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  • Nature Publishing Group (NPG)  (2)
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  • 1
    Publication Date: 2010-03-26
    Description: The Lyman-alpha (Lyalpha) emission line is the primary observational signature of star-forming galaxies at the highest redshifts, and has enabled the compilation of large samples of galaxies with which to study cosmic evolution. The resonant nature of the line, however, means that Lyalpha photons scatter in the neutral interstellar medium of their host galaxies, and their sensitivity to absorption by interstellar dust may therefore be greatly enhanced. This implies that the Lyalpha luminosity may be significantly reduced, or even completely suppressed. Hitherto, no unbiased empirical test of the escaping fraction (f(esc)) of Lyalpha photons has been performed at high redshifts. Here we report that the average f(esc) from star-forming galaxies at redshift z = 2.2 is just 5 per cent by performing a blind narrowband survey in Lyalpha and Halpha. This implies that numerous conclusions based on Lyalpha-selected samples will require upwards revision by an order of magnitude and we provide a benchmark for this revision. We demonstrate that almost 90 per cent of star-forming galaxies emit insufficient Lyalpha to be detected by standard selection criteria. Both samples show an anti-correlation of f(esc) with dust content, and we show that Lyalpha- and Halpha-selection recovers populations that differ substantially in dust content and f(esc).〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Hayes, Matthew -- Ostlin, Goran -- Schaerer, Daniel -- Mas-Hesse, J Miguel -- Leitherer, Claus -- Atek, Hakim -- Kunth, Daniel -- Verhamme, Anne -- de Barros, Stephane -- Melinder, Jens -- England -- Nature. 2010 Mar 25;464(7288):562-5. doi: 10.1038/nature08881.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Observatoire Astronomique de l'Universite de Geneve, 51 chemin des Maillettes, CH-1290 Sauverny, Switzerland. matthew.hayes@unige.ch〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/20336139" target="_blank"〉PubMed〈/a〉
    Print ISSN: 0028-0836
    Electronic ISSN: 1476-4687
    Topics: Biology , Chemistry and Pharmacology , Medicine , Natural Sciences in General , Physics
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  • 2
    Publication Date: 2016-01-15
    Description: One of the key questions in observational cosmology is the identification of the sources responsible for ionization of the Universe after the cosmic 'Dark Ages', when the baryonic matter was neutral. The currently identified distant galaxies are insufficient to fully reionize the Universe by redshift z approximately 6 (refs 1-3), but low-mass, star-forming galaxies are thought to be responsible for the bulk of the ionizing radiation. As direct observations at high redshift are difficult for a variety of reasons, one solution is to identify local proxies of this galaxy population. Starburst galaxies at low redshifts, however, generally are opaque to Lyman continuum photons. Small escape fractions of about 1 to 3 per cent, insufficient to ionize much surrounding gas, have been detected only in three low-redshift galaxies. Here we report far-ultraviolet observations of the nearby low-mass star-forming galaxy J0925+1403. The galaxy is leaking ionizing radiation with an escape fraction of about 8 per cent. The total number of photons emitted during the starburst phase is sufficient to ionize intergalactic medium material that is about 40 times as massive as the stellar mass of the galaxy.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Izotov, Y I -- Orlitova, I -- Schaerer, D -- Thuan, T X -- Verhamme, A -- Guseva, N G -- Worseck, G -- England -- Nature. 2016 Jan 14;529(7585):178-80. doi: 10.1038/nature16456.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Main Astronomical Observatory, National Academy of Sciences of Ukraine, 27 Zabolotnoho street, Kyiv 03680, Ukraine. ; Astronomical Institute, Czech Academy of Sciences, Boc ni II 1401, 141 00 Prague, Czech Republic. ; Observatoire de Geneve, Universite de Geneve, 51 Chemin des Maillettes, 1290 Versoix, Switzerland. ; CNRS, IRAP, 14 Avenue East Belin, 31400 Toulouse, France. ; Astronomy Department, University of Virginia, PO Box 400325, Charlottesville, Virginia 22904, USA. ; Max-Planck-Institut fur Astronomie, Konigstuhl 17, 69117 Heidelberg, Germany.〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/26762455" target="_blank"〉PubMed〈/a〉
    Print ISSN: 0028-0836
    Electronic ISSN: 1476-4687
    Topics: Biology , Chemistry and Pharmacology , Medicine , Natural Sciences in General , Physics
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