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- W2261374016 abstract "We use the stellar-mass-selected catalog from the Spitzer Large Area Survey with Hyper-Suprime-Cam (SPLASH) in the COSMOS field to study the environments of galaxies via galaxy density and clustering analyses up to The clustering strength of quiescent galaxies exceeds that of star-forming galaxies, implying that quiescent galaxies are preferentially located in more massive halos. When using local density measurement, we find a clear positive quiescent fraction–density relation at consistent with earlier results. However, the quiescent fraction–density relation reverses its trend at intermediate redshifts () with marginal significance (<1.8σ) and is found to be scale dependent (1.6σ). The lower fraction of quiescent galaxies seen in large-scale dense environments, if confirmed to be true, may be associated with the fact that the star formation can be more easily sustained via cold stream accretion in large-scale high-density regions, preventing galaxies from permanent quenching. Finally, at the quiescent fraction depends little on the local density, even though clustering shows that quiescent galaxies are in more massive halos. We argue that at high redshift the typical halo size falls below 1013 , where intrinsically the local density measurements are so varied that they do not trace the halo mass. Our results thus suggest that in the high-redshift universe, halo mass may be the key in quenching the star formation in galaxies, rather than the conventionally measured galaxy density." @default.
- W2261374016 created "2016-06-24" @default.
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- W2261374016 date "2016-01-26" @default.
- W2261374016 modified "2023-10-16" @default.
- W2261374016 title "THE SPLASH SURVEY: QUIESCENT GALAXIES ARE MORE STRONGLY CLUSTERED BUT ARE NOT NECESSARILY LOCATED IN HIGH-DENSITY ENVIRONMENTS" @default.
- W2261374016 cites W1815960455 @default.
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- W2261374016 cites W1970196846 @default.
- W2261374016 cites W1983114396 @default.
- W2261374016 cites W1985952407 @default.
- W2261374016 cites W1986761806 @default.
- W2261374016 cites W1989910526 @default.
- W2261374016 cites W1994671833 @default.
- W2261374016 cites W1995942510 @default.
- W2261374016 cites W1999402800 @default.
- W2261374016 cites W2001085255 @default.
- W2261374016 cites W2012576933 @default.
- W2261374016 cites W2012886609 @default.
- W2261374016 cites W2013964487 @default.
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- W2261374016 cites W2088107818 @default.
- W2261374016 cites W2090428815 @default.
- W2261374016 cites W2092051661 @default.
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- W2261374016 cites W2141709306 @default.
- W2261374016 cites W2142238829 @default.
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- W2261374016 cites W2963147361 @default.
- W2261374016 cites W3098017603 @default.
- W2261374016 cites W3098257997 @default.
- W2261374016 cites W3098339022 @default.
- W2261374016 cites W3099471130 @default.
- W2261374016 cites W3100024326 @default.
- W2261374016 cites W3100756254 @default.
- W2261374016 cites W3101682154 @default.
- W2261374016 cites W3102518111 @default.
- W2261374016 cites W3103850807 @default.
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- W2261374016 doi "https://doi.org/10.3847/0004-637x/817/2/97" @default.
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