[{"publication_status":"published","oa":1,"main_file_link":[{"url":"https://arxiv.org/abs/2108.03850","open_access":"1"}],"volume":925,"arxiv":1,"issue":"2","article_processing_charge":"No","article_number":"111","_id":"11509","date_published":"2022-01-31T00:00:00Z","abstract":[{"lang":"eng","text":"We present Keck/LRIS follow-up spectroscopy for 13 photometric candidates of extremely metal-poor galaxies (EMPGs) selected by a machine-learning technique applied to the deep (∼26 AB mag) optical and wide-area (∼500 deg2) Subaru imaging data in the EMPRESS survey. Nine out of the 13 candidates are EMPGs with an oxygen abundance (O/H) less than ∼10% solar value (O/H)⊙, and four sources are contaminants of moderately metal-rich galaxies or no emission-line objects. Notably, two out of the nine EMPGs have extremely low stellar masses and oxygen abundances of 5 × 10⁴x–7 × -10⁵ M⊙ and 2%–3% (O/H)⊙, respectively. With a sample of five EMPGs with (Fe/O) measurements, two (three) of which are taken from this study (the literature), we confirm that two EMPGs with the lowest (O/H) ratios of ∼2% (O/H)⊙ show high (Fe/O) ratios of ∼0.1, close to the solar abundance ratio. Comparing galaxy chemical enrichment models, we find that the two EMPGs cannot be explained by a scenario of metal-poor gas accretion/episodic star formation history due to their low (N/O) ratios. We conclude that the two EMPGs can be reproduced by the inclusion of bright hypernovae and/or hypothetical pair-instability supernovae (SNe) preferentially produced in a metal-poor environment. This conclusion implies that primordial galaxies at z ∼ 10 could have a high abundance of Fe that did not originate from Type Ia SNe with delays and that Fe may not serve as a cosmic clock for primordial galaxies."}],"user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","date_updated":"2022-07-21T05:51:25Z","external_id":{"arxiv":["2108.03850"]},"scopus_import":"1","publication_identifier":{"eissn":["1538-4357"],"issn":["0004-637X"]},"article_type":"original","oa_version":"Published Version","year":"2022","publisher":"IOP Publishing","quality_controlled":"1","publication":"The Astrophysical Journal","status":"public","intvolume":" 925","extern":"1","month":"01","date_created":"2022-07-06T12:01:48Z","acknowledgement":"We thank the referee for the valuable comments. We are also grateful to Koh Takahashi, Nozomu Tominaga, Chiaki Kobayashi, Yutaka Hirai, and Daichi Kashino for having useful discussions. This paper includes data gathered with the 10 m Keck Telescope located at W. M. Keck Observatory, Hawaii. We thank the staff of Keck Observatory for their help with the observations. The Hyper Suprime-Cam (HSC) collaboration includes the astronomical communities of Japan and Taiwan, and Princeton University. The HSC instrumentation and software were developed by the National Astronomical Observatory of Japan (NAOJ), the Kavli Institute for the Physics and Mathematics of the Universe (Kavli IPMU), the University of Tokyo, the High Energy Accelerator Research Organization (KEK), the Academia Sinica Institute for Astronomy and Astrophysics in Taiwan (ASIAA), and Princeton University. Based on data collected at the Subaru Telescope and retrieved from the HSC data archive system, which is operated by the Subaru Telescope and Astronomy Data Center at NAOJ. This work was supported by the joint research program of the Institute for Cosmic Ray Research (ICRR), University of Tokyo. The Cosmic Dawn Center is funded by the Danish National Research Foundation under grant No. 140. S.F. acknowledges support from the European Research Council (ERC) Consolidator Grant funding scheme (project ConTExt, grant No. 648179). This project has received funding from the European Union’s Horizon 2020 research and innovation program under the Marie Sklodowska-Curie grant agreement No. 847523 “INTERACTIONS.” This work is supported by World Premier International Research Center Initiative (WPI Initiative), MEXT, Japan, as well as the KAKENHI Grant-in-Aid for Scientific Research (A; 15H02064, 17H01110, 17H01114, 20H00180, and 21H04467) through the Japan Society for the Promotion of Science (JSPS). This work has been supported in part by JSPS KAKENHI grant Nos. JP17K05382, JP20K04024, and JP21H04499 (K.N.). Yuki Isobe, Kimihiko Nakajima, Yuichi Harikane, Takashi Kojima, and Masato Onodera are supported by JSPS KAKENHI grant Nos. 21J20785, 20K22373,19J01222, 18J12840, and 17K14257, respectively.","language":[{"iso":"eng"}],"keyword":["Space and Planetary Science","Astronomy and Astrophysics"],"doi":"10.3847/1538-4357/ac3509","citation":{"apa":"Isobe, Y., Ouchi, M., Suzuki, A., Moriya, T. J., Nakajima, K., Nomoto, K., … Xu, Y. (2022). EMPRESS. IV. Extremely metal-poor galaxies including very low-mass primordial systems with M∗= 104-105⊙ and 2%–3% (O/H): High (Fe/O) suggestive of metal enrichment by hypernovae/pair-instability supernovae. The Astrophysical Journal. IOP Publishing. https://doi.org/10.3847/1538-4357/ac3509","ama":"Isobe Y, Ouchi M, Suzuki A, et al. EMPRESS. IV. Extremely metal-poor galaxies including very low-mass primordial systems with M∗= 104-105⊙ and 2%–3% (O/H): High (Fe/O) suggestive of metal enrichment by hypernovae/pair-instability supernovae. The Astrophysical Journal. 2022;925(2). doi:10.3847/1538-4357/ac3509","short":"Y. Isobe, M. Ouchi, A. Suzuki, T.J. Moriya, K. Nakajima, K. Nomoto, M. Rauch, Y. Harikane, T. Kojima, Y. Ono, S. Fujimoto, A.K. Inoue, J.H. Kim, Y. Komiyama, H. Kusakabe, C.-H. Lee, M. Maseda, J.J. Matthee, L. Michel-Dansac, T. Nagao, T. Nanayakkara, M. Nishigaki, M. Onodera, Y. Sugahara, Y. Xu, The Astrophysical Journal 925 (2022).","mla":"Isobe, Yuki, et al. “EMPRESS. IV. Extremely Metal-Poor Galaxies Including Very Low-Mass Primordial Systems with M∗= 104-105⊙ and 2%–3% (O/H): High (Fe/O) Suggestive of Metal Enrichment by Hypernovae/Pair-Instability Supernovae.” The Astrophysical Journal, vol. 925, no. 2, 111, IOP Publishing, 2022, doi:10.3847/1538-4357/ac3509.","ista":"Isobe Y, Ouchi M, Suzuki A, Moriya TJ, Nakajima K, Nomoto K, Rauch M, Harikane Y, Kojima T, Ono Y, Fujimoto S, Inoue AK, Kim JH, Komiyama Y, Kusakabe H, Lee C-H, Maseda M, Matthee JJ, Michel-Dansac L, Nagao T, Nanayakkara T, Nishigaki M, Onodera M, Sugahara Y, Xu Y. 2022. EMPRESS. IV. Extremely metal-poor galaxies including very low-mass primordial systems with M∗= 104-105⊙ and 2%–3% (O/H): High (Fe/O) suggestive of metal enrichment by hypernovae/pair-instability supernovae. The Astrophysical Journal. 925(2), 111.","ieee":"Y. Isobe et al., “EMPRESS. IV. Extremely metal-poor galaxies including very low-mass primordial systems with M∗= 104-105⊙ and 2%–3% (O/H): High (Fe/O) suggestive of metal enrichment by hypernovae/pair-instability supernovae,” The Astrophysical Journal, vol. 925, no. 2. IOP Publishing, 2022.","chicago":"Isobe, Yuki, Masami Ouchi, Akihiro Suzuki, Takashi J. Moriya, Kimihiko Nakajima, Ken’ichi Nomoto, Michael Rauch, et al. “EMPRESS. IV. Extremely Metal-Poor Galaxies Including Very Low-Mass Primordial Systems with M∗= 104-105⊙ and 2%–3% (O/H): High (Fe/O) Suggestive of Metal Enrichment by Hypernovae/Pair-Instability Supernovae.” The Astrophysical Journal. IOP Publishing, 2022. https://doi.org/10.3847/1538-4357/ac3509."},"title":"EMPRESS. IV. Extremely metal-poor galaxies including very low-mass primordial systems with M∗= 10⁴-10⁵⊙ and 2%–3% (O/H): High (Fe/O) suggestive of metal enrichment by hypernovae/pair-instability supernovae","day":"31","author":[{"full_name":"Isobe, Yuki","first_name":"Yuki","last_name":"Isobe"},{"first_name":"Masami","full_name":"Ouchi, Masami","last_name":"Ouchi"},{"last_name":"Suzuki","full_name":"Suzuki, Akihiro","first_name":"Akihiro"},{"full_name":"Moriya, Takashi J.","first_name":"Takashi J.","last_name":"Moriya"},{"full_name":"Nakajima, Kimihiko","first_name":"Kimihiko","last_name":"Nakajima"},{"first_name":"Ken’ichi","full_name":"Nomoto, Ken’ichi","last_name":"Nomoto"},{"last_name":"Rauch","full_name":"Rauch, Michael","first_name":"Michael"},{"first_name":"Yuichi","full_name":"Harikane, Yuichi","last_name":"Harikane"},{"full_name":"Kojima, Takashi","first_name":"Takashi","last_name":"Kojima"},{"full_name":"Ono, Yoshiaki","first_name":"Yoshiaki","last_name":"Ono"},{"full_name":"Fujimoto, Seiji","first_name":"Seiji","last_name":"Fujimoto"},{"last_name":"Inoue","first_name":"Akio K.","full_name":"Inoue, Akio K."},{"first_name":"Ji Hoon","full_name":"Kim, Ji Hoon","last_name":"Kim"},{"first_name":"Yutaka","full_name":"Komiyama, Yutaka","last_name":"Komiyama"},{"last_name":"Kusakabe","full_name":"Kusakabe, Haruka","first_name":"Haruka"},{"last_name":"Lee","first_name":"Chien-Hsiu","full_name":"Lee, Chien-Hsiu"},{"first_name":"Michael","full_name":"Maseda, Michael","last_name":"Maseda"},{"full_name":"Matthee, Jorryt J","first_name":"Jorryt J","last_name":"Matthee","id":"7439a258-f3c0-11ec-9501-9df22fe06720","orcid":"0000-0003-2871-127X"},{"full_name":"Michel-Dansac, Leo","first_name":"Leo","last_name":"Michel-Dansac"},{"last_name":"Nagao","full_name":"Nagao, Tohru","first_name":"Tohru"},{"first_name":"Themiya","full_name":"Nanayakkara, Themiya","last_name":"Nanayakkara"},{"full_name":"Nishigaki, Moka","first_name":"Moka","last_name":"Nishigaki"},{"last_name":"Onodera","first_name":"Masato","full_name":"Onodera, Masato"},{"last_name":"Sugahara","full_name":"Sugahara, Yuma","first_name":"Yuma"},{"last_name":"Xu","full_name":"Xu, Yi","first_name":"Yi"}],"type":"journal_article"},{"oa":1,"main_file_link":[{"open_access":"1","url":"https://arxiv.org/abs/2112.08372"}],"publication_status":"published","volume":926,"issue":"2","article_processing_charge":"No","arxiv":1,"_id":"11510","date_published":"2022-02-17T00:00:00Z","abstract":[{"lang":"eng","text":"Galaxy evolution is driven by a variety of physical processes that are predicted to proceed at different rates for different dark matter haloes and environments across cosmic times. A record of this evolution is preserved in galaxy stellar populations, which we can access using absorption-line spectroscopy. Here we explore the large LEGA-C survey (DR3) to investigate the role of the environment and stellar mass on stellar populations at z ∼ 0.6–1 in the COSMOS field. Leveraging the statistical power and depth of LEGA-C, we reveal significant gradients in Dn4000 and Hδ equivalent widths (EWs) distributions over the stellar mass versus environment 2D spaces for the massive galaxy population (M > 1010 M⊙) at z ∼ 0.6–1.0. Dn4000 and Hδ EWs primarily depend on stellar mass, but they also depend on environment at fixed stellar mass. By splitting the sample into centrals and satellites, and in terms of star-forming galaxies and quiescent galaxies, we reveal that the significant environmental trends of Dn4000 and Hδ EW, when controlling for stellar mass, are driven by quiescent galaxies. Regardless of being centrals or satellites, star-forming galaxies reveal Dn4000 and Hδ EWs, which depend strongly on their stellar mass and are completely independent of the environment at 0.6 < z < 1.0. The environmental trends seen for satellite galaxies are fully driven by the trends that hold only for quiescent galaxies, combined with the strong environmental dependency of the quiescent fraction at fixed stellar mass. Our results are consistent with recent predictions from simulations that point toward massive galaxies forming first in overdensities or the most compact dark matter haloes."}],"article_number":"117","publication_identifier":{"issn":["0004-637X"],"eissn":["1538-4357"]},"date_updated":"2022-07-19T09:37:42Z","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","external_id":{"arxiv":["2112.08372"]},"scopus_import":"1","year":"2022","oa_version":"Published Version","article_type":"original","publisher":"IOP Publishing","status":"public","intvolume":" 926","quality_controlled":"1","publication":"The Astrophysical Journal","date_created":"2022-07-06T12:38:42Z","extern":"1","month":"02","acknowledgement":"We thank the reviewer for several valuable comments that improved the clarity of the manuscript. P.F.W. acknowledges the support of the fellowship by the East Asian Core Observatories Association. This work is based on observations made with ESO VLT Telescopes at the La Silla Paranal Observatory under programmes ID 194-A.2005 and 1100.A-0949 (The LEGA-C Public Spectroscopy Survey). This project has received funding from the European Research Council (ERC) under the European Union—Horizon 2020 research and innovation program (grant agreement No. 683184).","doi":"10.3847/1538-4357/ac4419","language":[{"iso":"eng"}],"keyword":["Space and Planetary Science","Astronomy and Astrophysics"],"title":"The LEGA-C of nature and nurture in stellar populations at z ∼ 0.6–1.0: Dn4000 and Hδ reveal different assembly histories for quiescent galaxies in different environments","citation":{"chicago":"Sobral, David, Arjen van der Wel, Rachel Bezanson, Eric Bell, Adam Muzzin, Francesco D’Eugenio, Behnam Darvish, et al. “The LEGA-C of Nature and Nurture in Stellar Populations at z ∼ 0.6–1.0: Dn4000 and Hδ Reveal Different Assembly Histories for Quiescent Galaxies in Different Environments.” The Astrophysical Journal. IOP Publishing, 2022. https://doi.org/10.3847/1538-4357/ac4419.","ista":"Sobral D, van der Wel A, Bezanson R, Bell E, Muzzin A, D’Eugenio F, Darvish B, Gallazzi A, Wu P-F, Maseda M, Matthee JJ, Paulino-Afonso A, Straatman C, van Dokkum PG. 2022. The LEGA-C of nature and nurture in stellar populations at z ∼ 0.6–1.0: Dn4000 and Hδ reveal different assembly histories for quiescent galaxies in different environments. The Astrophysical Journal. 926(2), 117.","ieee":"D. Sobral et al., “The LEGA-C of nature and nurture in stellar populations at z ∼ 0.6–1.0: Dn4000 and Hδ reveal different assembly histories for quiescent galaxies in different environments,” The Astrophysical Journal, vol. 926, no. 2. IOP Publishing, 2022.","mla":"Sobral, David, et al. “The LEGA-C of Nature and Nurture in Stellar Populations at z ∼ 0.6–1.0: Dn4000 and Hδ Reveal Different Assembly Histories for Quiescent Galaxies in Different Environments.” The Astrophysical Journal, vol. 926, no. 2, 117, IOP Publishing, 2022, doi:10.3847/1538-4357/ac4419.","short":"D. Sobral, A. van der Wel, R. Bezanson, E. Bell, A. Muzzin, F. D’Eugenio, B. Darvish, A. Gallazzi, P.-F. Wu, M. Maseda, J.J. Matthee, A. Paulino-Afonso, C. Straatman, P.G. van Dokkum, The Astrophysical Journal 926 (2022).","ama":"Sobral D, van der Wel A, Bezanson R, et al. The LEGA-C of nature and nurture in stellar populations at z ∼ 0.6–1.0: Dn4000 and Hδ reveal different assembly histories for quiescent galaxies in different environments. The Astrophysical Journal. 2022;926(2). doi:10.3847/1538-4357/ac4419","apa":"Sobral, D., van der Wel, A., Bezanson, R., Bell, E., Muzzin, A., D’Eugenio, F., … van Dokkum, P. G. (2022). The LEGA-C of nature and nurture in stellar populations at z ∼ 0.6–1.0: Dn4000 and Hδ reveal different assembly histories for quiescent galaxies in different environments. The Astrophysical Journal. IOP Publishing. https://doi.org/10.3847/1538-4357/ac4419"},"author":[{"full_name":"Sobral, David","first_name":"David","last_name":"Sobral"},{"first_name":"Arjen","full_name":"van der Wel, Arjen","last_name":"van der Wel"},{"last_name":"Bezanson","full_name":"Bezanson, Rachel","first_name":"Rachel"},{"full_name":"Bell, Eric","first_name":"Eric","last_name":"Bell"},{"first_name":"Adam","full_name":"Muzzin, Adam","last_name":"Muzzin"},{"last_name":"D’Eugenio","first_name":"Francesco","full_name":"D’Eugenio, Francesco"},{"last_name":"Darvish","first_name":"Behnam","full_name":"Darvish, Behnam"},{"full_name":"Gallazzi, Anna","first_name":"Anna","last_name":"Gallazzi"},{"first_name":"Po-Feng","full_name":"Wu, Po-Feng","last_name":"Wu"},{"first_name":"Michael","full_name":"Maseda, Michael","last_name":"Maseda"},{"id":"7439a258-f3c0-11ec-9501-9df22fe06720","orcid":"0000-0003-2871-127X","last_name":"Matthee","full_name":"Matthee, Jorryt J","first_name":"Jorryt J"},{"last_name":"Paulino-Afonso","first_name":"Ana","full_name":"Paulino-Afonso, Ana"},{"last_name":"Straatman","first_name":"Caroline","full_name":"Straatman, Caroline"},{"last_name":"van Dokkum","full_name":"van Dokkum, Pieter G.","first_name":"Pieter G."}],"type":"journal_article","day":"17"},{"main_file_link":[{"url":"https://arxiv.org/abs/2102.04561","open_access":"1"}],"oa":1,"publication_status":"published","volume":924,"issue":"2","article_processing_charge":"No","arxiv":1,"_id":"11511","abstract":[{"lang":"eng","text":"The ratio of α-elements to iron in galaxies holds valuable information about the star formation history (SFH) since their enrichment occurs on different timescales. The fossil record of stars in galaxies has mostly been excavated for passive galaxies, since the light of star-forming galaxies is dominated by young stars, which have much weaker atmospheric absorption features. Here we use the largest reference cosmological simulation of the EAGLE project to investigate the origin of variations in stellar α-enhancement among star-forming galaxies at z = 0, and their impact on integrated spectra. The definition of α-enhancement in a composite stellar population is ambiguous. We elucidate two definitions—termed “mean” and “galactic” α-enhancement—in more detail. While a star-forming galaxy has a high “mean” α-enhancement when its stars formed rapidly, a galaxy with a large “galactic” α-enhancement generally had a delayed SFH. We find that absorption-line strengths of Mg and Fe correlate with variations in α-enhancement. These correlations are strongest for the “galactic” α-enhancement. However, we show that these are mostly caused by other effects that are cross-correlated with α-enhancement, such as variations in the light-weighted age. This severely complicates the retrieval of α-enhancements in star-forming galaxies. The ambiguity is not severe for passive galaxies, and we confirm that spectral variations in these galaxies are caused by measurable variations in α-enhancements. We suggest that this more complex coupling between α-enhancement and SFHs can guide the interpretation of new observations of star-forming galaxies."}],"date_published":"2022-01-13T00:00:00Z","article_number":"73","publication_identifier":{"issn":["0004-637X"],"eissn":["1538-4357"]},"user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","date_updated":"2022-07-19T09:38:03Z","external_id":{"arxiv":["2102.04561"]},"scopus_import":"1","year":"2022","oa_version":"Published Version","article_type":"original","publisher":"IOP Publishing","status":"public","intvolume":" 924","quality_controlled":"1","publication":"The Astrophysical Journal","date_created":"2022-07-06T12:48:32Z","extern":"1","month":"01","acknowledgement":"We thank our anonymous referee for the constructive feedback. We extend our gratitude to Maarten Baes, Simon Lilly, Rafael Ottersberg, Gabriele Pezzulli, Alvio Renzini, and Andrea Weibel for insightful discussions. A.G. gratefully acknowledges financial support from the Fund for Scientific Research Flanders (FWO-Vlaanderen, project G.0G04.16N). This work used the DiRAC Data Centric system at Durham University, operated by the ICC on behalf of the STFC DiRAC HPC Facility (www.dirac.ac.uk). This equipment was funded by BIS National E-infrastructure capital grant ST/K00042X/1, STFC capital grant ST/H008519/1, and STFC DiRAC Operations grant ST/K003267/1 and Durham University. DiRAC is part of the National E-Infrastructure.\r\n\r\nWe have benefited from the data analysis tool Topcat (Taylor 2013) and the programming language Python, including the numpy (van der Walt et al. 2011), matplotlib (Hunter 2007), and scipy (Virtanen et al. 2020) packages.","doi":"10.3847/1538-4357/ac350b","language":[{"iso":"eng"}],"keyword":["Space and Planetary Science","Astronomy and Astrophysics"],"title":"On the variation in stellar α-enhancements of star-forming galaxies in the EAGLE simulation","citation":{"apa":"Gebek, A., & Matthee, J. J. (2022). On the variation in stellar α-enhancements of star-forming galaxies in the EAGLE simulation. The Astrophysical Journal. IOP Publishing. https://doi.org/10.3847/1538-4357/ac350b","ama":"Gebek A, Matthee JJ. On the variation in stellar α-enhancements of star-forming galaxies in the EAGLE simulation. The Astrophysical Journal. 2022;924(2). doi:10.3847/1538-4357/ac350b","short":"A. Gebek, J.J. Matthee, The Astrophysical Journal 924 (2022).","mla":"Gebek, Andrea, and Jorryt J. Matthee. “On the Variation in Stellar α-Enhancements of Star-Forming Galaxies in the EAGLE Simulation.” The Astrophysical Journal, vol. 924, no. 2, 73, IOP Publishing, 2022, doi:10.3847/1538-4357/ac350b.","ista":"Gebek A, Matthee JJ. 2022. On the variation in stellar α-enhancements of star-forming galaxies in the EAGLE simulation. The Astrophysical Journal. 924(2), 73.","ieee":"A. Gebek and J. J. Matthee, “On the variation in stellar α-enhancements of star-forming galaxies in the EAGLE simulation,” The Astrophysical Journal, vol. 924, no. 2. IOP Publishing, 2022.","chicago":"Gebek, Andrea, and Jorryt J Matthee. “On the Variation in Stellar α-Enhancements of Star-Forming Galaxies in the EAGLE Simulation.” The Astrophysical Journal. IOP Publishing, 2022. https://doi.org/10.3847/1538-4357/ac350b."},"type":"journal_article","author":[{"last_name":"Gebek","full_name":"Gebek, Andrea","first_name":"Andrea"},{"id":"7439a258-f3c0-11ec-9501-9df22fe06720","orcid":"0000-0003-2871-127X","last_name":"Matthee","first_name":"Jorryt J","full_name":"Matthee, Jorryt J"}],"day":"13"},{"publisher":"Oxford University Press","publication":"Monthly Notices of the Royal Astronomical Society","quality_controlled":"1","intvolume":" 512","status":"public","page":"5960-5977","month":"06","extern":"1","date_created":"2022-07-07T09:21:30Z","acknowledgement":"We thank an anonymous referee for an encouraging and constructive report that helped improving the quality of this work. We acknowledge illuminating conversations with Xiaohan Wu, Chris Cain, Anna-Christina Eilers, Simon Lilly and Ruari Mackenzie. RPN gratefully acknowledges an Ashford Fellowship granted by Harvard University. MG was supported by NASA through the NASA Hubble Fellowship grant HST-HF2-51409. PO acknowledges support from the Swiss National Science Foundation through the SNSF Professorship grant 190079. GP acknowledges support from the Netherlands Research School for Astronomy (NOVA). MH is fellow of the Knut and Alice Wallenberg Foundation. DE is supported by the US National Science Foundation (NSF) through Astronomy & Astrophysics grant AST-1909198. The Cosmic Dawn Center (DAWN) is funded by the Danish National Research Foundation under grant No. 140. RA acknowledges support from Fondecyt Regular Grant 1202007. ST is supported by the 2021 Research Fund 1.210134.01 of UNIST (Ulsan National Institute of Science & Technology). MLl acknowledges support from the ANID/Scholarship Program/Doctorado Nacional/2019-21191036. JC acknowledges support from the Spanish Ministry of Science and Innovation, project PID2019-107408GB-C43 (ESTALLIDOS) and from Gobierno de Canarias through EU FEDER funding, project PID2020010050.","keyword":["galaxies: high-redshift","intergalactic medium","cosmology: observations","dark ages","reionization","first stars","ultraviolet: galaxies"],"language":[{"iso":"eng"}],"doi":"10.1093/mnras/stac801","citation":{"mla":"Matthee, Jorryt J., et al. “(Re)Solving Reionization with Lyα: How Bright Lyα Emitters Account for the z ≈ 2 − 8 Cosmic Ionizing Background.” Monthly Notices of the Royal Astronomical Society, vol. 512, no. 4, Oxford University Press, 2022, pp. 5960–77, doi:10.1093/mnras/stac801.","ista":"Matthee JJ, Naidu RP, Pezzulli G, Gronke M, Sobral D, Oesch PA, Hayes M, Erb D, Schaerer D, Amorín R, Tacchella S, Ana Paulino-Afonso AP-A, Llerena M, Calhau J, Röttgering H. 2022. (Re)Solving reionization with Lyα: How bright Lyα emitters account for the z ≈ 2 − 8 cosmic ionizing background. Monthly Notices of the Royal Astronomical Society. 512(4), 5960–5977.","ieee":"J. J. Matthee et al., “(Re)Solving reionization with Lyα: How bright Lyα emitters account for the z ≈ 2 − 8 cosmic ionizing background,” Monthly Notices of the Royal Astronomical Society, vol. 512, no. 4. Oxford University Press, pp. 5960–5977, 2022.","chicago":"Matthee, Jorryt J, Rohan P. Naidu, Gabriele Pezzulli, Max Gronke, David Sobral, Pascal A. Oesch, Matthew Hayes, et al. “(Re)Solving Reionization with Lyα: How Bright Lyα Emitters Account for the z ≈ 2 − 8 Cosmic Ionizing Background.” Monthly Notices of the Royal Astronomical Society. Oxford University Press, 2022. https://doi.org/10.1093/mnras/stac801.","apa":"Matthee, J. J., Naidu, R. P., Pezzulli, G., Gronke, M., Sobral, D., Oesch, P. A., … Röttgering, H. (2022). (Re)Solving reionization with Lyα: How bright Lyα emitters account for the z ≈ 2 − 8 cosmic ionizing background. Monthly Notices of the Royal Astronomical Society. Oxford University Press. https://doi.org/10.1093/mnras/stac801","ama":"Matthee JJ, Naidu RP, Pezzulli G, et al. (Re)Solving reionization with Lyα: How bright Lyα emitters account for the z ≈ 2 − 8 cosmic ionizing background. Monthly Notices of the Royal Astronomical Society. 2022;512(4):5960-5977. doi:10.1093/mnras/stac801","short":"J.J. Matthee, R.P. Naidu, G. Pezzulli, M. Gronke, D. Sobral, P.A. Oesch, M. Hayes, D. Erb, D. Schaerer, R. Amorín, S. Tacchella, A.P.-A. Ana Paulino-Afonso, M. Llerena, J. Calhau, H. Röttgering, Monthly Notices of the Royal Astronomical Society 512 (2022) 5960–5977."},"title":"(Re)Solving reionization with Lyα: How bright Lyα emitters account for the z ≈ 2 − 8 cosmic ionizing background","day":"01","type":"journal_article","author":[{"last_name":"Matthee","full_name":"Matthee, Jorryt J","first_name":"Jorryt J","orcid":"0000-0003-2871-127X","id":"7439a258-f3c0-11ec-9501-9df22fe06720"},{"last_name":"Naidu","first_name":"Rohan P.","full_name":"Naidu, Rohan P."},{"last_name":"Pezzulli","first_name":"Gabriele","full_name":"Pezzulli, Gabriele"},{"full_name":"Gronke, Max","first_name":"Max","last_name":"Gronke"},{"full_name":"Sobral, David","first_name":"David","last_name":"Sobral"},{"full_name":"Oesch, Pascal A.","first_name":"Pascal A.","last_name":"Oesch"},{"full_name":"Hayes, Matthew","first_name":"Matthew","last_name":"Hayes"},{"first_name":"Dawn","full_name":"Erb, Dawn","last_name":"Erb"},{"first_name":"Daniel","full_name":"Schaerer, Daniel","last_name":"Schaerer"},{"first_name":"Ricardo","full_name":"Amorín, Ricardo","last_name":"Amorín"},{"full_name":"Tacchella, Sandro","first_name":"Sandro","last_name":"Tacchella"},{"full_name":"Ana Paulino-Afonso, Ana Paulino-Afonso","first_name":"Ana Paulino-Afonso","last_name":"Ana Paulino-Afonso"},{"last_name":"Llerena","full_name":"Llerena, Mario","first_name":"Mario"},{"last_name":"Calhau","full_name":"Calhau, João","first_name":"João"},{"full_name":"Röttgering, Huub","first_name":"Huub","last_name":"Röttgering"}],"publication_status":"published","oa":1,"main_file_link":[{"url":"https://arxiv.org/abs/2110.11967","open_access":"1"}],"volume":512,"arxiv":1,"article_processing_charge":"No","issue":"4","_id":"11521","date_published":"2022-06-01T00:00:00Z","abstract":[{"text":"The cosmic ionizing emissivity from star-forming galaxies has long been anchored to UV luminosity functions. Here, we introduce an emissivity framework based on Lyα emitters (LAEs), which naturally hones in on the subset of galaxies responsible for the ionizing background due to the intimate connection between production and escape of Lyα and LyC photons. Using constraints on the escape fractions of bright LAEs (LLyα > 0.2L*) at z ≈ 2 obtained from resolved Lyα profiles, and arguing for their redshift-invariance, we show that: (i) quasars and LAEs together reproduce the relatively flat emissivity at z ≈ 2–6, which is non-trivial given the strong evolution in both the star formation density and quasar number density at these epochs and (ii) LAEs produce late and rapid reionization between z ≈ 6−9 under plausible assumptions. Within this framework, the >10 × rise in the UV population-averaged fesc between z ≈ 3–7 naturally arises due to the same phenomena that drive the growing LAE fraction with redshift. Generally, a LAE dominated emissivity yields a peak in the distribution of the ionizing budget with UV luminosity as reported in latest simulations. Using our adopted parameters (fesc=50 per cent, ξion = 1025.9 Hz erg−1 for half the bright LAEs), a highly ionizing minority of galaxies with MUV < −17 accounts for the entire ionizing budget from star-forming galaxies. Rapid flashes of LyC from such rare galaxies produce a ‘disco’ ionizing background. We conclude proposing tests to further develop our suggested Lyα-anchored formalism.","lang":"eng"}],"external_id":{"arxiv":["2110.11967"]},"scopus_import":"1","date_updated":"2022-08-18T10:42:47Z","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","publication_identifier":{"eissn":["1365-2966"],"issn":["0035-8711"]},"article_type":"original","oa_version":"Preprint","year":"2022"},{"date_updated":"2024-02-21T12:34:51Z","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","doi":"10.15479/AT:ISTA:11542","related_material":{"link":[{"url":"https://www.biorxiv.org/content/10.1101/2021.06.21.449162v1","relation":"contains"}],"record":[{"relation":"used_in_publication","id":"11995","status":"public"}]},"contributor":[{"last_name":"Siegert","first_name":"Sandra","id":"36ACD32E-F248-11E8-B48F-1D18A9856A87","orcid":"0000-0001-8635-0877","contributor_type":"contact_person"}],"type":"research_data","author":[{"orcid":"0000-0001-5297-733X","id":"4C5E7B96-F248-11E8-B48F-1D18A9856A87","first_name":"Rouven","full_name":"Schulz, Rouven","last_name":"Schulz"}],"year":"2022","has_accepted_license":"1","oa_version":"None","citation":{"ista":"Schulz R. 2022. Source Data (Chimeric GPCRs mimic distinct signaling pathways and modulate microglia responses), Institute of Science and Technology Austria, 10.15479/AT:ISTA:11542.","ieee":"R. Schulz, “Source Data (Chimeric GPCRs mimic distinct signaling pathways and modulate microglia responses).” Institute of Science and Technology Austria, 2022.","chicago":"Schulz, Rouven. “Source Data (Chimeric GPCRs Mimic Distinct Signaling Pathways and Modulate Microglia Responses).” Institute of Science and Technology Austria, 2022. https://doi.org/10.15479/AT:ISTA:11542.","mla":"Schulz, Rouven. Source Data (Chimeric GPCRs Mimic Distinct Signaling Pathways and Modulate Microglia Responses). Institute of Science and Technology Austria, 2022, doi:10.15479/AT:ISTA:11542.","short":"R. Schulz, (2022).","apa":"Schulz, R. (2022). Source Data (Chimeric GPCRs mimic distinct signaling pathways and modulate microglia responses). Institute of Science and Technology Austria. https://doi.org/10.15479/AT:ISTA:11542","ama":"Schulz R. Source Data (Chimeric GPCRs mimic distinct signaling pathways and modulate microglia responses). 2022. doi:10.15479/AT:ISTA:11542"},"title":"Source Data (Chimeric GPCRs mimic distinct signaling pathways and modulate microglia responses)","file_date_updated":"2022-07-08T10:56:52Z","department":[{"_id":"GradSch"},{"_id":"SaSi"}],"tmp":{"legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","image":"/images/cc_by.png","short":"CC BY (4.0)"},"status":"public","publisher":"Institute of Science and Technology Austria","oa":1,"file":[{"checksum":"71e8186583f3adbb6c69a88ac9e6e49b","date_updated":"2022-07-08T10:56:52Z","access_level":"open_access","file_name":"Source Data.xlsx","file_size":135784571,"creator":"rschulz","date_created":"2022-07-08T10:56:52Z","success":1,"content_type":"application/vnd.openxmlformats-officedocument.spreadsheetml.sheet","relation":"main_file","file_id":"11543"}],"_id":"11542","date_created":"2022-07-08T11:03:02Z","date_published":"2022-01-01T00:00:00Z","article_processing_charge":"No"},{"date_created":"2022-07-08T11:40:07Z","month":"11","page":"145-179","status":"public","intvolume":" 609","quality_controlled":"1","department":[{"_id":"HeEd"}],"publication":"Journal of Algebra","isi":1,"publisher":"Elsevier","type":"journal_article","author":[{"full_name":"Brown, Adam","first_name":"Adam","last_name":"Brown","id":"70B7FDF6-608D-11E9-9333-8535E6697425"},{"last_name":"Romanov","full_name":"Romanov, Anna","first_name":"Anna"}],"day":"01","title":"Contravariant pairings between standard Whittaker modules and Verma modules","ec_funded":1,"citation":{"short":"A. Brown, A. Romanov, Journal of Algebra 609 (2022) 145–179.","ama":"Brown A, Romanov A. Contravariant pairings between standard Whittaker modules and Verma modules. Journal of Algebra. 2022;609(11):145-179. doi:10.1016/j.jalgebra.2022.06.017","apa":"Brown, A., & Romanov, A. (2022). Contravariant pairings between standard Whittaker modules and Verma modules. Journal of Algebra. Elsevier. https://doi.org/10.1016/j.jalgebra.2022.06.017","chicago":"Brown, Adam, and Anna Romanov. “Contravariant Pairings between Standard Whittaker Modules and Verma Modules.” Journal of Algebra. Elsevier, 2022. https://doi.org/10.1016/j.jalgebra.2022.06.017.","ieee":"A. Brown and A. Romanov, “Contravariant pairings between standard Whittaker modules and Verma modules,” Journal of Algebra, vol. 609, no. 11. Elsevier, pp. 145–179, 2022.","ista":"Brown A, Romanov A. 2022. Contravariant pairings between standard Whittaker modules and Verma modules. Journal of Algebra. 609(11), 145–179.","mla":"Brown, Adam, and Anna Romanov. “Contravariant Pairings between Standard Whittaker Modules and Verma Modules.” Journal of Algebra, vol. 609, no. 11, Elsevier, 2022, pp. 145–79, doi:10.1016/j.jalgebra.2022.06.017."},"doi":"10.1016/j.jalgebra.2022.06.017","ddc":["510"],"language":[{"iso":"eng"}],"keyword":["Algebra and Number Theory"],"acknowledgement":"We thank Catharina Stroppel and Jens Niklas Eberhardt for interesting discussions. The first author acknowledges the support of the European Union's Horizon 2020 research and innovation programme under the Marie Skłodowska-Curie Grant Agreement No. 754411. The second author is supported by the National Science Foundation Award No. 1803059 and the Australian Research Council grant DP170101579.","project":[{"call_identifier":"H2020","_id":"260C2330-B435-11E9-9278-68D0E5697425","name":"ISTplus - Postdoctoral Fellowships","grant_number":"754411"}],"_id":"11545","abstract":[{"lang":"eng","text":"We classify contravariant pairings between standard Whittaker modules and Verma modules over a complex semisimple Lie algebra. These contravariant pairings are useful in extending several classical techniques for category O to the Miličić–Soergel category N . We introduce a class of costandard modules which generalize dual Verma modules, and describe canonical maps from standard to costandard modules in terms of contravariant pairings.\r\nWe show that costandard modules have unique irreducible submodules and share the same composition factors as the corresponding standard Whittaker modules. We show that costandard modules give an algebraic characterization of the global sections of costandard twisted Harish-Chandra sheaves on the associated flag variety, which are defined using holonomic duality of D-modules. We prove that with these costandard modules, blocks of category\r\nN have the structure of highest weight categories and we establish a BGG reciprocity theorem for N ."}],"date_published":"2022-11-01T00:00:00Z","file":[{"checksum":"82abaee3d7837f703e499a9ecbb25b7c","access_level":"open_access","date_updated":"2023-02-02T07:32:48Z","file_size":582962,"creator":"dernst","file_name":"2022_JournalAlgebra_Brown.pdf","date_created":"2023-02-02T07:32:48Z","success":1,"file_id":"12473","relation":"main_file","content_type":"application/pdf"}],"issue":"11","article_processing_charge":"Yes (via OA deal)","volume":609,"tmp":{"legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","image":"/images/cc_by.png","short":"CC BY (4.0)"},"file_date_updated":"2023-02-02T07:32:48Z","oa":1,"publication_status":"published","year":"2022","oa_version":"Published Version","has_accepted_license":"1","article_type":"original","publication_identifier":{"issn":["0021-8693"]},"user_id":"4359f0d1-fa6c-11eb-b949-802e58b17ae8","date_updated":"2023-08-03T11:56:30Z","scopus_import":"1","external_id":{"isi":["000861841100004"]}},{"date_created":"2022-07-08T11:41:56Z","month":"08","status":"public","intvolume":" 377","publication":"Philosophical Transactions of the Royal Society B: Biological Sciences","quality_controlled":"1","department":[{"_id":"BeVi"},{"_id":"NiBa"}],"isi":1,"publisher":"Royal Society of London","type":"journal_article","author":[{"last_name":"Westram","first_name":"Anja M","full_name":"Westram, Anja M","orcid":"0000-0003-1050-4969","id":"3C147470-F248-11E8-B48F-1D18A9856A87"},{"full_name":"Faria, Rui","first_name":"Rui","last_name":"Faria"},{"last_name":"Johannesson","full_name":"Johannesson, Kerstin","first_name":"Kerstin"},{"last_name":"Butlin","full_name":"Butlin, Roger","first_name":"Roger"},{"id":"4880FE40-F248-11E8-B48F-1D18A9856A87","orcid":"0000-0002-8548-5240","full_name":"Barton, Nicholas H","first_name":"Nicholas H","last_name":"Barton"}],"day":"01","title":"Inversions and parallel evolution","citation":{"chicago":"Westram, Anja M, Rui Faria, Kerstin Johannesson, Roger Butlin, and Nicholas H Barton. “Inversions and Parallel Evolution.” Philosophical Transactions of the Royal Society B: Biological Sciences. Royal Society of London, 2022. https://doi.org/10.1098/rstb.2021.0203.","ista":"Westram AM, Faria R, Johannesson K, Butlin R, Barton NH. 2022. Inversions and parallel evolution. Philosophical Transactions of the Royal Society B: Biological Sciences. 377(1856), 20210203.","ieee":"A. M. Westram, R. Faria, K. Johannesson, R. Butlin, and N. H. Barton, “Inversions and parallel evolution,” Philosophical Transactions of the Royal Society B: Biological Sciences, vol. 377, no. 1856. Royal Society of London, 2022.","mla":"Westram, Anja M., et al. “Inversions and Parallel Evolution.” Philosophical Transactions of the Royal Society B: Biological Sciences, vol. 377, no. 1856, 20210203, Royal Society of London, 2022, doi:10.1098/rstb.2021.0203.","short":"A.M. Westram, R. Faria, K. Johannesson, R. Butlin, N.H. Barton, Philosophical Transactions of the Royal Society B: Biological Sciences 377 (2022).","ama":"Westram AM, Faria R, Johannesson K, Butlin R, Barton NH. Inversions and parallel evolution. Philosophical Transactions of the Royal Society B: Biological Sciences. 2022;377(1856). doi:10.1098/rstb.2021.0203","apa":"Westram, A. M., Faria, R., Johannesson, K., Butlin, R., & Barton, N. H. (2022). Inversions and parallel evolution. Philosophical Transactions of the Royal Society B: Biological Sciences. Royal Society of London. https://doi.org/10.1098/rstb.2021.0203"},"ddc":["570"],"doi":"10.1098/rstb.2021.0203","keyword":["General Agricultural and Biological Sciences","General Biochemistry","Genetics and Molecular Biology"],"language":[{"iso":"eng"}],"project":[{"_id":"05959E1C-7A3F-11EA-A408-12923DDC885E","name":"The maintenance of alternative adaptive peaks in snapdragons","grant_number":"P32166"}],"acknowledgement":"We thank the editor and two anonymous reviewers for their helpful and interesting comments on this manuscript.","abstract":[{"lang":"eng","text":"Local adaptation leads to differences between populations within a species. In many systems, similar environmental contrasts occur repeatedly, sometimes driving parallel phenotypic evolution. Understanding the genomic basis of local adaptation and parallel evolution is a major goal of evolutionary genomics. It is now known that by preventing the break-up of favourable combinations of alleles across multiple loci, genetic architectures that reduce recombination, like chromosomal inversions, can make an important contribution to local adaptation. However, little is known about whether inversions also contribute disproportionately to parallel evolution. Our aim here is to highlight this knowledge gap, to showcase existing studies, and to illustrate the differences between genomic architectures with and without inversions using simple models. We predict that by generating stronger effective selection, inversions can sometimes speed up the parallel adaptive process or enable parallel adaptation where it would be impossible otherwise, but this is highly dependent on the spatial setting. We highlight that further empirical work is needed, in particular to cover a broader taxonomic range and to understand the relative importance of inversions compared to genomic regions without inversions."}],"_id":"11546","date_published":"2022-08-01T00:00:00Z","article_number":"20210203","file":[{"checksum":"49f69428f3dcf5ce3ff281f7d199e9df","date_updated":"2023-02-02T08:20:29Z","access_level":"open_access","file_name":"2022_PhilosophicalTransactionsB_Westram.pdf","creator":"dernst","file_size":920304,"date_created":"2023-02-02T08:20:29Z","success":1,"content_type":"application/pdf","file_id":"12479","relation":"main_file"}],"article_processing_charge":"Yes (via OA deal)","issue":"1856","tmp":{"legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","image":"/images/cc_by.png","short":"CC BY (4.0)"},"volume":377,"file_date_updated":"2023-02-02T08:20:29Z","oa":1,"publication_status":"published","year":"2022","oa_version":"Published Version","has_accepted_license":"1","article_type":"original","publication_identifier":{"issn":["0962-8436"],"eissn":["1471-2970"]},"external_id":{"isi":["000812317300005"]},"scopus_import":"1","user_id":"4359f0d1-fa6c-11eb-b949-802e58b17ae8","date_updated":"2023-08-03T11:55:42Z"},{"scopus_import":"1","external_id":{"pmid":[" 35739187"],"isi":["000815098500002"]},"user_id":"4359f0d1-fa6c-11eb-b949-802e58b17ae8","date_updated":"2023-08-03T11:51:58Z","publication_identifier":{"eissn":["23993642"]},"year":"2022","oa_version":"Published Version","has_accepted_license":"1","publication_status":"published","oa":1,"file_date_updated":"2022-07-13T07:44:58Z","tmp":{"legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","image":"/images/cc_by.png","short":"CC BY (4.0)"},"volume":5,"article_processing_charge":"No","issue":"1","file":[{"success":1,"date_created":"2022-07-13T07:44:58Z","relation":"main_file","file_id":"11571","content_type":"application/pdf","access_level":"open_access","date_updated":"2022-07-13T07:44:58Z","checksum":"965f88bbcef3fd0c3e121340555c4467","creator":"kschuh","file_size":2335369,"file_name":"2022_communicationsbiology_Molina-Granada.pdf"}],"article_number":"620","_id":"11551","date_published":"2022-06-23T00:00:00Z","abstract":[{"text":"Imbalanced mitochondrial dNTP pools are known players in the pathogenesis of multiple human diseases. Here we show that, even under physiological conditions, dGTP is largely overrepresented among other dNTPs in mitochondria of mouse tissues and human cultured cells. In addition, a vast majority of mitochondrial dGTP is tightly bound to NDUFA10, an accessory subunit of complex I of the mitochondrial respiratory chain. NDUFA10 shares a deoxyribonucleoside kinase (dNK) domain with deoxyribonucleoside kinases in the nucleotide salvage pathway, though no specific function beyond stabilizing the complex I holoenzyme has been described for this subunit. We mutated the dNK domain of NDUFA10 in human HEK-293T cells while preserving complex I assembly and activity. The NDUFA10E160A/R161A shows reduced dGTP binding capacity in vitro and leads to a 50% reduction in mitochondrial dGTP content, proving that most dGTP is directly bound to the dNK domain of NDUFA10. This interaction may represent a hitherto unknown mechanism regulating mitochondrial dNTP availability and linking oxidative metabolism to DNA maintenance.","lang":"eng"}],"pmid":1,"acknowledgement":"We thank Dr, Luke Formosa (Department of Biochemistry and Molecular Biology, Monash Biomedicine Discovery Institute, Monash University, Melbourne, Australia) for his valuable advice and assistance on NDUFA10 molecular studies and Dr. Francesc Canals and his team (Proteomics Laboratory, Vall d’Hebron Institute of Oncology [VHIO], Universitat Autònoma de Barcelona, Barcelona, Spain) for their assistance with LC-MS/MS analyses. This work was supported by the Spanish Ministry of Industry, Economy and Competitiveness [grants BFU2014-52618-R, SAF2017-87506, and PID2020-112929RB-I00 to Y.C.], by the Spanish Instituto de Salud Carlos III [grants PI21/00554 and PMP15/00025 to R.M.], co-financed by the European Regional Development Fund (ERDF), and by an NHMRC Project grant to M.R. (GNT1164459).\r\n","language":[{"iso":"eng"}],"ddc":["570"],"doi":"10.1038/s42003-022-03568-6","citation":{"mla":"Molina-Granada, David, et al. “Most Mitochondrial DGTP Is Tightly Bound to Respiratory Complex I through the NDUFA10 Subunit.” Communications Biology, vol. 5, no. 1, 620, Springer Nature, 2022, doi:10.1038/s42003-022-03568-6.","chicago":"Molina-Granada, David, Emiliano González-Vioque, Marris G. Dibley, Raquel Cabrera-Pérez, Antoni Vallbona-Garcia, Javier Torres-Torronteras, Leonid A Sazanov, Michael T. Ryan, Yolanda Cámara, and Ramon Martí. “Most Mitochondrial DGTP Is Tightly Bound to Respiratory Complex I through the NDUFA10 Subunit.” Communications Biology. Springer Nature, 2022. https://doi.org/10.1038/s42003-022-03568-6.","ista":"Molina-Granada D, González-Vioque E, Dibley MG, Cabrera-Pérez R, Vallbona-Garcia A, Torres-Torronteras J, Sazanov LA, Ryan MT, Cámara Y, Martí R. 2022. Most mitochondrial dGTP is tightly bound to respiratory complex I through the NDUFA10 subunit. Communications Biology. 5(1), 620.","ieee":"D. Molina-Granada et al., “Most mitochondrial dGTP is tightly bound to respiratory complex I through the NDUFA10 subunit,” Communications Biology, vol. 5, no. 1. Springer Nature, 2022.","ama":"Molina-Granada D, González-Vioque E, Dibley MG, et al. Most mitochondrial dGTP is tightly bound to respiratory complex I through the NDUFA10 subunit. Communications Biology. 2022;5(1). doi:10.1038/s42003-022-03568-6","apa":"Molina-Granada, D., González-Vioque, E., Dibley, M. G., Cabrera-Pérez, R., Vallbona-Garcia, A., Torres-Torronteras, J., … Martí, R. (2022). Most mitochondrial dGTP is tightly bound to respiratory complex I through the NDUFA10 subunit. Communications Biology. Springer Nature. https://doi.org/10.1038/s42003-022-03568-6","short":"D. Molina-Granada, E. González-Vioque, M.G. Dibley, R. Cabrera-Pérez, A. Vallbona-Garcia, J. Torres-Torronteras, L.A. Sazanov, M.T. Ryan, Y. Cámara, R. Martí, Communications Biology 5 (2022)."},"title":"Most mitochondrial dGTP is tightly bound to respiratory complex I through the NDUFA10 subunit","day":"23","author":[{"last_name":"Molina-Granada","first_name":"David","full_name":"Molina-Granada, David"},{"first_name":"Emiliano","full_name":"González-Vioque, Emiliano","last_name":"González-Vioque"},{"first_name":"Marris G.","full_name":"Dibley, Marris G.","last_name":"Dibley"},{"last_name":"Cabrera-Pérez","first_name":"Raquel","full_name":"Cabrera-Pérez, Raquel"},{"first_name":"Antoni","full_name":"Vallbona-Garcia, Antoni","last_name":"Vallbona-Garcia"},{"full_name":"Torres-Torronteras, Javier","first_name":"Javier","last_name":"Torres-Torronteras"},{"full_name":"Sazanov, Leonid A","first_name":"Leonid A","last_name":"Sazanov","id":"338D39FE-F248-11E8-B48F-1D18A9856A87","orcid":"0000-0002-0977-7989"},{"full_name":"Ryan, Michael T.","first_name":"Michael T.","last_name":"Ryan"},{"full_name":"Cámara, Yolanda","first_name":"Yolanda","last_name":"Cámara"},{"full_name":"Martí, Ramon","first_name":"Ramon","last_name":"Martí"}],"type":"journal_article","publisher":"Springer Nature","isi":1,"publication":"Communications Biology","department":[{"_id":"LeSa"}],"quality_controlled":"1","status":"public","intvolume":" 5","month":"06","date_created":"2022-07-10T22:01:52Z"},{"article_processing_charge":"No","issue":"24","arxiv":1,"_id":"11552","abstract":[{"text":"Rotational dynamics of D2 molecules inside helium nanodroplets is induced by a moderately intense femtosecond pump pulse and measured as a function of time by recording the yield of HeD+ ions, created through strong-field dissociative ionization with a delayed femtosecond probe pulse. The yield oscillates with a period of 185 fs, reflecting field-free rotational wave packet dynamics, and the oscillation persists for more than 500 periods. Within the experimental uncertainty, the rotational constant BHe of the in-droplet D2 molecule, determined by Fourier analysis, is the same as Bgas for an isolated D2 molecule. Our observations show that the D2 molecules inside helium nanodroplets essentially rotate as free D2 molecules.","lang":"eng"}],"date_published":"2022-06-16T00:00:00Z","article_number":"243201","main_file_link":[{"open_access":"1","url":"https://doi.org/10.48550/arXiv.2201.09281"}],"oa":1,"publication_status":"published","volume":128,"oa_version":"Submitted Version","year":"2022","publication_identifier":{"issn":["00319007"],"eissn":["10797114"]},"external_id":{"isi":["000820659700002"],"arxiv":["2201.09281"]},"scopus_import":"1","date_updated":"2023-08-03T11:54:14Z","user_id":"4359f0d1-fa6c-11eb-b949-802e58b17ae8","date_created":"2022-07-10T22:01:52Z","month":"06","isi":1,"publisher":"American Physical Society","intvolume":" 128","status":"public","publication":"Physical Review Letters","department":[{"_id":"MiLe"}],"quality_controlled":"1","title":"Femtosecond rotational dynamics of D2 molecules in superfluid helium nanodroplets","citation":{"mla":"Qiang, Junjie, et al. “Femtosecond Rotational Dynamics of D2 Molecules in Superfluid Helium Nanodroplets.” Physical Review Letters, vol. 128, no. 24, 243201, American Physical Society, 2022, doi:10.1103/PhysRevLett.128.243201.","chicago":"Qiang, Junjie, Lianrong Zhou, Peifen Lu, Kang Lin, Yongzhe Ma, Shengzhe Pan, Chenxu Lu, et al. “Femtosecond Rotational Dynamics of D2 Molecules in Superfluid Helium Nanodroplets.” Physical Review Letters. American Physical Society, 2022. https://doi.org/10.1103/PhysRevLett.128.243201.","ista":"Qiang J, Zhou L, Lu P, Lin K, Ma Y, Pan S, Lu C, Jiang W, Sun F, Zhang W, Li H, Gong X, Averbukh IS, Prior Y, Schouder CA, Stapelfeldt H, Cherepanov I, Lemeshko M, Jäger W, Wu J. 2022. Femtosecond rotational dynamics of D2 molecules in superfluid helium nanodroplets. Physical Review Letters. 128(24), 243201.","ieee":"J. Qiang et al., “Femtosecond rotational dynamics of D2 molecules in superfluid helium nanodroplets,” Physical Review Letters, vol. 128, no. 24. American Physical Society, 2022.","ama":"Qiang J, Zhou L, Lu P, et al. Femtosecond rotational dynamics of D2 molecules in superfluid helium nanodroplets. Physical Review Letters. 2022;128(24). doi:10.1103/PhysRevLett.128.243201","apa":"Qiang, J., Zhou, L., Lu, P., Lin, K., Ma, Y., Pan, S., … Wu, J. (2022). Femtosecond rotational dynamics of D2 molecules in superfluid helium nanodroplets. Physical Review Letters. American Physical Society. https://doi.org/10.1103/PhysRevLett.128.243201","short":"J. Qiang, L. Zhou, P. Lu, K. Lin, Y. Ma, S. Pan, C. Lu, W. Jiang, F. Sun, W. Zhang, H. Li, X. Gong, I.S. Averbukh, Y. Prior, C.A. Schouder, H. Stapelfeldt, I. Cherepanov, M. Lemeshko, W. Jäger, J. Wu, Physical Review Letters 128 (2022)."},"ec_funded":1,"author":[{"full_name":"Qiang, Junjie","first_name":"Junjie","last_name":"Qiang"},{"last_name":"Zhou","first_name":"Lianrong","full_name":"Zhou, Lianrong"},{"first_name":"Peifen","full_name":"Lu, Peifen","last_name":"Lu"},{"full_name":"Lin, Kang","first_name":"Kang","last_name":"Lin"},{"last_name":"Ma","full_name":"Ma, Yongzhe","first_name":"Yongzhe"},{"last_name":"Pan","full_name":"Pan, Shengzhe","first_name":"Shengzhe"},{"last_name":"Lu","full_name":"Lu, Chenxu","first_name":"Chenxu"},{"last_name":"Jiang","full_name":"Jiang, Wenyu","first_name":"Wenyu"},{"last_name":"Sun","first_name":"Fenghao","full_name":"Sun, Fenghao"},{"first_name":"Wenbin","full_name":"Zhang, Wenbin","last_name":"Zhang"},{"first_name":"Hui","full_name":"Li, Hui","last_name":"Li"},{"first_name":"Xiaochun","full_name":"Gong, Xiaochun","last_name":"Gong"},{"last_name":"Averbukh","first_name":"Ilya Sh","full_name":"Averbukh, Ilya Sh"},{"last_name":"Prior","first_name":"Yehiam","full_name":"Prior, Yehiam"},{"first_name":"Constant A.","full_name":"Schouder, Constant A.","last_name":"Schouder"},{"first_name":"Henrik","full_name":"Stapelfeldt, Henrik","last_name":"Stapelfeldt"},{"id":"339C7E5A-F248-11E8-B48F-1D18A9856A87","first_name":"Igor","full_name":"Cherepanov, Igor","last_name":"Cherepanov"},{"last_name":"Lemeshko","first_name":"Mikhail","full_name":"Lemeshko, Mikhail","orcid":"0000-0002-6990-7802","id":"37CB05FA-F248-11E8-B48F-1D18A9856A87"},{"full_name":"Jäger, Wolfgang","first_name":"Wolfgang","last_name":"Jäger"},{"last_name":"Wu","first_name":"Jian","full_name":"Wu, Jian"}],"type":"journal_article","day":"16","project":[{"call_identifier":"H2020","_id":"2688CF98-B435-11E9-9278-68D0E5697425","grant_number":"801770","name":"Angulon: physics and applications of a new quasiparticle"},{"name":"International IST Doctoral Program","grant_number":"665385","_id":"2564DBCA-B435-11E9-9278-68D0E5697425","call_identifier":"H2020"}],"doi":"10.1103/PhysRevLett.128.243201","language":[{"iso":"eng"}]},{"oa_version":"None","has_accepted_license":"1","year":"2022","article_type":"original","publication_identifier":{"eissn":["2199-6806"],"issn":["2199-6792"]},"date_updated":"2023-02-16T10:02:12Z","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","scopus_import":"1","date_published":"2022-06-01T00:00:00Z","_id":"11553","abstract":[{"lang":"eng","text":"In holomorphic dynamics, complex box mappings arise as first return maps to wellchosen domains. They are a generalization of polynomial-like mapping, where the domain of the return map can have infinitely many components. They turned out to be extremely useful in tackling diverse problems. The purpose of this paper is:\r\n• To illustrate some pathologies that can occur when a complex box mapping is not induced by a globally defined map and when its domain has infinitely many components, and to give conditions to avoid these issues.\r\n• To show that once one has a box mapping for a rational map, these conditions can be assumed to hold in a very natural setting. Thus, we call such complex box mappings dynamically natural. Having such box mappings is the first step in tackling many problems in one-dimensional dynamics.\r\n• Many results in holomorphic dynamics rely on an interplay between combinatorial and analytic techniques. In this setting, some of these tools are:\r\n • the Enhanced Nest (a nest of puzzle pieces around critical points) from Kozlovski, Shen, van Strien (AnnMath 165:749–841, 2007), referred to below as KSS;\r\n • the Covering Lemma (which controls the moduli of pullbacks of annuli) from Kahn and Lyubich (Ann Math 169(2):561–593, 2009);\r\n • the QC-Criterion and the Spreading Principle from KSS.\r\nThe purpose of this paper is to make these tools more accessible so that they can be used as a ‘black box’, so one does not have to redo the proofs in new settings.\r\n• To give an intuitive, but also rather detailed, outline of the proof from KSS and Kozlovski and van Strien (Proc Lond Math Soc (3) 99:275–296, 2009) of the following results for non-renormalizable dynamically natural complex box mappings:\r\n • puzzle pieces shrink to points,\r\n • (under some assumptions) topologically conjugate non-renormalizable polynomials and box mappings are quasiconformally conjugate.\r\n• We prove the fundamental ergodic properties for dynamically natural box mappings. This leads to some necessary conditions for when such a box mapping supports a measurable invariant line field on its filled Julia set. These mappings\r\nare the analogues of Lattès maps in this setting.\r\n• We prove a version of Mañé’s Theorem for complex box mappings concerning expansion along orbits of points that avoid a neighborhood of the set of critical points."}],"file":[{"date_created":"2022-07-12T10:04:55Z","success":1,"relation":"main_file","file_id":"11559","content_type":"application/pdf","checksum":"16e7c659dee9073c6c8aeb87316ef201","access_level":"open_access","date_updated":"2022-07-12T10:04:55Z","file_size":2509915,"creator":"kschuh","file_name":"2022_ArnoldMathematicalJournal_Clark.pdf"}],"issue":"2","article_processing_charge":"No","volume":8,"tmp":{"legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","image":"/images/cc_by.png","short":"CC BY (4.0)"},"file_date_updated":"2022-07-12T10:04:55Z","oa":1,"publication_status":"published","type":"journal_article","author":[{"last_name":"Clark","first_name":"Trevor","full_name":"Clark, Trevor"},{"orcid":"0000-0002-9156-8616","id":"fe8209e2-906f-11eb-847d-950f8fc09115","first_name":"Kostiantyn","full_name":"Drach, Kostiantyn","last_name":"Drach"},{"last_name":"Kozlovski","full_name":"Kozlovski, Oleg","first_name":"Oleg"},{"last_name":"Strien","first_name":"Sebastian Van","full_name":"Strien, Sebastian Van"}],"day":"01","title":"The dynamics of complex box mappings","ec_funded":1,"citation":{"ama":"Clark T, Drach K, Kozlovski O, Strien SV. The dynamics of complex box mappings. Arnold Mathematical Journal. 2022;8(2):319-410. doi:10.1007/s40598-022-00200-7","apa":"Clark, T., Drach, K., Kozlovski, O., & Strien, S. V. (2022). The dynamics of complex box mappings. Arnold Mathematical Journal. Springer Nature. https://doi.org/10.1007/s40598-022-00200-7","short":"T. Clark, K. Drach, O. Kozlovski, S.V. Strien, Arnold Mathematical Journal 8 (2022) 319–410.","mla":"Clark, Trevor, et al. “The Dynamics of Complex Box Mappings.” Arnold Mathematical Journal, vol. 8, no. 2, Springer Nature, 2022, pp. 319–410, doi:10.1007/s40598-022-00200-7.","chicago":"Clark, Trevor, Kostiantyn Drach, Oleg Kozlovski, and Sebastian Van Strien. “The Dynamics of Complex Box Mappings.” Arnold Mathematical Journal. Springer Nature, 2022. https://doi.org/10.1007/s40598-022-00200-7.","ista":"Clark T, Drach K, Kozlovski O, Strien SV. 2022. The dynamics of complex box mappings. Arnold Mathematical Journal. 8(2), 319–410.","ieee":"T. Clark, K. Drach, O. Kozlovski, and S. V. Strien, “The dynamics of complex box mappings,” Arnold Mathematical Journal, vol. 8, no. 2. Springer Nature, pp. 319–410, 2022."},"ddc":["500"],"doi":"10.1007/s40598-022-00200-7","language":[{"iso":"eng"}],"acknowledgement":"We would also like to thank Dzmitry Dudko and Dierk Schleicher for many stimulating discussions and encouragement during our work on this project, and Weixiao Shen, Mikhail Hlushchanka and the referee for helpful comments. We are grateful to Leon Staresinic who carefully read the revised version of the manuscript and provided many helpful suggestions.","related_material":{"link":[{"relation":"erratum","url":"https://doi.org/10.1007/s40598-022-00209-y"},{"url":"https://doi.org/10.1007/s40598-022-00218-x","relation":"erratum"}]},"project":[{"grant_number":"885707","name":"Spectral rigidity and integrability for billiards and geodesic flows","call_identifier":"H2020","_id":"9B8B92DE-BA93-11EA-9121-9846C619BF3A"}],"date_created":"2022-07-10T22:01:53Z","month":"06","page":"319-410","status":"public","intvolume":" 8","quality_controlled":"1","department":[{"_id":"VaKa"}],"publication":"Arnold Mathematical Journal","publisher":"Springer Nature"},{"publisher":"Elsevier","isi":1,"publication":"Journal of Computational Physics","department":[{"_id":"GradSch"},{"_id":"ChWo"}],"quality_controlled":"1","intvolume":" 467","status":"public","month":"10","date_created":"2022-07-11T12:19:59Z","acknowledgement":"Zhores supercomputer of Skolkovo Institute of Science and Technology [68] has been used in the present research. S.A.M. was supported by Moscow Center for Fundamental and Applied Mathematics (the agreement with the Ministry of Education and Science of the Russian Federation No. 075-15-2019-1624). A.I.O. acknowledges RFBR project No. 20-31-90022. N.V.B. acknowledges the support of the Analytical Center (subsidy agreement 000000D730321P5Q0002, Grant No. 70-2021-00145 02.11.2021).","keyword":["Computer Science Applications","Physics and Astronomy (miscellaneous)","Applied Mathematics","Computational Mathematics","Modeling and Simulation","Numerical Analysis"],"language":[{"iso":"eng"}],"doi":"10.1016/j.jcp.2022.111439","ddc":["518"],"citation":{"mla":"Kalinov, Aleksei, et al. “Direct Simulation Monte Carlo for New Regimes in Aggregation-Fragmentation Kinetics.” Journal of Computational Physics, vol. 467, 111439, Elsevier, 2022, doi:10.1016/j.jcp.2022.111439.","chicago":"Kalinov, Aleksei, A.I. Osinskiy, S.A. Matveev, W. Otieno, and N.V. Brilliantov. “Direct Simulation Monte Carlo for New Regimes in Aggregation-Fragmentation Kinetics.” Journal of Computational Physics. Elsevier, 2022. https://doi.org/10.1016/j.jcp.2022.111439.","ieee":"A. Kalinov, A. I. Osinskiy, S. A. Matveev, W. Otieno, and N. V. Brilliantov, “Direct simulation Monte Carlo for new regimes in aggregation-fragmentation kinetics,” Journal of Computational Physics, vol. 467. Elsevier, 2022.","ista":"Kalinov A, Osinskiy AI, Matveev SA, Otieno W, Brilliantov NV. 2022. Direct simulation Monte Carlo for new regimes in aggregation-fragmentation kinetics. Journal of Computational Physics. 467, 111439.","ama":"Kalinov A, Osinskiy AI, Matveev SA, Otieno W, Brilliantov NV. Direct simulation Monte Carlo for new regimes in aggregation-fragmentation kinetics. Journal of Computational Physics. 2022;467. doi:10.1016/j.jcp.2022.111439","apa":"Kalinov, A., Osinskiy, A. I., Matveev, S. A., Otieno, W., & Brilliantov, N. V. (2022). Direct simulation Monte Carlo for new regimes in aggregation-fragmentation kinetics. Journal of Computational Physics. Elsevier. https://doi.org/10.1016/j.jcp.2022.111439","short":"A. Kalinov, A.I. Osinskiy, S.A. Matveev, W. Otieno, N.V. Brilliantov, Journal of Computational Physics 467 (2022)."},"title":"Direct simulation Monte Carlo for new regimes in aggregation-fragmentation kinetics","day":"15","author":[{"first_name":"Aleksei","full_name":"Kalinov, Aleksei","last_name":"Kalinov","orcid":"0000-0003-2189-3904","id":"44b7120e-eb97-11eb-a6c2-e1557aa81d02"},{"last_name":"Osinskiy","full_name":"Osinskiy, A.I.","first_name":"A.I."},{"first_name":"S.A.","full_name":"Matveev, S.A.","last_name":"Matveev"},{"last_name":"Otieno","full_name":"Otieno, W.","first_name":"W."},{"first_name":"N.V.","full_name":"Brilliantov, N.V.","last_name":"Brilliantov"}],"type":"journal_article","publication_status":"published","main_file_link":[{"url":"https://doi.org/10.48550/arXiv.2103.09481","open_access":"1"}],"oa":1,"volume":467,"arxiv":1,"article_processing_charge":"No","article_number":"111439","date_published":"2022-10-15T00:00:00Z","_id":"11556","abstract":[{"text":"We revisit two basic Direct Simulation Monte Carlo Methods to model aggregation kinetics and extend them for aggregation processes with collisional fragmentation (shattering). We test the performance and accuracy of the extended methods and compare their performance with efficient deterministic finite-difference method applied to the same model. We validate the stochastic methods on the test problems and apply them to verify the existence of oscillating regimes in the aggregation-fragmentation kinetics recently detected in deterministic simulations. We confirm the emergence of steady oscillations of densities in such systems and prove the stability of the\r\noscillations with respect to fluctuations and noise.","lang":"eng"}],"external_id":{"isi":["000917225500013"],"arxiv":["2103.09481"]},"date_updated":"2023-08-03T11:55:06Z","user_id":"4359f0d1-fa6c-11eb-b949-802e58b17ae8","publication_identifier":{"issn":["0021-9991"]},"article_type":"original","oa_version":"Preprint","year":"2022"},{"month":"07","date_created":"2022-07-17T22:01:53Z","publisher":"BioMed Central","isi":1,"publication":"Genome Biology","quality_controlled":"1","department":[{"_id":"FyKo"}],"status":"public","intvolume":" 23","citation":{"short":"R. Zhang, R. Kuo, M. Coulter, C.P.G. Calixto, J.C. Entizne, W. Guo, Y. Marquez, L. Milne, S. Riegler, A. Matsui, M. Tanaka, S. Harvey, Y. Gao, T. Wießner-Kroh, A. Paniagua, M. Crespi, K. Denby, A.B. Hur, E. Huq, M. Jantsch, A. Jarmolowski, T. Koester, S. Laubinger, Q.Q. Li, L. Gu, M. Seki, D. Staiger, R. Sunkar, Z. Szweykowska-Kulinska, S.L. Tu, A. Wachter, R. Waugh, L. Xiong, X.N. Zhang, A. Conesa, A.S.N. Reddy, A. Barta, M. Kalyna, J.W.S. Brown, Genome Biology 23 (2022).","ama":"Zhang R, Kuo R, Coulter M, et al. A high-resolution single-molecule sequencing-based Arabidopsis transcriptome using novel methods of Iso-seq analysis. Genome Biology. 2022;23. doi:10.1186/s13059-022-02711-0","apa":"Zhang, R., Kuo, R., Coulter, M., Calixto, C. P. G., Entizne, J. C., Guo, W., … Brown, J. W. S. (2022). A high-resolution single-molecule sequencing-based Arabidopsis transcriptome using novel methods of Iso-seq analysis. Genome Biology. BioMed Central. https://doi.org/10.1186/s13059-022-02711-0","chicago":"Zhang, Runxuan, Richard Kuo, Max Coulter, Cristiane P.G. Calixto, Juan Carlos Entizne, Wenbin Guo, Yamile Marquez, et al. “A High-Resolution Single-Molecule Sequencing-Based Arabidopsis Transcriptome Using Novel Methods of Iso-Seq Analysis.” Genome Biology. BioMed Central, 2022. https://doi.org/10.1186/s13059-022-02711-0.","ieee":"R. Zhang et al., “A high-resolution single-molecule sequencing-based Arabidopsis transcriptome using novel methods of Iso-seq analysis,” Genome Biology, vol. 23. BioMed Central, 2022.","ista":"Zhang R, Kuo R, Coulter M, Calixto CPG, Entizne JC, Guo W, Marquez Y, Milne L, Riegler S, Matsui A, Tanaka M, Harvey S, Gao Y, Wießner-Kroh T, Paniagua A, Crespi M, Denby K, Hur AB, Huq E, Jantsch M, Jarmolowski A, Koester T, Laubinger S, Li QQ, Gu L, Seki M, Staiger D, Sunkar R, Szweykowska-Kulinska Z, Tu SL, Wachter A, Waugh R, Xiong L, Zhang XN, Conesa A, Reddy ASN, Barta A, Kalyna M, Brown JWS. 2022. A high-resolution single-molecule sequencing-based Arabidopsis transcriptome using novel methods of Iso-seq analysis. Genome Biology. 23, 149.","mla":"Zhang, Runxuan, et al. “A High-Resolution Single-Molecule Sequencing-Based Arabidopsis Transcriptome Using Novel Methods of Iso-Seq Analysis.” Genome Biology, vol. 23, 149, BioMed Central, 2022, doi:10.1186/s13059-022-02711-0."},"title":"A high-resolution single-molecule sequencing-based Arabidopsis transcriptome using novel methods of Iso-seq analysis","day":"07","author":[{"last_name":"Zhang","full_name":"Zhang, Runxuan","first_name":"Runxuan"},{"full_name":"Kuo, Richard","first_name":"Richard","last_name":"Kuo"},{"last_name":"Coulter","full_name":"Coulter, Max","first_name":"Max"},{"full_name":"Calixto, Cristiane P.G.","first_name":"Cristiane P.G.","last_name":"Calixto"},{"first_name":"Juan Carlos","full_name":"Entizne, Juan Carlos","last_name":"Entizne"},{"last_name":"Guo","full_name":"Guo, Wenbin","first_name":"Wenbin"},{"full_name":"Marquez, Yamile","first_name":"Yamile","last_name":"Marquez"},{"first_name":"Linda","full_name":"Milne, Linda","last_name":"Milne"},{"full_name":"Riegler, Stefan","first_name":"Stefan","last_name":"Riegler","id":"FF6018E0-D806-11E9-8E43-0B14E6697425","orcid":"0000-0003-3413-1343"},{"first_name":"Akihiro","full_name":"Matsui, Akihiro","last_name":"Matsui"},{"last_name":"Tanaka","full_name":"Tanaka, Maho","first_name":"Maho"},{"last_name":"Harvey","full_name":"Harvey, Sarah","first_name":"Sarah"},{"full_name":"Gao, Yubang","first_name":"Yubang","last_name":"Gao"},{"full_name":"Wießner-Kroh, Theresa","first_name":"Theresa","last_name":"Wießner-Kroh"},{"full_name":"Paniagua, Alejandro","first_name":"Alejandro","last_name":"Paniagua"},{"last_name":"Crespi","first_name":"Martin","full_name":"Crespi, Martin"},{"first_name":"Katherine","full_name":"Denby, Katherine","last_name":"Denby"},{"last_name":"Hur","full_name":"Hur, Asa Ben","first_name":"Asa Ben"},{"last_name":"Huq","full_name":"Huq, Enamul","first_name":"Enamul"},{"last_name":"Jantsch","first_name":"Michael","full_name":"Jantsch, Michael"},{"first_name":"Artur","full_name":"Jarmolowski, Artur","last_name":"Jarmolowski"},{"full_name":"Koester, Tino","first_name":"Tino","last_name":"Koester"},{"last_name":"Laubinger","full_name":"Laubinger, Sascha","first_name":"Sascha"},{"last_name":"Li","first_name":"Qingshun Quinn","full_name":"Li, Qingshun Quinn"},{"full_name":"Gu, Lianfeng","first_name":"Lianfeng","last_name":"Gu"},{"last_name":"Seki","full_name":"Seki, Motoaki","first_name":"Motoaki"},{"full_name":"Staiger, Dorothee","first_name":"Dorothee","last_name":"Staiger"},{"last_name":"Sunkar","full_name":"Sunkar, Ramanjulu","first_name":"Ramanjulu"},{"last_name":"Szweykowska-Kulinska","first_name":"Zofia","full_name":"Szweykowska-Kulinska, Zofia"},{"full_name":"Tu, Shih Long","first_name":"Shih Long","last_name":"Tu"},{"last_name":"Wachter","full_name":"Wachter, Andreas","first_name":"Andreas"},{"first_name":"Robbie","full_name":"Waugh, Robbie","last_name":"Waugh"},{"full_name":"Xiong, Liming","first_name":"Liming","last_name":"Xiong"},{"last_name":"Zhang","full_name":"Zhang, Xiao Ning","first_name":"Xiao Ning"},{"full_name":"Conesa, Ana","first_name":"Ana","last_name":"Conesa"},{"last_name":"Reddy","first_name":"Anireddy S.N.","full_name":"Reddy, Anireddy S.N."},{"first_name":"Andrea","full_name":"Barta, Andrea","last_name":"Barta"},{"last_name":"Kalyna","first_name":"Maria","full_name":"Kalyna, Maria"},{"last_name":"Brown","full_name":"Brown, John W.S.","first_name":"John W.S."}],"type":"journal_article","acknowledgement":"This work was jointly supported by funding from the Biotechnology and Biological Sciences Research Council (BBSRC) BB/P009751/1 to JB; BB/R014582/1 to RW and RZ; BB/S020160/1 to RZ; BB/S004610/1 (16 ERA-CAPS BARN) to RW; the Scottish Government Rural and Environment Science and Analytical Services division (RESAS) [to RZ, RW, and JB]; the\r\nNational Science Foundation (MCB-2014408) and the National Institute of Health (NIH) (GM-114297) to E.H.; S. H. was supported by funding to K.D. from the University of York; the Austrian Science Fund (FWF) SFB F43 to AB and MJ and [P26333] to MK; The French Agence Nationale de la Recherche grant ANR-16-CE12-0032 to MC; the Japan Science and\r\nTechnology Agency (JST), the Core Research for Evolutionary Science and Technology (CREST; Grant Number JPMJCR13B4) to M.S.; the National Science Foundation (Grant No. DBI1949036 to A.b.H and A.S.N.R, and Grant No. MCB 2014542 to E.H. and A.S.N.R.); and the DOE Office of Science, Office of Biological and Environmental Research (Grant\r\nNo. DE-SC0010733) to A.S.N.R and A.b.H.; the Deutsche Forschungsgemeinschaft (DFG) STA653/14-1 and STA653/15-1 to DS; the National Science Foundation grant (IOS-154173) to Q.Q.L.; the German Research Foundation (DFG) WA2167/8-1 to AW and SFB1101/C03 to AW and TWK; the Research Grants Council (RGC) of Hong Kong (GRF 12103020) to LX. NSF grant IOS-1849708 and NSF EPSCoR grant 1826836 to RS; the Academia Sinica to S.-L. T.","language":[{"iso":"eng"}],"ddc":["570"],"doi":"10.1186/s13059-022-02711-0","article_processing_charge":"No","file":[{"file_id":"11597","relation":"main_file","content_type":"application/pdf","date_created":"2022-07-18T08:15:24Z","success":1,"creator":"dernst","file_size":3146207,"file_name":"2022_GenomeBiology_Zhang.pdf","checksum":"2c30ef84151d257a6b835b4e069b70ac","access_level":"open_access","date_updated":"2022-07-18T08:15:24Z"}],"article_number":"149","_id":"11587","date_published":"2022-07-07T00:00:00Z","abstract":[{"text":"Background: Accurate and comprehensive annotation of transcript sequences is essential for transcript quantification and differential gene and transcript expression analysis. Single-molecule long-read sequencing technologies provide improved integrity of transcript structures including alternative splicing, and transcription start and polyadenylation sites. However, accuracy is significantly affected by sequencing errors, mRNA degradation, or incomplete cDNA synthesis.\r\nResults: We present a new and comprehensive Arabidopsis thaliana Reference Transcript Dataset 3 (AtRTD3). AtRTD3 contains over 169,000 transcripts—twice that of the best current Arabidopsis transcriptome and including over 1500 novel genes. Seventy-eight percent of transcripts are from Iso-seq with accurately defined splice junctions and transcription start and end sites. We develop novel methods to determine splice junctions and transcription start and end sites accurately. Mismatch profiles around splice junctions provide a powerful feature to distinguish correct splice junctions and remove false splice junctions. Stratified approaches identify high-confidence transcription start and end sites and remove fragmentary transcripts due to degradation. AtRTD3 is a major improvement over existing transcriptomes as demonstrated by analysis of an Arabidopsis cold response RNA-seq time-series. AtRTD3 provides higher resolution of transcript expression profiling and identifies cold-induced differential transcription start and polyadenylation site usage.\r\nConclusions: AtRTD3 is the most comprehensive Arabidopsis transcriptome currently. It improves the precision of differential gene and transcript expression, differential alternative splicing, and transcription start/end site usage analysis from RNA-seq data. The novel methods for identifying accurate splice junctions and transcription start/end sites are widely applicable and will improve single-molecule sequencing analysis from any species.","lang":"eng"}],"publication_status":"published","oa":1,"file_date_updated":"2022-07-18T08:15:24Z","tmp":{"legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","image":"/images/cc_by.png","short":"CC BY (4.0)"},"volume":23,"article_type":"original","year":"2022","oa_version":"Published Version","has_accepted_license":"1","scopus_import":"1","external_id":{"isi":["000821915500002"]},"user_id":"4359f0d1-fa6c-11eb-b949-802e58b17ae8","date_updated":"2023-08-03T12:04:18Z","publication_identifier":{"eissn":["1474-760X"]}},{"user_id":"4359f0d1-fa6c-11eb-b949-802e58b17ae8","date_updated":"2023-08-03T12:01:01Z","scopus_import":"1","external_id":{"isi":["000823746100018"]},"publication_identifier":{"eissn":["1592-8721"],"issn":["0390-6078"]},"article_type":"original","oa_version":"Published Version","has_accepted_license":"1","year":"2022","license":"https://creativecommons.org/licenses/by-nc/4.0/","publication_status":"published","oa":1,"file_date_updated":"2022-07-18T07:51:55Z","volume":107,"tmp":{"short":"CC BY-NC (4.0)","legal_code_url":"https://creativecommons.org/licenses/by-nc/4.0/legalcode","image":"/images/cc_by_nc.png","name":"Creative Commons Attribution-NonCommercial 4.0 International (CC BY-NC 4.0)"},"issue":"7","article_processing_charge":"No","file":[{"content_type":"application/pdf","relation":"main_file","file_id":"11595","success":1,"date_created":"2022-07-18T07:51:55Z","file_name":"2022_Haematologica_Nicolai.pdf","file_size":1722094,"creator":"dernst","date_updated":"2022-07-18T07:51:55Z","access_level":"open_access","checksum":"9b47830945f3c30428fe9cfee2dc4a8a"}],"_id":"11588","abstract":[{"lang":"eng","text":"Visualizing cell behavior and effector function on a single cell level has been crucial for understanding key aspects of mammalian biology. Due to their small size, large number and rapid recruitment into thrombi, there is a lack of data on fate and behavior of individual platelets in thrombosis and hemostasis. Here we report the use of platelet lineage restricted multi-color reporter mouse strains to delineate platelet function on a single cell level. We show that genetic labeling allows for single platelet and megakaryocyte (MK) tracking and morphological analysis in vivo and in vitro, while not affecting lineage functions. Using Cre-driven Confetti expression, we provide insights into temporal gene expression patterns as well as spatial clustering of MK in the bone marrow. In the vasculature, shape analysis of activated platelets recruited to thrombi identifies ubiquitous filopodia formation with no evidence of lamellipodia formation. Single cell tracking in complex thrombi reveals prominent myosin-dependent motility of platelets and highlights thrombus formation as a highly dynamic process amenable to modification and intervention of the acto-myosin cytoskeleton. Platelet function assays combining flow cytrometry, as well as in vivo, ex vivo and in vitro imaging show unaltered platelet functions of multicolor reporter mice compared to wild-type controls. In conclusion, platelet lineage multicolor reporter mice prove useful in furthering our understanding of platelet and MK biology on a single cell level."}],"date_published":"2022-07-01T00:00:00Z","acknowledgement":"This study was supported by the Deutsche Forschungsgemeinschaft (DFG) SFB 914 ( to SM [B02 and Z01]), the DFG SFB 1123 (to SM [B06]), the DFG FOR 2033 (to SM), the German\r\nCenter for Cardiovascular Research (DZHK) (Clinician Scientist Programme), MHA 1.4VD (to SM), Postdoc Start-up Grant, 81X3600213 (to FG), 81X3600222 (to LN), the FP7 program\r\n(project 260309, PRESTIGE [to SM]). This project has received funding from the European Research Council (ERC) under the European Union’s Horizon 2020 research and innovation programme (grant agreement No. 83344, ERC-2018-ADG “IMMUNOTHROMBOSIS” [to SM] and the Marie Skłodowska Curie Individual Fellowship (EU project 747687, LamelliActin [to FG]). ","project":[{"name":"Mechanical Adaptation of Lamellipodial Actin Networks in Migrating Cells","grant_number":"747687","_id":"260AA4E2-B435-11E9-9278-68D0E5697425","call_identifier":"H2020"}],"language":[{"iso":"eng"}],"ddc":["570"],"doi":"10.3324/haematol.2021.278896","ec_funded":1,"citation":{"apa":"Nicolai, L., Kaiser, R., Escaig, R., Hoffknecht, M. L., Anjum, A., Leunig, A., … Gärtner, F. R. (2022). Single platelet and megakaryocyte morpho-dynamics uncovered by multicolor reporter mouse strains in vitro and in vivo. Haematologica. Ferrata Storti Foundation. https://doi.org/10.3324/haematol.2021.278896","ama":"Nicolai L, Kaiser R, Escaig R, et al. Single platelet and megakaryocyte morpho-dynamics uncovered by multicolor reporter mouse strains in vitro and in vivo. Haematologica. 2022;107(7):1669-1680. doi:10.3324/haematol.2021.278896","short":"L. Nicolai, R. Kaiser, R. Escaig, M.L. Hoffknecht, A. Anjum, A. Leunig, J. Pircher, A. Ehrlich, M. Lorenz, H. Ishikawa-Ankerhold, W.C. Aird, S. Massberg, F.R. Gärtner, Haematologica 107 (2022) 1669–1680.","mla":"Nicolai, Leo, et al. “Single Platelet and Megakaryocyte Morpho-Dynamics Uncovered by Multicolor Reporter Mouse Strains in Vitro and in Vivo.” Haematologica, vol. 107, no. 7, Ferrata Storti Foundation, 2022, pp. 1669–80, doi:10.3324/haematol.2021.278896.","ieee":"L. Nicolai et al., “Single platelet and megakaryocyte morpho-dynamics uncovered by multicolor reporter mouse strains in vitro and in vivo,” Haematologica, vol. 107, no. 7. Ferrata Storti Foundation, pp. 1669–1680, 2022.","ista":"Nicolai L, Kaiser R, Escaig R, Hoffknecht ML, Anjum A, Leunig A, Pircher J, Ehrlich A, Lorenz M, Ishikawa-Ankerhold H, Aird WC, Massberg S, Gärtner FR. 2022. Single platelet and megakaryocyte morpho-dynamics uncovered by multicolor reporter mouse strains in vitro and in vivo. Haematologica. 107(7), 1669–1680.","chicago":"Nicolai, Leo, Rainer Kaiser, Raphael Escaig, Marie Louise Hoffknecht, Afra Anjum, Alexander Leunig, Joachim Pircher, et al. “Single Platelet and Megakaryocyte Morpho-Dynamics Uncovered by Multicolor Reporter Mouse Strains in Vitro and in Vivo.” Haematologica. Ferrata Storti Foundation, 2022. https://doi.org/10.3324/haematol.2021.278896."},"title":"Single platelet and megakaryocyte morpho-dynamics uncovered by multicolor reporter mouse strains in vitro and in vivo","day":"01","type":"journal_article","author":[{"last_name":"Nicolai","first_name":"Leo","full_name":"Nicolai, Leo"},{"first_name":"Rainer","full_name":"Kaiser, Rainer","last_name":"Kaiser"},{"last_name":"Escaig","full_name":"Escaig, Raphael","first_name":"Raphael"},{"last_name":"Hoffknecht","full_name":"Hoffknecht, Marie Louise","first_name":"Marie Louise"},{"full_name":"Anjum, Afra","first_name":"Afra","last_name":"Anjum"},{"last_name":"Leunig","full_name":"Leunig, Alexander","first_name":"Alexander"},{"full_name":"Pircher, Joachim","first_name":"Joachim","last_name":"Pircher"},{"first_name":"Andreas","full_name":"Ehrlich, Andreas","last_name":"Ehrlich"},{"first_name":"Michael","full_name":"Lorenz, Michael","last_name":"Lorenz"},{"full_name":"Ishikawa-Ankerhold, Hellen","first_name":"Hellen","last_name":"Ishikawa-Ankerhold"},{"last_name":"Aird","first_name":"William C.","full_name":"Aird, William C."},{"first_name":"Steffen","full_name":"Massberg, Steffen","last_name":"Massberg"},{"first_name":"Florian R","full_name":"Gärtner, Florian R","last_name":"Gärtner","id":"397A88EE-F248-11E8-B48F-1D18A9856A87","orcid":"0000-0001-6120-3723"}],"publisher":"Ferrata Storti Foundation","isi":1,"quality_controlled":"1","department":[{"_id":"MiSi"}],"publication":"Haematologica","intvolume":" 107","status":"public","page":"1669-1680","month":"07","date_created":"2022-07-17T22:01:54Z"},{"month":"06","date_created":"2022-07-17T22:01:54Z","publisher":"Frontiers","isi":1,"quality_controlled":"1","department":[{"_id":"JiFr"}],"publication":"Frontiers in Plant Science","intvolume":" 13","status":"public","citation":{"chicago":"Wang, Ren, Ellie Himschoot, Jian Chen, Marie Boudsocq, Danny Geelen, Jiří Friml, Tom Beeckman, and Steffen Vanneste. “Constitutive Active CPK30 Interferes with Root Growth and Endomembrane Trafficking in Arabidopsis Thaliana.” Frontiers in Plant Science. Frontiers, 2022. https://doi.org/10.3389/fpls.2022.862398.","ista":"Wang R, Himschoot E, Chen J, Boudsocq M, Geelen D, Friml J, Beeckman T, Vanneste S. 2022. Constitutive active CPK30 interferes with root growth and endomembrane trafficking in Arabidopsis thaliana. Frontiers in Plant Science. 13, 862398.","ieee":"R. Wang et al., “Constitutive active CPK30 interferes with root growth and endomembrane trafficking in Arabidopsis thaliana,” Frontiers in Plant Science, vol. 13. Frontiers, 2022.","mla":"Wang, Ren, et al. “Constitutive Active CPK30 Interferes with Root Growth and Endomembrane Trafficking in Arabidopsis Thaliana.” Frontiers in Plant Science, vol. 13, 862398, Frontiers, 2022, doi:10.3389/fpls.2022.862398.","short":"R. Wang, E. Himschoot, J. Chen, M. Boudsocq, D. Geelen, J. Friml, T. Beeckman, S. Vanneste, Frontiers in Plant Science 13 (2022).","ama":"Wang R, Himschoot E, Chen J, et al. Constitutive active CPK30 interferes with root growth and endomembrane trafficking in Arabidopsis thaliana. Frontiers in Plant Science. 2022;13. doi:10.3389/fpls.2022.862398","apa":"Wang, R., Himschoot, E., Chen, J., Boudsocq, M., Geelen, D., Friml, J., … Vanneste, S. (2022). Constitutive active CPK30 interferes with root growth and endomembrane trafficking in Arabidopsis thaliana. Frontiers in Plant Science. Frontiers. https://doi.org/10.3389/fpls.2022.862398"},"title":"Constitutive active CPK30 interferes with root growth and endomembrane trafficking in Arabidopsis thaliana","day":"16","author":[{"last_name":"Wang","first_name":"Ren","full_name":"Wang, Ren"},{"full_name":"Himschoot, Ellie","first_name":"Ellie","last_name":"Himschoot"},{"first_name":"Jian","full_name":"Chen, Jian","last_name":"Chen"},{"last_name":"Boudsocq","first_name":"Marie","full_name":"Boudsocq, Marie"},{"full_name":"Geelen, Danny","first_name":"Danny","last_name":"Geelen"},{"id":"4159519E-F248-11E8-B48F-1D18A9856A87","orcid":"0000-0002-8302-7596","first_name":"Jiří","full_name":"Friml, Jiří","last_name":"Friml"},{"last_name":"Beeckman","first_name":"Tom","full_name":"Beeckman, Tom"},{"full_name":"Vanneste, Steffen","first_name":"Steffen","last_name":"Vanneste"}],"type":"journal_article","acknowledgement":"RW and JC predoctoral fellows that were supported by the Chinese Science Counsil. The IPS2 benefits from the support of the LabEx Saclay Plant Sciences-SPS (ANR-10-LABX-0040-SPS).\r\nWe thank Jen Sheen for establishing and generously sharing the CKP family clone sets, and for providing useful feedback on the manuscript.","pmid":1,"related_material":{"link":[{"relation":"erratum","url":"https://doi.org/10.3389/fpls.2022.1100792"}]},"language":[{"iso":"eng"}],"ddc":["580"],"doi":"10.3389/fpls.2022.862398","article_processing_charge":"No","article_number":"862398","file":[{"content_type":"application/pdf","relation":"main_file","file_id":"11596","success":1,"date_created":"2022-07-18T08:05:15Z","file_name":"2022_FrontiersPlantScience_Wang.pdf","creator":"dernst","file_size":5040638,"date_updated":"2022-07-18T08:05:15Z","access_level":"open_access","checksum":"95313515637c0f84de591d204375d764"}],"_id":"11589","abstract":[{"text":"Calcium-dependent protein kinases (CPK) are key components of a wide array of signaling pathways, translating stress and nutrient signaling into the modulation of cellular processes such as ion transport and transcription. However, not much is known about CPKs in endomembrane trafficking. Here, we screened for CPKs that impact on root growth and gravitropism, by overexpressing constitutively active forms of CPKs under the control of an inducible promoter in Arabidopsis thaliana. We found that inducible overexpression of an constitutive active CPK30 (CA-CPK30) resulted in a loss of root gravitropism and ectopic auxin accumulation in the root tip. Immunolocalization revealed that CA-CPK30 roots have reduced PIN protein levels, PIN1 polarity defects and impaired Brefeldin A (BFA)-sensitive trafficking. Moreover, FM4-64 uptake was reduced, indicative of a defect in endocytosis. The effects on BFA-sensitive trafficking were not specific to PINs, as BFA could not induce aggregation of ARF1- and CHC-labeled endosomes in CA-CPK30. Interestingly, the interference with BFA-body formation, could be reverted by increasing the extracellular pH, indicating a pH-dependence of this CA-CPK30 effect. Altogether, our data reveal an important role for CPK30 in root growth regulation and endomembrane trafficking in Arabidopsis thaliana.","lang":"eng"}],"date_published":"2022-06-16T00:00:00Z","publication_status":"published","oa":1,"file_date_updated":"2022-07-18T08:05:15Z","volume":13,"tmp":{"legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","image":"/images/cc_by.png","short":"CC BY (4.0)"},"article_type":"original","has_accepted_license":"1","oa_version":"Published Version","year":"2022","date_updated":"2023-08-03T12:01:47Z","user_id":"4359f0d1-fa6c-11eb-b949-802e58b17ae8","external_id":{"pmid":["35783951"],"isi":["000819250500001"]},"scopus_import":"1","publication_identifier":{"eissn":["1664-462X"]}},{"publication_status":"published","oa":1,"file_date_updated":"2022-07-18T06:33:13Z","tmp":{"legal_code_url":"https://creativecommons.org/licenses/by/4.0/legalcode","name":"Creative Commons Attribution 4.0 International Public License (CC-BY 4.0)","image":"/images/cc_by.png","short":"CC BY (4.0)"},"volume":24,"article_processing_charge":"No","issue":"6","file":[{"content_type":"application/pdf","relation":"main_file","file_id":"11594","date_created":"2022-07-18T06:33:13Z","success":1,"file_name":"2022_NewJournalPhysics_Brauneis.pdf","file_size":3415721,"creator":"dernst","checksum":"dc67b60f2e50e9ef2bd820ca0d7333d2","date_updated":"2022-07-18T06:33:13Z","access_level":"open_access"}],"article_number":"063036","date_published":"2022-06-01T00:00:00Z","_id":"11590","abstract":[{"text":"We investigate the ground-state properties of weakly repulsive one-dimensional bosons in the presence of an attractive zero-range impurity potential. First, we derive mean-field solutions to the problem on a finite ring for the two asymptotic cases: (i) all bosons are bound to the impurity and (ii) all bosons are in a scattering state. Moreover, we derive the critical line that separates these regimes in the parameter space. In the thermodynamic limit, this critical line determines the maximum number of bosons that can be bound by the impurity potential, forming an artificial atom. Second, we validate the mean-field results using the flow equation approach and the multi-layer multi-configuration time-dependent Hartree method for atomic mixtures. While beyond-mean-field effects destroy long-range order in the Bose gas, the critical boson number is unaffected. Our findings are important for understanding such artificial atoms in low-density Bose gases with static and mobile impurities.","lang":"eng"}],"scopus_import":"1","external_id":{"isi":["000818530000001"]},"user_id":"4359f0d1-fa6c-11eb-b949-802e58b17ae8","date_updated":"2023-08-03T11:57:41Z","publication_identifier":{"issn":["1367-2630"]},"article_type":"original","year":"2022","oa_version":"Published Version","has_accepted_license":"1","publisher":"IOP Publishing","isi":1,"publication":"New Journal of Physics","quality_controlled":"1","department":[{"_id":"MiLe"}],"status":"public","intvolume":" 24","month":"06","date_created":"2022-07-17T22:01:55Z","project":[{"call_identifier":"H2020","_id":"260C2330-B435-11E9-9278-68D0E5697425","name":"ISTplus - Postdoctoral Fellowships","grant_number":"754411"},{"_id":"2688CF98-B435-11E9-9278-68D0E5697425","call_identifier":"H2020","grant_number":"801770","name":"Angulon: physics and applications of a new quasiparticle"}],"acknowledgement":"This work has received funding from the DFG Project No. 413495248 [VO 2437/1-1] (FB, H-WH, AGV) and European Union's Horizon 2020 research and innovation programme under the Marie Skĺodowska-Curie Grant Agreement No. 754411 (AGV). ML acknowledges support by the European Research Council (ERC) Starting Grant No. 801770 (ANGULON). SIM acknowledges support from the NSF through a grant for ITAMP at Harvard University.","language":[{"iso":"eng"}],"doi":"10.1088/1367-2630/ac78d8","ddc":["530"],"citation":{"mla":"Brauneis, Fabian, et al. “Artificial Atoms from Cold Bosons in One Dimension.” New Journal of Physics, vol. 24, no. 6, 063036, IOP Publishing, 2022, doi:10.1088/1367-2630/ac78d8.","chicago":"Brauneis, Fabian, Timothy G. Backert, Simeon I. Mistakidis, Mikhail Lemeshko, Hans Werner Hammer, and Artem Volosniev. “Artificial Atoms from Cold Bosons in One Dimension.” New Journal of Physics. IOP Publishing, 2022. https://doi.org/10.1088/1367-2630/ac78d8.","ista":"Brauneis F, Backert TG, Mistakidis SI, Lemeshko M, Hammer HW, Volosniev A. 2022. Artificial atoms from cold bosons in one dimension. New Journal of Physics. 24(6), 063036.","ieee":"F. Brauneis, T. G. Backert, S. I. Mistakidis, M. Lemeshko, H. W. Hammer, and A. Volosniev, “Artificial atoms from cold bosons in one dimension,” New Journal of Physics, vol. 24, no. 6. IOP Publishing, 2022.","ama":"Brauneis F, Backert TG, Mistakidis SI, Lemeshko M, Hammer HW, Volosniev A. Artificial atoms from cold bosons in one dimension. New Journal of Physics. 2022;24(6). doi:10.1088/1367-2630/ac78d8","apa":"Brauneis, F., Backert, T. G., Mistakidis, S. I., Lemeshko, M., Hammer, H. W., & Volosniev, A. (2022). Artificial atoms from cold bosons in one dimension. New Journal of Physics. IOP Publishing. https://doi.org/10.1088/1367-2630/ac78d8","short":"F. Brauneis, T.G. Backert, S.I. Mistakidis, M. Lemeshko, H.W. Hammer, A. Volosniev, New Journal of Physics 24 (2022)."},"ec_funded":1,"title":"Artificial atoms from cold bosons in one dimension","day":"01","author":[{"first_name":"Fabian","full_name":"Brauneis, Fabian","last_name":"Brauneis"},{"first_name":"Timothy G.","full_name":"Backert, Timothy G.","last_name":"Backert"},{"first_name":"Simeon I.","full_name":"Mistakidis, Simeon I.","last_name":"Mistakidis"},{"orcid":"0000-0002-6990-7802","id":"37CB05FA-F248-11E8-B48F-1D18A9856A87","last_name":"Lemeshko","full_name":"Lemeshko, Mikhail","first_name":"Mikhail"},{"last_name":"Hammer","full_name":"Hammer, Hans Werner","first_name":"Hans Werner"},{"orcid":"0000-0003-0393-5525","id":"37D278BC-F248-11E8-B48F-1D18A9856A87","first_name":"Artem","full_name":"Volosniev, Artem","last_name":"Volosniev"}],"type":"journal_article"},{"doi":"10.1103/PhysRevA.105.062454","language":[{"iso":"eng"}],"project":[{"call_identifier":"H2020","_id":"9B868D20-BA93-11EA-9121-9846C619BF3A","grant_number":"899354","name":"Quantum Local Area Networks with Superconducting Qubits"}],"acknowledgement":"We thank T. Mavrogordatos and D. Zhu for initial contribution on the presented topic and K. Fedorov for stimulating discussions on entangled microwave beams. This work was supported by the Austrian Science Fund (FWF) through Grant No. P32299 (PHONED) and the European Union’s Horizon 2020 research and innovation programme under Grant Agreement No. 899354 (SuperQuLAN). Most of the computational results presented were obtained using the CLIP cluster [65].","type":"journal_article","author":[{"last_name":"Agustí","first_name":"J.","full_name":"Agustí, J."},{"last_name":"Minoguchi","first_name":"Y.","full_name":"Minoguchi, Y."},{"last_name":"Fink","full_name":"Fink, Johannes M","first_name":"Johannes M","orcid":"0000-0001-8112-028X","id":"4B591CBA-F248-11E8-B48F-1D18A9856A87"},{"full_name":"Rabl, P.","first_name":"P.","last_name":"Rabl"}],"day":"29","title":"Long-distance distribution of qubit-qubit entanglement using Gaussian-correlated photonic beams","citation":{"short":"J. Agustí, Y. Minoguchi, J.M. Fink, P. Rabl, Physical Review A 105 (2022).","apa":"Agustí, J., Minoguchi, Y., Fink, J. M., & Rabl, P. (2022). Long-distance distribution of qubit-qubit entanglement using Gaussian-correlated photonic beams. Physical Review A. American Physical Society. https://doi.org/10.1103/PhysRevA.105.062454","ama":"Agustí J, Minoguchi Y, Fink JM, Rabl P. Long-distance distribution of qubit-qubit entanglement using Gaussian-correlated photonic beams. Physical Review A. 2022;105(6). doi:10.1103/PhysRevA.105.062454","ieee":"J. Agustí, Y. Minoguchi, J. M. Fink, and P. Rabl, “Long-distance distribution of qubit-qubit entanglement using Gaussian-correlated photonic beams,” Physical Review A, vol. 105, no. 6. American Physical Society, 2022.","ista":"Agustí J, Minoguchi Y, Fink JM, Rabl P. 2022. Long-distance distribution of qubit-qubit entanglement using Gaussian-correlated photonic beams. Physical Review A. 105(6), 062454.","chicago":"Agustí, J., Y. Minoguchi, Johannes M Fink, and P. Rabl. “Long-Distance Distribution of Qubit-Qubit Entanglement Using Gaussian-Correlated Photonic Beams.” Physical Review A. American Physical Society, 2022. https://doi.org/10.1103/PhysRevA.105.062454.","mla":"Agustí, J., et al. “Long-Distance Distribution of Qubit-Qubit Entanglement Using Gaussian-Correlated Photonic Beams.” Physical Review A, vol. 105, no. 6, 062454, American Physical Society, 2022, doi:10.1103/PhysRevA.105.062454."},"ec_funded":1,"status":"public","intvolume":" 105","publication":"Physical Review A","quality_controlled":"1","department":[{"_id":"JoFi"}],"isi":1,"publisher":"American Physical Society","date_created":"2022-07-17T22:01:55Z","month":"06","publication_identifier":{"issn":["2469-9926"],"eissn":["2469-9934"]},"external_id":{"arxiv":["2204.02993"],"isi":["000824330200003"]},"scopus_import":"1","user_id":"4359f0d1-fa6c-11eb-b949-802e58b17ae8","date_updated":"2023-08-03T11:58:16Z","oa_version":"Preprint","year":"2022","article_type":"original","volume":105,"oa":1,"main_file_link":[{"url":" https://doi.org/10.48550/arXiv.2204.02993","open_access":"1"}],"publication_status":"published","_id":"11591","date_published":"2022-06-29T00:00:00Z","abstract":[{"text":"We investigate the deterministic generation and distribution of entanglement in large quantum networks by driving distant qubits with the output fields of a nondegenerate parametric amplifier. In this setting, the amplifier produces a continuous Gaussian two-mode squeezed state, which acts as a quantum-correlated reservoir for the qubits and relaxes them into a highly entangled steady state. Here we are interested in the maximal amount of entanglement and the optimal entanglement generation rates that can be achieved with this scheme under realistic conditions taking, in particular, the finite amplifier bandwidth, waveguide losses, and propagation delays into account. By combining exact numerical simulations of the full network with approximate analytic results, we predict the optimal working point for the amplifier and the corresponding qubit-qubit entanglement under various conditions. Our findings show that this passive conversion of Gaussian into discrete-variable entanglement offers a robust and experimentally very attractive approach for operating large optical, microwave, or hybrid quantum networks, for which efficient parametric amplifiers are currently developed.","lang":"eng"}],"article_number":"062454","article_processing_charge":"No","issue":"6","arxiv":1},{"publication_status":"published","main_file_link":[{"url":" https://doi.org/10.48550/arXiv.2206.03924","open_access":"1"}],"oa":1,"volume":105,"arxiv":1,"article_processing_charge":"No","issue":"6","article_number":"063329","_id":"11592","date_published":"2022-06-30T00:00:00Z","abstract":[{"text":"We compare recent experimental results [Science 375, 528 (2022)] of the superfluid unitary Fermi gas near the critical temperature with a thermodynamic model based on the elementary excitations of the system. We find good agreement between experimental data and our theory for several quantities such as first sound, second sound, and superfluid fraction. We also show that mode mixing between first and second sound occurs. Finally, we characterize the response amplitude to a density perturbation: Close to the critical temperature both first and second sound can be excited through a density perturbation, whereas at lower temperatures only the first sound mode exhibits a significant response.","lang":"eng"}],"scopus_import":"1","external_id":{"arxiv":["2206.03924"],"isi":["000829758500010"]},"user_id":"4359f0d1-fa6c-11eb-b949-802e58b17ae8","date_updated":"2023-08-03T12:00:11Z","publication_identifier":{"eissn":["2469-9934"],"issn":["2469-9926"]},"article_type":"original","oa_version":"Preprint","year":"2022","publisher":"American Physical Society","isi":1,"publication":"Physical Review A","quality_controlled":"1","department":[{"_id":"MiLe"}],"intvolume":" 105","status":"public","month":"06","date_created":"2022-07-17T22:01:55Z","acknowledgement":"The authors gratefully acknowledge stimulating discussions with T. Enss, and thank an anonymous referee for suggestions and remarks that allowed us to improve the original manuscript. This work is supported by the Deutsche Forschungsgemeinschaft (DFG, German Research Foundation) under Germany’s Excellence Strategy EXC2181/1-390900948 (the Heidelberg STRUCTURES Excellence Cluster).","language":[{"iso":"eng"}],"doi":"10.1103/PhysRevA.105.063329","citation":{"short":"G. Bighin, A. Cappellaro, L. Salasnich, Physical Review A 105 (2022).","ama":"Bighin G, Cappellaro A, Salasnich L. Unitary Fermi superfluid near the critical temperature: Thermodynamics and sound modes from elementary excitations. Physical Review A. 2022;105(6). doi:10.1103/PhysRevA.105.063329","apa":"Bighin, G., Cappellaro, A., & Salasnich, L. (2022). Unitary Fermi superfluid near the critical temperature: Thermodynamics and sound modes from elementary excitations. Physical Review A. American Physical Society. https://doi.org/10.1103/PhysRevA.105.063329","chicago":"Bighin, Giacomo, Alberto Cappellaro, and L. Salasnich. “Unitary Fermi Superfluid near the Critical Temperature: Thermodynamics and Sound Modes from Elementary Excitations.” Physical Review A. American Physical Society, 2022. https://doi.org/10.1103/PhysRevA.105.063329.","ista":"Bighin G, Cappellaro A, Salasnich L. 2022. Unitary Fermi superfluid near the critical temperature: Thermodynamics and sound modes from elementary excitations. Physical Review A. 105(6), 063329.","ieee":"G. Bighin, A. Cappellaro, and L. Salasnich, “Unitary Fermi superfluid near the critical temperature: Thermodynamics and sound modes from elementary excitations,” Physical Review A, vol. 105, no. 6. American Physical Society, 2022.","mla":"Bighin, Giacomo, et al. “Unitary Fermi Superfluid near the Critical Temperature: Thermodynamics and Sound Modes from Elementary Excitations.” Physical Review A, vol. 105, no. 6, 063329, American Physical Society, 2022, doi:10.1103/PhysRevA.105.063329."},"title":"Unitary Fermi superfluid near the critical temperature: Thermodynamics and sound modes from elementary excitations","day":"30","author":[{"orcid":"0000-0001-8823-9777","id":"4CA96FD4-F248-11E8-B48F-1D18A9856A87","last_name":"Bighin","first_name":"Giacomo","full_name":"Bighin, Giacomo"},{"last_name":"Cappellaro","full_name":"Cappellaro, Alberto","first_name":"Alberto","id":"9d13b3cb-30a2-11eb-80dc-f772505e8660","orcid":"0000-0001-6110-2359"},{"full_name":"Salasnich, L.","first_name":"L.","last_name":"Salasnich"}],"type":"journal_article"},{"oa_version":"Preprint","year":"2022","article_type":"original","publication_identifier":{"eissn":["1432-0444"],"issn":["0179-5376"]},"user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","date_updated":"2023-08-14T12:43:52Z","external_id":{"arxiv":["1803.05085"],"isi":["000825014500001"]},"scopus_import":"1","date_published":"2022-09-01T00:00:00Z","_id":"11593","abstract":[{"lang":"eng","text":"A drawing of a graph on a surface is independently even if every pair of nonadjacent edges in the drawing crosses an even number of times. The Z2 -genus of a graph G is the minimum g such that G has an independently even drawing on the orientable surface of genus g. An unpublished result by Robertson and Seymour implies that for every t, every graph of sufficiently large genus contains as a minor a projective t×t grid or one of the following so-called t -Kuratowski graphs: K3,t, or t copies of K5 or K3,3 sharing at most two common vertices. We show that the Z2-genus of graphs in these families is unbounded in t; in fact, equal to their genus. Together, this implies that the genus of a graph is bounded from above by a function of its Z2-genus, solving a problem posed by Schaefer and Štefankovič, and giving an approximate version of the Hanani–Tutte theorem on orientable surfaces. We also obtain an analogous result for Euler genus and Euler Z2-genus of graphs."}],"article_processing_charge":"No","arxiv":1,"volume":68,"oa":1,"main_file_link":[{"url":"https://arxiv.org/abs/1803.05085","open_access":"1"}],"publication_status":"published","type":"journal_article","author":[{"orcid":"0000-0001-8485-1774","id":"39F3FFE4-F248-11E8-B48F-1D18A9856A87","last_name":"Fulek","full_name":"Fulek, Radoslav","first_name":"Radoslav"},{"first_name":"Jan","full_name":"Kynčl, Jan","last_name":"Kynčl"}],"day":"01","title":"The Z2-Genus of Kuratowski minors","citation":{"chicago":"Fulek, Radoslav, and Jan Kynčl. “The Z2-Genus of Kuratowski Minors.” Discrete and Computational Geometry. Springer Nature, 2022. https://doi.org/10.1007/s00454-022-00412-w.","ieee":"R. Fulek and J. Kynčl, “The Z2-Genus of Kuratowski minors,” Discrete and Computational Geometry, vol. 68. Springer Nature, pp. 425–447, 2022.","ista":"Fulek R, Kynčl J. 2022. The Z2-Genus of Kuratowski minors. Discrete and Computational Geometry. 68, 425–447.","mla":"Fulek, Radoslav, and Jan Kynčl. “The Z2-Genus of Kuratowski Minors.” Discrete and Computational Geometry, vol. 68, Springer Nature, 2022, pp. 425–47, doi:10.1007/s00454-022-00412-w.","short":"R. Fulek, J. Kynčl, Discrete and Computational Geometry 68 (2022) 425–447.","ama":"Fulek R, Kynčl J. The Z2-Genus of Kuratowski minors. Discrete and Computational Geometry. 2022;68:425-447. doi:10.1007/s00454-022-00412-w","apa":"Fulek, R., & Kynčl, J. (2022). The Z2-Genus of Kuratowski minors. Discrete and Computational Geometry. Springer Nature. https://doi.org/10.1007/s00454-022-00412-w"},"doi":"10.1007/s00454-022-00412-w","language":[{"iso":"eng"}],"acknowledgement":"We thank Zdeněk Dvořák, Xavier Goaoc, and Pavel Paták for helpful discussions. We also thank Bojan Mohar, Paul Seymour, Gelasio Salazar, Jim Geelen, and John Maharry for information about their unpublished results related to Conjecture 3.1. Finally we thank the reviewers for corrections and suggestions for improving the presentation.\r\nSupported by Austrian Science Fund (FWF): M2281-N35. Supported by project 19-04113Y of the Czech Science Foundation (GAČR), by the Czech-French collaboration project EMBEDS II (CZ: 7AMB17FR029, FR: 38087RM), and by Charles University project UNCE/SCI/004.","related_material":{"record":[{"status":"public","id":"186","relation":"earlier_version"}]},"project":[{"name":"Eliminating intersections in drawings of graphs","grant_number":"M02281","_id":"261FA626-B435-11E9-9278-68D0E5697425","call_identifier":"FWF"}],"date_created":"2022-07-17T22:01:56Z","month":"09","page":"425-447","status":"public","intvolume":" 68","department":[{"_id":"UlWa"}],"quality_controlled":"1","publication":"Discrete and Computational Geometry","isi":1,"publisher":"Springer Nature"},{"quality_controlled":"1","publication":"Nature Astronomy","volume":6,"status":"public","intvolume":" 6","publisher":"Springer Nature","publication_status":"published","extern":"1","month":"05","_id":"11600","date_created":"2022-07-18T09:34:37Z","abstract":[{"text":"The Sun’s surface hosts varying magnetic activities and rotation rates (from equator to pole), and unique solar weather. Now, a combination of ground and space observations has unveiled a previously undetected magnetized plasma current.","lang":"eng"}],"date_published":"2022-05-18T00:00:00Z","page":"631-632","article_processing_charge":"No","language":[{"iso":"eng"}],"date_updated":"2022-08-19T09:52:21Z","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","keyword":["Astronomy and Astrophysics"],"scopus_import":"1","doi":"10.1038/s41550-022-01683-2","publication_identifier":{"eissn":["2397-3366"]},"day":"18","article_type":"letter_note","year":"2022","oa_version":"None","author":[{"id":"d9edb345-f866-11ec-9b37-d119b5234501","orcid":"0000-0003-0142-4000","full_name":"Bugnet, Lisa Annabelle","first_name":"Lisa Annabelle","last_name":"Bugnet"}],"type":"journal_article","citation":{"chicago":"Bugnet, Lisa Annabelle. “Hidden Currents at the Sun’s Surface.” Nature Astronomy. Springer Nature, 2022. https://doi.org/10.1038/s41550-022-01683-2.","ista":"Bugnet LA. 2022. Hidden currents at the Sun’s surface. Nature Astronomy. 6, 631–632.","ieee":"L. A. Bugnet, “Hidden currents at the Sun’s surface,” Nature Astronomy, vol. 6. Springer Nature, pp. 631–632, 2022.","mla":"Bugnet, Lisa Annabelle. “Hidden Currents at the Sun’s Surface.” Nature Astronomy, vol. 6, Springer Nature, 2022, pp. 631–32, doi:10.1038/s41550-022-01683-2.","short":"L.A. Bugnet, Nature Astronomy 6 (2022) 631–632.","ama":"Bugnet LA. Hidden currents at the Sun’s surface. Nature Astronomy. 2022;6:631-632. doi:10.1038/s41550-022-01683-2","apa":"Bugnet, L. A. (2022). Hidden currents at the Sun’s surface. Nature Astronomy. Springer Nature. https://doi.org/10.1038/s41550-022-01683-2"},"title":"Hidden currents at the Sun’s surface"},{"title":"The K2 Galactic Archaeology Program data release 3: Age-abundance patterns in C1–C8 and C10–C18","citation":{"apa":"Zinn, J. C., Stello, D., Elsworth, Y., García, R. A., Kallinger, T., Mathur, S., … Silva Aguirre, V. (2022). The K2 Galactic Archaeology Program data release 3: Age-abundance patterns in C1–C8 and C10–C18. The Astrophysical Journal. IOP Publishing. https://doi.org/10.3847/1538-4357/ac2c83","ama":"Zinn JC, Stello D, Elsworth Y, et al. The K2 Galactic Archaeology Program data release 3: Age-abundance patterns in C1–C8 and C10–C18. The Astrophysical Journal. 2022;926(2). doi:10.3847/1538-4357/ac2c83","short":"J.C. Zinn, D. Stello, Y. Elsworth, R.A. García, T. Kallinger, S. Mathur, B. Mosser, M. Hon, L.A. Bugnet, C. Jones, C. Reyes, S. Sharma, R. Schönrich, J.T. Warfield, R. Luger, A. Vanderburg, C. Kobayashi, M.H. Pinsonneault, J.A. Johnson, D. Huber, S. Buder, M. Joyce, J. Bland-Hawthorn, L. Casagrande, G.F. Lewis, A. Miglio, T. Nordlander, G.R. Davies, G.D. Silva, W.J. Chaplin, V. Silva Aguirre, The Astrophysical Journal 926 (2022).","mla":"Zinn, Joel C., et al. “The K2 Galactic Archaeology Program Data Release 3: Age-Abundance Patterns in C1–C8 and C10–C18.” The Astrophysical Journal, vol. 926, no. 2, 191, IOP Publishing, 2022, doi:10.3847/1538-4357/ac2c83.","ista":"Zinn JC, Stello D, Elsworth Y, García RA, Kallinger T, Mathur S, Mosser B, Hon M, Bugnet LA, Jones C, Reyes C, Sharma S, Schönrich R, Warfield JT, Luger R, Vanderburg A, Kobayashi C, Pinsonneault MH, Johnson JA, Huber D, Buder S, Joyce M, Bland-Hawthorn J, Casagrande L, Lewis GF, Miglio A, Nordlander T, Davies GR, Silva GD, Chaplin WJ, Silva Aguirre V. 2022. The K2 Galactic Archaeology Program data release 3: Age-abundance patterns in C1–C8 and C10–C18. The Astrophysical Journal. 926(2), 191.","ieee":"J. C. Zinn et al., “The K2 Galactic Archaeology Program data release 3: Age-abundance patterns in C1–C8 and C10–C18,” The Astrophysical Journal, vol. 926, no. 2. IOP Publishing, 2022.","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 3: Age-Abundance Patterns in C1–C8 and C10–C18.” The Astrophysical Journal. IOP Publishing, 2022. https://doi.org/10.3847/1538-4357/ac2c83."},"author":[{"last_name":"Zinn","first_name":"Joel C.","full_name":"Zinn, Joel C."},{"first_name":"Dennis","full_name":"Stello, Dennis","last_name":"Stello"},{"full_name":"Elsworth, Yvonne","first_name":"Yvonne","last_name":"Elsworth"},{"last_name":"García","first_name":"Rafael A.","full_name":"García, Rafael A."},{"last_name":"Kallinger","full_name":"Kallinger, Thomas","first_name":"Thomas"},{"full_name":"Mathur, Savita","first_name":"Savita","last_name":"Mathur"},{"last_name":"Mosser","full_name":"Mosser, Benoît","first_name":"Benoît"},{"first_name":"Marc","full_name":"Hon, Marc","last_name":"Hon"},{"full_name":"Bugnet, Lisa Annabelle","first_name":"Lisa Annabelle","last_name":"Bugnet","id":"d9edb345-f866-11ec-9b37-d119b5234501","orcid":"0000-0003-0142-4000"},{"first_name":"Caitlin","full_name":"Jones, Caitlin","last_name":"Jones"},{"last_name":"Reyes","first_name":"Claudia","full_name":"Reyes, Claudia"},{"last_name":"Sharma","full_name":"Sharma, Sanjib","first_name":"Sanjib"},{"full_name":"Schönrich, Ralph","first_name":"Ralph","last_name":"Schönrich"},{"last_name":"Warfield","full_name":"Warfield, Jack T.","first_name":"Jack T."},{"full_name":"Luger, Rodrigo","first_name":"Rodrigo","last_name":"Luger"},{"last_name":"Vanderburg","full_name":"Vanderburg, Andrew","first_name":"Andrew"},{"first_name":"Chiaki","full_name":"Kobayashi, Chiaki","last_name":"Kobayashi"},{"last_name":"Pinsonneault","first_name":"Marc H.","full_name":"Pinsonneault, Marc H."},{"last_name":"Johnson","full_name":"Johnson, Jennifer A.","first_name":"Jennifer A."},{"last_name":"Huber","first_name":"Daniel","full_name":"Huber, Daniel"},{"full_name":"Buder, Sven","first_name":"Sven","last_name":"Buder"},{"last_name":"Joyce","first_name":"Meridith","full_name":"Joyce, Meridith"},{"first_name":"Joss","full_name":"Bland-Hawthorn, Joss","last_name":"Bland-Hawthorn"},{"last_name":"Casagrande","full_name":"Casagrande, Luca","first_name":"Luca"},{"full_name":"Lewis, Geraint F.","first_name":"Geraint F.","last_name":"Lewis"},{"last_name":"Miglio","full_name":"Miglio, Andrea","first_name":"Andrea"},{"last_name":"Nordlander","full_name":"Nordlander, Thomas","first_name":"Thomas"},{"last_name":"Davies","first_name":"Guy R.","full_name":"Davies, Guy R."},{"last_name":"Silva","full_name":"Silva, Gayandhi De","first_name":"Gayandhi De"},{"first_name":"William J.","full_name":"Chaplin, William J.","last_name":"Chaplin"},{"last_name":"Silva Aguirre","first_name":"Victor","full_name":"Silva Aguirre, Victor"}],"type":"journal_article","day":"24","acknowledgement":"We would like to thank the anonymous referee whose comments significantly improved the manuscript. J.C.Z. is supported by an NSF Astronomy and Astrophysics Postdoctoral Fellowship under award AST-2001869. 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. acknowledges support from the Spanish Ministry of Science and Innovation with the Ramon y Cajal fellowship number RYC-2015-17697 and the grant number PID2019-107187GB-I00. R.A.G. acknowledges funding received from the PLATO CNES grant. C.K. acknowledges funding from the UK Science and Technology Facilities Council (STFC) through grants ST/M000958/1, ST/R000905/1, and ST/V000632/1.\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. This 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 paper includes data collected by the Kepler mission. Funding for the Kepler mission is provided by the NASA Science Mission directorate.\r\n\r\nParts of this research were supported by the Australian Research Council Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D), through project number CE170100013.\r\n\r\nThis research was partially conducted during the Exostar19 program at the Kavli Institute for Theoretical Physics at UC Santa Barbara, which was supported in part by the National Science Foundation under grant No. NSF PHY-1748958.\r\n\r\nBased in part on data obtained at Siding Spring Observatory via GALAH. We acknowledge the traditional owners of the land on which the AAT stands, the Gamilaraay people, and pay our respects to elders past and present.\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 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 (www.sdss.org).\r\n\r\nSoftware: asfgrid (Sharma & Stello 2016), corner (Foreman-Mackey 2016), emcee (Foreman-Mackey et al. 2013), NumPy (Walt 2011), pandas (McKinney 2010), Matplotlib (Hunter 2007), IPython (Pérez & Granger 2007), SciPy (Virtanen et al.2020).","doi":"10.3847/1538-4357/ac2c83","keyword":["Space and Planetary Science","Astronomy and Astrophysics"],"language":[{"iso":"eng"}],"date_created":"2022-07-18T10:57:30Z","month":"02","extern":"1","publisher":"IOP Publishing","intvolume":" 926","status":"public","publication":"The Astrophysical Journal","quality_controlled":"1","year":"2022","oa_version":"Preprint","article_type":"original","publication_identifier":{"issn":["0004-637X"],"eissn":["1538-4357"]},"scopus_import":"1","external_id":{"arxiv":["2108.05455"]},"date_updated":"2022-08-19T09:52:08Z","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","article_processing_charge":"No","issue":"2","arxiv":1,"_id":"11601","abstract":[{"text":"We present the third and final data release of the K2 Galactic Archaeology Program (K2 GAP) for Campaigns C1–C8 and C10–C18. We provide asteroseismic radius and mass coefficients, κR and κM, for ∼19,000 red giant stars, which translate directly to radius and mass given a temperature. As such, K2 GAP DR3 represents the largest asteroseismic sample in the literature to date. K2 GAP DR3 stellar parameters are calibrated to be on an absolute parallactic scale based on Gaia DR2, with red giant branch and red clump evolutionary state classifications provided via a machine-learning approach. Combining these stellar parameters with GALAH DR3 spectroscopy, we determine asteroseismic ages with precisions of ∼20%–30% and compare age-abundance relations to Galactic chemical evolution models among both low- and high-α populations for α, light, iron-peak, and neutron-capture elements. We confirm recent indications in the literature of both increased Ba production at late Galactic times as well as significant contributions to r-process enrichment from prompt sources associated with, e.g., core-collapse supernovae. With an eye toward other Galactic archeology applications, we characterize K2 GAP DR3 uncertainties and completeness using injection tests, suggesting that K2 GAP DR3 is largely unbiased in mass/age, with uncertainties of 2.9% (stat.) ± 0.1% (syst.) and 6.7% (stat.) ± 0.3% (syst.) in κR and κM for red giant branch stars and 4.7% (stat.) ± 0.3% (syst.) and 11% (stat.) ± 0.9% (syst.) for red clump stars. We also identify percent-level asteroseismic systematics, which are likely related to the time baseline of the underlying data, and which therefore should be considered in TESS asteroseismic analysis.","lang":"eng"}],"date_published":"2022-02-24T00:00:00Z","article_number":"191","main_file_link":[{"open_access":"1","url":"https://arxiv.org/abs/2108.05455"}],"oa":1,"publication_status":"published","volume":926}]