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20 April 2024
 
  » arxiv » 1604.2214

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A New Constraint on the Ly$alpha$ Fraction of UV Very Bright Galaxies at Redshift 7
Hisanori Furusawa ; Nobunari Kashikawa ; Masakazu A. R. Kobayashi ; James S. Dunlop ; Kazuhiro Shimasaku ; Tadafumi Takata ; Kazuhiro Sekiguchi ; Yoshiaki Naito ; Junko Furusawa ; Masami Ouchi ; Fumiaki Nakata ; Naoki Yasuda ; Yuki Okura ; Yoshiaki Taniguchi ; Toru Yamada ; Masaru Kajisawa ; Johan P. U. Fynbo ; Olivier Le Fevre ;
Date 8 Apr 2016
AbstractWe study the extent to which very bright (-23.0 < MUV < -21.75) Lyman-break selected galaxies at redshifts z~7 display detectable Lya emission. To explore this issue, we have obtained follow-up optical spectroscopy of 9 z~7 galaxies from a parent sample of 24 z~7 galaxy candidates selected from the 1.65 sq.deg COSMOS-UltraVISTA and SXDS-UDS survey fields using the latest near-infrared public survey data, and new ultra-deep Subaru z’-band imaging (which we also present and describe in this paper). Our spectroscopy has yielded only one possible detection of Lya at z=7.168 with a rest-frame equivalent width EW_0 = 3.7 (+1.7/-1.1) Angstrom. The relative weakness of this line, combined with our failure to detect Lya emission from the other spectroscopic targets allows us to place a new upper limit on the prevalence of strong Lya emission at these redshifts. For conservative calculation and to facilitate comparison with previous studies at lower redshifts, we derive a 1-sigma upper limit on the fraction of UV bright galaxies at z~7 that display EW_0 > 50 Angstrom, which we estimate to be < 0.23. This result may indicate a weak trend where the fraction of strong Lya emitters ceases to rise, and possibly falls between z~6 and z~7. Our results also leave open the possibility that strong Lya may still be more prevalent in the brightest galaxies in the reionization era than their fainter counterparts. A larger spectroscopic sample of galaxies is required to derive a more reliable constraint on the neutral hydrogen fraction at z~7 based on the Lya fraction in the bright galaxies.
Source arXiv, 1604.2214
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