name":"Ralph","last_name":"Schönrich"},{"full_name":"Warfield, Jack T.","first_name":"Jack T.","last_name":"Warfield"},{"last_name":"Luger","first_name":"Rodrigo","full_name":"Luger, Rodrigo"},{"full_name":"Pinsonneault, Marc H.","first_name":"Marc H.","last_name":"Pinsonneault"},{"full_name":"Johnson, Jennifer A.","last_name":"Johnson","first_name":"Jennifer A."},{"full_name":"Huber, Daniel","last_name":"Huber","first_name":"Daniel"},{"last_name":"Aguirre","first_name":"Victor Silva","full_name":"Aguirre, Victor Silva"},{"first_name":"William J.","last_name":"Chaplin","full_name":"Chaplin, William J."},{"first_name":"Guy R.","last_name":"Davies","full_name":"Davies, Guy R."},{"last_name":"Miglio","first_name":"Andrea","full_name":"Miglio, Andrea"}]},{"author":[{"first_name":"William J.","last_name":"Chaplin","full_name":"Chaplin, William J."},{"full_name":"Serenelli, Aldo M.","last_name":"Serenelli","first_name":"Aldo M."},{"last_name":"Miglio","first_name":"Andrea","full_name":"Miglio, Andrea"},{"full_name":"Morel, Thierry","last_name":"Morel","first_name":"Thierry"},{"full_name":"Mackereth, J. Ted","first_name":"J. Ted","last_name":"Mackereth"},{"first_name":"Fiorenzo","last_name":"Vincenzo","full_name":"Vincenzo, Fiorenzo"},{"last_name":"Kjeldsen","first_name":"Hans","full_name":"Kjeldsen, Hans"},{"first_name":"Sarbani","last_name":"Basu","full_name":"Basu, Sarbani"},{"first_name":"Warrick H.","last_name":"Ball","full_name":"Ball, Warrick H."},{"full_name":"Stokholm, Amalie","first_name":"Amalie","last_name":"Stokholm"},{"last_name":"Verma","first_name":"Kuldeep","full_name":"Verma, Kuldeep"},{"first_name":"Jakob Rørsted","last_name":"Mosumgaard","full_name":"Mosumgaard, Jakob Rørsted"},{"full_name":"Silva Aguirre, Victor","first_name":"Victor","last_name":"Silva Aguirre"},{"full_name":"Mazumdar, Anwesh","first_name":"Anwesh","last_name":"Mazumdar"},{"full_name":"Ranadive, Pritesh","last_name":"Ranadive","first_name":"Pritesh"},{"last_name":"Antia","first_name":"H. M.","full_name":"Antia, H. M."},{"last_name":"Lebreton","first_name":"Yveline","full_name":"Lebreton, Yveline"},{"full_name":"Ong, Joel","last_name":"Ong","first_name":"Joel"},{"first_name":"Thierry","last_name":"Appourchaux","full_name":"Appourchaux, Thierry"},{"last_name":"Bedding","first_name":"Timothy R.","full_name":"Bedding, Timothy R."},{"last_name":"Christensen-Dalsgaard","first_name":"Jørgen","full_name":"Christensen-Dalsgaard, Jørgen"},{"last_name":"Creevey","first_name":"Orlagh","full_name":"Creevey, Orlagh"},{"full_name":"García, Rafael A.","last_name":"García","first_name":"Rafael A."},{"first_name":"Rasmus","last_name":"Handberg","full_name":"Handberg, Rasmus"},{"full_name":"Huber, Daniel","first_name":"Daniel","last_name":"Huber"},{"full_name":"Kawaler, Steven D.","last_name":"Kawaler","first_name":"Steven D."},{"first_name":"Mikkel N.","last_name":"Lund","full_name":"Lund, Mikkel N."},{"first_name":"Travis S.","last_name":"Metcalfe","full_name":"Metcalfe, Travis S."},{"first_name":"Keivan G.","last_name":"Stassun","full_name":"Stassun, Keivan G."},{"full_name":"Bazot, Michäel","first_name":"Michäel","last_name":"Bazot"},{"full_name":"Beck, Paul G.","first_name":"Paul G.","last_name":"Beck"},{"last_name":"Bell","first_name":"Keaton J.","full_name":"Bell, Keaton J."},{"last_name":"Bergemann","first_name":"Maria","full_name":"Bergemann, Maria"},{"first_name":"Derek L.","last_name":"Buzasi","full_name":"Buzasi, Derek L."},{"last_name":"Benomar","first_name":"Othman","full_name":"Benomar, Othman"},{"last_name":"Bossini","first_name":"Diego","full_name":"Bossini, Diego"},{"full_name":"Bugnet, Lisa Annabelle","id":"d9edb345-f866-11ec-9b37-d119b5234501","last_name":"Bugnet","first_name":"Lisa Annabelle","orcid":"0000-0003-0142-4000"},{"first_name":"Tiago L.","last_name":"Campante","full_name":"Campante, Tiago L."},{"last_name":"Orhan","first_name":"Zeynep Çelik","full_name":"Orhan, Zeynep Çelik"},{"full_name":"Corsaro, Enrico","first_name":"Enrico","last_name":"Corsaro"},{"full_name":"González-Cuesta, Lucía","last_name":"González-Cuesta","first_name":"Lucía"},{"full_name":"Davies, Guy R.","last_name":"Davies","first_name":"Guy R."},{"full_name":"Di Mauro, Maria Pia","last_name":"Di Mauro","first_name":"Maria Pia"},{"full_name":"Egeland, Ricky","first_name":"Ricky","last_name":"Egeland"},{"full_name":"Elsworth, Yvonne P.","last_name":"Elsworth","first_name":"Yvonne P."},{"full_name":"Gaulme, Patrick","last_name":"Gaulme","first_name":"Patrick"},{"full_name":"Ghasemi, Hamed","last_name":"Ghasemi","first_name":"Hamed"},{"first_name":"Zhao","last_name":"Guo","full_name":"Guo, Zhao"},{"first_name":"Oliver J.","last_name":"Hall","full_name":"Hall, Oliver J."},{"first_name":"Amir","last_name":"Hasanzadeh","full_name":"Hasanzadeh, Amir"},{"full_name":"Hekker, Saskia","last_name":"Hekker","first_name":"Saskia"},{"last_name":"Howe","first_name":"Rachel","full_name":"Howe, Rachel"},{"full_name":"Jenkins, Jon M.","last_name":"Jenkins","first_name":"Jon M."},{"last_name":"Jiménez","first_name":"Antonio","full_name":"Jiménez, Antonio"},{"full_name":"Kiefer, René","first_name":"René","last_name":"Kiefer"},{"first_name":"James S.","last_name":"Kuszlewicz","full_name":"Kuszlewicz, James S."},{"first_name":"Thomas","last_name":"Kallinger","full_name":"Kallinger, Thomas"},{"first_name":"David W.","last_name":"Latham","full_name":"Latham, David W."},{"full_name":"Lundkvist, Mia S.","last_name":"Lundkvist","first_name":"Mia S."},{"last_name":"Mathur","first_name":"Savita","full_name":"Mathur, Savita"},{"last_name":"Montalbán","first_name":"Josefina","full_name":"Montalbán, Josefina"},{"first_name":"Benoit","last_name":"Mosser","full_name":"Mosser, Benoit"},{"full_name":"Bedón, Andres Moya","first_name":"Andres Moya","last_name":"Bedón"},{"last_name":"Nielsen","first_name":"Martin Bo","full_name":"Nielsen, Martin Bo"},{"full_name":"Örtel, Sibel","first_name":"Sibel","last_name":"Örtel"},{"first_name":"Ben M.","last_name":"Rendle","full_name":"Rendle, Ben M."},{"full_name":"Ricker, George R.","last_name":"Ricker","first_name":"George R."},{"first_name":"Thaíse S.","last_name":"Rodrigues","full_name":"Rodrigues, Thaíse S."},{"full_name":"Roxburgh, Ian W.","last_name":"Roxburgh","first_name":"Ian W."},{"full_name":"Safari, Hossein","first_name":"Hossein","last_name":"Safari"},{"last_name":"Schofield","first_name":"Mathew","full_name":"Schofield, Mathew"},{"full_name":"Seager, Sara","first_name":"Sara","last_name":"Seager"},{"full_name":"Smalley, Barry","first_name":"Barry","last_name":"Smalley"},{"first_name":"Dennis","last_name":"Stello","full_name":"Stello, Dennis"},{"first_name":"Róbert","last_name":"Szabó","full_name":"Szabó, Róbert"},{"full_name":"Tayar, Jamie","first_name":"Jamie","last_name":"Tayar"},{"full_name":"Themeßl, Nathalie","last_name":"Themeßl","first_name":"Nathalie"},{"full_name":"Thomas, Alexandra E. L.","first_name":"Alexandra E. L.","last_name":"Thomas"},{"first_name":"Roland K.","last_name":"Vanderspek","full_name":"Vanderspek, Roland K."},{"full_name":"van Rossem, Walter E.","first_name":"Walter E.","last_name":"van Rossem"},{"last_name":"Vrard","first_name":"Mathieu","full_name":"Vrard, Mathieu"},{"last_name":"Weiss","first_name":"Achim","full_name":"Weiss, Achim"},{"first_name":"Timothy R.","last_name":"White","full_name":"White, Timothy R."},{"full_name":"Winn, Joshua N.","first_name":"Joshua N.","last_name":"Winn"},{"last_name":"Yıldız","first_name":"Mutlu","full_name":"Yıldız, Mutlu"}],"date_published":"2020-04-01T00:00:00Z","volume":4,"abstract":[{"text":"Over the course of its history, the Milky Way has ingested multiple smaller satellite galaxies1. Although these accreted stellar populations can be forensically identified as kinematically distinct structures within the Galaxy, it is difficult in general to date precisely the age at which any one merger occurred. Recent results have revealed a population of stars that were accreted via the collision of a dwarf galaxy, called Gaia–Enceladus1, leading to substantial pollution of the chemical and dynamical properties of the Milky Way. Here we identify the very bright, naked-eye star ν Indi as an indicator of the age of the early in situ population of the Galaxy. We combine asteroseismic, spectroscopic, astrometric and kinematic observations to show that this metal-poor, alpha-element-rich star was an indigenous member of the halo, and we measure its age to be 11.0±0.7 (stat) ±0.8 (sys) billion years. The star bears hallmarks consistent with having been kinematically heated by the Gaia–Enceladus collision. Its age implies that the earliest the merger could have begun was 11.6 and 13.2 billion years ago, at 68% and 95% confidence, respectively. Computations based on hierarchical cosmological models slightly reduce the above limits.","lang":"eng"}],"issue":"4","keyword":["Astronomy and Astrophysics"],"publication":"Nature Astronomy","year":"2020","language":[{"iso":"eng"}],"day":"01","scopus_import":"1","main_file_link":[{"open_access":"1","url":"https://arxiv.org/abs/2001.04653"}],"publisher":"Springer Nature","article_type":"letter_note","date_created":"2022-07-18T13:36:19Z","arxiv":1,"oa":1,"publication_status":"published","publication_identifier":{"eissn":["2397-3366"]},"date_updated":"2022-08-22T07:08:29Z","month":"04","oa_version":"Preprint","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","title":"Age dating of an early Milky Way merger via asteroseismology of the naked-eye star ν Indi","type":"journal_article","status":"public","extern":"1","citation":{"ieee":"W. J. Chaplin <i>et al.</i>, “Age dating of an early Milky Way merger via asteroseismology of the naked-eye star ν Indi,” <i>Nature Astronomy</i>, vol. 4, no. 4. Springer Nature, pp. 382–389, 2020.","ista":"Chaplin WJ, Serenelli AM, Miglio A, Morel T, Mackereth JT, Vincenzo F, Kjeldsen H, Basu S, Ball WH, Stokholm A, Verma K, Mosumgaard JR, Silva Aguirre V, Mazumdar A, Ranadive P, Antia HM, Lebreton Y, Ong J, Appourchaux T, Bedding TR, Christensen-Dalsgaard J, Creevey O, García RA, Handberg R, Huber D, Kawaler SD, Lund MN, Metcalfe TS, Stassun KG, Bazot M, Beck PG, Bell KJ, Bergemann M, Buzasi DL, Benomar O, Bossini D, Bugnet LA, Campante TL, Orhan ZÇ, Corsaro E, González-Cuesta L, Davies GR, Di Mauro MP, Egeland R, Elsworth YP, Gaulme P, Ghasemi H, Guo Z, Hall OJ, Hasanzadeh A, Hekker S, Howe R, Jenkins JM, Jiménez A, Kiefer R, Kuszlewicz JS, Kallinger T, Latham DW, Lundkvist MS, Mathur S, Montalbán J, Mosser B, Bedón AM, Nielsen MB, Örtel S, Rendle BM, Ricker GR, Rodrigues TS, Roxburgh IW, Safari H, Schofield M, Seager S, Smalley B, Stello D, Szabó R, Tayar J, Themeßl N, Thomas AEL, Vanderspek RK, van Rossem WE, Vrard M, Weiss A, White TR, Winn JN, Yıldız M. 2020. Age dating of an early Milky Way merger via asteroseismology of the naked-eye star ν Indi. Nature Astronomy. 4(4), 382–389.","chicago":"Chaplin, William J., Aldo M. Serenelli, Andrea Miglio, Thierry Morel, J. Ted Mackereth, Fiorenzo Vincenzo, Hans Kjeldsen, et al. “Age Dating of an Early Milky Way Merger via Asteroseismology of the Naked-Eye Star ν Indi.” <i>Nature Astronomy</i>. Springer Nature, 2020. <a href=\"https://doi.org/10.1038/s41550-019-0975-9\">https://doi.org/10.1038/s41550-019-0975-9</a>.","ama":"Chaplin WJ, Serenelli AM, Miglio A, et al. Age dating of an early Milky Way merger via asteroseismology of the naked-eye star ν Indi. <i>Nature Astronomy</i>. 2020;4(4):382-389. doi:<a href=\"https://doi.org/10.1038/s41550-019-0975-9\">10.1038/s41550-019-0975-9</a>","short":"W.J. Chaplin, A.M. Serenelli, A. Miglio, T. Morel, J.T. Mackereth, F. Vincenzo, H. Kjeldsen, S. Basu, W.H. Ball, A. Stokholm, K. Verma, J.R. Mosumgaard, V. Silva Aguirre, A. Mazumdar, P. Ranadive, H.M. Antia, Y. Lebreton, J. Ong, T. Appourchaux, T.R. Bedding, J. Christensen-Dalsgaard, O. Creevey, R.A. García, R. Handberg, D. Huber, S.D. Kawaler, M.N. Lund, T.S. Metcalfe, K.G. Stassun, M. Bazot, P.G. Beck, K.J. Bell, M. Bergemann, D.L. Buzasi, O. Benomar, D. Bossini, L.A. Bugnet, T.L. Campante, Z.Ç. Orhan, E. Corsaro, L. González-Cuesta, G.R. Davies, M.P. Di Mauro, R. Egeland, Y.P. Elsworth, P. Gaulme, H. Ghasemi, Z. Guo, O.J. Hall, A. Hasanzadeh, S. Hekker, R. Howe, J.M. Jenkins, A. Jiménez, R. Kiefer, J.S. Kuszlewicz, T. Kallinger, D.W. Latham, M.S. Lundkvist, S. Mathur, J. Montalbán, B. Mosser, A.M. Bedón, M.B. Nielsen, S. Örtel, B.M. Rendle, G.R. Ricker, T.S. Rodrigues, I.W. Roxburgh, H. Safari, M. Schofield, S. Seager, B. Smalley, D. Stello, R. Szabó, J. Tayar, N. Themeßl, A.E.L. Thomas, R.K. Vanderspek, W.E. van Rossem, M. Vrard, A. Weiss, T.R. White, J.N. Winn, M. Yıldız, Nature Astronomy 4 (2020) 382–389.","mla":"Chaplin, William J., et al. “Age Dating of an Early Milky Way Merger via Asteroseismology of the Naked-Eye Star ν Indi.” <i>Nature Astronomy</i>, vol. 4, no. 4, Springer Nature, 2020, pp. 382–89, doi:<a href=\"https://doi.org/10.1038/s41550-019-0975-9\">10.1038/s41550-019-0975-9</a>.","apa":"Chaplin, W. J., Serenelli, A. M., Miglio, A., Morel, T., Mackereth, J. T., Vincenzo, F., … Yıldız, M. (2020). Age dating of an early Milky Way merger via asteroseismology of the naked-eye star ν Indi. <i>Nature Astronomy</i>. Springer Nature. <a href=\"https://doi.org/10.1038/s41550-019-0975-9\">https://doi.org/10.1038/s41550-019-0975-9</a>"},"article_processing_charge":"No","quality_controlled":"1","acknowledgement":"This paper includes data collected by the TESS mission, which are publicly available from the Mikulski Archive for Space Telescopes (MAST). Resources supporting this work were provided by the NASA High-End Computing (HEC) Program through the NASA Advanced Supercomputing (NAS) Division at Ames Research Center for the production of the SPOC data products. W.J.C. acknowledges support from the UK Science and Technology Facilities Council (STFC) and UK Space Agency. Funding for the Stellar Astrophysics Centre is provided by The Danish National Research Foundation (grant agreement number DNRF106). This research was partially conducted during the Exostar19 programme at the Kavli Institute for Theoretical Physics at UC Santa Barbara, which was supported in part by the National Science Foundation under grant number NSF PHY-1748958. A.M., J.T.M., F.V. and J.M. acknowledge support from the ERC Consolidator Grant funding scheme (project ASTEROCHRONOMETRY, grant agreement number 772293). F.V. acknowledges the support of a Fellowship from the Center for Cosmology and AstroParticle Physics at The Ohio State University. W.H.B. and M.B.N. acknowledge support from the UK Space Agency. K.J.B. is supported by the National Science Foundation under award AST-1903828. M.B.N. acknowledges partial support from the NYU Abu Dhabi Center for Space Science under grant number G1502. A.M.S. is partially supported by the Spanish Government (ESP2017-82674-R) and Generalitat de Catalunya (2017-SGR-1131). T.M. acknowledges financial support from Belspo for contract PRODEX PLATO. H.K. acknowledges support from the European Social Fund via the Lithuanian Science Council grant number 09.3.3-LMT-K-712-01-0103. S.B. acknowledges support from NSF grant AST-1514676 and NASA grant 80NSSC19K0374. V.S.A. acknowledges support from the Independent Research Fund Denmark (research grant 7027-00096B). D.H. acknowledges support by the National Aeronautics and Space Administration (80NSSC18K1585, 80NSSC19K0379) awarded through the TESS Guest Investigator Program and by the National Science Foundation (AST-1717000). T.S.M. acknowledges support from a visiting fellowship at the Max Planck Institute for Solar System Research. Computational resources were provided through XSEDE allocation TG-AST090107. D.L.B. acknowledges support from NASA under grant NNX16AB76G. T.L.C. acknowledges support from the European Union’s Horizon 2020 research and innovation programme under the Marie Skłodowska-Curie grant agreement number 792848 (PULSATION). This work was supported by FCT/MCTES through national funds (PIDDAC) by means of grant UID/FIS/04434/2019. K.J.B., S.H., J.S.K. and N.T. are supported by the European Research Council under the European Community’s Seventh Framework Programme (FP7/2007-2013)/ERC grant agreement number 338251 (StellarAges). E.C. is funded by the European Union’s Horizon 2020 research and innovation program under the Marie Sklodowska-Curie grant agreement number 664931. L.G.-C. acknowledges support from the MINECO FPI-SO doctoral research project SEV-2015-0548-17-2 and predoctoral contract BES-2017-082610. P.G. is supported by the German space agency (Deutsches Zentrum für Luft- und Raumfahrt) under PLATO data grant 50OO1501. R.K. acknowledges support from the UK Science and Technology Facilities Council (STFC), under consolidated grant ST/L000733/1. M.S.L. is supported by the Carlsberg Foundation (grant agreement number CF17-076). Z.C.O., S.O. and M.Y. acknowledge support from the Scientific and Technological Research Council of Turkey (TÜBİTAK:118F352). S.M. acknowledges support from the Spanish ministry through the Ramon y Cajal fellowship number RYC-2015-17697. T.S.R. acknowledges financial support from Premiale 2015 MITiC (PI B. Garilli). R.Sz. acknowledges the support from NKFIH grant project No. K-115709, and the Lendület program of the Hungarian Academy of Science (project number 2018-7/2019). J.T. acknowledges support was provided by NASA through the NASA Hubble Fellowship grant number 51424 awarded by the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., for NASA, under contract NAS5-26555. This work was supported by FEDER through COMPETE2020 (POCI-01-0145-FEDER-030389. A.M.B. acknowledges funding from the European Union’s Horizon 2020 research and innovation program under the Marie Sklodowska-Curie grant agreement No 749962 (project THOT). A.M. and P.R. acknowledge the support of the Government of India, Department of Atomic Energy, under Project No. 12-R&D-TFR-6.04-0600. K.J.B. is an NSF Astronomy and Astrophysics Postdoctoral Fellow and DIRAC Fellow.","external_id":{"arxiv":["2001.04653"]},"doi":"10.1038/s41550-019-0975-9","intvolume":"         4","_id":"11611","page":"382-389"},{"month":"02","oa_version":"Preprint","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","publication_status":"published","oa":1,"date_updated":"2022-08-22T07:25:51Z","publication_identifier":{"issn":["0004-637X"],"eissn":["1538-4357"]},"arxiv":1,"article_number":"L34","doi":"10.3847/2041-8213/ab6443","external_id":{"arxiv":["1912.07604"]},"_id":"11612","intvolume":"       889","acknowledgement":"This Letter includes data collected by the TESS mission, which are publicly available from the Mikulski Archive for Space Telescopes (MAST). Funding for the TESS mission is provided by NASA's Science Mission directorate. Funding for the TESS Asteroseismic Science Operations Centre is provided by the Danish National Research Foundation (grant agreement No. DNRF106), ESA PRODEX (PEA 4000119301), and Stellar Astrophysics Centre (SAC) at Aarhus University. V.S.A. acknowledges support from the Independent Research Fund Denmark (Research grant 7027-00096B). D.B. is supported in the form of work contract FCT/MCTES through national funds and by FEDER through COMPETE2020 in connection to these grants: UID/FIS/04434/2019; PTDC/FIS-AST/30389/2017 & POCI-01-0145-FEDER-030389. L.B., R.A.G., and B.M. acknowledge the support from the CNES/PLATO grant. D.B. acknowledges NASA grant NNX16AB76G. T.L.C. acknowledges support from the European Union's Horizon 2020 research and innovation programme under the Marie Skłodowska-Curie grant agreement No. 792848 (PULSATION). This work was supported by FCT/MCTES through national funds (UID/FIS/04434/2019). E.C. is funded by the European Union's Horizon 2020 research and innovation program under the Marie Skłodowska-Curie grant agreement No. 664931. R.H. and M.N.L. acknowledge the support of the ESA PRODEX programme. T.S.R. acknowledges financial support from Premiale 2015 MITiC (PI B. Garilli). K.J.B. is supported by the National Science Foundation under Award AST-1903828. M.S.L. is supported by the Carlsberg Foundation (grant agreement No. CF17-0760). M.C. is funded by FCT//MCTES through national funds and by FEDER through COMPETE2020 through these grants: UID/FIS/04434/2019, PTDC/FIS-AST/30389/2017 & POCI-01-0145-FEDER-030389, CEECIND/02619/2017. The research leading to the presented results has received funding from the European Research Council under the European Community's Seventh Framework Programme (FP7/2007-2013)/ERC grant agreement no 338251 (StellarAges). A.M. acknowledges support from the European Research Council Consolidator Grant funding scheme (project ASTEROCHRONOMETRY, grant agreement No. 772293, http://www.asterochronometry.eu). A.M.S. is partially supported by MINECO grant ESP2017-82674-R. J.C.S. acknowledges funding support from Spanish public funds for research under projects ESP2017-87676-2-2, and from project RYC-2012-09913 under the 'Ramón y Cajal' program of the Spanish Ministry of Science and Education. Resources supporting this work were provided by the NASA High-End Computing (HEC) Program through the NASA Advanced Supercomputing (NAS) Division at Ames Research Center for the production of the SPOC data products.","quality_controlled":"1","article_processing_charge":"No","extern":"1","citation":{"apa":"Aguirre, V. S., Stello, D., Stokholm, A., Mosumgaard, J. R., Ball, W. H., Basu, S., … Vanderspek, R. (2020). Detection and characterization of oscillating red giants: First results from the TESS satellite. <i>The Astrophysical Journal Letters</i>. IOP Publishing. <a href=\"https://doi.org/10.3847/2041-8213/ab6443\">https://doi.org/10.3847/2041-8213/ab6443</a>","mla":"Aguirre, Víctor Silva, et al. “Detection and Characterization of Oscillating Red Giants: First Results from the TESS Satellite.” <i>The Astrophysical Journal Letters</i>, vol. 889, no. 2, L34, IOP Publishing, 2020, doi:<a href=\"https://doi.org/10.3847/2041-8213/ab6443\">10.3847/2041-8213/ab6443</a>.","short":"V.S. Aguirre, D. Stello, A. Stokholm, J.R. Mosumgaard, W.H. Ball, S. Basu, D. Bossini, L.A. Bugnet, D. Buzasi, T.L. Campante, L. Carboneau, W.J. Chaplin, E. Corsaro, G.R. Davies, Y. Elsworth, R.A. García, P. Gaulme, O.J. Hall, R. Handberg, M. Hon, T. Kallinger, L. Kang, M.N. Lund, S. Mathur, A. Mints, B. Mosser, Z. Çelik Orhan, T.S. Rodrigues, M. Vrard, M. Yıldız, J.C. Zinn, S. Örtel, P.G. Beck, K.J. Bell, Z. Guo, C. Jiang, J.S. Kuszlewicz, C.A. Kuehn, T. Li, M.S. Lundkvist, M. Pinsonneault, J. Tayar, M.S. Cunha, S. Hekker, D. Huber, A. Miglio, M.J.P. F. G. Monteiro, D. Slumstrup, M.L. Winther, G. Angelou, O. Benomar, A. Bódi, B.L. De Moura, S. Deheuvels, A. Derekas, M.P. Di Mauro, M.-A. Dupret, A. Jiménez, Y. Lebreton, J. Matthews, N. Nardetto, J.D. do Nascimento, F. Pereira, L.F. Rodríguez Díaz, A.M. Serenelli, E. Spitoni, E. Stonkutė, J.C. Suárez, R. Szabó, V. Van Eylen, R. Ventura, K. Verma, A. Weiss, T. Wu, T. Barclay, J. Christensen-Dalsgaard, J.M. Jenkins, H. Kjeldsen, G.R. Ricker, S. Seager, R. Vanderspek, The Astrophysical Journal Letters 889 (2020).","chicago":"Aguirre, Víctor Silva, Dennis Stello, Amalie Stokholm, Jakob R. Mosumgaard, Warrick H. Ball, Sarbani Basu, Diego Bossini, et al. “Detection and Characterization of Oscillating Red Giants: First Results from the TESS Satellite.” <i>The Astrophysical Journal Letters</i>. IOP Publishing, 2020. <a href=\"https://doi.org/10.3847/2041-8213/ab6443\">https://doi.org/10.3847/2041-8213/ab6443</a>.","ama":"Aguirre VS, Stello D, Stokholm A, et al. Detection and characterization of oscillating red giants: First results from the TESS satellite. <i>The Astrophysical Journal Letters</i>. 2020;889(2). doi:<a href=\"https://doi.org/10.3847/2041-8213/ab6443\">10.3847/2041-8213/ab6443</a>","ieee":"V. S. Aguirre <i>et al.</i>, “Detection and characterization of oscillating red giants: First results from the TESS satellite,” <i>The Astrophysical Journal Letters</i>, vol. 889, no. 2. IOP Publishing, 2020.","ista":"Aguirre VS, Stello D, Stokholm A, Mosumgaard JR, Ball WH, Basu S, Bossini D, Bugnet LA, Buzasi D, Campante TL, Carboneau L, Chaplin WJ, Corsaro E, Davies GR, Elsworth Y, García RA, Gaulme P, Hall OJ, Handberg R, Hon M, Kallinger T, Kang L, Lund MN, Mathur S, Mints A, Mosser B, Çelik Orhan Z, Rodrigues TS, Vrard M, Yıldız M, Zinn JC, Örtel S, Beck PG, Bell KJ, Guo Z, Jiang C, Kuszlewicz JS, Kuehn CA, Li T, Lundkvist MS, Pinsonneault M, Tayar J, Cunha MS, Hekker S, Huber D, Miglio A, F. G. Monteiro MJP, Slumstrup D, Winther ML, Angelou G, Benomar O, Bódi A, De Moura BL, Deheuvels S, Derekas A, Di Mauro MP, Dupret M-A, Jiménez A, Lebreton Y, Matthews J, Nardetto N, do Nascimento JD, Pereira F, Rodríguez Díaz LF, Serenelli AM, Spitoni E, Stonkutė E, Suárez JC, Szabó R, Van Eylen V, Ventura R, Verma K, Weiss A, Wu T, Barclay T, Christensen-Dalsgaard J, Jenkins JM, Kjeldsen H, Ricker GR, Seager S, Vanderspek R. 2020. Detection and characterization of oscillating red giants: First results from the TESS satellite. The Astrophysical Journal Letters. 889(2), L34."},"title":"Detection and characterization of oscillating red giants: First results from the TESS satellite","status":"public","type":"journal_article","publication":"The Astrophysical Journal Letters","day":"01","language":[{"iso":"eng"}],"year":"2020","keyword":["Space and Planetary Science","Astronomy and Astrophysics"],"issue":"2","author":[{"full_name":"Aguirre, Víctor Silva","last_name":"Aguirre","first_name":"Víctor Silva"},{"full_name":"Stello, Dennis","first_name":"Dennis","last_name":"Stello"},{"full_name":"Stokholm, Amalie","first_name":"Amalie","last_name":"Stokholm"},{"full_name":"Mosumgaard, Jakob R.","last_name":"Mosumgaard","first_name":"Jakob R."},{"full_name":"Ball, Warrick H.","last_name":"Ball","first_name":"Warrick H."},{"last_name":"Basu","first_name":"Sarbani","full_name":"Basu, Sarbani"},{"first_name":"Diego","last_name":"Bossini","full_name":"Bossini, Diego"},{"id":"d9edb345-f866-11ec-9b37-d119b5234501","full_name":"Bugnet, Lisa Annabelle","first_name":"Lisa Annabelle","last_name":"Bugnet","orcid":"0000-0003-0142-4000"},{"full_name":"Buzasi, Derek","last_name":"Buzasi","first_name":"Derek"},{"full_name":"Campante, Tiago L.","last_name":"Campante","first_name":"Tiago L."},{"first_name":"Lindsey","last_name":"Carboneau","full_name":"Carboneau, Lindsey"},{"full_name":"Chaplin, William J.","first_name":"William J.","last_name":"Chaplin"},{"last_name":"Corsaro","first_name":"Enrico","full_name":"Corsaro, Enrico"},{"first_name":"Guy R.","last_name":"Davies","full_name":"Davies, Guy R."},{"first_name":"Yvonne","last_name":"Elsworth","full_name":"Elsworth, Yvonne"},{"full_name":"García, Rafael A.","first_name":"Rafael A.","last_name":"García"},{"full_name":"Gaulme, Patrick","last_name":"Gaulme","first_name":"Patrick"},{"first_name":"Oliver J.","last_name":"Hall","full_name":"Hall, Oliver J."},{"first_name":"Rasmus","last_name":"Handberg","full_name":"Handberg, Rasmus"},{"full_name":"Hon, Marc","first_name":"Marc","last_name":"Hon"},{"full_name":"Kallinger, Thomas","last_name":"Kallinger","first_name":"Thomas"},{"full_name":"Kang, Liu","first_name":"Liu","last_name":"Kang"},{"full_name":"Lund, Mikkel N.","last_name":"Lund","first_name":"Mikkel N."},{"full_name":"Mathur, Savita","first_name":"Savita","last_name":"Mathur"},{"full_name":"Mints, Alexey","last_name":"Mints","first_name":"Alexey"},{"first_name":"Benoit","last_name":"Mosser","full_name":"Mosser, Benoit"},{"full_name":"Çelik Orhan, Zeynep","first_name":"Zeynep","last_name":"Çelik Orhan"},{"full_name":"Rodrigues, Thaíse S.","last_name":"Rodrigues","first_name":"Thaíse S."},{"last_name":"Vrard","first_name":"Mathieu","full_name":"Vrard, Mathieu"},{"first_name":"Mutlu","last_name":"Yıldız","full_name":"Yıldız, Mutlu"},{"full_name":"Zinn, Joel C.","first_name":"Joel C.","last_name":"Zinn"},{"last_name":"Örtel","first_name":"Sibel","full_name":"Örtel, Sibel"},{"full_name":"Beck, Paul G.","last_name":"Beck","first_name":"Paul G."},{"first_name":"Keaton J.","last_name":"Bell","full_name":"Bell, Keaton J."},{"last_name":"Guo","first_name":"Zhao","full_name":"Guo, Zhao"},{"last_name":"Jiang","first_name":"Chen","full_name":"Jiang, Chen"},{"last_name":"Kuszlewicz","first_name":"James S.","full_name":"Kuszlewicz, James S."},{"full_name":"Kuehn, Charles A.","last_name":"Kuehn","first_name":"Charles A."},{"full_name":"Li, Tanda","last_name":"Li","first_name":"Tanda"},{"last_name":"Lundkvist","first_name":"Mia S.","full_name":"Lundkvist, Mia S."},{"last_name":"Pinsonneault","first_name":"Marc","full_name":"Pinsonneault, Marc"},{"last_name":"Tayar","first_name":"Jamie","full_name":"Tayar, Jamie"},{"first_name":"Margarida S.","last_name":"Cunha","full_name":"Cunha, Margarida S."},{"first_name":"Saskia","last_name":"Hekker","full_name":"Hekker, Saskia"},{"first_name":"Daniel","last_name":"Huber","full_name":"Huber, Daniel"},{"first_name":"Andrea","last_name":"Miglio","full_name":"Miglio, Andrea"},{"full_name":"F. G. Monteiro, Mario J. P.","last_name":"F. G. Monteiro","first_name":"Mario J. P."},{"last_name":"Slumstrup","first_name":"Ditte","full_name":"Slumstrup, Ditte"},{"last_name":"Winther","first_name":"Mark L.","full_name":"Winther, Mark L."},{"full_name":"Angelou, George","first_name":"George","last_name":"Angelou"},{"full_name":"Benomar, Othman","last_name":"Benomar","first_name":"Othman"},{"first_name":"Attila","last_name":"Bódi","full_name":"Bódi, Attila"},{"last_name":"De Moura","first_name":"Bruno L.","full_name":"De Moura, Bruno L."},{"full_name":"Deheuvels, Sébastien","last_name":"Deheuvels","first_name":"Sébastien"},{"last_name":"Derekas","first_name":"Aliz","full_name":"Derekas, Aliz"},{"first_name":"Maria Pia","last_name":"Di Mauro","full_name":"Di Mauro, Maria Pia"},{"full_name":"Dupret, Marc-Antoine","first_name":"Marc-Antoine","last_name":"Dupret"},{"first_name":"Antonio","last_name":"Jiménez","full_name":"Jiménez, Antonio"},{"full_name":"Lebreton, Yveline","first_name":"Yveline","last_name":"Lebreton"},{"full_name":"Matthews, Jaymie","last_name":"Matthews","first_name":"Jaymie"},{"first_name":"Nicolas","last_name":"Nardetto","full_name":"Nardetto, Nicolas"},{"first_name":"Jose D.","last_name":"do Nascimento","full_name":"do Nascimento, Jose D."},{"full_name":"Pereira, Filipe","first_name":"Filipe","last_name":"Pereira"},{"first_name":"Luisa F.","last_name":"Rodríguez Díaz","full_name":"Rodríguez Díaz, Luisa F."},{"last_name":"Serenelli","first_name":"Aldo M.","full_name":"Serenelli, Aldo M."},{"first_name":"Emanuele","last_name":"Spitoni","full_name":"Spitoni, Emanuele"},{"full_name":"Stonkutė, Edita","last_name":"Stonkutė","first_name":"Edita"},{"first_name":"Juan Carlos","last_name":"Suárez","full_name":"Suárez, Juan Carlos"},{"last_name":"Szabó","first_name":"Robert","full_name":"Szabó, Robert"},{"last_name":"Van Eylen","first_name":"Vincent","full_name":"Van Eylen, Vincent"},{"full_name":"Ventura, Rita","first_name":"Rita","last_name":"Ventura"},{"last_name":"Verma","first_name":"Kuldeep","full_name":"Verma, Kuldeep"},{"last_name":"Weiss","first_name":"Achim","full_name":"Weiss, Achim"},{"full_name":"Wu, Tao","first_name":"Tao","last_name":"Wu"},{"first_name":"Thomas","last_name":"Barclay","full_name":"Barclay, Thomas"},{"full_name":"Christensen-Dalsgaard, Jørgen","first_name":"Jørgen","last_name":"Christensen-Dalsgaard"},{"full_name":"Jenkins, Jon M.","last_name":"Jenkins","first_name":"Jon M."},{"full_name":"Kjeldsen, Hans","first_name":"Hans","last_name":"Kjeldsen"},{"full_name":"Ricker, George R.","last_name":"Ricker","first_name":"George R."},{"full_name":"Seager, Sara","last_name":"Seager","first_name":"Sara"},{"full_name":"Vanderspek, Roland","last_name":"Vanderspek","first_name":"Roland"}],"abstract":[{"text":"Since the onset of the \"space revolution\" of high-precision high-cadence photometry, asteroseismology has been demonstrated as a powerful tool for informing Galactic archeology investigations. The launch of the NASA Transiting Exoplanet Survey Satellite (TESS) mission has enabled seismic-based inferences to go full sky—providing a clear advantage for large ensemble studies of the different Milky Way components. Here we demonstrate its potential for investigating the Galaxy by carrying out the first asteroseismic ensemble study of red giant stars observed by TESS. We use a sample of 25 stars for which we measure their global asteroseimic observables and estimate their fundamental stellar properties, such as radius, mass, and age. Significant improvements are seen in the uncertainties of our estimates when combining seismic observables from TESS with astrometric measurements from the Gaia mission compared to when the seismology and astrometry are applied separately. Specifically, when combined we show that stellar radii can be determined to a precision of a few percent, masses to 5%–10%, and ages to the 20% level. This is comparable to the precision typically obtained using end-of-mission Kepler data.","lang":"eng"}],"volume":889,"date_published":"2020-02-01T00:00:00Z","article_type":"original","date_created":"2022-07-18T13:52:54Z","publisher":"IOP Publishing","main_file_link":[{"url":"https://arxiv.org/abs/1912.07604","open_access":"1"}],"scopus_import":"1"},{"publisher":"Springer Nature","main_file_link":[{"url":"https://arxiv.org/abs/2012.08684","open_access":"1"}],"scopus_import":"1","series_title":"ASSSP","date_created":"2022-07-19T08:25:41Z","author":[{"full_name":"Bugnet, Lisa Annabelle","id":"d9edb345-f866-11ec-9b37-d119b5234501","last_name":"Bugnet","first_name":"Lisa Annabelle","orcid":"0000-0003-0142-4000"},{"last_name":"Prat","first_name":"V.","full_name":"Prat, V."},{"last_name":"Mathis","first_name":"S.","full_name":"Mathis, S."},{"full_name":"García, R. A.","last_name":"García","first_name":"R. A."},{"first_name":"S.","last_name":"Mathur","full_name":"Mathur, S."},{"first_name":"K.","last_name":"Augustson","full_name":"Augustson, K."},{"full_name":"Neiner, C.","first_name":"C.","last_name":"Neiner"},{"last_name":"Thompson","first_name":"M. J.","full_name":"Thompson, M. J."}],"volume":57,"abstract":[{"lang":"eng","text":"The recent discovery of low-amplitude dipolar oscillation mixed modes in massive red giants indicates the presence of a missing physical process inside their cores. Stars more massive than ∼ 1.3 M⊙ are known to develop a convective core during the main-sequence: the dynamo process triggered by this convection could be the origin of a strong magnetic field inside the core of the star, trapped when it becomes stably stratified and for the rest of its evolution. The presence of highly magnetized white dwarfs strengthens the hypothesis of buried fossil magnetic fields inside the core of evolved low-mass stars. If such a fossil field exists, it should affect the mixed modes of red giants as they are sensitive to processes affecting the deepest layers of these stars. The impact of a magnetic field on dipolar oscillations modes was one of Pr. Michael J. Thompson’s research topics during the 90s when preparing the helioseismic SoHO space mission. As the detection of gravity modes in the Sun is still controversial, the investigation of the solar oscillation modes did not provide any hint of the existence of a magnetic field in the solar radiative core. Today we have access to the core of evolved stars thanks to the asteroseismic observation of mixed modes from CoRoT, Kepler, K2 and TESS missions. The idea of applying and generalizing the work done for the Sun came from discussions with Pr. Michael Thompson in early 2018 before we lost him. Following the path we drew together, we theoretically investigate the effect of a stable axisymmetric mixed poloidal and toroidal magnetic field, aligned with the rotation axis of the star, on the mixed modes frequencies of a typical evolved low-mass star. This enables us to estimate the magnetic perturbations to the eigenfrequencies of mixed dipolar modes, depending on the magnetic field strength and the evolutionary state of the star. We conclude that strong magnetic fields of ∼ 1MG should perturb the mixed-mode frequency pattern enough for its effects to be detectable inside current asteroseismic data."}],"edition":"1","date_published":"2020-12-19T00:00:00Z","publication":"Dynamics of the Sun and Stars","day":"19","year":"2020","language":[{"iso":"eng"}],"citation":{"short":"L.A. Bugnet, V. Prat, S. Mathis, R.A. García, S. Mathur, K. Augustson, C. Neiner, M.J. Thompson, in:, M. Monteiro, R.A. Garcia, J. Christensen-Dalsgaard, S.W. McIntosh (Eds.), Dynamics of the Sun and Stars, 1st ed., Springer Nature, Cham, 2020, pp. 251–257.","ama":"Bugnet LA, Prat V, Mathis S, et al. The impact of a fossil magnetic field on dipolar mixed-mode frequencies in sub- and red-giant stars. In: Monteiro M, Garcia RA, Christensen-Dalsgaard J, McIntosh SW, eds. <i>Dynamics of the Sun and Stars</i>. Vol 57. 1st ed. ASSSP. Cham: Springer Nature; 2020:251-257. doi:<a href=\"https://doi.org/10.1007/978-3-030-55336-4_33\">10.1007/978-3-030-55336-4_33</a>","chicago":"Bugnet, Lisa Annabelle, V. Prat, S. Mathis, R. A. García, S. Mathur, K. Augustson, C. Neiner, and M. J. Thompson. “The Impact of a Fossil Magnetic Field on Dipolar Mixed-Mode Frequencies in Sub- and Red-Giant Stars.” In <i>Dynamics of the Sun and Stars</i>, edited by Mario Monteiro, Rafael A Garcia, Jorgen Christensen-Dalsgaard, and Scott W McIntosh, 1st ed., 57:251–57. ASSSP. Cham: Springer Nature, 2020. <a href=\"https://doi.org/10.1007/978-3-030-55336-4_33\">https://doi.org/10.1007/978-3-030-55336-4_33</a>.","apa":"Bugnet, L. A., Prat, V., Mathis, S., García, R. A., Mathur, S., Augustson, K., … Thompson, M. J. (2020). The impact of a fossil magnetic field on dipolar mixed-mode frequencies in sub- and red-giant stars. In M. Monteiro, R. A. Garcia, J. Christensen-Dalsgaard, &#38; S. W. McIntosh (Eds.), <i>Dynamics of the Sun and Stars</i> (1st ed., Vol. 57, pp. 251–257). Cham: Springer Nature. <a href=\"https://doi.org/10.1007/978-3-030-55336-4_33\">https://doi.org/10.1007/978-3-030-55336-4_33</a>","mla":"Bugnet, Lisa Annabelle, et al. “The Impact of a Fossil Magnetic Field on Dipolar Mixed-Mode Frequencies in Sub- and Red-Giant Stars.” <i>Dynamics of the Sun and Stars</i>, edited by Mario Monteiro et al., 1st ed., vol. 57, Springer Nature, 2020, pp. 251–57, doi:<a href=\"https://doi.org/10.1007/978-3-030-55336-4_33\">10.1007/978-3-030-55336-4_33</a>.","ieee":"L. A. Bugnet <i>et al.</i>, “The impact of a fossil magnetic field on dipolar mixed-mode frequencies in sub- and red-giant stars,” in <i>Dynamics of the Sun and Stars</i>, 1st ed., vol. 57, M. Monteiro, R. A. Garcia, J. Christensen-Dalsgaard, and S. W. McIntosh, Eds. Cham: Springer Nature, 2020, pp. 251–257.","ista":"Bugnet LA, Prat V, Mathis S, García RA, Mathur S, Augustson K, Neiner C, Thompson MJ. 2020.The impact of a fossil magnetic field on dipolar mixed-mode frequencies in sub- and red-giant stars. In: Dynamics of the Sun and Stars. Astrophysics and Space Science Proceedings, vol. 57, 251–257."},"article_processing_charge":"No","extern":"1","title":"The impact of a fossil magnetic field on dipolar mixed-mode frequencies in sub- and red-giant stars","type":"book_chapter","status":"public","doi":"10.1007/978-3-030-55336-4_33","external_id":{"arxiv":["2012.08684"]},"page":"251-257","_id":"11622","intvolume":"        57","acknowledgement":"The authors of this work acknowledge the support received from the PLATO CNES grant, the National Aeronautics and Space Administration under Grant NNX15AF13G, by the National Science Foundation grant AST-1411685, the Ramon y Cajal fellowship number RYC-2015-17697, the ERC SPIRE grant (647383), and the Fundation L’Oréal-Unesco-Académie des sciences.","quality_controlled":"1","place":"Cham","editor":[{"last_name":"Monteiro","first_name":"Mario","full_name":"Monteiro, Mario"},{"full_name":"Garcia, Rafael A","last_name":"Garcia","first_name":"Rafael A"},{"full_name":"Christensen-Dalsgaard, Jorgen","last_name":"Christensen-Dalsgaard","first_name":"Jorgen"},{"last_name":"McIntosh","first_name":"Scott W","full_name":"McIntosh, Scott W"}],"arxiv":1,"alternative_title":["Astrophysics and Space Science Proceedings"],"oa_version":"Preprint","month":"12","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","publication_status":"published","oa":1,"date_updated":"2022-08-22T08:07:42Z","publication_identifier":{"eissn":["1570-6605"],"isbn":["978-3-030-55335-7"],"issn":["1570-6591"],"eisbn":["978-3-030-55336-4"]}},{"citation":{"ieee":"M. H. Henzinger, D. Leniowski, and C. Mathieu, “Dynamic clustering to minimize the sum of radii,” <i>Algorithmica</i>, vol. 82, no. 11. Springer Nature, pp. 3183–3194, 2020.","ista":"Henzinger MH, Leniowski D, Mathieu C. 2020. Dynamic clustering to minimize the sum of radii. Algorithmica. 82(11), 3183–3194.","ama":"Henzinger MH, Leniowski D, Mathieu C. Dynamic clustering to minimize the sum of radii. <i>Algorithmica</i>. 2020;82(11):3183-3194. doi:<a href=\"https://doi.org/10.1007/s00453-020-00721-7\">10.1007/s00453-020-00721-7</a>","chicago":"Henzinger, Monika H, Dariusz Leniowski, and Claire Mathieu. “Dynamic Clustering to Minimize the Sum of Radii.” <i>Algorithmica</i>. Springer Nature, 2020. <a href=\"https://doi.org/10.1007/s00453-020-00721-7\">https://doi.org/10.1007/s00453-020-00721-7</a>.","short":"M.H. Henzinger, D. Leniowski, C. Mathieu, Algorithmica 82 (2020) 3183–3194.","apa":"Henzinger, M. H., Leniowski, D., &#38; Mathieu, C. (2020). Dynamic clustering to minimize the sum of radii. <i>Algorithmica</i>. Springer Nature. <a href=\"https://doi.org/10.1007/s00453-020-00721-7\">https://doi.org/10.1007/s00453-020-00721-7</a>","mla":"Henzinger, Monika H., et al. “Dynamic Clustering to Minimize the Sum of Radii.” <i>Algorithmica</i>, vol. 82, no. 11, Springer Nature, 2020, pp. 3183–94, doi:<a href=\"https://doi.org/10.1007/s00453-020-00721-7\">10.1007/s00453-020-00721-7</a>."},"extern":"1","article_processing_charge":"No","status":"public","type":"journal_article","title":"Dynamic clustering to minimize the sum of radii","page":"3183-3194","_id":"11674","intvolume":"        82","doi":"10.1007/s00453-020-00721-7","external_id":{"arxiv":["1707.02577"]},"quality_controlled":"1","arxiv":1,"user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","month":"11","oa_version":"Preprint","date_updated":"2022-09-12T08:50:14Z","publication_identifier":{"issn":["0178-4617"],"eissn":["1432-0541"]},"oa":1,"publication_status":"published","publisher":"Springer Nature","main_file_link":[{"open_access":"1","url":"https://doi.org/10.48550/arXiv.1707.02577"}],"scopus_import":"1","date_created":"2022-07-27T13:58:58Z","article_type":"original","issue":"11","abstract":[{"lang":"eng","text":"In this paper, we study the problem of opening centers to cluster a set of clients in a metric space so as to minimize the sum of the costs of the centers and of the cluster radii, in a dynamic environment where clients arrive and depart, and the solution must be updated efficiently while remaining competitive with respect to the current optimal solution. We call this dynamic sum-of-radii clustering problem. We present a data structure that maintains a solution whose cost is within a constant factor of the cost of an optimal solution in metric spaces with bounded doubling dimension and whose worst-case update time is logarithmic in the parameters of the problem."}],"volume":82,"date_published":"2020-11-01T00:00:00Z","author":[{"id":"540c9bbd-f2de-11ec-812d-d04a5be85630","full_name":"Henzinger, Monika H","last_name":"Henzinger","first_name":"Monika H","orcid":"0000-0002-5008-6530"},{"full_name":"Leniowski, Dariusz","last_name":"Leniowski","first_name":"Dariusz"},{"full_name":"Mathieu, Claire","first_name":"Claire","last_name":"Mathieu"}],"day":"01","language":[{"iso":"eng"}],"year":"2020","publication":"Algorithmica"},{"author":[{"last_name":"Bhattacharya","first_name":"Sayan","full_name":"Bhattacharya, Sayan"},{"full_name":"Chakrabarty, Deeparnab","last_name":"Chakrabarty","first_name":"Deeparnab"},{"orcid":"0000-0002-5008-6530","last_name":"Henzinger","first_name":"Monika H","id":"540c9bbd-f2de-11ec-812d-d04a5be85630","full_name":"Henzinger, Monika H"}],"date_published":"2020-04-01T00:00:00Z","abstract":[{"text":"We consider the problems of maintaining an approximate maximum matching and an approximate minimum vertex cover in a dynamic graph undergoing a sequence of edge insertions/deletions. Starting with the seminal work of Onak and Rubinfeld (in: Proceedings of the ACM symposium on theory of computing (STOC), 2010), this problem has received significant attention in recent years. Very recently, extending the framework of Baswana et al. (in: Proceedings of the IEEE symposium on foundations of computer science (FOCS), 2011) , Solomon (in: Proceedings of the IEEE symposium on foundations of computer science (FOCS), 2016) gave a randomized dynamic algorithm for this problem that has an approximation ratio of 2 and an amortized update time of O(1) with high probability. This algorithm requires the assumption of an oblivious adversary, meaning that the future sequence of edge insertions/deletions in the graph cannot depend in any way on the algorithm’s past output. A natural way to remove the assumption on oblivious adversary is to give a deterministic dynamic algorithm for the same problem in O(1) update time. In this paper, we resolve this question. We present a new deterministic fully dynamic algorithm that maintains a O(1)-approximate minimum vertex cover and maximum fractional matching, with an amortized update time of O(1). Previously, the best deterministic algorithm for this problem was due to Bhattacharya et al. (in: Proceedings of the ACM-SIAM symposium on discrete algorithms (SODA), 2015); it had an approximation ratio of (2+ε) and an amortized update time of O(logn/ε2). Our result can be generalized to give a fully dynamic O(f3)-approximate algorithm with O(f2) amortized update time for the hypergraph vertex cover and fractional hypergraph matching problem, where every hyperedge has at most f vertices.","lang":"eng"}],"volume":82,"issue":"4","keyword":["Dynamic algorithms","Data structures","Graph algorithms","Matching","Vertex cover"],"publication":"Algorithmica","year":"2020","language":[{"iso":"eng"}],"day":"01","scopus_import":"1","main_file_link":[{"url":"https://doi.org/10.1007/s00453-019-00630-4","open_access":"1"}],"publisher":"Springer Nature","date_created":"2022-07-27T14:31:06Z","article_type":"original","oa":1,"publication_status":"published","publication_identifier":{"eissn":["1432-0541"],"issn":["0178-4617"]},"date_updated":"2022-09-12T08:55:46Z","oa_version":"Published Version","month":"04","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","title":"Deterministic dynamic matching in O(1) update time","type":"journal_article","status":"public","citation":{"ieee":"S. Bhattacharya, D. Chakrabarty, and M. H. Henzinger, “Deterministic dynamic matching in O(1) update time,” <i>Algorithmica</i>, vol. 82, no. 4. Springer Nature, pp. 1057–1080, 2020.","ista":"Bhattacharya S, Chakrabarty D, Henzinger MH. 2020. Deterministic dynamic matching in O(1) update time. Algorithmica. 82(4), 1057–1080.","short":"S. Bhattacharya, D. Chakrabarty, M.H. Henzinger, Algorithmica 82 (2020) 1057–1080.","ama":"Bhattacharya S, Chakrabarty D, Henzinger MH. Deterministic dynamic matching in O(1) update time. <i>Algorithmica</i>. 2020;82(4):1057-1080. doi:<a href=\"https://doi.org/10.1007/s00453-019-00630-4\">10.1007/s00453-019-00630-4</a>","chicago":"Bhattacharya, Sayan, Deeparnab Chakrabarty, and Monika H Henzinger. “Deterministic Dynamic Matching in O(1) Update Time.” <i>Algorithmica</i>. Springer Nature, 2020. <a href=\"https://doi.org/10.1007/s00453-019-00630-4\">https://doi.org/10.1007/s00453-019-00630-4</a>.","apa":"Bhattacharya, S., Chakrabarty, D., &#38; Henzinger, M. H. (2020). Deterministic dynamic matching in O(1) update time. <i>Algorithmica</i>. Springer Nature. <a href=\"https://doi.org/10.1007/s00453-019-00630-4\">https://doi.org/10.1007/s00453-019-00630-4</a>","mla":"Bhattacharya, Sayan, et al. “Deterministic Dynamic Matching in O(1) Update Time.” <i>Algorithmica</i>, vol. 82, no. 4, Springer Nature, 2020, pp. 1057–80, doi:<a href=\"https://doi.org/10.1007/s00453-019-00630-4\">10.1007/s00453-019-00630-4</a>."},"article_processing_charge":"No","extern":"1","quality_controlled":"1","doi":"10.1007/s00453-019-00630-4","intvolume":"        82","page":"1057-1080","_id":"11675"},{"article_number":"eabc1939","has_accepted_license":"1","date_updated":"2021-04-12T08:35:19Z","ddc":["570"],"publication_status":"published","oa":1,"user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","oa_version":"Published Version","month":"12","type":"journal_article","status":"public","title":"Self-assembly-based posttranslational protein oscillators","tmp":{"short":"CC BY (4.0)","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","image":"/images/cc_by.png","name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)"},"extern":"1","citation":{"ista":"Kimchi O, Goodrich CP, Courbet A, Curatolo AI, Woodall NB, Baker D, Brenner MP. 2020. Self-assembly-based posttranslational protein oscillators. Science Advances. 6(51), eabc1939.","ieee":"O. Kimchi <i>et al.</i>, “Self-assembly-based posttranslational protein oscillators,” <i>Science Advances</i>, vol. 6, no. 51. 2020.","apa":"Kimchi, O., Goodrich, C. P., Courbet, A., Curatolo, A. I., Woodall, N. B., Baker, D., &#38; Brenner, M. P. (2020). Self-assembly-based posttranslational protein oscillators. <i>Science Advances</i>. <a href=\"https://doi.org/10.1126/sciadv.abc1939\">https://doi.org/10.1126/sciadv.abc1939</a>","mla":"Kimchi, Ofer, et al. “Self-Assembly-Based Posttranslational Protein Oscillators.” <i>Science Advances</i>, vol. 6, no. 51, eabc1939, 2020, doi:<a href=\"https://doi.org/10.1126/sciadv.abc1939\">10.1126/sciadv.abc1939</a>.","chicago":"Kimchi, Ofer, Carl Peter Goodrich, Alexis Courbet, Agnese I. Curatolo, Nicholas B. Woodall, David Baker, and Michael P. Brenner. “Self-Assembly-Based Posttranslational Protein Oscillators.” <i>Science Advances</i>, 2020. <a href=\"https://doi.org/10.1126/sciadv.abc1939\">https://doi.org/10.1126/sciadv.abc1939</a>.","ama":"Kimchi O, Goodrich CP, Courbet A, et al. Self-assembly-based posttranslational protein oscillators. <i>Science Advances</i>. 2020;6(51). doi:<a href=\"https://doi.org/10.1126/sciadv.abc1939\">10.1126/sciadv.abc1939</a>","short":"O. Kimchi, C.P. Goodrich, A. Courbet, A.I. Curatolo, N.B. Woodall, D. Baker, M.P. Brenner, Science Advances 6 (2020)."},"article_processing_charge":"No","quality_controlled":"1","_id":"7778","intvolume":"         6","doi":"10.1126/sciadv.abc1939","volume":6,"abstract":[{"lang":"eng","text":"Recent advances in synthetic posttranslational protein circuits are substantially impacting the landscape of cellular engineering and offer several advantages compared to traditional gene circuits. However, engineering dynamic phenomena such as oscillations in protein-level circuits remains an outstanding challenge. Few examples of biological posttranslational oscillators are known, necessitating theoretical progress to determine realizable oscillators. We construct mathematical models for two posttranslational oscillators, using few components that interact only through reversible binding and phosphorylation/dephosphorylation reactions. Our designed oscillators rely on the self-assembly of two protein species into multimeric functional enzymes that respectively inhibit and enhance this self-assembly. We limit our analysis to within experimental constraints, finding (i) significant portions of the restricted parameter space yielding oscillations and (ii) that oscillation periods can be tuned by several orders of magnitude using recent advances in computational protein design. Our work paves the way for the rational design and realization of protein-based dynamic systems."}],"date_published":"2020-12-16T00:00:00Z","author":[{"full_name":"Kimchi, Ofer","last_name":"Kimchi","first_name":"Ofer"},{"orcid":"0000-0002-1307-5074","first_name":"Carl Peter","last_name":"Goodrich","full_name":"Goodrich, Carl Peter","id":"EB352CD2-F68A-11E9-89C5-A432E6697425"},{"last_name":"Courbet","first_name":"Alexis","full_name":"Courbet, Alexis"},{"full_name":"Curatolo, Agnese I.","first_name":"Agnese I.","last_name":"Curatolo"},{"full_name":"Woodall, Nicholas B.","last_name":"Woodall","first_name":"Nicholas B."},{"last_name":"Baker","first_name":"David","full_name":"Baker, David"},{"full_name":"Brenner, Michael P.","last_name":"Brenner","first_name":"Michael P."}],"issue":"51","file_date_updated":"2021-04-12T08:33:23Z","day":"16","language":[{"iso":"eng"}],"year":"2020","publication":"Science Advances","file":[{"success":1,"access_level":"open_access","file_size":1259758,"file_name":"2020_ScienceAdv_Kimchi.pdf","content_type":"application/pdf","date_updated":"2021-04-12T08:33:23Z","checksum":"eb6d950b6a68ddc4a2fb31ec80a2a1bd","relation":"main_file","date_created":"2021-04-12T08:33:23Z","creator":"dernst","file_id":"9320"}],"article_type":"original","date_created":"2020-04-30T12:07:55Z"},{"article_type":"original","date_created":"2020-05-03T22:00:47Z","scopus_import":"1","publisher":"Elsevier","file":[{"file_id":"7798","relation":"main_file","checksum":"a9b152381307cf45fe266a8dc5640388","date_created":"2020-05-04T12:25:19Z","creator":"dernst","content_type":"application/pdf","date_updated":"2020-07-14T12:48:03Z","access_level":"open_access","file_size":3826792,"file_name":"2020_BBA_Adjobo_Hermans.pdf"}],"pmid":1,"publication":"Biochimica et Biophysica Acta - Bioenergetics","day":"01","year":"2020","language":[{"iso":"eng"}],"author":[{"last_name":"Adjobo-Hermans","first_name":"Merel J.W.","full_name":"Adjobo-Hermans, Merel J.W."},{"last_name":"De Haas","first_name":"Ria","full_name":"De Haas, Ria"},{"full_name":"Willems, Peter H.G.M.","first_name":"Peter H.G.M.","last_name":"Willems"},{"full_name":"Wojtala, Aleksandra","last_name":"Wojtala","first_name":"Aleksandra"},{"first_name":"Sjenet E.","last_name":"Van Emst-De Vries","full_name":"Van Emst-De Vries, Sjenet E."},{"full_name":"Wagenaars, Jori A.","last_name":"Wagenaars","first_name":"Jori A."},{"full_name":"Van Den Brand, Mariel","first_name":"Mariel","last_name":"Van Den Brand"},{"full_name":"Rodenburg, Richard J.","first_name":"Richard J.","last_name":"Rodenburg"},{"last_name":"Smeitink","first_name":"Jan A.M.","full_name":"Smeitink, Jan A.M."},{"first_name":"Leo G.","last_name":"Nijtmans","full_name":"Nijtmans, Leo G."},{"last_name":"Sazanov","first_name":"Leonid A","orcid":"0000-0002-0977-7989","full_name":"Sazanov, Leonid A","id":"338D39FE-F248-11E8-B48F-1D18A9856A87"},{"first_name":"Mariusz R.","last_name":"Wieckowski","full_name":"Wieckowski, Mariusz R."},{"last_name":"Koopman","first_name":"Werner J.H.","full_name":"Koopman, Werner J.H."}],"volume":1861,"abstract":[{"text":"Mutations in NDUFS4, which encodes an accessory subunit of mitochondrial oxidative phosphorylation (OXPHOS) complex I (CI), induce Leigh syndrome (LS). LS is a poorly understood pediatric disorder featuring brain-specific anomalies and early death. To study the LS pathomechanism, we here compared OXPHOS proteomes between various Ndufs4−/− mouse tissues. Ndufs4−/− animals displayed significantly lower CI subunit levels in brain/diaphragm relative to other tissues (liver/heart/kidney/skeletal muscle), whereas other OXPHOS subunit levels were not reduced. Absence of NDUFS4 induced near complete absence of the NDUFA12 accessory subunit, a 50% reduction in other CI subunit levels, and an increase in specific CI assembly factors. Among the latter, NDUFAF2 was most highly increased. Regarding NDUFS4, NDUFA12 and NDUFAF2, identical results were obtained in Ndufs4−/− mouse embryonic fibroblasts (MEFs) and NDUFS4-mutated LS patient cells. Ndufs4−/− MEFs contained active CI in situ but blue-native-PAGE highlighted that NDUFAF2 attached to an inactive CI subcomplex (CI-830) and inactive assemblies of higher MW. In NDUFA12-mutated LS patient cells, NDUFA12 absence did not reduce NDUFS4 levels but triggered NDUFAF2 association to active CI. BN-PAGE revealed no such association in LS patient fibroblasts with mutations in other CI subunit-encoding genes where NDUFAF2 was attached to CI-830 (NDUFS1, NDUFV1 mutation) or not detected (NDUFS7 mutation). Supported by enzymological and CI in silico structural analysis, we conclude that absence of NDUFS4 induces near complete absence of NDUFA12 but not vice versa, and that NDUFAF2 stabilizes active CI in Ndufs4−/− mice and LS patient cells, perhaps in concert with mitochondrial inner membrane lipids.","lang":"eng"}],"date_published":"2020-08-01T00:00:00Z","file_date_updated":"2020-07-14T12:48:03Z","issue":"8","quality_controlled":"1","department":[{"_id":"LeSa"}],"doi":"10.1016/j.bbabio.2020.148213","external_id":{"pmid":["32335026"],"isi":["000540842000012"]},"_id":"7788","intvolume":"      1861","title":"NDUFS4 deletion triggers loss of NDUFA12 in Ndufs4−/− mice and Leigh syndrome patients: A stabilizing role for NDUFAF2","tmp":{"short":"CC BY (4.0)","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","image":"/images/cc_by.png","name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)"},"type":"journal_article","status":"public","article_processing_charge":"No","citation":{"ieee":"M. J. W. Adjobo-Hermans <i>et al.</i>, “NDUFS4 deletion triggers loss of NDUFA12 in Ndufs4−/− mice and Leigh syndrome patients: A stabilizing role for NDUFAF2,” <i>Biochimica et Biophysica Acta - Bioenergetics</i>, vol. 1861, no. 8. Elsevier, 2020.","ista":"Adjobo-Hermans MJW, De Haas R, Willems PHGM, Wojtala A, Van Emst-De Vries SE, Wagenaars JA, Van Den Brand M, Rodenburg RJ, Smeitink JAM, Nijtmans LG, Sazanov LA, Wieckowski MR, Koopman WJH. 2020. NDUFS4 deletion triggers loss of NDUFA12 in Ndufs4−/− mice and Leigh syndrome patients: A stabilizing role for NDUFAF2. Biochimica et Biophysica Acta - Bioenergetics. 1861(8), 148213.","mla":"Adjobo-Hermans, Merel J. W., et al. “NDUFS4 Deletion Triggers Loss of NDUFA12 in Ndufs4−/− Mice and Leigh Syndrome Patients: A Stabilizing Role for NDUFAF2.” <i>Biochimica et Biophysica Acta - Bioenergetics</i>, vol. 1861, no. 8, 148213, Elsevier, 2020, doi:<a href=\"https://doi.org/10.1016/j.bbabio.2020.148213\">10.1016/j.bbabio.2020.148213</a>.","apa":"Adjobo-Hermans, M. J. W., De Haas, R., Willems, P. H. G. M., Wojtala, A., Van Emst-De Vries, S. E., Wagenaars, J. A., … Koopman, W. J. H. (2020). NDUFS4 deletion triggers loss of NDUFA12 in Ndufs4−/− mice and Leigh syndrome patients: A stabilizing role for NDUFAF2. <i>Biochimica et Biophysica Acta - Bioenergetics</i>. Elsevier. <a href=\"https://doi.org/10.1016/j.bbabio.2020.148213\">https://doi.org/10.1016/j.bbabio.2020.148213</a>","short":"M.J.W. Adjobo-Hermans, R. De Haas, P.H.G.M. Willems, A. Wojtala, S.E. Van Emst-De Vries, J.A. Wagenaars, M. Van Den Brand, R.J. Rodenburg, J.A.M. Smeitink, L.G. Nijtmans, L.A. Sazanov, M.R. Wieckowski, W.J.H. Koopman, Biochimica et Biophysica Acta - Bioenergetics 1861 (2020).","chicago":"Adjobo-Hermans, Merel J.W., Ria De Haas, Peter H.G.M. Willems, Aleksandra Wojtala, Sjenet E. Van Emst-De Vries, Jori A. Wagenaars, Mariel Van Den Brand, et al. “NDUFS4 Deletion Triggers Loss of NDUFA12 in Ndufs4−/− Mice and Leigh Syndrome Patients: A Stabilizing Role for NDUFAF2.” <i>Biochimica et Biophysica Acta - Bioenergetics</i>. Elsevier, 2020. <a href=\"https://doi.org/10.1016/j.bbabio.2020.148213\">https://doi.org/10.1016/j.bbabio.2020.148213</a>.","ama":"Adjobo-Hermans MJW, De Haas R, Willems PHGM, et al. NDUFS4 deletion triggers loss of NDUFA12 in Ndufs4−/− mice and Leigh syndrome patients: A stabilizing role for NDUFAF2. <i>Biochimica et Biophysica Acta - Bioenergetics</i>. 2020;1861(8). doi:<a href=\"https://doi.org/10.1016/j.bbabio.2020.148213\">10.1016/j.bbabio.2020.148213</a>"},"isi":1,"oa":1,"publication_status":"published","ddc":["570"],"date_updated":"2023-08-21T06:19:18Z","publication_identifier":{"issn":["00052728"],"eissn":["18792650"]},"oa_version":"Published Version","month":"08","user_id":"4359f0d1-fa6c-11eb-b949-802e58b17ae8","article_number":"148213","has_accepted_license":"1"},{"pmid":1,"file":[{"date_updated":"2020-07-14T12:48:03Z","content_type":"application/pdf","file_name":"2020_Cell_Dekoninck.pdf","access_level":"open_access","file_size":17992888,"file_id":"7795","date_created":"2020-05-04T10:20:55Z","creator":"dernst","relation":"main_file","checksum":"e2114902f4e9d75a752e9efb5ae06011"}],"publisher":"Elsevier","scopus_import":"1","date_created":"2020-05-03T22:00:48Z","article_type":"original","issue":"3","file_date_updated":"2020-07-14T12:48:03Z","date_published":"2020-04-30T00:00:00Z","volume":181,"abstract":[{"lang":"eng","text":"During embryonic and postnatal development, organs and tissues grow steadily to achieve their final size at the end of puberty. However, little is known about the cellular dynamics that mediate postnatal growth. By combining in vivo clonal lineage tracing, proliferation kinetics, single-cell transcriptomics, andin vitro micro-pattern experiments, we resolved the cellular dynamics taking place during postnatal skin epidermis expansion. Our data revealed that harmonious growth is engineered by a single population of developmental progenitors presenting a fixed fate imbalance of self-renewing divisions with an ever-decreasing proliferation rate. Single-cell RNA sequencing revealed that epidermal developmental progenitors form a more uniform population compared with adult stem and progenitor cells. Finally, we found that the spatial pattern of cell division orientation is dictated locally by the underlying collagen fiber orientation. Our results uncover a simple design principle of organ growth where progenitors and differentiated cells expand in harmony with their surrounding tissues."}],"author":[{"full_name":"Dekoninck, Sophie","first_name":"Sophie","last_name":"Dekoninck"},{"orcid":"0000-0001-6005-1561","first_name":"Edouard B","last_name":"Hannezo","id":"3A9DB764-F248-11E8-B48F-1D18A9856A87","full_name":"Hannezo, Edouard B"},{"full_name":"Sifrim, Alejandro","first_name":"Alejandro","last_name":"Sifrim"},{"first_name":"Yekaterina A.","last_name":"Miroshnikova","full_name":"Miroshnikova, Yekaterina A."},{"full_name":"Aragona, Mariaceleste","first_name":"Mariaceleste","last_name":"Aragona"},{"first_name":"Milan","last_name":"Malfait","full_name":"Malfait, Milan"},{"last_name":"Gargouri","first_name":"Souhir","full_name":"Gargouri, Souhir"},{"full_name":"De Neunheuser, Charlotte","first_name":"Charlotte","last_name":"De Neunheuser"},{"first_name":"Christine","last_name":"Dubois","full_name":"Dubois, Christine"},{"full_name":"Voet, Thierry","first_name":"Thierry","last_name":"Voet"},{"full_name":"Wickström, Sara A.","first_name":"Sara A.","last_name":"Wickström"},{"full_name":"Simons, Benjamin D.","first_name":"Benjamin D.","last_name":"Simons"},{"full_name":"Blanpain, Cédric","last_name":"Blanpain","first_name":"Cédric"}],"year":"2020","language":[{"iso":"eng"}],"day":"30","publication":"Cell","isi":1,"citation":{"apa":"Dekoninck, S., Hannezo, E. B., Sifrim, A., Miroshnikova, Y. A., Aragona, M., Malfait, M., … Blanpain, C. (2020). Defining the design principles of skin epidermis postnatal growth. <i>Cell</i>. Elsevier. <a href=\"https://doi.org/10.1016/j.cell.2020.03.015\">https://doi.org/10.1016/j.cell.2020.03.015</a>","mla":"Dekoninck, Sophie, et al. “Defining the Design Principles of Skin Epidermis Postnatal Growth.” <i>Cell</i>, vol. 181, no. 3, Elsevier, 2020, p. 604–620.e22, doi:<a href=\"https://doi.org/10.1016/j.cell.2020.03.015\">10.1016/j.cell.2020.03.015</a>.","ama":"Dekoninck S, Hannezo EB, Sifrim A, et al. Defining the design principles of skin epidermis postnatal growth. <i>Cell</i>. 2020;181(3):604-620.e22. doi:<a href=\"https://doi.org/10.1016/j.cell.2020.03.015\">10.1016/j.cell.2020.03.015</a>","short":"S. Dekoninck, E.B. Hannezo, A. Sifrim, Y.A. Miroshnikova, M. Aragona, M. Malfait, S. Gargouri, C. De Neunheuser, C. Dubois, T. Voet, S.A. Wickström, B.D. Simons, C. Blanpain, Cell 181 (2020) 604–620.e22.","chicago":"Dekoninck, Sophie, Edouard B Hannezo, Alejandro Sifrim, Yekaterina A. Miroshnikova, Mariaceleste Aragona, Milan Malfait, Souhir Gargouri, et al. “Defining the Design Principles of Skin Epidermis Postnatal Growth.” <i>Cell</i>. Elsevier, 2020. <a href=\"https://doi.org/10.1016/j.cell.2020.03.015\">https://doi.org/10.1016/j.cell.2020.03.015</a>.","ista":"Dekoninck S, Hannezo EB, Sifrim A, Miroshnikova YA, Aragona M, Malfait M, Gargouri S, De Neunheuser C, Dubois C, Voet T, Wickström SA, Simons BD, Blanpain C. 2020. Defining the design principles of skin epidermis postnatal growth. Cell. 181(3), 604–620.e22.","ieee":"S. Dekoninck <i>et al.</i>, “Defining the design principles of skin epidermis postnatal growth,” <i>Cell</i>, vol. 181, no. 3. Elsevier, p. 604–620.e22, 2020."},"article_processing_charge":"No","status":"public","type":"journal_article","tmp":{"short":"CC BY-NC-ND (4.0)","legal_code_url":"https://creativecommons.org/licenses/by-nc-nd/4.0/legalcode","image":"/images/cc_by_nc_nd.png","name":"Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International (CC BY-NC-ND 4.0)"},"title":"Defining the design principles of skin epidermis postnatal growth","intvolume":"       181","license":"https://creativecommons.org/licenses/by-nc-nd/4.0/","_id":"7789","page":"604-620.e22","external_id":{"isi":["000530708400016"],"pmid":["32259486"]},"doi":"10.1016/j.cell.2020.03.015","department":[{"_id":"EdHa"}],"quality_controlled":"1","has_accepted_license":"1","user_id":"4359f0d1-fa6c-11eb-b949-802e58b17ae8","oa_version":"Published Version","month":"04","publication_identifier":{"eissn":["10974172"],"issn":["00928674"]},"date_updated":"2023-08-21T06:17:43Z","ddc":["570"],"oa":1,"publication_status":"published"},{"publication_identifier":{"eissn":["20505094"]},"ddc":["510"],"date_updated":"2023-08-21T06:18:49Z","oa":1,"publication_status":"published","user_id":"4359f0d1-fa6c-11eb-b949-802e58b17ae8","related_material":{"record":[{"id":"7524","relation":"earlier_version","status":"public"}]},"oa_version":"Published Version","month":"03","article_number":"e20","arxiv":1,"has_accepted_license":"1","department":[{"_id":"RoSe"}],"quality_controlled":"1","intvolume":"         8","_id":"7790","external_id":{"arxiv":["1910.03372"],"isi":["000527342000001"]},"doi":"10.1017/fms.2020.17","type":"journal_article","status":"public","title":"The free energy of the two-dimensional dilute Bose gas. I. Lower bound","tmp":{"short":"CC BY (4.0)","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","image":"/images/cc_by.png","name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)"},"isi":1,"citation":{"short":"A. Deuchert, S. Mayer, R. Seiringer, Forum of Mathematics, Sigma 8 (2020).","chicago":"Deuchert, Andreas, Simon Mayer, and Robert Seiringer. “The Free Energy of the Two-Dimensional Dilute Bose Gas. I. Lower Bound.” <i>Forum of Mathematics, Sigma</i>. Cambridge University Press, 2020. <a href=\"https://doi.org/10.1017/fms.2020.17\">https://doi.org/10.1017/fms.2020.17</a>.","ama":"Deuchert A, Mayer S, Seiringer R. The free energy of the two-dimensional dilute Bose gas. I. Lower bound. <i>Forum of Mathematics, Sigma</i>. 2020;8. doi:<a href=\"https://doi.org/10.1017/fms.2020.17\">10.1017/fms.2020.17</a>","apa":"Deuchert, A., Mayer, S., &#38; Seiringer, R. (2020). The free energy of the two-dimensional dilute Bose gas. I. Lower bound. <i>Forum of Mathematics, Sigma</i>. Cambridge University Press. <a href=\"https://doi.org/10.1017/fms.2020.17\">https://doi.org/10.1017/fms.2020.17</a>","mla":"Deuchert, Andreas, et al. “The Free Energy of the Two-Dimensional Dilute Bose Gas. I. Lower Bound.” <i>Forum of Mathematics, Sigma</i>, vol. 8, e20, Cambridge University Press, 2020, doi:<a href=\"https://doi.org/10.1017/fms.2020.17\">10.1017/fms.2020.17</a>.","ista":"Deuchert A, Mayer S, Seiringer R. 2020. The free energy of the two-dimensional dilute Bose gas. I. Lower bound. Forum of Mathematics, Sigma. 8, e20.","ieee":"A. Deuchert, S. Mayer, and R. Seiringer, “The free energy of the two-dimensional dilute Bose gas. I. Lower bound,” <i>Forum of Mathematics, Sigma</i>, vol. 8. Cambridge University Press, 2020."},"article_processing_charge":"No","ec_funded":1,"language":[{"iso":"eng"}],"year":"2020","day":"14","publication":"Forum of Mathematics, Sigma","date_published":"2020-03-14T00:00:00Z","volume":8,"abstract":[{"lang":"eng","text":"We prove a lower bound for the free energy (per unit volume) of the two-dimensional Bose gas in the thermodynamic limit. We show that the free energy at density 𝜌 and inverse temperature 𝛽 differs from the one of the noninteracting system by the correction term 𝜋𝜌𝜌𝛽𝛽 . Here, is the scattering length of the interaction potential, and 𝛽 is the inverse Berezinskii–Kosterlitz–Thouless critical temperature for superfluidity. The result is valid in the dilute limit 𝜌 and if 𝛽𝜌 ."}],"author":[{"last_name":"Deuchert","first_name":"Andreas","orcid":"0000-0003-3146-6746","full_name":"Deuchert, Andreas","id":"4DA65CD0-F248-11E8-B48F-1D18A9856A87"},{"full_name":"Mayer, Simon","id":"30C4630A-F248-11E8-B48F-1D18A9856A87","first_name":"Simon","last_name":"Mayer"},{"id":"4AFD0470-F248-11E8-B48F-1D18A9856A87","full_name":"Seiringer, Robert","orcid":"0000-0002-6781-0521","last_name":"Seiringer","first_name":"Robert"}],"file_date_updated":"2020-07-14T12:48:03Z","article_type":"original","project":[{"name":"Analysis of quantum many-body systems","_id":"25C6DC12-B435-11E9-9278-68D0E5697425","grant_number":"694227","call_identifier":"H2020"}],"date_created":"2020-05-03T22:00:48Z","scopus_import":"1","file":[{"file_id":"7797","date_created":"2020-05-04T12:02:41Z","creator":"dernst","relation":"main_file","checksum":"8a64da99d107686997876d7cad8cfe1e","date_updated":"2020-07-14T12:48:03Z","content_type":"application/pdf","file_name":"2020_ForumMath_Deuchert.pdf","access_level":"open_access","file_size":692530}],"publisher":"Cambridge University Press"},{"article_type":"original","date_created":"2020-05-04T08:50:47Z","pmid":1,"file":[{"date_updated":"2020-07-14T12:48:03Z","content_type":"application/pdf","file_name":"2020_eLife_Kuhn.pdf","file_size":2893082,"access_level":"open_access","file_id":"7794","date_created":"2020-05-04T09:06:43Z","creator":"dernst","relation":"main_file","checksum":"15d740de1a741fdcc6ec128c48eed017"}],"publisher":"eLife Sciences Publications","scopus_import":"1","publication":"eLife","year":"2020","language":[{"iso":"eng"}],"day":"08","file_date_updated":"2020-07-14T12:48:03Z","author":[{"first_name":"André","last_name":"Kuhn","full_name":"Kuhn, André"},{"first_name":"Sigurd","last_name":"Ramans Harborough","full_name":"Ramans Harborough, Sigurd"},{"full_name":"McLaughlin, Heather M","first_name":"Heather M","last_name":"McLaughlin"},{"full_name":"Natarajan, Bhavani","last_name":"Natarajan","first_name":"Bhavani"},{"full_name":"Verstraeten, Inge","id":"362BF7FE-F248-11E8-B48F-1D18A9856A87","first_name":"Inge","last_name":"Verstraeten","orcid":"0000-0001-7241-2328"},{"full_name":"Friml, Jiří","id":"4159519E-F248-11E8-B48F-1D18A9856A87","orcid":"0000-0002-8302-7596","last_name":"Friml","first_name":"Jiří"},{"full_name":"Kepinski, Stefan","first_name":"Stefan","last_name":"Kepinski"},{"last_name":"Østergaard","first_name":"Lars","full_name":"Østergaard, Lars"}],"date_published":"2020-04-08T00:00:00Z","volume":9,"abstract":[{"lang":"eng","text":"Hormonal signalling in animals often involves direct transcription factor-hormone interactions that modulate gene expression. In contrast, plant hormone signalling is most commonly based on de-repression via the degradation of transcriptional repressors. Recently, we uncovered a non-canonical signalling mechanism for the plant hormone auxin whereby auxin directly affects the activity of the atypical auxin response factor (ARF), ETTIN towards target genes without the requirement for protein degradation. Here we show that ETTIN directly binds auxin, leading to dissociation from co-repressor proteins of the TOPLESS/TOPLESS-RELATED family followed by histone acetylation and induction of gene expression. This mechanism is reminiscent of animal hormone signalling as it affects the activity towards regulation of target genes and provides the first example of a DNA-bound hormone receptor in plants. Whilst auxin affects canonical ARFs indirectly by facilitating degradation of Aux/IAA repressors, direct ETTIN-auxin interactions allow switching between repressive and de-repressive chromatin states in an instantly-reversible manner."}],"external_id":{"isi":["000527752200001"],"pmid":["32267233"]},"doi":"10.7554/elife.51787","intvolume":"         9","_id":"7793","quality_controlled":"1","department":[{"_id":"JiFr"}],"citation":{"mla":"Kuhn, André, et al. “Direct ETTIN-Auxin Interaction Controls Chromatin States in Gynoecium Development.” <i>ELife</i>, vol. 9, e51787, eLife Sciences Publications, 2020, doi:<a href=\"https://doi.org/10.7554/elife.51787\">10.7554/elife.51787</a>.","apa":"Kuhn, A., Ramans Harborough, S., McLaughlin, H. M., Natarajan, B., Verstraeten, I., Friml, J., … Østergaard, L. (2020). Direct ETTIN-auxin interaction controls chromatin states in gynoecium development. <i>ELife</i>. eLife Sciences Publications. <a href=\"https://doi.org/10.7554/elife.51787\">https://doi.org/10.7554/elife.51787</a>","chicago":"Kuhn, André, Sigurd Ramans Harborough, Heather M McLaughlin, Bhavani Natarajan, Inge Verstraeten, Jiří Friml, Stefan Kepinski, and Lars Østergaard. “Direct ETTIN-Auxin Interaction Controls Chromatin States in Gynoecium Development.” <i>ELife</i>. eLife Sciences Publications, 2020. <a href=\"https://doi.org/10.7554/elife.51787\">https://doi.org/10.7554/elife.51787</a>.","ama":"Kuhn A, Ramans Harborough S, McLaughlin HM, et al. Direct ETTIN-auxin interaction controls chromatin states in gynoecium development. <i>eLife</i>. 2020;9. doi:<a href=\"https://doi.org/10.7554/elife.51787\">10.7554/elife.51787</a>","short":"A. Kuhn, S. Ramans Harborough, H.M. McLaughlin, B. Natarajan, I. Verstraeten, J. Friml, S. Kepinski, L. Østergaard, ELife 9 (2020).","ieee":"A. Kuhn <i>et al.</i>, “Direct ETTIN-auxin interaction controls chromatin states in gynoecium development,” <i>eLife</i>, vol. 9. eLife Sciences Publications, 2020.","ista":"Kuhn A, Ramans Harborough S, McLaughlin HM, Natarajan B, Verstraeten I, Friml J, Kepinski S, Østergaard L. 2020. Direct ETTIN-auxin interaction controls chromatin states in gynoecium development. eLife. 9, e51787."},"article_processing_charge":"No","isi":1,"title":"Direct ETTIN-auxin interaction controls chromatin states in gynoecium development","tmp":{"short":"CC BY (4.0)","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","image":"/images/cc_by.png","name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)"},"type":"journal_article","status":"public","oa_version":"Published Version","month":"04","user_id":"4359f0d1-fa6c-11eb-b949-802e58b17ae8","publication_status":"published","oa":1,"publication_identifier":{"issn":["2050-084X"]},"date_updated":"2023-08-21T06:17:12Z","ddc":["580"],"has_accepted_license":"1","article_number":"e51787"},{"_id":"7800","doi":"10.1101/2020.01.10.902064 ","department":[{"_id":"JoDa"},{"_id":"GaNo"},{"_id":"LifeSc"}],"acknowledged_ssus":[{"_id":"PreCl"}],"citation":{"short":"J. Morandell, L.A. Schwarz, B. Basilico, S. Tasciyan, A. Nicolas, C.M. Sommer, C. Kreuzinger, L. Knaus, Z. Dobler, E. Cacci, J.G. Danzl, G. Novarino, BioRxiv (n.d.).","chicago":"Morandell, Jasmin, Lena A Schwarz, Bernadette Basilico, Saren Tasciyan, Armel Nicolas, Christoph M Sommer, Caroline Kreuzinger, et al. “Cul3 Regulates Cytoskeleton Protein Homeostasis and Cell Migration during a Critical Window of Brain Development.” <i>BioRxiv</i>. Cold Spring Harbor Laboratory, n.d. <a href=\"https://doi.org/10.1101/2020.01.10.902064 \">https://doi.org/10.1101/2020.01.10.902064 </a>.","ama":"Morandell J, Schwarz LA, Basilico B, et al. Cul3 regulates cytoskeleton protein homeostasis and cell migration during a critical window of brain development. <i>bioRxiv</i>. doi:<a href=\"https://doi.org/10.1101/2020.01.10.902064 \">10.1101/2020.01.10.902064 </a>","apa":"Morandell, J., Schwarz, L. A., Basilico, B., Tasciyan, S., Nicolas, A., Sommer, C. M., … Novarino, G. (n.d.). Cul3 regulates cytoskeleton protein homeostasis and cell migration during a critical window of brain development. <i>bioRxiv</i>. Cold Spring Harbor Laboratory. <a href=\"https://doi.org/10.1101/2020.01.10.902064 \">https://doi.org/10.1101/2020.01.10.902064 </a>","mla":"Morandell, Jasmin, et al. “Cul3 Regulates Cytoskeleton Protein Homeostasis and Cell Migration during a Critical Window of Brain Development.” <i>BioRxiv</i>, Cold Spring Harbor Laboratory, doi:<a href=\"https://doi.org/10.1101/2020.01.10.902064 \">10.1101/2020.01.10.902064 </a>.","ieee":"J. Morandell <i>et al.</i>, “Cul3 regulates cytoskeleton protein homeostasis and cell migration during a critical window of brain development,” <i>bioRxiv</i>. Cold Spring Harbor Laboratory.","ista":"Morandell J, Schwarz LA, Basilico B, Tasciyan S, Nicolas A, Sommer CM, Kreuzinger C, Knaus L, Dobler Z, Cacci E, Danzl JG, Novarino G. Cul3 regulates cytoskeleton protein homeostasis and cell migration during a critical window of brain development. bioRxiv, <a href=\"https://doi.org/10.1101/2020.01.10.902064 \">10.1101/2020.01.10.902064 </a>."},"article_processing_charge":"No","type":"preprint","status":"public","title":"Cul3 regulates cytoskeleton protein homeostasis and cell migration during a critical window of brain development","tmp":{"short":"CC BY-NC-ND (4.0)","legal_code_url":"https://creativecommons.org/licenses/by-nc-nd/4.0/legalcode","image":"/images/cc_by_nc_nd.png","name":"Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International (CC BY-NC-ND 4.0)"},"user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","related_material":{"record":[{"id":"8620","relation":"dissertation_contains","status":"public"},{"status":"public","id":"9429","relation":"later_version"}]},"oa_version":"Preprint","month":"01","date_updated":"2024-09-10T12:04:26Z","ddc":["570"],"oa":1,"publication_status":"submitted","has_accepted_license":"1","date_created":"2020-05-05T14:31:33Z","project":[{"call_identifier":"FWF","grant_number":"I03600","name":"Optical control of synaptic function via adhesion molecules","_id":"265CB4D0-B435-11E9-9278-68D0E5697425"},{"call_identifier":"FWF","grant_number":"W1232-B24","name":"Molecular Drug Targets","_id":"2548AE96-B435-11E9-9278-68D0E5697425"}],"file":[{"date_created":"2020-05-05T14:31:19Z","creator":"rsix","relation":"main_file","checksum":"c6799ab5daba80efe8e2ed63c15f8c81","file_id":"7801","file_name":"2020.01.10.902064v1.full.pdf","access_level":"open_access","file_size":2931370,"date_updated":"2020-07-14T12:48:03Z","content_type":"application/pdf"}],"publisher":"Cold Spring Harbor Laboratory","year":"2020","language":[{"iso":"eng"}],"day":"11","publication":"bioRxiv","file_date_updated":"2020-07-14T12:48:03Z","date_published":"2020-01-11T00:00:00Z","abstract":[{"text":"De novo loss of function mutations in the ubiquitin ligase-encoding gene Cullin3 (CUL3) lead to autism spectrum disorder (ASD). Here, we used Cul3 mouse models to evaluate the consequences of Cul3 mutations in vivo. Our results show that Cul3 haploinsufficient mice exhibit deficits in motor coordination as well as ASD-relevant social and cognitive impairments. Cul3 mutant brain displays cortical lamination abnormalities due to defective neuronal migration and reduced numbers of excitatory and inhibitory neurons. In line with the observed abnormal columnar organization, Cul3 haploinsufficiency is associated with decreased spontaneous excitatory and inhibitory activity in the cortex. At the molecular level, employing a quantitative proteomic approach, we show that Cul3 regulates cytoskeletal and adhesion protein abundance in mouse embryos. Abnormal regulation of cytoskeletal proteins in Cul3 mutant neuronal cells results in atypical organization of the actin mesh at the cell leading edge, likely causing the observed migration deficits. In contrast to these important functions early in development, Cul3 deficiency appears less relevant at adult stages. In fact, induction of Cul3 haploinsufficiency in adult mice does not result in the behavioral defects observed in constitutive Cul3 haploinsufficient animals. Taken together, our data indicate that Cul3 has a critical role in the regulation of cytoskeletal proteins and neuronal migration and that ASD-associated defects and behavioral abnormalities are primarily due to Cul3 functions at early developmental stages.","lang":"eng"}],"author":[{"full_name":"Morandell, Jasmin","id":"4739D480-F248-11E8-B48F-1D18A9856A87","first_name":"Jasmin","last_name":"Morandell"},{"first_name":"Lena A","last_name":"Schwarz","full_name":"Schwarz, Lena A","id":"29A8453C-F248-11E8-B48F-1D18A9856A87"},{"last_name":"Basilico","first_name":"Bernadette","orcid":"0000-0003-1843-3173","id":"36035796-5ACA-11E9-A75E-7AF2E5697425","full_name":"Basilico, Bernadette"},{"full_name":"Tasciyan, Saren","id":"4323B49C-F248-11E8-B48F-1D18A9856A87","first_name":"Saren","last_name":"Tasciyan","orcid":"0000-0003-1671-393X"},{"first_name":"Armel","last_name":"Nicolas","full_name":"Nicolas, Armel","id":"2A103192-F248-11E8-B48F-1D18A9856A87"},{"orcid":"0000-0003-1216-9105","last_name":"Sommer","first_name":"Christoph M","id":"4DF26D8C-F248-11E8-B48F-1D18A9856A87","full_name":"Sommer, Christoph M"},{"first_name":"Caroline","last_name":"Kreuzinger","full_name":"Kreuzinger, Caroline","id":"382077BA-F248-11E8-B48F-1D18A9856A87"},{"full_name":"Knaus, Lisa","id":"3B2ABCF4-F248-11E8-B48F-1D18A9856A87","last_name":"Knaus","first_name":"Lisa"},{"last_name":"Dobler","first_name":"Zoe","full_name":"Dobler, Zoe","id":"D23090A2-9057-11EA-883A-A8396FC7A38F"},{"last_name":"Cacci","first_name":"Emanuele","full_name":"Cacci, Emanuele"},{"id":"42EFD3B6-F248-11E8-B48F-1D18A9856A87","full_name":"Danzl, Johann G","first_name":"Johann G","last_name":"Danzl","orcid":"0000-0001-8559-3973"},{"first_name":"Gaia","last_name":"Novarino","orcid":"0000-0002-7673-7178","full_name":"Novarino, Gaia","id":"3E57A680-F248-11E8-B48F-1D18A9856A87"}]},{"date_created":"2020-05-06T08:53:34Z","project":[{"name":"ISTplus - Postdoctoral Fellowships","_id":"260C2330-B435-11E9-9278-68D0E5697425","call_identifier":"H2020","grant_number":"754411"}],"publisher":"Association for Computing Machinery","main_file_link":[{"open_access":"1","url":"https://arxiv.org/abs/1912.05390"}],"scopus_import":"1","day":"01","language":[{"iso":"eng"}],"year":"2020","publication":"Proceedings of the 32nd ACM Symposium on Parallelism in Algorithms and Architectures (SPAA 2020)","ec_funded":1,"issue":"7","abstract":[{"lang":"eng","text":"The Massively Parallel Computation (MPC) model is an emerging model which distills core  aspects of distributed and parallel computation. It has been developed as a tool to solve (typically graph) problems in systems where the input is distributed over many machines with limited space.\r\n\t\r\nRecent work has focused on the regime in which machines have sublinear (in $n$, the number of nodes in the input graph) space, with randomized algorithms presented for fundamental graph problems of Maximal Matching and Maximal Independent Set. However, there have been no prior corresponding deterministic algorithms.\r\n\t\r\n\tA major challenge underlying the sublinear space setting is that the local space of each machine might be too small to store all the edges incident to a single node. This poses a considerable obstacle compared to the classical models in which each node is assumed to know and have easy access to its incident edges. To overcome this barrier we introduce a new graph sparsification technique that deterministically computes a low-degree subgraph with additional desired properties. The degree of the nodes in this subgraph is small in the sense that the edges of each node can be now stored on a single machine. This low-degree subgraph also has the property that solving the problem on this subgraph provides \\emph{significant} global progress, i.e., progress towards solving the problem for the original input graph.\r\n\t\r\nUsing this framework to derandomize the well-known randomized algorithm of Luby [SICOMP'86], we obtain $O(\\log \\Delta+\\log\\log n)$-round deterministic MPC algorithms for solving the fundamental problems of Maximal Matching and Maximal Independent Set with $O(n^{\\epsilon})$ space on each machine for any constant $\\epsilon > 0$. Based on the recent work of Ghaffari et al. [FOCS'18], this additive $O(\\log\\log n)$ factor is conditionally essential. These algorithms can also be shown to run in $O(\\log \\Delta)$ rounds in the closely related model of CONGESTED CLIQUE, improving upon the state-of-the-art bound of $O(\\log^2 \\Delta)$ rounds by Censor-Hillel et al. [DISC'17]."}],"date_published":"2020-07-01T00:00:00Z","author":[{"orcid":"0000-0002-5646-9524","first_name":"Artur","last_name":"Czumaj","full_name":"Czumaj, Artur"},{"orcid":"0000-0002-5646-9524","first_name":"Peter","last_name":"Davies","id":"11396234-BB50-11E9-B24C-90FCE5697425","full_name":"Davies, Peter"},{"first_name":"Merav","last_name":"Parter","full_name":"Parter, Merav"}],"_id":"7802","page":"175-185","doi":"10.1145/3350755.3400282","external_id":{"isi":["000744436200015"],"arxiv":["1912.05390"]},"department":[{"_id":"DaAl"}],"quality_controlled":"1","isi":1,"article_processing_charge":"No","citation":{"ama":"Czumaj A, Davies P, Parter M. Graph sparsification for derandomizing massively parallel computation with low space. In: <i>Proceedings of the 32nd ACM Symposium on Parallelism in Algorithms and Architectures (SPAA 2020)</i>. Association for Computing Machinery; 2020:175-185. doi:<a href=\"https://doi.org/10.1145/3350755.3400282\">10.1145/3350755.3400282</a>","chicago":"Czumaj, Artur, Peter Davies, and Merav Parter. “Graph Sparsification for Derandomizing Massively Parallel Computation with Low Space.” In <i>Proceedings of the 32nd ACM Symposium on Parallelism in Algorithms and Architectures (SPAA 2020)</i>, 175–85. Association for Computing Machinery, 2020. <a href=\"https://doi.org/10.1145/3350755.3400282\">https://doi.org/10.1145/3350755.3400282</a>.","short":"A. Czumaj, P. Davies, M. Parter, in:, Proceedings of the 32nd ACM Symposium on Parallelism in Algorithms and Architectures (SPAA 2020), Association for Computing Machinery, 2020, pp. 175–185.","mla":"Czumaj, Artur, et al. “Graph Sparsification for Derandomizing Massively Parallel Computation with Low Space.” <i>Proceedings of the 32nd ACM Symposium on Parallelism in Algorithms and Architectures (SPAA 2020)</i>, no. 7, Association for Computing Machinery, 2020, pp. 175–85, doi:<a href=\"https://doi.org/10.1145/3350755.3400282\">10.1145/3350755.3400282</a>.","apa":"Czumaj, A., Davies, P., &#38; Parter, M. (2020). Graph sparsification for derandomizing massively parallel computation with low space. In <i>Proceedings of the 32nd ACM Symposium on Parallelism in Algorithms and Architectures (SPAA 2020)</i> (pp. 175–185). Virtual Event, United States: Association for Computing Machinery. <a href=\"https://doi.org/10.1145/3350755.3400282\">https://doi.org/10.1145/3350755.3400282</a>","ieee":"A. Czumaj, P. Davies, and M. Parter, “Graph sparsification for derandomizing massively parallel computation with low space,” in <i>Proceedings of the 32nd ACM Symposium on Parallelism in Algorithms and Architectures (SPAA 2020)</i>, Virtual Event, United States, 2020, no. 7, pp. 175–185.","ista":"Czumaj A, Davies P, Parter M. 2020. Graph sparsification for derandomizing massively parallel computation with low space. Proceedings of the 32nd ACM Symposium on Parallelism in Algorithms and Architectures (SPAA 2020). SPAA: Symposium on Parallelism in Algorithms and Architectures, 175–185."},"type":"conference","status":"public","title":"Graph sparsification for derandomizing massively parallel computation with low space","user_id":"4359f0d1-fa6c-11eb-b949-802e58b17ae8","related_material":{"record":[{"id":"9541","relation":"later_version","status":"public"}]},"oa_version":"Preprint","month":"07","date_updated":"2024-02-28T12:53:09Z","oa":1,"publication_status":"published","conference":{"name":"SPAA: Symposium on Parallelism in Algorithms and Architectures","start_date":"2020-07-15","end_date":"2020-07-17","location":"Virtual Event, United States"},"arxiv":1},{"project":[{"name":"ISTplus - Postdoctoral Fellowships","_id":"260C2330-B435-11E9-9278-68D0E5697425","call_identifier":"H2020","grant_number":"754411"}],"date_created":"2020-05-06T09:02:14Z","file":[{"success":1,"content_type":"application/pdf","date_updated":"2020-10-08T08:17:36Z","file_size":520051,"access_level":"open_access","file_name":"ColoringArxiv.pdf","file_id":"8624","relation":"main_file","checksum":"46fe4fc58a64eb04068115573f631d4c","date_created":"2020-10-08T08:17:36Z","creator":"pdavies"}],"publisher":"Association for Computing Machinery","publication":"Proceedings of the 2020 ACM Symposium on Principles of Distributed Computing","day":"01","year":"2020","language":[{"iso":"eng"}],"ec_funded":1,"file_date_updated":"2020-10-08T08:17:36Z","author":[{"last_name":"Czumaj","first_name":"Artur","orcid":"0000-0002-5646-9524","full_name":"Czumaj, Artur"},{"orcid":"0000-0002-5646-9524","first_name":"Peter","last_name":"Davies","id":"11396234-BB50-11E9-B24C-90FCE5697425","full_name":"Davies, Peter"},{"first_name":"Merav","last_name":"Parter","full_name":"Parter, Merav"}],"abstract":[{"lang":"eng","text":"We settle the complexity of the (Δ+1)-coloring and (Δ+1)-list coloring problems in the CONGESTED CLIQUE model by presenting a simple deterministic algorithm for both problems running in a constant number of rounds. This matches the complexity of the recent breakthrough randomized constant-round (Δ+1)-list coloring algorithm due to Chang et al. (PODC'19), and significantly improves upon the state-of-the-art O(logΔ)-round deterministic (Δ+1)-coloring bound of Parter (ICALP'18).\r\nA remarkable property of our algorithm is its simplicity. Whereas the state-of-the-art randomized algorithms for this problem are based on the quite involved local coloring algorithm of Chang et al. (STOC'18), our algorithm can be described in just a few lines. At a high level, it applies a careful derandomization of a recursive procedure which partitions the nodes and their respective palettes into separate bins. We show that after O(1) recursion steps, the remaining uncolored subgraph within each bin has linear size, and thus can be solved locally by collecting it to a single node. This algorithm can also be implemented in the Massively Parallel Computation (MPC) model provided that each machine has linear (in n, the number of nodes in the input graph) space.\r\nWe also show an extension of our algorithm to the MPC regime in which machines have sublinear space: we present the first deterministic (Δ+1)-list coloring algorithm designed for sublinear-space MPC, which runs in O(logΔ+loglogn) rounds."}],"date_published":"2020-07-01T00:00:00Z","doi":"10.1145/3382734.3405751","external_id":{"arxiv":["2009.06043"]},"_id":"7803","page":"309-318","quality_controlled":"1","department":[{"_id":"DaAl"}],"article_processing_charge":"No","citation":{"ista":"Czumaj A, Davies P, Parter M. 2020. Simple, deterministic, constant-round coloring in the congested clique. Proceedings of the 2020 ACM Symposium on Principles of Distributed Computing. PODC: Symposium on Principles of Distributed Computing, 309–318.","ieee":"A. Czumaj, P. Davies, and M. Parter, “Simple, deterministic, constant-round coloring in the congested clique,” in <i>Proceedings of the 2020 ACM Symposium on Principles of Distributed Computing</i>, Salerno, Italy, 2020, pp. 309–318.","mla":"Czumaj, Artur, et al. “Simple, Deterministic, Constant-Round Coloring in the Congested Clique.” <i>Proceedings of the 2020 ACM Symposium on Principles of Distributed Computing</i>, Association for Computing Machinery, 2020, pp. 309–18, doi:<a href=\"https://doi.org/10.1145/3382734.3405751\">10.1145/3382734.3405751</a>.","apa":"Czumaj, A., Davies, P., &#38; Parter, M. (2020). Simple, deterministic, constant-round coloring in the congested clique. In <i>Proceedings of the 2020 ACM Symposium on Principles of Distributed Computing</i> (pp. 309–318). Salerno, Italy: Association for Computing Machinery. <a href=\"https://doi.org/10.1145/3382734.3405751\">https://doi.org/10.1145/3382734.3405751</a>","chicago":"Czumaj, Artur, Peter Davies, and Merav Parter. “Simple, Deterministic, Constant-Round Coloring in the Congested Clique.” In <i>Proceedings of the 2020 ACM Symposium on Principles of Distributed Computing</i>, 309–18. Association for Computing Machinery, 2020. <a href=\"https://doi.org/10.1145/3382734.3405751\">https://doi.org/10.1145/3382734.3405751</a>.","ama":"Czumaj A, Davies P, Parter M. Simple, deterministic, constant-round coloring in the congested clique. In: <i>Proceedings of the 2020 ACM Symposium on Principles of Distributed Computing</i>. Association for Computing Machinery; 2020:309-318. doi:<a href=\"https://doi.org/10.1145/3382734.3405751\">10.1145/3382734.3405751</a>","short":"A. Czumaj, P. Davies, M. Parter, in:, Proceedings of the 2020 ACM Symposium on Principles of Distributed Computing, Association for Computing Machinery, 2020, pp. 309–318."},"title":"Simple, deterministic, constant-round coloring in the congested clique","status":"public","type":"conference","oa_version":"Submitted Version","month":"07","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","oa":1,"publication_status":"published","conference":{"location":"Salerno, Italy","start_date":"2020-08-03","end_date":"2020-08-07","name":"PODC: Symposium on Principles of Distributed Computing"},"ddc":["000"],"date_updated":"2021-01-12T08:15:37Z","has_accepted_license":"1","arxiv":1},{"tmp":{"short":"CC BY (4.0)","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","image":"/images/cc_by.png","name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)"},"title":"MALT-1 mediates IL-17 neural signaling to regulate C. elegans behavior, immunity and longevity","type":"journal_article","status":"public","citation":{"apa":"Flynn, S. M., Chen, C., Artan, M., Barratt, S., Crisp, A., Nelson, G. M., … de Bono, M. (2020). MALT-1 mediates IL-17 neural signaling to regulate C. elegans behavior, immunity and longevity. <i>Nature Communications</i>. Springer Nature. <a href=\"https://doi.org/10.1038/s41467-020-15872-y\">https://doi.org/10.1038/s41467-020-15872-y</a>","mla":"Flynn, Sean M., et al. “MALT-1 Mediates IL-17 Neural Signaling to Regulate C. Elegans Behavior, Immunity and Longevity.” <i>Nature Communications</i>, vol. 11, 2099, Springer Nature, 2020, doi:<a href=\"https://doi.org/10.1038/s41467-020-15872-y\">10.1038/s41467-020-15872-y</a>.","chicago":"Flynn, Sean M., Changchun Chen, Murat Artan, Stephen Barratt, Alastair Crisp, Geoffrey M. Nelson, Sew Yeu Peak-Chew, Farida Begum, Mark Skehel, and Mario de Bono. “MALT-1 Mediates IL-17 Neural Signaling to Regulate C. Elegans Behavior, Immunity and Longevity.” <i>Nature Communications</i>. Springer Nature, 2020. <a href=\"https://doi.org/10.1038/s41467-020-15872-y\">https://doi.org/10.1038/s41467-020-15872-y</a>.","ama":"Flynn SM, Chen C, Artan M, et al. MALT-1 mediates IL-17 neural signaling to regulate C. elegans behavior, immunity and longevity. <i>Nature Communications</i>. 2020;11. doi:<a href=\"https://doi.org/10.1038/s41467-020-15872-y\">10.1038/s41467-020-15872-y</a>","short":"S.M. Flynn, C. Chen, M. Artan, S. Barratt, A. Crisp, G.M. Nelson, S.Y. Peak-Chew, F. Begum, M. Skehel, M. de Bono, Nature Communications 11 (2020).","ieee":"S. M. Flynn <i>et al.</i>, “MALT-1 mediates IL-17 neural signaling to regulate C. elegans behavior, immunity and longevity,” <i>Nature Communications</i>, vol. 11. Springer Nature, 2020.","ista":"Flynn SM, Chen C, Artan M, Barratt S, Crisp A, Nelson GM, Peak-Chew SY, Begum F, Skehel M, de Bono M. 2020. MALT-1 mediates IL-17 neural signaling to regulate C. elegans behavior, immunity and longevity. Nature Communications. 11, 2099."},"article_processing_charge":"No","isi":1,"quality_controlled":"1","department":[{"_id":"MaDe"}],"external_id":{"isi":["000531855500029"]},"doi":"10.1038/s41467-020-15872-y","intvolume":"        11","_id":"7804","article_number":"2099","has_accepted_license":"1","publication_status":"published","oa":1,"publication_identifier":{"eissn":["20411723"]},"ddc":["570"],"date_updated":"2023-08-21T06:21:14Z","oa_version":"Published Version","month":"04","user_id":"4359f0d1-fa6c-11eb-b949-802e58b17ae8","scopus_import":"1","file":[{"date_updated":"2020-07-14T12:48:03Z","content_type":"application/pdf","file_name":"2020_NatureComm_Flynn.pdf","file_size":4609120,"access_level":"open_access","file_id":"7817","date_created":"2020-05-11T10:36:33Z","creator":"dernst","checksum":"dce367abf2c1a1d15f58fe6f7de82893","relation":"main_file"}],"publisher":"Springer Nature","date_created":"2020-05-10T22:00:47Z","article_type":"original","author":[{"full_name":"Flynn, Sean M.","first_name":"Sean M.","last_name":"Flynn"},{"full_name":"Chen, Changchun","first_name":"Changchun","last_name":"Chen"},{"id":"C407B586-6052-11E9-B3AE-7006E6697425","full_name":"Artan, Murat","first_name":"Murat","last_name":"Artan","orcid":"0000-0001-8945-6992"},{"last_name":"Barratt","first_name":"Stephen","full_name":"Barratt, Stephen"},{"full_name":"Crisp, Alastair","first_name":"Alastair","last_name":"Crisp"},{"last_name":"Nelson","first_name":"Geoffrey M.","full_name":"Nelson, Geoffrey M."},{"full_name":"Peak-Chew, Sew Yeu","first_name":"Sew Yeu","last_name":"Peak-Chew"},{"full_name":"Begum, Farida","first_name":"Farida","last_name":"Begum"},{"full_name":"Skehel, Mark","first_name":"Mark","last_name":"Skehel"},{"full_name":"De Bono, Mario","id":"4E3FF80E-F248-11E8-B48F-1D18A9856A87","orcid":"0000-0001-8347-0443","last_name":"De Bono","first_name":"Mario"}],"date_published":"2020-04-29T00:00:00Z","volume":11,"abstract":[{"lang":"eng","text":"Besides pro-inflammatory roles, the ancient cytokine interleukin-17 (IL-17) modulates neural circuit function. We investigate IL-17 signaling in neurons, and the extent it can alter organismal phenotypes. We combine immunoprecipitation and mass spectrometry to biochemically characterize endogenous signaling complexes that function downstream of IL-17 receptors in C. elegans neurons. We identify the paracaspase MALT-1 as a critical output of the pathway. MALT1 mediates signaling from many immune receptors in mammals, but was not previously implicated in IL-17 signaling or nervous system function. C. elegans MALT-1 forms a complex with homologs of Act1 and IRAK and appears to function both as a scaffold and a protease. MALT-1 is expressed broadly in the C. elegans nervous system, and neuronal IL-17–MALT-1 signaling regulates multiple phenotypes, including escape behavior, associative learning, immunity and longevity. Our data suggest MALT1 has an ancient role modulating neural circuit function downstream of IL-17 to remodel physiology and behavior."}],"file_date_updated":"2020-07-14T12:48:03Z","publication":"Nature Communications","year":"2020","language":[{"iso":"eng"}],"day":"29"},{"file":[{"success":1,"creator":"dernst","date_created":"2020-10-06T07:47:53Z","checksum":"2cba327c9e9416d75cb96be54b0fb441","relation":"main_file","file_id":"8614","file_name":"2020_NatureComm_Hurny.pdf","access_level":"open_access","file_size":4743576,"date_updated":"2020-10-06T07:47:53Z","content_type":"application/pdf"}],"publisher":"Springer Nature","pmid":1,"scopus_import":"1","date_created":"2020-05-10T22:00:48Z","project":[{"name":"Hormone cross-talk drives nutrient dependent plant development","_id":"2542D156-B435-11E9-9278-68D0E5697425","call_identifier":"FWF","grant_number":"I 1774-B16"},{"call_identifier":"FP7","grant_number":"291734","_id":"25681D80-B435-11E9-9278-68D0E5697425","name":"International IST Postdoc Fellowship Programme"}],"article_type":"original","file_date_updated":"2020-10-06T07:47:53Z","author":[{"last_name":"Hurny","first_name":"Andrej","orcid":"0000-0003-3638-1426","id":"4DC4AF46-F248-11E8-B48F-1D18A9856A87","full_name":"Hurny, Andrej"},{"id":"33A3C818-F248-11E8-B48F-1D18A9856A87","full_name":"Cuesta, Candela","last_name":"Cuesta","first_name":"Candela","orcid":"0000-0003-1923-2410"},{"first_name":"Nicola","last_name":"Cavallari","full_name":"Cavallari, Nicola","id":"457160E6-F248-11E8-B48F-1D18A9856A87"},{"orcid":"0000-0002-5503-4983","first_name":"Krisztina","last_name":"Ötvös","full_name":"Ötvös, Krisztina","id":"29B901B0-F248-11E8-B48F-1D18A9856A87"},{"full_name":"Duclercq, Jerome","first_name":"Jerome","last_name":"Duclercq"},{"first_name":"Ladislav","last_name":"Dokládal","full_name":"Dokládal, Ladislav"},{"last_name":"Montesinos López","first_name":"Juan C","orcid":"0000-0001-9179-6099","id":"310A8E3E-F248-11E8-B48F-1D18A9856A87","full_name":"Montesinos López, Juan C"},{"first_name":"Marçal","last_name":"Gallemi","orcid":"0000-0003-4675-6893","id":"460C6802-F248-11E8-B48F-1D18A9856A87","full_name":"Gallemi, Marçal"},{"id":"42FE702E-F248-11E8-B48F-1D18A9856A87","full_name":"Semeradova, Hana","last_name":"Semeradova","first_name":"Hana"},{"first_name":"Thomas","last_name":"Rauter","full_name":"Rauter, Thomas","id":"A0385D1A-9376-11EA-A47D-9862C5E3AB22"},{"full_name":"Stenzel, Irene","first_name":"Irene","last_name":"Stenzel"},{"full_name":"Persiau, Geert","first_name":"Geert","last_name":"Persiau"},{"first_name":"Freia","last_name":"Benade","full_name":"Benade, Freia"},{"full_name":"Bhalearo, Rishikesh","last_name":"Bhalearo","first_name":"Rishikesh"},{"full_name":"Sýkorová, Eva","last_name":"Sýkorová","first_name":"Eva"},{"first_name":"András","last_name":"Gorzsás","full_name":"Gorzsás, András"},{"full_name":"Sechet, Julien","first_name":"Julien","last_name":"Sechet"},{"last_name":"Mouille","first_name":"Gregory","full_name":"Mouille, Gregory"},{"first_name":"Ingo","last_name":"Heilmann","full_name":"Heilmann, Ingo"},{"first_name":"Geert","last_name":"De Jaeger","full_name":"De Jaeger, Geert"},{"first_name":"Jutta","last_name":"Ludwig-Müller","full_name":"Ludwig-Müller, Jutta"},{"full_name":"Benková, Eva","id":"38F4F166-F248-11E8-B48F-1D18A9856A87","last_name":"Benková","first_name":"Eva","orcid":"0000-0002-8510-9739"}],"volume":11,"abstract":[{"lang":"eng","text":"Plants as non-mobile organisms constantly integrate varying environmental signals to flexibly adapt their growth and development. Local fluctuations in water and nutrient availability, sudden changes in temperature or other abiotic and biotic stresses can trigger changes in the growth of plant organs. Multiple mutually interconnected hormonal signaling cascades act as essential endogenous translators of these exogenous signals in the adaptive responses of plants. Although the molecular backbones of hormone transduction pathways have been identified, the mechanisms underlying their interactions are largely unknown. Here, using genome wide transcriptome profiling we identify an auxin and cytokinin cross-talk component; SYNERGISTIC ON AUXIN AND CYTOKININ 1 (SYAC1), whose expression in roots is strictly dependent on both of these hormonal pathways. We show that SYAC1 is a regulator of secretory pathway, whose enhanced activity interferes with deposition of cell wall components and can fine-tune organ growth and sensitivity to soil pathogens."}],"date_published":"2020-05-01T00:00:00Z","publication":"Nature Communications","day":"01","language":[{"iso":"eng"}],"year":"2020","ec_funded":1,"article_processing_charge":"No","citation":{"ieee":"A. Hurny <i>et al.</i>, “Synergistic on Auxin and Cytokinin 1 positively regulates growth and attenuates soil pathogen resistance,” <i>Nature Communications</i>, vol. 11. Springer Nature, 2020.","ista":"Hurny A, Cuesta C, Cavallari N, Ötvös K, Duclercq J, Dokládal L, Montesinos López JC, Gallemi M, Semerádová H, Rauter T, Stenzel I, Persiau G, Benade F, Bhalearo R, Sýkorová E, Gorzsás A, Sechet J, Mouille G, Heilmann I, De Jaeger G, Ludwig-Müller J, Benková E. 2020. Synergistic on Auxin and Cytokinin 1 positively regulates growth and attenuates soil pathogen resistance. Nature Communications. 11, 2170.","short":"A. Hurny, C. Cuesta, N. Cavallari, K. Ötvös, J. Duclercq, L. Dokládal, J.C. Montesinos López, M. Gallemi, H. Semerádová, T. Rauter, I. Stenzel, G. Persiau, F. Benade, R. Bhalearo, E. Sýkorová, A. Gorzsás, J. Sechet, G. Mouille, I. Heilmann, G. De Jaeger, J. Ludwig-Müller, E. Benková, Nature Communications 11 (2020).","ama":"Hurny A, Cuesta C, Cavallari N, et al. Synergistic on Auxin and Cytokinin 1 positively regulates growth and attenuates soil pathogen resistance. <i>Nature Communications</i>. 2020;11. doi:<a href=\"https://doi.org/10.1038/s41467-020-15895-5\">10.1038/s41467-020-15895-5</a>","chicago":"Hurny, Andrej, Candela Cuesta, Nicola Cavallari, Krisztina Ötvös, Jerome Duclercq, Ladislav Dokládal, Juan C Montesinos López, et al. “Synergistic on Auxin and Cytokinin 1 Positively Regulates Growth and Attenuates Soil Pathogen Resistance.” <i>Nature Communications</i>. Springer Nature, 2020. <a href=\"https://doi.org/10.1038/s41467-020-15895-5\">https://doi.org/10.1038/s41467-020-15895-5</a>.","mla":"Hurny, Andrej, et al. “Synergistic on Auxin and Cytokinin 1 Positively Regulates Growth and Attenuates Soil Pathogen Resistance.” <i>Nature Communications</i>, vol. 11, 2170, Springer Nature, 2020, doi:<a href=\"https://doi.org/10.1038/s41467-020-15895-5\">10.1038/s41467-020-15895-5</a>.","apa":"Hurny, A., Cuesta, C., Cavallari, N., Ötvös, K., Duclercq, J., Dokládal, L., … Benková, E. (2020). Synergistic on Auxin and Cytokinin 1 positively regulates growth and attenuates soil pathogen resistance. <i>Nature Communications</i>. Springer Nature. <a href=\"https://doi.org/10.1038/s41467-020-15895-5\">https://doi.org/10.1038/s41467-020-15895-5</a>"},"isi":1,"acknowledged_ssus":[{"_id":"Bio"},{"_id":"LifeSc"}],"title":"Synergistic on Auxin and Cytokinin 1 positively regulates growth and attenuates soil pathogen resistance","tmp":{"short":"CC BY (4.0)","legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","image":"/images/cc_by.png","name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)"},"status":"public","type":"journal_article","doi":"10.1038/s41467-020-15895-5","external_id":{"pmid":["32358503"],"isi":["000531425900012"]},"_id":"7805","intvolume":"        11","acknowledgement":"We thank Daria Siekhaus, Jiri Friml and Alexander Johnson for critical reading of the manuscript, Peter Pimpl, Christian Luschnig and Liwen Jiang for sharing published material, Lesia Rodriguez Solovey for technical assistance. This work was supported by the Austrian Science Fund (FWF01_I1774S) to A.H., K.Ö., and E.B., the German Research Foundation (DFG; He3424/6-1 to I.H.), by the People Programme (Marie Curie Actions) of the European Union’s Seventh Framework Programme (FP7/2007-2013) under REA grant agreement n° [291734] (to N.C.), by the EU in the framework of the Marie-Curie FP7 COFUND People Programme through the award of an AgreenSkills+ fellowship No. 609398 (to J.S.) and by the Scientific Service Units of IST-Austria through resources provided by the Bioimaging Facility, the Life Science Facility. The IJPB benefits from the support of Saclay Plant Sciences-SPS (ANR-17-EUR-0007).","quality_controlled":"1","department":[{"_id":"EvBe"}],"has_accepted_license":"1","article_number":"2170","month":"05","oa_version":"Published Version","user_id":"4359f0d1-fa6c-11eb-b949-802e58b17ae8","oa":1,"publication_status":"published","date_updated":"2023-08-21T06:21:56Z","ddc":["570"],"publication_identifier":{"eissn":["20411723"]}}]