dc.contributor.author | Sobral, D. | |
dc.contributor.author | Best, P.N. | |
dc.contributor.author | Geach, J.E. | |
dc.contributor.author | Smail, I. | |
dc.contributor.author | Kurk, J. | |
dc.contributor.author | Cirasuolo, M. | |
dc.contributor.author | Casali, M. | |
dc.contributor.author | Ivison, R.J. | |
dc.contributor.author | Coppin, Kristen | |
dc.contributor.author | Dalton, G.B. | |
dc.date.accessioned | 2014-01-27T11:00:30Z | |
dc.date.available | 2014-01-27T11:00:30Z | |
dc.date.issued | 2009-09-01 | |
dc.identifier.citation | Sobral , D , Best , P N , Geach , J E , Smail , I , Kurk , J , Cirasuolo , M , Casali , M , Ivison , R J , Coppin , K & Dalton , G B 2009 , ' Bright Lyα emitters at z ~ 9 : Constraints on the LF from HizELS ' , Monthly Notices of the Royal Astronomical Society: Letters , vol. 398 , no. 1 , pp. L68-L72 . https://doi.org/10.1111/j.1745-3933.2009.00712.x | |
dc.identifier.issn | 1745-3933 | |
dc.identifier.other | ORCID: /0000-0002-0729-2988/work/30423103 | |
dc.identifier.uri | http://hdl.handle.net/2299/12676 | |
dc.description | Copyright Royal Astronomical Society | |
dc.description.abstract | New results are presented, as part of the Hi-z Emission Line Survey (HizELS), from the largest area survey to date (1.4 deg ) for Lyα emitters (LAEs) at z ~ 9. The survey, which is primarily targeting Hα emitters at z <3, uses the Wide Field CAMera on the United Kingdom Infrared Telescope and a custom narrow-band filter in the J band and reaches a Lyα luminosity limit of ~10 ergs over a co-moving volume of 1.12 × 10 Mpc at z = 8.96 ± 0.06. Only two candidates were found out of 1517 line emitters and those were rejected as LAEs after follow-up observations. The limit on the space density of bright LAEs is improved by three orders of magnitude, consistent with suppression of the bright end of the Lyα luminosity function beyond z ~ 6. Combined with upper limits from smaller but deeper surveys, this rules out some of the most extreme models for high-redshift LAEs. The potential contamination of future narrow-band Lyα surveys at z > 7 by Galactic brown dwarf stars is also examined, leading to the conclusion that such contamination may well be significant for searches at 7.7 <z <8.0, 9.1 <z <9.5 and 11.7 <z <12.2. | en |
dc.format.extent | 1101551 | |
dc.language.iso | eng | |
dc.relation.ispartof | Monthly Notices of the Royal Astronomical Society: Letters | |
dc.title | Bright Lyα emitters at z ~ 9 : Constraints on the LF from HizELS | en |
dc.contributor.institution | Centre for Astrophysics Research | |
dc.contributor.institution | Centre for Climate Change Research (C3R) | |
dc.contributor.institution | School of Physics, Engineering & Computer Science | |
dc.contributor.institution | Department of Physics, Astronomy and Mathematics | |
dc.contributor.institution | Centre of Data Innovation Research | |
dc.description.status | Peer reviewed | |
dc.identifier.url | http://www.scopus.com/inward/record.url?scp=70549101627&partnerID=8YFLogxK | |
rioxxterms.versionofrecord | 10.1111/j.1745-3933.2009.00712.x | |
rioxxterms.type | Journal Article/Review | |
herts.preservation.rarelyaccessed | true | |