Matches in SemOpenAlex for { <https://semopenalex.org/work/W2465893476> ?p ?o ?g. }
- W2465893476 endingPage "76" @default.
- W2465893476 startingPage "76" @default.
- W2465893476 abstract "The Wide Field Camera 3 (WFC3) on the Hubble Space Telescope (HST) enabled the search for the first galaxies observed at z ~ 8 - 11 (500 - 700 Myr after the Big Bang). To continue quantifying the number density of the most luminous galaxies (M_AB ~ -22.0) at the earliest epoch observable with HST, we search for z ~ 10 galaxies (F125W-dropouts) in archival data from the Brightest of Reionizing Galaxies (BoRG[z8]) survey, originally designed for detection of z ~ 8 galaxies (F098M-dropouts). By focusing on the deepest 293 arcmin^2 of the data along 62 independent lines of sight, we identify six z ~ 10 candidates satisfying the color selection criteria, detected at S/N > 8 in F160W with M_AB = -22.8 to -21.1 if at z = 10. Three of the six sources, including the two brightest, are in a single WFC3 pointing (~ 4 arcmin^2), suggestive of significant clustering, which is expected from bright galaxies at z ~ 10. However, the two brightest galaxies are too extended to be likely at z ~ 10, and one additional source is unresolved and possibly a brown dwarf. The remaining three candidates have m_AB ~ 26, and given the area and completeness of our search, our best estimate is a number density of sources that is marginally higher but consistent at 2{sigma} with searches in legacy fields. Our study highlights that z ~ 10 searches can yield a small number of candidates, making tailored follow-ups of HST pure-parallel observations viable and effective." @default.
- W2465893476 created "2016-07-22" @default.
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- W2465893476 date "2016-08-09" @default.
- W2465893476 modified "2023-09-25" @default.
- W2465893476 title "GALAXY CANDIDATES AT<i>z</i>∼ 10 IN ARCHIVAL DATA FROM THE BRIGHTEST OF REIONIZING GALAXIES (BORG[z8]) SURVEY" @default.
- W2465893476 cites W1525855014 @default.
- W2465893476 cites W1572126587 @default.
- W2465893476 cites W1582953240 @default.
- W2465893476 cites W1603995462 @default.
- W2465893476 cites W1665497759 @default.
- W2465893476 cites W1722819912 @default.
- W2465893476 cites W1908085087 @default.
- W2465893476 cites W1932159333 @default.
- W2465893476 cites W1960284331 @default.
- W2465893476 cites W1962697969 @default.
- W2465893476 cites W1967532042 @default.
- W2465893476 cites W1970381301 @default.
- W2465893476 cites W1978498913 @default.
- W2465893476 cites W1981864500 @default.
- W2465893476 cites W1990937453 @default.
- W2465893476 cites W1994915027 @default.
- W2465893476 cites W2009886487 @default.
- W2465893476 cites W2012035798 @default.
- W2465893476 cites W2016966639 @default.
- W2465893476 cites W2019365096 @default.
- W2465893476 cites W2023842147 @default.
- W2465893476 cites W2024297548 @default.
- W2465893476 cites W2025717087 @default.
- W2465893476 cites W2029343094 @default.
- W2465893476 cites W2040634438 @default.
- W2465893476 cites W2048195627 @default.
- W2465893476 cites W2057016571 @default.
- W2465893476 cites W2067558684 @default.
- W2465893476 cites W2068368465 @default.
- W2465893476 cites W2071407353 @default.
- W2465893476 cites W2076653098 @default.
- W2465893476 cites W2077944558 @default.
- W2465893476 cites W2078991135 @default.
- W2465893476 cites W2082592033 @default.
- W2465893476 cites W2093520301 @default.
- W2465893476 cites W2094871238 @default.
- W2465893476 cites W2095914404 @default.
- W2465893476 cites W2097790409 @default.
- W2465893476 cites W2120040287 @default.
- W2465893476 cites W2133581151 @default.
- W2465893476 cites W2136246999 @default.
- W2465893476 cites W2142238829 @default.
- W2465893476 cites W2150819820 @default.
- W2465893476 cites W2155705849 @default.
- W2465893476 cites W2158454843 @default.
- W2465893476 cites W2185979087 @default.
- W2465893476 cites W2254519591 @default.
- W2465893476 cites W2288607592 @default.
- W2465893476 cites W2332378549 @default.
- W2465893476 cites W2552643820 @default.
- W2465893476 cites W2593327244 @default.
- W2465893476 cites W2951385617 @default.
- W2465893476 cites W3098906824 @default.
- W2465893476 cites W3099155372 @default.
- W2465893476 cites W3099975679 @default.
- W2465893476 cites W3100206529 @default.
- W2465893476 cites W3100361538 @default.
- W2465893476 cites W3100564066 @default.
- W2465893476 cites W3101004763 @default.
- W2465893476 cites W3102047411 @default.
- W2465893476 cites W3102242441 @default.
- W2465893476 cites W3102587696 @default.
- W2465893476 cites W3102597523 @default.
- W2465893476 cites W3102706913 @default.
- W2465893476 cites W3102799427 @default.
- W2465893476 cites W3102804033 @default.
- W2465893476 cites W3103446530 @default.
- W2465893476 cites W3104123668 @default.
- W2465893476 cites W3104592512 @default.
- W2465893476 cites W3104906118 @default.
- W2465893476 cites W3105037965 @default.
- W2465893476 cites W3105439098 @default.
- W2465893476 cites W3105652047 @default.
- W2465893476 cites W3121553509 @default.
- W2465893476 cites W3123147540 @default.
- W2465893476 cites W3123261968 @default.
- W2465893476 cites W3124349042 @default.
- W2465893476 cites W3124368117 @default.
- W2465893476 cites W3124919044 @default.
- W2465893476 doi "https://doi.org/10.3847/0004-637x/827/1/76" @default.
- W2465893476 hasPublicationYear "2016" @default.