{"day":"01","publisher":"Oxford University Press","year":"2015","article_type":"original","date_published":"2015-11-01T00:00:00Z","keyword":["Space and Planetary Science","Astronomy and Astrophysics","black hole physics","stars: Population III","galaxies: high-redshift"],"title":"The brightest Lyα emitter: Pop III or black hole?","scopus_import":"1","quality_controlled":"1","main_file_link":[{"url":"https://arxiv.org/abs/1506.07173","open_access":"1"}],"oa_version":"Preprint","issue":"3","language":[{"iso":"eng"}],"intvolume":"       453","external_id":{"arxiv":["1506.07173"]},"page":"2465-2470","status":"public","oa":1,"user_id":"2DF688A6-F248-11E8-B48F-1D18A9856A87","article_processing_charge":"No","acknowledgement":"SS acknowledges support from the Netherlands Organization for Scientific research (NWO), VENI grant 639.041.233. RS acknowledges support from the European Research Council under the European Union (FP/2007-2013)/ERC grant agreement no. 306476. DS acknowledges (i) financial support from the NWO through a Veni fellowship and (ii) funding from FCT through a FCT Investigator Starting Grant and Start-up Grant (IF/01154/2012/CP0189/CT0010) and from FCT grant PEstOE/FIS/UI2751/2014.","date_created":"2022-07-14T08:58:36Z","month":"11","citation":{"short":"A. Pallottini, A. Ferrara, F. Pacucci, S. Gallerani, S. Salvadori, R. Schneider, D. Schaerer, D. Sobral, J.J. Matthee, Monthly Notices of the Royal Astronomical Society 453 (2015) 2465–2470.","ama":"Pallottini A, Ferrara A, Pacucci F, et al. The brightest Lyα emitter: Pop III or black hole? <i>Monthly Notices of the Royal Astronomical Society</i>. 2015;453(3):2465-2470. doi:<a href=\"https://doi.org/10.1093/mnras/stv1795\">10.1093/mnras/stv1795</a>","mla":"Pallottini, A., et al. “The Brightest Lyα Emitter: Pop III or Black Hole?” <i>Monthly Notices of the Royal Astronomical Society</i>, vol. 453, no. 3, Oxford University Press, 2015, pp. 2465–70, doi:<a href=\"https://doi.org/10.1093/mnras/stv1795\">10.1093/mnras/stv1795</a>.","ieee":"A. Pallottini <i>et al.</i>, “The brightest Lyα emitter: Pop III or black hole?,” <i>Monthly Notices of the Royal Astronomical Society</i>, vol. 453, no. 3. Oxford University Press, pp. 2465–2470, 2015.","ista":"Pallottini A, Ferrara A, Pacucci F, Gallerani S, Salvadori S, Schneider R, Schaerer D, Sobral D, Matthee JJ. 2015. The brightest Lyα emitter: Pop III or black hole? Monthly Notices of the Royal Astronomical Society. 453(3), 2465–2470.","chicago":"Pallottini, A., A. Ferrara, F. Pacucci, S. Gallerani, S. Salvadori, R. Schneider, D. Schaerer, D. Sobral, and Jorryt J Matthee. “The Brightest Lyα Emitter: Pop III or Black Hole?” <i>Monthly Notices of the Royal Astronomical Society</i>. Oxford University Press, 2015. <a href=\"https://doi.org/10.1093/mnras/stv1795\">https://doi.org/10.1093/mnras/stv1795</a>.","apa":"Pallottini, A., Ferrara, A., Pacucci, F., Gallerani, S., Salvadori, S., Schneider, R., … Matthee, J. J. (2015). The brightest Lyα emitter: Pop III or black hole? <i>Monthly Notices of the Royal Astronomical Society</i>. Oxford University Press. <a href=\"https://doi.org/10.1093/mnras/stv1795\">https://doi.org/10.1093/mnras/stv1795</a>"},"doi":"10.1093/mnras/stv1795","author":[{"first_name":"A.","full_name":"Pallottini, A.","last_name":"Pallottini"},{"last_name":"Ferrara","full_name":"Ferrara, A.","first_name":"A."},{"last_name":"Pacucci","full_name":"Pacucci, F.","first_name":"F."},{"first_name":"S.","full_name":"Gallerani, S.","last_name":"Gallerani"},{"first_name":"S.","full_name":"Salvadori, S.","last_name":"Salvadori"},{"last_name":"Schneider","full_name":"Schneider, R.","first_name":"R."},{"last_name":"Schaerer","full_name":"Schaerer, D.","first_name":"D."},{"first_name":"D.","full_name":"Sobral, D.","last_name":"Sobral"},{"id":"7439a258-f3c0-11ec-9501-9df22fe06720","last_name":"Matthee","orcid":"0000-0003-2871-127X","full_name":"Matthee, Jorryt J","first_name":"Jorryt J"}],"_id":"11579","abstract":[{"lang":"eng","text":"CR7 is the brightest z = 6.6 Ly α emitter (LAE) known to date, and spectroscopic follow-up by Sobral et al. suggests that CR7 might host Population (Pop) III stars. We examine this interpretation using cosmological hydrodynamical simulations. Several simulated galaxies show the same ‘Pop III wave’ pattern observed in CR7. However, to reproduce the extreme CR7 Ly α/He II1640 line luminosities (⁠Lα/HeII⁠) a top-heavy initial mass function and a massive ( ≳ 107 M⊙) Pop III burst with age ≲ 2 Myr are required. Assuming that the observed properties of Ly α and He II emission are typical for Pop III, we predict that in the COSMOS/UDS/SA22 fields, 14 out of the 30 LAEs at z = 6.6 with Lα > 1043.3 erg s−1 should also host Pop III stars producing an observable LHeII≳1042.7ergs−1⁠. As an alternate explanation, we explore the possibility that CR7 is instead powered by accretion on to a direct collapse black hole. Our model predicts Lα, LHeII⁠, and X-ray luminosities that are in agreement with the observations. In any case, the observed properties of CR7 indicate that this galaxy is most likely powered by sources formed from pristine gas. We propose that further X-ray observations can distinguish between the two above scenarios."}],"publication":"Monthly Notices of the Royal Astronomical Society","publication_status":"published","type":"journal_article","extern":"1","volume":453,"date_updated":"2022-08-19T08:19:23Z","publication_identifier":{"eissn":["1365-2966"],"issn":["0035-8711"]}}