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タイトルSearching for Neutral Hydrogen Halos Around z approx. 2.1 and z approx. 3.1 Ly(alpha) Emitting Galaxies
本文(外部サイト)http://hdl.handle.net/2060/20160001317
著者(英)Cronwall, Caryl; Kurczynski, Peter; Feldmeier, John J.; Guaita, Lucia; Orsi, Alvaro; Bond, Nicholas A.; Hagen, Lea. M. Z.; Ciardullo, Robin; Blanc, Guillermo A.; Acquaviva, Viviana; Gawiser, Eric; Hagen, Alex
著者所属(英)NASA Goddard Space Flight Center
発行日2013-09-30
言語eng
内容記述We search for evidence of diffuse Ly(alpha) emission from extended neutral hydrogen surrounding Ly(alpha) emitting galaxies (LAEs) using deep narrow-band images of the Extended Chandra Deep Field South. By stacking the profiles of 187 LAEs at z = 2.06, 241 LAEs at z = 3.10, and 179 LAEs at z = 3.12, and carefully performing low-surface brightness photometry, we obtain mean surface brightness maps that reach 9.9, 8.7, and 6.2 10(exp 19) erg/sq cm/s/sq arcsec in the emission line. We undertake a thorough investigation of systematic uncertainties in our surface brightness measurements and find that our limits are 5-10 times larger than would be expected from Poisson background fluctuations; these uncertainties are often underestimated in the literature. At z approx. 3.1, we find evidence for extended halos with small-scale lengths of 5-8 kpc in some but not all of our sub-samples. We demonstrate that sub-samples of LAEs with low equivalent widths and brighter continuum magnitudes are more likely to possess such halos. At z approx. 2.1, we find no evidence of extended Ly emission down to our detection limits. Through Monte-Carlo simulations, we also show that we would have detected large diffuse LAE halos if they were present in our data sets. We compare these findings to other measurements in the literature and discuss possible instrumental and astrophysical reasons for the discrepancies.
NASA分類Astrophysics
レポートNOGSFC-E-DAA-TN12517
権利Copyright, Distribution under U.S. Government purpose rights
URIhttps://repository.exst.jaxa.jp/dspace/handle/a-is/558756


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