[{"month":"07","quality_controlled":"1","publication_identifier":{"eissn":["1538-4357"],"issn":["0004-637X"]},"volume":808,"article_type":"original","date_created":"2022-07-07T09:00:58Z","acknowledgement":"We thank the anonymous reviewer for useful and constructive comments and suggestions which greatly improved the quality and clarity of our work. D.S. acknowledges financial support from the Netherlands Organisation for Scientific research (NWO) through a Veni fellowship, from FCT through a FCT Investigator Starting Grant and Start-up Grant (IF/01154/2012/CP0189/CT0010), from FCT grant UID/FIS/04434/2013, and from LSF and LKBF. J.M. acknowledges the award of a Huygens PhD fellowship. H.R. acknowledges support from the ERC Advanced Investigator program NewClusters 321271. The authors thank Mark Dijkstra, Bhaskar Agarwal, Jarrett Johnson, Andrea Ferrara, Jarle Brinchmann, Rebecca Bowler, George Becker, Emma Curtis-Lake, Milos Milosavljevic, Raffaella Schneider, Paul Shapiro, and Erik Zackrisson for interesting, stimulating and helpful discussions. The authors are extremely grateful to ESO for the award of ESO DDT time (294.A-5018 and 294.A-5039) which allowed the spectroscopic confirmation of both sources and the detailed investigation of their nature. Observations are also based on data from W.M. Keck Observatory. The W.M. Keck Observatory is operated as a scientific partnership of Caltech, the University of California and the National Aeronautics and Space Administration. Based on observations obtained with MegaPrime/Megacam, a joint project of CFHT and CEA/IRFU, at the Canada–France–Hawaii Telescope (CFHT) which is operated by the National Research Council (NRC) of Canada, the Institut National des Science de lUnivers of the Centre National de la Recherche Scientifique (CNRS) of France, and the University of Hawaii. This work is based in part on data products produced at Terapix available at the Canadian Astronomy Data Centre as part of the Canada–France–Hawaii Telescope Legacy Survey, a collaborative project of NRC and CNRS. Based on data products from observations made with ESO Telescopes at the La Silla Paranal Observatory under ESO programme IDs 294.A-5018, 294.A-5039, and 179.A-2005, and on data products produced by TERAPIX and the Cambridge Astronomy Survey Unit on behalf of the UltraVISTA consortium. The authors acknowledge the award of service time (SW2014b20) on the William Herschel Telescope (WHT). WHT and its service programme are operated on the island of La Palma by the Isaac Newton Group in the Spanish Observatorio del Roque de los Muchachos of the Instituto de Astrofisica de Canarias.","extern":"1","article_processing_charge":"No","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","keyword":["Space and Planetary Science","Astronomy and Astrophysics","dark ages","reionization","first stars – early universe – galaxies: evolution"],"intvolume":"       808","author":[{"first_name":"David","full_name":"Sobral, David","last_name":"Sobral"},{"full_name":"Matthee, Jorryt J","first_name":"Jorryt J","id":"7439a258-f3c0-11ec-9501-9df22fe06720","last_name":"Matthee","orcid":"0000-0003-2871-127X"},{"last_name":"Darvish","first_name":"Behnam","full_name":"Darvish, Behnam"},{"full_name":"Schaerer, Daniel","first_name":"Daniel","last_name":"Schaerer"},{"full_name":"Mobasher, Bahram","first_name":"Bahram","last_name":"Mobasher"},{"first_name":"Huub","full_name":"Röttgering, Huub","last_name":"Röttgering"},{"full_name":"Santos, Sérgio","first_name":"Sérgio","last_name":"Santos"},{"last_name":"Hemmati","full_name":"Hemmati, Shoubaneh","first_name":"Shoubaneh"}],"oa":1,"_id":"11519","date_published":"2015-07-28T00:00:00Z","language":[{"iso":"eng"}],"doi":"10.1088/0004-637X/808/2/139","publisher":"IOP Publishing","year":"2015","type":"journal_article","main_file_link":[{"url":"https://arxiv.org/abs/1504.01734","open_access":"1"}],"publication":"The Astrophysical Journal","external_id":{"arxiv":["1504.01734"]},"title":"Evidence for PopIII-like stellar populations in the most luminous Lyα emitters at the epoch of reionisation: Spectroscopic confirmation","citation":{"ista":"Sobral D, Matthee JJ, Darvish B, Schaerer D, Mobasher B, Röttgering H, Santos S, Hemmati S. 2015. Evidence for PopIII-like stellar populations in the most luminous Lyα emitters at the epoch of reionisation: Spectroscopic confirmation. The Astrophysical Journal. 808(2), 139.","apa":"Sobral, D., Matthee, J. J., Darvish, B., Schaerer, D., Mobasher, B., Röttgering, H., … Hemmati, S. (2015). Evidence for PopIII-like stellar populations in the most luminous Lyα emitters at the epoch of reionisation: Spectroscopic confirmation. <i>The Astrophysical Journal</i>. IOP Publishing. <a href=\"https://doi.org/10.1088/0004-637X/808/2/139\">https://doi.org/10.1088/0004-637X/808/2/139</a>","short":"D. Sobral, J.J. Matthee, B. Darvish, D. Schaerer, B. Mobasher, H. Röttgering, S. Santos, S. Hemmati, The Astrophysical Journal 808 (2015) 139.","mla":"Sobral, David, et al. “Evidence for PopIII-like Stellar Populations in the Most Luminous Lyα Emitters at the Epoch of Reionisation: Spectroscopic Confirmation.” <i>The Astrophysical Journal</i>, vol. 808, no. 2, IOP Publishing, 2015, p. 139, doi:<a href=\"https://doi.org/10.1088/0004-637X/808/2/139\">10.1088/0004-637X/808/2/139</a>.","ama":"Sobral D, Matthee JJ, Darvish B, et al. Evidence for PopIII-like stellar populations in the most luminous Lyα emitters at the epoch of reionisation: Spectroscopic confirmation. <i>The Astrophysical Journal</i>. 2015;808(2):139. doi:<a href=\"https://doi.org/10.1088/0004-637X/808/2/139\">10.1088/0004-637X/808/2/139</a>","chicago":"Sobral, David, Jorryt J Matthee, Behnam Darvish, Daniel Schaerer, Bahram Mobasher, Huub Röttgering, Sérgio Santos, and Shoubaneh Hemmati. “Evidence for PopIII-like Stellar Populations in the Most Luminous Lyα Emitters at the Epoch of Reionisation: Spectroscopic Confirmation.” <i>The Astrophysical Journal</i>. IOP Publishing, 2015. <a href=\"https://doi.org/10.1088/0004-637X/808/2/139\">https://doi.org/10.1088/0004-637X/808/2/139</a>.","ieee":"D. Sobral <i>et al.</i>, “Evidence for PopIII-like stellar populations in the most luminous Lyα emitters at the epoch of reionisation: Spectroscopic confirmation,” <i>The Astrophysical Journal</i>, vol. 808, no. 2. IOP Publishing, p. 139, 2015."},"arxiv":1,"issue":"2","scopus_import":"1","publication_status":"published","oa_version":"Preprint","page":"139","day":"28","abstract":[{"text":"Faint Lyα emitters become increasingly rarer toward the reionization epoch (z ∼ 6–7). However, observations from a very large (∼5 deg2) Lyα narrow-band survey at z = 6.6 show that this is not the case for the most luminous emitters, capable of ionizing their own local bubbles. Here we present follow-up observations of the two most luminous Lyα candidates in the COSMOS field: “MASOSA” and “CR7.” We used X-SHOOTER, SINFONI, and FORS2 on the Very Large Telescope, and DEIMOS on Keck, to confirm both candidates beyond any doubt. We find redshifts of z = 6.541 and z = 6.604 for “MASOSA” and “CR7,” respectively. MASOSA has a strong detection in Lyα with a line width of 386 ± 30 km s−1 (FWHM) and with very high EW0 (>200 Å), but undetected in the continuum, implying very low stellar mass and a likely young, metal-poor stellar population. “CR7,” with an observed Lyα luminosity of 1043.92±0.05 erg s−1 is the most luminous Lyα emitter ever found at z > 6 and is spatially extended (∼16 kpc). “CR7” reveals a narrow Lyα line with 266 ± 15 km s−1 FWHM, being detected in the near-infrared (NIR) (rest-frame UV; β = −2.3 ± 0.1) and in IRAC/Spitzer. We detect a narrow He II 1640 Å emission line (6σ, FWHM = 130 ± 30 km s−1 ) in CR7 which can explain the clear excess seen in the J-band photometry (EW0 ∼ 80 Å). We find no other emission lines from the UV to the NIR in our X-SHOOTER spectra (He II/O III] 1663 Å > 3 and He II/C III] 1908 Å > 2.5). We conclude that CR7 is best explained by a combination of a PopIII-like population, which dominates the rest-frame UV and the nebular emission, and a more normal stellar population, which presumably dominates the mass. Hubble Space Telescope/WFC3 observations show that the light is indeed spatially separated between a very blue component, coincident with Lyα and He II emission, and two red components (∼5 kpc away), which dominate the mass. Our findings are consistent with theoretical predictions of a PopIII wave, with PopIII star formation migrating away from the original sites of star formation.","lang":"eng"}],"date_updated":"2022-08-18T10:30:13Z","status":"public"},{"scopus_import":"1","issue":"3","citation":{"ama":"Sobral D, Matthee JJ, Best PN, et al. CF-HiZELS, an ∼10 deg2 emission-line survey with spectroscopic follow-up: Hα, [O III] + Hβ and [O II] luminosity functions at z = 0.8, 1.4 and 2.2 . <i>Monthly Notices of the Royal Astronomical Society</i>. 2015;451(3):2303-2323. doi:<a href=\"https://doi.org/10.1093/mnras/stv1076\">10.1093/mnras/stv1076</a>","apa":"Sobral, D., Matthee, J. J., Best, P. N., Smail, I., Khostovan, A. A., Milvang-Jensen, B., … Mobasher, B. (2015). CF-HiZELS, an ∼10 deg2 emission-line survey with spectroscopic follow-up: Hα, [O III] + Hβ and [O II] luminosity functions at z = 0.8, 1.4 and 2.2 . <i>Monthly Notices of the Royal Astronomical Society</i>. Oxford University Press. <a href=\"https://doi.org/10.1093/mnras/stv1076\">https://doi.org/10.1093/mnras/stv1076</a>","mla":"Sobral, D., et al. “CF-HiZELS, an ∼10 Deg2 Emission-Line Survey with Spectroscopic Follow-up: Hα, [O III] + Hβ and [O II] Luminosity Functions at z = 0.8, 1.4 and 2.2 .” <i>Monthly Notices of the Royal Astronomical Society</i>, vol. 451, no. 3, Oxford University Press, 2015, pp. 2303–23, doi:<a href=\"https://doi.org/10.1093/mnras/stv1076\">10.1093/mnras/stv1076</a>.","short":"D. Sobral, J.J. Matthee, P.N. Best, I. Smail, A.A. Khostovan, B. Milvang-Jensen, J.-W. Kim, J. Stott, J. Calhau, H. Nayyeri, B. Mobasher, Monthly Notices of the Royal Astronomical Society 451 (2015) 2303–2323.","ista":"Sobral D, Matthee JJ, Best PN, Smail I, Khostovan AA, Milvang-Jensen B, Kim J-W, Stott J, Calhau J, Nayyeri H, Mobasher B. 2015. CF-HiZELS, an ∼10 deg2 emission-line survey with spectroscopic follow-up: Hα, [O III] + Hβ and [O II] luminosity functions at z = 0.8, 1.4 and 2.2 . Monthly Notices of the Royal Astronomical Society. 451(3), 2303–2323.","ieee":"D. Sobral <i>et al.</i>, “CF-HiZELS, an ∼10 deg2 emission-line survey with spectroscopic follow-up: Hα, [O III] + Hβ and [O II] luminosity functions at z = 0.8, 1.4 and 2.2 ,” <i>Monthly Notices of the Royal Astronomical Society</i>, vol. 451, no. 3. Oxford University Press, pp. 2303–2323, 2015.","chicago":"Sobral, D., Jorryt J Matthee, P. N. Best, I. Smail, A. A. Khostovan, B. Milvang-Jensen, J.-W. Kim, et al. “CF-HiZELS, an ∼10 Deg2 Emission-Line Survey with Spectroscopic Follow-up: Hα, [O III] + Hβ and [O II] Luminosity Functions at z = 0.8, 1.4 and 2.2 .” <i>Monthly Notices of the Royal Astronomical Society</i>. Oxford University Press, 2015. <a href=\"https://doi.org/10.1093/mnras/stv1076\">https://doi.org/10.1093/mnras/stv1076</a>."},"arxiv":1,"title":"CF-HiZELS, an ∼10 deg2 emission-line survey with spectroscopic follow-up: Hα, [O III] + Hβ and [O II] luminosity functions at z = 0.8, 1.4 and 2.2 ","external_id":{"arxiv":["1502.06602"]},"publication":"Monthly Notices of the Royal Astronomical Society","main_file_link":[{"url":"https://arxiv.org/abs/1502.06602","open_access":"1"}],"status":"public","date_updated":"2022-08-19T08:23:18Z","abstract":[{"lang":"eng","text":"We present results from the largest contiguous narrow-band survey in the near-infrared. We have used the wide-field infrared camera/Canada–France–Hawaii Telescope and the lowOH2 filter (1.187 ± 0.005 μm) to survey ≈10 deg2 of contiguous extragalactic sky in the SA22 field. A total of ∼6000 candidate emission-line galaxies are found. We use deep ugrizJK data to obtain robust photometric redshifts. We combine our data with the High-redshift(Z) Emission Line Survey (HiZELS), explore spectroscopic surveys (VVDS, VIPERS) and obtain our own spectroscopic follow-up with KMOS, FMOS and MOSFIRE to derive large samples of high-redshift emission-line selected galaxies: 3471 Hα emitters at z = 0.8, 1343 [O III] + Hβ emitters at z = 1.4 and 572 [O II] emitters at z = 2.2. We probe comoving volumes of >106 Mpc3 and find significant overdensities, including an 8.5σ (spectroscopically confirmed) overdensity of Hα emitters at z = 0.81. We derive Hα, [O III] + Hβ and [O II] luminosity functions at z = 0.8, 1.4, 2.2, respectively, and present implications for future surveys such as Euclid. Our uniquely large volumes/areas allow us to subdivide the samples in thousands of randomized combinations of areas and provide a robust empirical measurement of sample/cosmic variance. We show that surveys for star-forming/emission-line galaxies at a depth similar to ours can only overcome cosmic-variance (errors <10 per cent) if they are based on volumes >5 × 105 Mpc3; errors on L* and ϕ* due to sample (cosmic) variance on surveys probing ∼104 and ∼105 Mpc3 are typically very high: ∼300 and ∼40–60 per cent, respectively."}],"day":"11","page":"2303-2323","publication_status":"published","oa_version":"Preprint","intvolume":"       451","keyword":["Space and Planetary Science","Astronomy and Astrophysics","galaxies: evolution","galaxies: formation","galaxies: luminosity function","mass function","cosmology: observations","early Universe","large-scale structure of Universe"],"user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","extern":"1","article_processing_charge":"No","acknowledgement":"The authors wish to thank the anonymous reviewer for many helpful comments and suggestions which greatly improved the clarity and quality of this work. DS acknowledges financial support from the Netherlands Organization for Scientific research (NWO) through a Veni fellowship, from FCT through an FCT Investigator Starting Grant and Start-up Grant (IF/01154/2012/CP0189/CT0010), from FCT grant PEst-OE/FIS/UI2751/2014, and from LSF and LKBF. JM acknowledges the award of a Huygens PhD fellowship. PNB is grateful for support from STFC. IRS acknowledges support from STFC, a Leverhulme Fellowship, the ERC Advanced Investigator programme DUSTYGAL and a Royal Society/Wolfson Merit Award. BMJ acknowledges support from the ERC-StG grant EGGS-278202. The Dark Cosmology Centre is funded by the DNRF. The Dark Cosmology Centre is funded by the DNRF. JWK acknowledges support from the National Research Foundation of Korea (NRF) grant, no. 2008-0060544, funded by the Korea government (MSIP). JPS acknowledges support from STFC (ST/I001573/1). JC acknowledges support from the FCT-IF grant IF/01154/2012/CP0189/CT0010. The work was only possible due to OPTICON/FP7 and the invaluable access that it granted to the CFHT telescope. We would also like to acknowledge the excellent work done by CFHT staff in conducting the observations in service mode, and on delivering truly excellent data. We are also tremendously thankful to Kentaro Aoki for the incredible support while observing at Subaru with FMOS, and also to the Keck staff for the help with the observations with MOSFIRE. This work is based on observations obtained with WIRCam on the CFHT, OPTICON programme 2011B/029, 2012A019 and 2012B/016. Based on observations made with ESO telescopes at the La Silla Paranal Observatory under programmes IDs 60.A-9460 (data can be accessed through the ESO data archive), 087.A 0337 and 089.A-0965. Based on observations done with FMOS on Subaru under programme S14A-084, and on MOSFIRE/Keck observations under programme U066M. Part of the data on which this analysis is based are available from Sobral et al. (2013a). Dedicated to the memory of C. M. Sobral (1953-2014).","date_created":"2022-07-14T09:02:22Z","volume":451,"article_type":"original","publication_identifier":{"issn":["0035-8711"],"eissn":["1365-2966"]},"quality_controlled":"1","month":"08","type":"journal_article","year":"2015","publisher":"Oxford University Press","doi":"10.1093/mnras/stv1076","language":[{"iso":"eng"}],"date_published":"2015-08-11T00:00:00Z","_id":"11580","oa":1,"author":[{"full_name":"Sobral, D.","first_name":"D.","last_name":"Sobral"},{"full_name":"Matthee, Jorryt J","first_name":"Jorryt J","orcid":"0000-0003-2871-127X","id":"7439a258-f3c0-11ec-9501-9df22fe06720","last_name":"Matthee"},{"last_name":"Best","full_name":"Best, P. N.","first_name":"P. N."},{"last_name":"Smail","first_name":"I.","full_name":"Smail, I."},{"full_name":"Khostovan, A. A.","first_name":"A. A.","last_name":"Khostovan"},{"full_name":"Milvang-Jensen, B.","first_name":"B.","last_name":"Milvang-Jensen"},{"first_name":"J.-W.","full_name":"Kim, J.-W.","last_name":"Kim"},{"first_name":"J.","full_name":"Stott, J.","last_name":"Stott"},{"last_name":"Calhau","full_name":"Calhau, J.","first_name":"J."},{"full_name":"Nayyeri, H.","first_name":"H.","last_name":"Nayyeri"},{"last_name":"Mobasher","first_name":"B.","full_name":"Mobasher, B."}]},{"citation":{"chicago":"Stott, John P., David Sobral, A. M. Swinbank, Ian Smail, Richard Bower, Philip N. Best, Ray M. Sharples, James E. Geach, and Jorryt J Matthee. “A Relationship between Specific Star Formation Rate and Metallicity Gradient within z ∼ 1 Galaxies from KMOS-HiZELS.” <i>Monthly Notices of the Royal Astronomical Society</i>. Oxford University Press, 2014. <a href=\"https://doi.org/10.1093/mnras/stu1343\">https://doi.org/10.1093/mnras/stu1343</a>.","ieee":"J. P. Stott <i>et al.</i>, “A relationship between specific star formation rate and metallicity gradient within z ∼ 1 galaxies from KMOS-HiZELS,” <i>Monthly Notices of the Royal Astronomical Society</i>, vol. 443, no. 3. Oxford University Press, pp. 2695–2704, 2014.","apa":"Stott, J. P., Sobral, D., Swinbank, A. M., Smail, I., Bower, R., Best, P. N., … Matthee, J. J. (2014). A relationship between specific star formation rate and metallicity gradient within z ∼ 1 galaxies from KMOS-HiZELS. <i>Monthly Notices of the Royal Astronomical Society</i>. Oxford University Press. <a href=\"https://doi.org/10.1093/mnras/stu1343\">https://doi.org/10.1093/mnras/stu1343</a>","ista":"Stott JP, Sobral D, Swinbank AM, Smail I, Bower R, Best PN, Sharples RM, Geach JE, Matthee JJ. 2014. A relationship between specific star formation rate and metallicity gradient within z ∼ 1 galaxies from KMOS-HiZELS. Monthly Notices of the Royal Astronomical Society. 443(3), 2695–2704.","short":"J.P. Stott, D. Sobral, A.M. Swinbank, I. Smail, R. Bower, P.N. Best, R.M. Sharples, J.E. Geach, J.J. Matthee, Monthly Notices of the Royal Astronomical Society 443 (2014) 2695–2704.","mla":"Stott, John P., et al. “A Relationship between Specific Star Formation Rate and Metallicity Gradient within z ∼ 1 Galaxies from KMOS-HiZELS.” <i>Monthly Notices of the Royal Astronomical Society</i>, vol. 443, no. 3, Oxford University Press, 2014, pp. 2695–704, doi:<a href=\"https://doi.org/10.1093/mnras/stu1343\">10.1093/mnras/stu1343</a>.","ama":"Stott JP, Sobral D, Swinbank AM, et al. A relationship between specific star formation rate and metallicity gradient within z ∼ 1 galaxies from KMOS-HiZELS. <i>Monthly Notices of the Royal Astronomical Society</i>. 2014;443(3):2695-2704. doi:<a href=\"https://doi.org/10.1093/mnras/stu1343\">10.1093/mnras/stu1343</a>"},"arxiv":1,"issue":"3","scopus_import":"1","main_file_link":[{"url":"https://arxiv.org/abs/1407.1047","open_access":"1"}],"external_id":{"arxiv":["1407.1047"]},"title":"A relationship between specific star formation rate and metallicity gradient within z ∼ 1 galaxies from KMOS-HiZELS","publication":"Monthly Notices of the Royal Astronomical Society","date_updated":"2022-08-19T08:27:25Z","status":"public","abstract":[{"lang":"eng","text":"We have observed a sample of typical z ∼ 1 star-forming galaxies, selected from the HiZELS survey, with the new K-band Multi-Object Spectrograph (KMOS) near-infrared, multi-integral field unit instrument on the Very Large Telescope (VLT), in order to obtain their dynamics and metallicity gradients. The majority of our galaxies have a metallicity gradient consistent with being flat or negative (i.e. higher metallicity cores than outskirts). Intriguingly, we find a trend between metallicity gradient and specific star formation rate (sSFR), such that galaxies with a high sSFR tend to have relatively metal poor centres, a result which is strengthened when combined with data sets from the literature. This result appears to explain the discrepancies reported between different high-redshift studies and varying claims for evolution. From a galaxy evolution perspective, the trend we see would mean that a galaxy's sSFR is governed by the amount of metal-poor gas that can be funnelled into its core, triggered either by merging or through efficient accretion. In fact, merging may play a significant role as it is the starburst galaxies at all epochs, which have the more positive metallicity gradients. Our results may help to explain the origin of the fundamental metallicity relation, in which galaxies at a fixed mass are observed to have lower metallicities at higher star formation rates, especially if the metallicity is measured in an aperture encompassing only the central regions of the galaxy. Finally, we note that this study demonstrates the power of KMOS as an efficient instrument for large-scale resolved galaxy surveys."}],"publication_status":"published","page":"2695-2704","oa_version":"Preprint","day":"21","acknowledgement":"First, we acknowledge the referee for their comments, which have improved the clarity of this paper. JPS and IRS acknowledge support from STFC (ST/I001573/1). IRS also acknowledges support from the ERC Advanced Investigator programme DUSTYGAL and a Royal Society/Wolfson Merit Award. DS acknowledges financial support from NWO through a Veni fellowship and from FCT through the award of an FCT-IF starting grant. PNB acknowledges STFC for financial support.","date_created":"2022-07-14T12:16:10Z","keyword":["Space and Planetary Science","Astronomy and Astrophysics","galaxies: abundances","galaxies: evolution","galaxies: kinematics and dynamics"],"intvolume":"       443","extern":"1","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","article_processing_charge":"No","quality_controlled":"1","publication_identifier":{"eissn":["1365-2966"],"issn":["0035-8711"]},"month":"09","volume":443,"article_type":"original","publisher":"Oxford University Press","year":"2014","language":[{"iso":"eng"}],"doi":"10.1093/mnras/stu1343","type":"journal_article","oa":1,"_id":"11582","author":[{"last_name":"Stott","full_name":"Stott, John P.","first_name":"John P."},{"full_name":"Sobral, David","first_name":"David","last_name":"Sobral"},{"first_name":"A. M.","full_name":"Swinbank, A. M.","last_name":"Swinbank"},{"first_name":"Ian","full_name":"Smail, Ian","last_name":"Smail"},{"last_name":"Bower","full_name":"Bower, Richard","first_name":"Richard"},{"full_name":"Best, Philip N.","first_name":"Philip N.","last_name":"Best"},{"last_name":"Sharples","first_name":"Ray M.","full_name":"Sharples, Ray M."},{"full_name":"Geach, James E.","first_name":"James E.","last_name":"Geach"},{"orcid":"0000-0003-2871-127X","last_name":"Matthee","id":"7439a258-f3c0-11ec-9501-9df22fe06720","first_name":"Jorryt J","full_name":"Matthee, Jorryt J"}],"date_published":"2014-09-21T00:00:00Z"},{"publication":"Monthly Notices of the Royal Astronomical Society","external_id":{"arxiv":["1402.6697"]},"title":"A 10 deg2 Lyman α survey at z=8.8 with spectroscopic follow-up: Strong constraints on the luminosity function and implications for other surveys","main_file_link":[{"open_access":"1","url":"https://arxiv.org/abs/1402.6697"}],"issue":"3","scopus_import":"1","arxiv":1,"citation":{"apa":"Matthee, J. J., Sobral, D., Swinbank, A. M., Smail, I., Best, P. N., Kim, J.-W., … Fynbo, J. (2014). A 10 deg2 Lyman α survey at z=8.8 with spectroscopic follow-up: Strong constraints on the luminosity function and implications for other surveys. <i>Monthly Notices of the Royal Astronomical Society</i>. Oxford University Press. <a href=\"https://doi.org/10.1093/mnras/stu392\">https://doi.org/10.1093/mnras/stu392</a>","short":"J.J. Matthee, D. Sobral, A.M. Swinbank, I. Smail, P.N. Best, J.-W. Kim, M. Franx, B. Milvang-Jensen, J. Fynbo, Monthly Notices of the Royal Astronomical Society 440 (2014) 2375–2387.","ista":"Matthee JJ, Sobral D, Swinbank AM, Smail I, Best PN, Kim J-W, Franx M, Milvang-Jensen B, Fynbo J. 2014. A 10 deg2 Lyman α survey at z=8.8 with spectroscopic follow-up: Strong constraints on the luminosity function and implications for other surveys. Monthly Notices of the Royal Astronomical Society. 440(3), 2375–2387.","mla":"Matthee, Jorryt J., et al. “A 10 Deg2 Lyman α Survey at Z=8.8 with Spectroscopic Follow-up: Strong Constraints on the Luminosity Function and Implications for Other Surveys.” <i>Monthly Notices of the Royal Astronomical Society</i>, vol. 440, no. 3, Oxford University Press, 2014, pp. 2375–87, doi:<a href=\"https://doi.org/10.1093/mnras/stu392\">10.1093/mnras/stu392</a>.","ama":"Matthee JJ, Sobral D, Swinbank AM, et al. A 10 deg2 Lyman α survey at z=8.8 with spectroscopic follow-up: Strong constraints on the luminosity function and implications for other surveys. <i>Monthly Notices of the Royal Astronomical Society</i>. 2014;440(3):2375-2387. doi:<a href=\"https://doi.org/10.1093/mnras/stu392\">10.1093/mnras/stu392</a>","chicago":"Matthee, Jorryt J, David Sobral, A. M. Swinbank, Ian Smail, P. N. Best, Jae-Woo Kim, Marijn Franx, Bo Milvang-Jensen, and Johan Fynbo. “A 10 Deg2 Lyman α Survey at Z=8.8 with Spectroscopic Follow-up: Strong Constraints on the Luminosity Function and Implications for Other Surveys.” <i>Monthly Notices of the Royal Astronomical Society</i>. Oxford University Press, 2014. <a href=\"https://doi.org/10.1093/mnras/stu392\">https://doi.org/10.1093/mnras/stu392</a>.","ieee":"J. J. Matthee <i>et al.</i>, “A 10 deg2 Lyman α survey at z=8.8 with spectroscopic follow-up: Strong constraints on the luminosity function and implications for other surveys,” <i>Monthly Notices of the Royal Astronomical Society</i>, vol. 440, no. 3. Oxford University Press, pp. 2375–2387, 2014."},"page":"2375-2387","oa_version":"Preprint","publication_status":"published","day":"21","abstract":[{"text":"Candidate galaxies at redshifts of z ∼ 10 are now being found in extremely deep surveys, probing very small areas. As a consequence, candidates are very faint, making spectroscopic confirmation practically impossible. In order to overcome such limitations, we have undertaken the CF-HiZELS survey, which is a large-area, medium-depth near-infrared narrow-band survey targeted at z = 8.8 Lyman α (Lyα) emitters (LAEs) and covering 10 deg2 in part of the SSA22 field with the Canada–France–Hawaii Telescope (CFHT). We surveyed a comoving volume of 4.7 × 106 Mpc3 to a Lyα luminosity limit of 6.3 × 1043舁erg舁s−1. We look for Lyα candidates by applying the following criteria: (i) clear emission-line source, (ii) no optical detections (ugriz from CFHTLS), (iii) no visible detection in the optical stack (ugriz > 27), (iv) visually checked reliable NBJ and J detections and (v) J − K ≤ 0. We compute photometric redshifts and remove a significant amount of dusty lower redshift line-emitters at z ∼ 1.4 or 2.2. A total of 13 Lyα candidates were found, of which two are marked as strong candidates, but the majority have very weak constraints on their spectral energy distributions. Using follow-up observations with SINFONI/VLT, we are able to exclude the most robust candidates as LAEs. We put a strong constraint on the Lyα luminosity function at z ∼ 9 and make realistic predictions for ongoing and future surveys. Our results show that surveys for the highest redshift LAEs are susceptible of multiple contaminations and that spectroscopic follow-up is absolutely necessary.","lang":"eng"}],"status":"public","date_updated":"2022-08-19T08:30:30Z","volume":440,"article_type":"original","month":"05","quality_controlled":"1","publication_identifier":{"eissn":["1365-2966"],"issn":["0035-8711"]},"user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","article_processing_charge":"No","extern":"1","keyword":["Space and Planetary Science","Astronomy and Astrophysics","galaxies: evolution","galaxies: high-redshift","cosmology: observations","dark ages","reionization","first stars"],"intvolume":"       440","date_created":"2022-07-14T12:33:24Z","acknowledgement":"We thank the anonymous referee for the comments and suggestions which improved both the quality and clarity of this work. DS acknowledges financial support from the Netherlands Organisation for Scientific Research (NWO) through a Veni fellowship. IRS acknowledges support from STFC (ST/I001573/1), a Leverhulme Fellowship, the ERC Advanced Investigator programme DUSTYGAL 321334 and a Royal Society/Wolfson Merit Award. PNB acknowledges support from the Leverhulme Trust. JWK acknowledges the support from the Creative Research Initiative Program, no. 2008- 0060544, of the National Research Foundation of Korea (NRF) funded by the Korean government (MSIP). JPUF and BMJ acknowledge support from the ERC-StG grant EGGS-278202. The Dark Cosmology Centre is funded by the Danish National Research Foundation. This work is based in part on data obtained as part of the UKIRT Infrared Deep Sky Survey. Based on observations obtained with MegaPrime/MegaCam, a joint project of CFHT and CEA/IRFU, at the Canada–France–Hawaii Telescope (CFHT) which is operated by the National Research Council (NRC) of Canada, the Institut National des Science de l’Univers of the Centre National de la Recherche Scientifique (CNRS) of France and the University of Hawaii. This work is based in part on data products produced at Terapix available at the Canadian Astronomy Data Centre as part of the Canada-France-Hawaii Telescope Legacy Survey, a collaborative project of NRC and CNRS. This work was only possible due to OPTICON/FP7 and the access that it granted to the CFHT telescope. The authors also wish to acknowledge the CFHTLS and UKIDSS surveys for their excellent legacy and complementary value – without such high-quality data sets, this research would not have been possible.","date_published":"2014-05-21T00:00:00Z","author":[{"orcid":"0000-0003-2871-127X","id":"7439a258-f3c0-11ec-9501-9df22fe06720","last_name":"Matthee","first_name":"Jorryt J","full_name":"Matthee, Jorryt J"},{"first_name":"David","full_name":"Sobral, David","last_name":"Sobral"},{"full_name":"Swinbank, A. M.","first_name":"A. M.","last_name":"Swinbank"},{"first_name":"Ian","full_name":"Smail, Ian","last_name":"Smail"},{"first_name":"P. N.","full_name":"Best, P. N.","last_name":"Best"},{"last_name":"Kim","full_name":"Kim, Jae-Woo","first_name":"Jae-Woo"},{"first_name":"Marijn","full_name":"Franx, Marijn","last_name":"Franx"},{"first_name":"Bo","full_name":"Milvang-Jensen, Bo","last_name":"Milvang-Jensen"},{"first_name":"Johan","full_name":"Fynbo, Johan","last_name":"Fynbo"}],"oa":1,"_id":"11583","type":"journal_article","language":[{"iso":"eng"}],"doi":"10.1093/mnras/stu392","publisher":"Oxford University Press","year":"2014"},{"publication":"Plants","external_id":{"pmid":["27137397"]},"file":[{"checksum":"fb4ff2e820e344e253c9197544610be6","file_id":"10916","date_created":"2022-03-21T12:12:56Z","success":1,"date_updated":"2022-03-21T12:12:56Z","file_name":"2013_Plants_Vanneste.pdf","file_size":670188,"access_level":"open_access","content_type":"application/pdf","relation":"main_file","creator":"dernst"}],"title":"Calcium: The missing link in auxin action","issue":"4","scopus_import":"1","has_accepted_license":"1","citation":{"apa":"Vanneste, S., &#38; Friml, J. (2013). Calcium: The missing link in auxin action. <i>Plants</i>. MDPI. <a href=\"https://doi.org/10.3390/plants2040650\">https://doi.org/10.3390/plants2040650</a>","ista":"Vanneste S, Friml J. 2013. Calcium: The missing link in auxin action. Plants. 2(4), 650–675.","short":"S. Vanneste, J. Friml, Plants 2 (2013) 650–675.","mla":"Vanneste, Steffen, and Jiří Friml. “Calcium: The Missing Link in Auxin Action.” <i>Plants</i>, vol. 2, no. 4, MDPI, 2013, pp. 650–75, doi:<a href=\"https://doi.org/10.3390/plants2040650\">10.3390/plants2040650</a>.","ama":"Vanneste S, Friml J. Calcium: The missing link in auxin action. <i>Plants</i>. 2013;2(4):650-675. doi:<a href=\"https://doi.org/10.3390/plants2040650\">10.3390/plants2040650</a>","chicago":"Vanneste, Steffen, and Jiří Friml. “Calcium: The Missing Link in Auxin Action.” <i>Plants</i>. MDPI, 2013. <a href=\"https://doi.org/10.3390/plants2040650\">https://doi.org/10.3390/plants2040650</a>.","ieee":"S. Vanneste and J. Friml, “Calcium: The missing link in auxin action,” <i>Plants</i>, vol. 2, no. 4. MDPI, pp. 650–675, 2013."},"oa_version":"Published Version","page":"650-675","publication_status":"published","day":"21","tmp":{"image":"/images/cc_by.png","short":"CC BY (3.0)","name":"Creative Commons Attribution 3.0 Unported (CC BY 3.0)","legal_code_url":"https://creativecommons.org/licenses/by/3.0/legalcode"},"abstract":[{"lang":"eng","text":"Due to their sessile lifestyles, plants need to deal with the limitations and stresses imposed by the changing environment. Plants cope with these by a remarkable developmental flexibility, which is embedded in their strategy to survive. Plants can adjust their size, shape and number of organs, bend according to gravity and light, and regenerate tissues that were damaged, utilizing a coordinating, intercellular signal, the plant hormone, auxin. Another versatile signal is the cation, Ca2+, which is a crucial second messenger for many rapid cellular processes during responses to a wide range of endogenous and environmental signals, such as hormones, light, drought stress and others. Auxin is a good candidate for one of these Ca2+-activating signals. However, the role of auxin-induced Ca2+ signaling is poorly understood. Here, we will provide an overview of possible developmental and physiological roles, as well as mechanisms underlying the interconnection of Ca2+ and auxin signaling. "}],"status":"public","license":"https://creativecommons.org/licenses/by/3.0/","date_updated":"2022-03-21T12:15:29Z","volume":2,"article_type":"original","month":"10","quality_controlled":"1","publication_identifier":{"issn":["2223-7747"]},"ddc":["580"],"user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","article_processing_charge":"No","file_date_updated":"2022-03-21T12:12:56Z","keyword":["Plant Science","Ecology","Ecology","Evolution","Behavior and Systematics"],"intvolume":"         2","date_created":"2022-03-21T07:13:49Z","pmid":1,"department":[{"_id":"JiFr"}],"date_published":"2013-10-21T00:00:00Z","author":[{"last_name":"Vanneste","first_name":"Steffen","full_name":"Vanneste, Steffen"},{"first_name":"Jiří","full_name":"Friml, Jiří","last_name":"Friml","id":"4159519E-F248-11E8-B48F-1D18A9856A87","orcid":"0000-0002-8302-7596"}],"oa":1,"_id":"10895","type":"journal_article","language":[{"iso":"eng"}],"doi":"10.3390/plants2040650","publisher":"MDPI","year":"2013"},{"status":"public","date_updated":"2022-07-18T08:45:58Z","abstract":[{"text":"Faithful execution of developmental gene expression programs occurs at multiple levels and involves many different components such as transcription factors, histone-modification enzymes, and mRNA processing proteins. Recent evidence suggests that nucleoporins, well known components that control nucleo-cytoplasmic trafficking, have wide-ranging functions in developmental gene regulation that potentially extend beyond their role in nuclear transport. Whether the unexpected role of nuclear pore proteins in transcription regulation, which initially has been described in fungi and flies, also applies to human cells is unknown. Here we show at a genome-wide level that the nuclear pore protein NUP98 associates with developmentally regulated genes active during human embryonic stem cell differentiation. Overexpression of a dominant negative fragment of NUP98 levels decreases expression levels of NUP98-bound genes. In addition, we identify two modes of developmental gene regulation by NUP98 that are differentiated by the spatial localization of NUP98 target genes. Genes in the initial stage of developmental induction can associate with NUP98 that is embedded in the nuclear pores at the nuclear periphery. Alternatively, genes that are highly induced can interact with NUP98 in the nuclear interior, away from the nuclear pores. This work demonstrates for the first time that NUP98 dynamically associates with the human genome during differentiation, revealing a role of a nuclear pore protein in regulating developmental gene expression programs.","lang":"eng"}],"day":"28","oa_version":"Published Version","publication_status":"published","scopus_import":"1","issue":"2","citation":{"ama":"Liang Y, Franks TM, Marchetto MC, Gage FH, Hetzer M. Dynamic association of NUP98 with the human genome. <i>PLoS Genetics</i>. 2013;9(2). doi:<a href=\"https://doi.org/10.1371/journal.pgen.1003308\">10.1371/journal.pgen.1003308</a>","ista":"Liang Y, Franks TM, Marchetto MC, Gage FH, Hetzer M. 2013. Dynamic association of NUP98 with the human genome. PLoS Genetics. 9(2), e1003308.","apa":"Liang, Y., Franks, T. M., Marchetto, M. C., Gage, F. H., &#38; Hetzer, M. (2013). Dynamic association of NUP98 with the human genome. <i>PLoS Genetics</i>. Public Library of Science. <a href=\"https://doi.org/10.1371/journal.pgen.1003308\">https://doi.org/10.1371/journal.pgen.1003308</a>","mla":"Liang, Yun, et al. “Dynamic Association of NUP98 with the Human Genome.” <i>PLoS Genetics</i>, vol. 9, no. 2, e1003308, Public Library of Science, 2013, doi:<a href=\"https://doi.org/10.1371/journal.pgen.1003308\">10.1371/journal.pgen.1003308</a>.","short":"Y. Liang, T.M. Franks, M.C. Marchetto, F.H. Gage, M. Hetzer, PLoS Genetics 9 (2013).","ieee":"Y. Liang, T. M. Franks, M. C. Marchetto, F. H. Gage, and M. Hetzer, “Dynamic association of NUP98 with the human genome,” <i>PLoS Genetics</i>, vol. 9, no. 2. Public Library of Science, 2013.","chicago":"Liang, Yun, Tobias M. Franks, Maria C. Marchetto, Fred H. Gage, and Martin Hetzer. “Dynamic Association of NUP98 with the Human Genome.” <i>PLoS Genetics</i>. Public Library of Science, 2013. <a href=\"https://doi.org/10.1371/journal.pgen.1003308\">https://doi.org/10.1371/journal.pgen.1003308</a>."},"title":"Dynamic association of NUP98 with the human genome","external_id":{"pmid":["23468646"]},"publication":"PLoS Genetics","main_file_link":[{"url":"https://doi.org/10.1371/journal.pgen.1003308","open_access":"1"}],"type":"journal_article","year":"2013","publisher":"Public Library of Science","doi":"10.1371/journal.pgen.1003308","language":[{"iso":"eng"}],"date_published":"2013-02-28T00:00:00Z","_id":"11086","oa":1,"author":[{"last_name":"Liang","first_name":"Yun","full_name":"Liang, Yun"},{"full_name":"Franks, Tobias M.","first_name":"Tobias M.","last_name":"Franks"},{"last_name":"Marchetto","full_name":"Marchetto, Maria C.","first_name":"Maria C."},{"full_name":"Gage, Fred H.","first_name":"Fred H.","last_name":"Gage"},{"full_name":"HETZER, Martin W","first_name":"Martin W","id":"86c0d31b-b4eb-11ec-ac5a-eae7b2e135ed","last_name":"HETZER","orcid":"0000-0002-2111-992X"}],"intvolume":"         9","keyword":["Cancer Research","Genetics (clinical)","Genetics","Molecular Biology","Ecology","Evolution","Behavior and Systematics"],"article_processing_charge":"No","user_id":"72615eeb-f1f3-11ec-aa25-d4573ddc34fd","extern":"1","pmid":1,"date_created":"2022-04-07T07:50:59Z","article_number":"e1003308","volume":9,"article_type":"original","publication_identifier":{"issn":["1553-7404"]},"quality_controlled":"1","month":"02"},{"oa":1,"_id":"11520","author":[{"last_name":"Sobral","full_name":"Sobral, D.","first_name":"D."},{"first_name":"A. M.","full_name":"Swinbank, A. M.","last_name":"Swinbank"},{"first_name":"J. P.","full_name":"Stott, J. P.","last_name":"Stott"},{"first_name":"Jorryt J","full_name":"Matthee, Jorryt J","orcid":"0000-0003-2871-127X","last_name":"Matthee","id":"7439a258-f3c0-11ec-9501-9df22fe06720"},{"full_name":"Bower, R. G.","first_name":"R. G.","last_name":"Bower"},{"last_name":"Smail","full_name":"Smail, Ian","first_name":"Ian"},{"full_name":"Best, P.","first_name":"P.","last_name":"Best"},{"last_name":"Geach","full_name":"Geach, J. E.","first_name":"J. E."},{"full_name":"Sharples, R. M.","first_name":"R. M.","last_name":"Sharples"}],"date_published":"2013-12-03T00:00:00Z","publisher":"IOP Publishing","year":"2013","language":[{"iso":"eng"}],"doi":"10.1088/0004-637x/779/2/139","type":"journal_article","quality_controlled":"1","publication_identifier":{"eissn":["1538-4357"],"issn":["0004-637X"]},"month":"12","article_type":"original","volume":779,"acknowledgement":"We thank the referee for many helpful comments and suggestions which greatly improved the clarity and quality of this work. D.S. acknowledges financial support from the Netherlands Organisation for Scientific research (NWO) through a Veni fellowship and also funding from the European Community Seventh Framework Programme (FP7/2007-2013) under grant agreement number RG226604 (OPTICON) which allowed access to CFHT time (proposals: 11BO29 & 12AO19). A.M.S. gratefully acknowledges an STFC Advanced Fellowship through grant number ST/H005234/1. I.R.S., J.P.S., and R.G.B. acknowledge support from the UK Science and Technology Facilities Council (STFC) under ST/I001573/1. I.R.S. acknowledges STFC (ST/J001422/1), the ERC Advanced Investigator program DUSTYGAL and a Royal Society/Wolfson Merit Award. P.N.B. acknowledges support from STFC. R.M.S. acknowledges support from the grant ST/1001573/1. The data presented here are based on observations with the KMOS spectrograph on the ESO/VLT under program 60.A-9460 and can be accessed through the ESO data archive. The authors also wish to acknowledge the help from Michael Hilker in preparing the KMOS observations.","article_number":"139","date_created":"2022-07-07T09:14:48Z","keyword":["Space and Planetary Science","Astronomy and Astrophysics","galaxies: evolution – galaxies","high-redshift – galaxies","starburst"],"intvolume":"       779","extern":"1","user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","article_processing_charge":"No","abstract":[{"lang":"eng","text":"We present the spatially resolved Hα dynamics of 16 star-forming galaxies at z ∼ 0.81 using the new KMOS multi-object integral field spectrograph on the ESO Very Large Telescope. These galaxies, selected using 1.18 μm narrowband imaging from the 10 deg2 CFHT-HiZELS survey of the SA 22 hr field, are found in a ∼4 Mpc overdensity of Hα emitters and likely reside in a group/intermediate environment, but not a cluster. We confirm and identify a rich group of star-forming galaxies at z = 0.813 ± 0.003, with 13 galaxies within 1000 km s−1 of each other, and seven within a diameter of 3 Mpc. All of our galaxies are “typical” star-forming galaxies at their redshift, 0.8 ± 0.4 SFR$^*_{z = 0.8}$, spanning a range of specific star formation rates (sSFRs) of 0.2–1.1 Gyr−1 and have a median metallicity very close to solar of 12 + log(O/H) = 8.62 ± 0.06. We measure the spatially resolved Hα dynamics of the galaxies in our sample and show that 13 out of 16 galaxies can be described by rotating disks and use the data to derive inclination corrected rotation speeds of 50–275 km s−1. The fraction of disks within our sample is 75% ± 8%, consistent with previous results based on Hubble Space Telescope morphologies of Hα-selected galaxies at z ∼ 1 and confirming that disks dominate the SFR density at z ∼ 1. Our Hα galaxies are well fitted by the z ∼ 1–2 Tully–Fisher (TF) relation, confirming the evolution seen in the zero point. Apart from having, on average, higher stellar masses and lower sSFRs, our group galaxies at z = 0.81 present the same mass–metallicity and TF relation as z ∼ 1 field galaxies and are all disk galaxies."}],"oa_version":"Preprint","publication_status":"published","day":"03","date_updated":"2022-08-18T10:43:07Z","status":"public","main_file_link":[{"url":"https://arxiv.org/abs/1310.3822","open_access":"1"}],"external_id":{"arxiv":["1310.3822"]},"title":"The dynamics of z=0.8 H-alpha-selected star-forming galaxies from KMOS/CF-HiZELS","publication":"The Astrophysical Journal","citation":{"chicago":"Sobral, D., A. M. Swinbank, J. P. Stott, Jorryt J Matthee, R. G. Bower, Ian Smail, P. Best, J. E. Geach, and R. M. Sharples. “The Dynamics of Z=0.8 H-Alpha-Selected Star-Forming Galaxies from KMOS/CF-HiZELS.” <i>The Astrophysical Journal</i>. IOP Publishing, 2013. <a href=\"https://doi.org/10.1088/0004-637x/779/2/139\">https://doi.org/10.1088/0004-637x/779/2/139</a>.","ieee":"D. Sobral <i>et al.</i>, “The dynamics of z=0.8 H-alpha-selected star-forming galaxies from KMOS/CF-HiZELS,” <i>The Astrophysical Journal</i>, vol. 779, no. 2. IOP Publishing, 2013.","apa":"Sobral, D., Swinbank, A. M., Stott, J. P., Matthee, J. J., Bower, R. G., Smail, I., … Sharples, R. M. (2013). The dynamics of z=0.8 H-alpha-selected star-forming galaxies from KMOS/CF-HiZELS. <i>The Astrophysical Journal</i>. IOP Publishing. <a href=\"https://doi.org/10.1088/0004-637x/779/2/139\">https://doi.org/10.1088/0004-637x/779/2/139</a>","ista":"Sobral D, Swinbank AM, Stott JP, Matthee JJ, Bower RG, Smail I, Best P, Geach JE, Sharples RM. 2013. The dynamics of z=0.8 H-alpha-selected star-forming galaxies from KMOS/CF-HiZELS. The Astrophysical Journal. 779(2), 139.","mla":"Sobral, D., et al. “The Dynamics of Z=0.8 H-Alpha-Selected Star-Forming Galaxies from KMOS/CF-HiZELS.” <i>The Astrophysical Journal</i>, vol. 779, no. 2, 139, IOP Publishing, 2013, doi:<a href=\"https://doi.org/10.1088/0004-637x/779/2/139\">10.1088/0004-637x/779/2/139</a>.","short":"D. Sobral, A.M. Swinbank, J.P. Stott, J.J. Matthee, R.G. Bower, I. Smail, P. Best, J.E. Geach, R.M. Sharples, The Astrophysical Journal 779 (2013).","ama":"Sobral D, Swinbank AM, Stott JP, et al. The dynamics of z=0.8 H-alpha-selected star-forming galaxies from KMOS/CF-HiZELS. <i>The Astrophysical Journal</i>. 2013;779(2). doi:<a href=\"https://doi.org/10.1088/0004-637x/779/2/139\">10.1088/0004-637x/779/2/139</a>"},"arxiv":1,"issue":"2","scopus_import":"1"},{"type":"journal_article","publisher":"Genetics Society of America","year":"1996","language":[{"iso":"eng"}],"date_published":"1996-10-01T00:00:00Z","oa":1,"_id":"6161","author":[{"last_name":"de Bono","id":"4E3FF80E-F248-11E8-B48F-1D18A9856A87","orcid":"0000-0001-8347-0443","full_name":"de Bono, Mario","first_name":"Mario"},{"last_name":"Hodgkin","first_name":"J.","full_name":"Hodgkin, J."}],"keyword":["amino acid sequence","article","caenorhabditis elegans","evolution","genetic variability","nonhuman","priority journal","sex determination","Amino Acid Sequence","Animals","Animals","Genetically Modified","Base Sequence","Caenorhabditis","Caenorhabditis elegans","Caenorhabditis elegans Proteins","DNA","Helminth","DNA-Binding Proteins","Evolution","Molecular","Female","Helminth Proteins","Membrane Proteins","Molecular Sequence Data","Mutagenesis","RNA","Messenger","Sequence Homology","Amino Acid","Sex Determination (Analysis)","Transcription Factors","Transgenes","Turner Syndrome","Animalia","Caenorhabditis","Caenorhabditis briggsae","Caenorhabditis elegans","Nematoda"],"intvolume":"       144","extern":"1","user_id":"3E5EF7F0-F248-11E8-B48F-1D18A9856A87","pmid":1,"date_created":"2019-03-21T11:50:37Z","volume":144,"quality_controlled":"1","publication_identifier":{"issn":["00166731"]},"month":"10","status":"public","date_updated":"2021-01-12T08:06:28Z","abstract":[{"text":"The tra-1 gene is a terminal regulator of somatic sex in Caenorhabditis elegans: high tra-1 activity elicits female development, low tra-1 activity elicits male development. To investigate the function and evolution of tra- 1, we examined the tra-1 gene from the closely related nematode C. briggsae. Ce-tra-1 and Cb-tra-1 are unusually divergent. Each gene generates two transcripts, but only one of these is present in both species. This common transcript encodes TRA-1A, which shows only 44% amino acid identity between the species, a figure much lower than that for previously compared genes. A Cb-tra-1 transgene rescues many tissues of tra-1(null) mutants of C. elegans but not the somatic gonad or germ line. This transgene also causes nongonadal feminization of XO animals, indicating incorrect sexual regulation. Alignment of Ce-TRA-1A and Cb-TRA-1A defined several conserved regions likely to be important for tra-1 function. The phenotype differences between Ce-tra- 1(null) mutants rescued by Cb-tra-1 transgenes and wild-type C. elegans indicate significant divergence of regulatory regions. These molecular and functional studies suggest that evolution of sex determination in nematodes is rapid and genetically complex.","lang":"eng"}],"publication_status":"published","oa_version":"Published Version","page":"587-595","day":"01","issue":"2","citation":{"ieee":"M. de Bono and J. Hodgkin, “Evolution of sex determination in Caenorhabditis: Unusually high divergence of tra-1 and its functional consequences,” <i>Genetics</i>, vol. 144, no. 2. Genetics Society of America, pp. 587–595, 1996.","chicago":"Bono, Mario de, and J. Hodgkin. “Evolution of Sex Determination in Caenorhabditis: Unusually High Divergence of Tra-1 and Its Functional Consequences.” <i>Genetics</i>. Genetics Society of America, 1996.","ama":"de Bono M, Hodgkin J. Evolution of sex determination in Caenorhabditis: Unusually high divergence of tra-1 and its functional consequences. <i>Genetics</i>. 1996;144(2):587-595.","ista":"de Bono M, Hodgkin J. 1996. Evolution of sex determination in Caenorhabditis: Unusually high divergence of tra-1 and its functional consequences. Genetics. 144(2), 587–595.","apa":"de Bono, M., &#38; Hodgkin, J. (1996). Evolution of sex determination in Caenorhabditis: Unusually high divergence of tra-1 and its functional consequences. <i>Genetics</i>. Genetics Society of America.","mla":"de Bono, Mario, and J. Hodgkin. “Evolution of Sex Determination in Caenorhabditis: Unusually High Divergence of Tra-1 and Its Functional Consequences.” <i>Genetics</i>, vol. 144, no. 2, Genetics Society of America, 1996, pp. 587–95.","short":"M. de Bono, J. Hodgkin, Genetics 144 (1996) 587–595."},"external_id":{"pmid":["8889522"]},"title":"Evolution of sex determination in Caenorhabditis: Unusually high divergence of tra-1 and its functional consequences","publication":"Genetics","main_file_link":[{"url":"https://www.ncbi.nlm.nih.gov/pmc/articles/PMC1207552/","open_access":"1"}]},{"publication":"Analytical biogeography: An integrated approach to the study of animal and plant distributions","title":"Speciation","month":"01","publist_id":"1736","main_file_link":[{"url":"https://link.springer.com/book/10.1007/978-94-009-0435-4#toc"}],"publication_identifier":{"isbn":["978-0-412-40050-6"],"eissn":["978-94-009-0435-4"]},"quality_controlled":"1","editor":[{"full_name":"Myers, Alan","first_name":"Alan","last_name":"Myers"},{"last_name":"Giller","first_name":"Paul","full_name":"Giller, Paul"}],"scopus_import":"1","extern":"1","article_processing_charge":"No","user_id":"ea97e931-d5af-11eb-85d4-e6957dddbf17","keyword":["biogeography","biology","complexity","distribution","evolution","geology"],"date_created":"2018-12-11T12:08:13Z","citation":{"chicago":"Barton, Nicholas H. “Speciation.” In <i>Analytical Biogeography: An Integrated Approach to the Study of Animal and Plant Distributions</i>, edited by Alan Myers and Paul Giller, 1st ed., 185–218. Springer, 1988. <a href=\"https://doi.org/10.1007/978-94-009-0435-4\">https://doi.org/10.1007/978-94-009-0435-4</a>.","ieee":"N. H. Barton, “Speciation,” in <i>Analytical biogeography: An integrated approach to the study of animal and plant distributions</i>, 1st ed., A. Myers and P. Giller, Eds. Springer, 1988, pp. 185–218.","mla":"Barton, Nicholas H. “Speciation.” <i>Analytical Biogeography: An Integrated Approach to the Study of Animal and Plant Distributions</i>, edited by Alan Myers and Paul Giller, 1st ed., Springer, 1988, pp. 185–218, doi:<a href=\"https://doi.org/10.1007/978-94-009-0435-4\">10.1007/978-94-009-0435-4</a>.","ista":"Barton NH. 1988.Speciation. In: Analytical biogeography: An integrated approach to the study of animal and plant distributions. , 185–218.","apa":"Barton, N. H. (1988). Speciation. In A. Myers &#38; P. Giller (Eds.), <i>Analytical biogeography: An integrated approach to the study of animal and plant distributions</i> (1st ed., pp. 185–218). Springer. <a href=\"https://doi.org/10.1007/978-94-009-0435-4\">https://doi.org/10.1007/978-94-009-0435-4</a>","short":"N.H. Barton, in:, A. Myers, P. Giller (Eds.), Analytical Biogeography: An Integrated Approach to the Study of Animal and Plant Distributions, 1st ed., Springer, 1988, pp. 185–218.","ama":"Barton NH. Speciation. In: Myers A, Giller P, eds. <i>Analytical Biogeography: An Integrated Approach to the Study of Animal and Plant Distributions</i>. 1st ed. 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