Matches in SemOpenAlex for { <https://semopenalex.org/work/W2949874561> ?p ?o ?g. }
- W2949874561 endingPage "84" @default.
- W2949874561 startingPage "84" @default.
- W2949874561 abstract "We introduce a new color selection technique to identify high-redshift, massive galaxies that are systematically missed by Lyman-break selection. The new selection is based on the H160 (H) and Infrared Array Camera (IRAC) 4.5 μm bands, specifically mag. These galaxies, called HIEROs, include two major populations that can be separated with an additional J − H color. The populations are massive and dusty star-forming galaxies at () and extremely dusty galaxies at (). The 350 arcmin2 of the GOODS-North and GOODS-South fields with the deepest Hubble Space Telescope (HST)/Wide Field Camera 3 (WFC3) near-infrared and IRAC data contain as many as 285 HIEROs down to mag. Inclusion of the most extreme HIEROs, not even detected in the H band, makes this selection particularly complete for the identification of massive high-redshift galaxies. We focus here primarily on () HIEROs, which have a median photometric redshift and stellar mass and are much fainter in the rest-frame UV than similarly massive Lyman-break galaxies (LBGs). Their star formation rates (SFRs), derived from their stacked infrared spectral energy distributions (SEDs), reach ∼240 yr−1, leading to a specific SFR, Gyr−1, suggesting that the sSFRs for massive galaxies continue to grow at but at a lower growth rate than from z = 0 to z = 2. With a median half-light radius of 2 kpc, including as compact as quiescent (QS) galaxies at similar redshifts, HIEROs represent perfect star-forming progenitors of the most massive ( ) compact QS galaxies at and have the right number density. HIEROs make up of all galaxies with identified at from their photometric redshifts. This is five times more than LBGs with nearly no overlap between the two populations. While HIEROs make up 15%–25% of the total SFR density at –5, they completely dominate the SFR density taking place in galaxies, and HIEROs are therefore crucial to understanding the very early phase of massive galaxy formation." @default.
- W2949874561 created "2019-06-27" @default.
- W2949874561 creator A5001676664 @default.
- W2949874561 creator A5002397192 @default.
- W2949874561 creator A5004163126 @default.
- W2949874561 creator A5015409091 @default.
- W2949874561 creator A5017176794 @default.
- W2949874561 creator A5017490289 @default.
- W2949874561 creator A5020310880 @default.
- W2949874561 creator A5024410226 @default.
- W2949874561 creator A5029531883 @default.
- W2949874561 creator A5031355390 @default.
- W2949874561 creator A5036257511 @default.
- W2949874561 creator A5038955740 @default.
- W2949874561 creator A5039140400 @default.
- W2949874561 creator A5041494992 @default.
- W2949874561 creator A5043083140 @default.
- W2949874561 creator A5054628656 @default.
- W2949874561 creator A5056214913 @default.
- W2949874561 creator A5056216981 @default.
- W2949874561 creator A5058519861 @default.
- W2949874561 creator A5061200355 @default.
- W2949874561 creator A5062477074 @default.
- W2949874561 creator A5063009942 @default.
- W2949874561 creator A5065415667 @default.
- W2949874561 creator A5066369555 @default.
- W2949874561 creator A5066819594 @default.
- W2949874561 creator A5073619828 @default.
- W2949874561 creator A5076100952 @default.
- W2949874561 creator A5080778381 @default.
- W2949874561 creator A5082697625 @default.
- W2949874561 creator A5085764209 @default.
- W2949874561 creator A5086583377 @default.
- W2949874561 creator A5088582472 @default.
- W2949874561 date "2016-01-14" @default.
- W2949874561 modified "2023-10-18" @default.
- W2949874561 title "INFRARED COLOR SELECTION OF MASSIVE GALAXIES AT<i>z</i>> 3" @default.
- W2949874561 cites W1508863994 @default.
- W2949874561 cites W1524555145 @default.
- W2949874561 cites W1596864409 @default.
- W2949874561 cites W1842880767 @default.
- W2949874561 cites W1908085087 @default.
- W2949874561 cites W1913812026 @default.
- W2949874561 cites W1973977373 @default.
- W2949874561 cites W1979789803 @default.
- W2949874561 cites W1984895372 @default.
- W2949874561 cites W1985952407 @default.
- W2949874561 cites W1986834411 @default.
- W2949874561 cites W1994097808 @default.
- W2949874561 cites W1994662943 @default.
- W2949874561 cites W1994671833 @default.
- W2949874561 cites W1999046479 @default.
- W2949874561 cites W2008777327 @default.
- W2949874561 cites W2008991538 @default.
- W2949874561 cites W2009743038 @default.
- W2949874561 cites W2017450908 @default.
- W2949874561 cites W2019398523 @default.
- W2949874561 cites W2028398011 @default.
- W2949874561 cites W2033803356 @default.
- W2949874561 cites W2034244381 @default.
- W2949874561 cites W2034288205 @default.
- W2949874561 cites W2041084195 @default.
- W2949874561 cites W2042994140 @default.
- W2949874561 cites W2043235658 @default.
- W2949874561 cites W2044360592 @default.
- W2949874561 cites W2047156688 @default.
- W2949874561 cites W2047758030 @default.
- W2949874561 cites W2047970181 @default.
- W2949874561 cites W2048274049 @default.
- W2949874561 cites W2049698250 @default.
- W2949874561 cites W2057589371 @default.
- W2949874561 cites W2058678220 @default.
- W2949874561 cites W2066233280 @default.
- W2949874561 cites W2069396164 @default.
- W2949874561 cites W2070696493 @default.
- W2949874561 cites W2070887798 @default.
- W2949874561 cites W2073925265 @default.
- W2949874561 cites W2074259895 @default.
- W2949874561 cites W2075414028 @default.
- W2949874561 cites W2076455056 @default.
- W2949874561 cites W2084780057 @default.
- W2949874561 cites W2084830951 @default.
- W2949874561 cites W2090046995 @default.
- W2949874561 cites W2090689284 @default.
- W2949874561 cites W2091867375 @default.
- W2949874561 cites W2092458937 @default.
- W2949874561 cites W2093468672 @default.
- W2949874561 cites W2107308864 @default.
- W2949874561 cites W2110709935 @default.
- W2949874561 cites W2110830624 @default.
- W2949874561 cites W2124572431 @default.
- W2949874561 cites W2126790576 @default.
- W2949874561 cites W2135052708 @default.
- W2949874561 cites W2144910248 @default.
- W2949874561 cites W2147847259 @default.
- W2949874561 cites W2151062050 @default.
- W2949874561 cites W2155705849 @default.
- W2949874561 cites W2158454843 @default.