Matches in SemOpenAlex for { <https://semopenalex.org/work/W3098623648> ?p ?o ?g. }
- W3098623648 endingPage "A2" @default.
- W3098623648 startingPage "A2" @default.
- W3098623648 abstract "We carried out a photometric and structural analysis in the rest-frame $V$ band of a mass-selected ($log M/M_odot >10.7$) sample of red-sequence galaxies in 14 galaxy clusters, 6 of which are at $z>1.45$. To this end, we reduced/analyzed about 300 orbits of multicolor images taken with the Advanced Camera for Survey and the Wide Field Camera 3 on the Hubble Space Telescope. We uniformly morphologically classified galaxies from $z=0.023$ to $z=1.803$, and we homogeneously derived sizes (effective radii) for the entire sample. Furthermore, our size derivation allows, and therefore is not biased by, the presence of the usual variety of morphological structures seen in early-type galaxies, such as bulges, bars, disks, isophote twists, and ellipiticy gradients. By using such a mass-selected sample, composed of 244 red-sequence early-type galaxies, we find that the $log$ of the galaxy size at a fixed stellar mass, $log M/M_odot= 11$ has increased with time at a rate of $0.023pm0.002$ dex per Gyr over the last 10 Gyr, in marked contrast with the threefold increase found in the literature for galaxies in the general field over the same period. This suggests, at face value, that secular processes should be excluded as the primary drivers of size evolution because we observed an environmental environmental dependent size growth. Using spectroscopic ages of Coma early-type galaxies we also find that recently quenched early-type galaxies are a numerically minor population not different enough in size to alter the mean size at a given mass, which implies that the progenitor bias is minor, i.e., that the size evolution measured by selecting galaxies at the redshift of observation is indistinguishable from the one that compares ancestors and descendents." @default.
- W3098623648 created "2020-11-23" @default.
- W3098623648 creator A5015736261 @default.
- W3098623648 creator A5024567984 @default.
- W3098623648 creator A5028903582 @default.
- W3098623648 date "2016-08-29" @default.
- W3098623648 modified "2023-10-12" @default.
- W3098623648 title "Size growth of red-sequence early-type galaxies in clusters in the last 10 Gyr" @default.
- W3098623648 cites W1501370474 @default.
- W3098623648 cites W1598567242 @default.
- W3098623648 cites W1791095791 @default.
- W3098623648 cites W1794475290 @default.
- W3098623648 cites W1813536970 @default.
- W3098623648 cites W1887378386 @default.
- W3098623648 cites W1937529881 @default.
- W3098623648 cites W1964402260 @default.
- W3098623648 cites W1968771143 @default.
- W3098623648 cites W1980708053 @default.
- W3098623648 cites W1983932997 @default.
- W3098623648 cites W1985370957 @default.
- W3098623648 cites W1987597328 @default.
- W3098623648 cites W1992898138 @default.
- W3098623648 cites W1993225027 @default.
- W3098623648 cites W1993950853 @default.
- W3098623648 cites W1994671833 @default.
- W3098623648 cites W1995606657 @default.
- W3098623648 cites W1999468056 @default.
- W3098623648 cites W2000244530 @default.
- W3098623648 cites W2005376313 @default.
- W3098623648 cites W2009736281 @default.
- W3098623648 cites W2011651094 @default.
- W3098623648 cites W2012143947 @default.
- W3098623648 cites W2012478338 @default.
- W3098623648 cites W2020019783 @default.
- W3098623648 cites W2024409675 @default.
- W3098623648 cites W2025020969 @default.
- W3098623648 cites W2025181530 @default.
- W3098623648 cites W2031763498 @default.
- W3098623648 cites W2032767306 @default.
- W3098623648 cites W2033539580 @default.
- W3098623648 cites W2033803356 @default.
- W3098623648 cites W2034065802 @default.
- W3098623648 cites W2039082913 @default.
- W3098623648 cites W2042905846 @default.
- W3098623648 cites W2044141001 @default.
- W3098623648 cites W2052458093 @default.
- W3098623648 cites W2053791382 @default.
- W3098623648 cites W2059588423 @default.
- W3098623648 cites W2063375039 @default.
- W3098623648 cites W2064725598 @default.
- W3098623648 cites W2066645046 @default.
- W3098623648 cites W2068405714 @default.
- W3098623648 cites W2071384997 @default.
- W3098623648 cites W2079227246 @default.
- W3098623648 cites W2082331906 @default.
- W3098623648 cites W2084091264 @default.
- W3098623648 cites W2086491236 @default.
- W3098623648 cites W2087766564 @default.
- W3098623648 cites W2089065774 @default.
- W3098623648 cites W2089191176 @default.
- W3098623648 cites W2098236249 @default.
- W3098623648 cites W2101470472 @default.
- W3098623648 cites W2108238747 @default.
- W3098623648 cites W2109146631 @default.
- W3098623648 cites W2111162453 @default.
- W3098623648 cites W2116035762 @default.
- W3098623648 cites W2119352430 @default.
- W3098623648 cites W2141515548 @default.
- W3098623648 cites W2142238829 @default.
- W3098623648 cites W2145954987 @default.
- W3098623648 cites W2152668089 @default.
- W3098623648 cites W2153050977 @default.
- W3098623648 cites W2155385043 @default.
- W3098623648 cites W2159657041 @default.
- W3098623648 cites W2160843940 @default.
- W3098623648 cites W2162399571 @default.
- W3098623648 cites W2166814121 @default.
- W3098623648 cites W2167129914 @default.
- W3098623648 cites W2169318301 @default.
- W3098623648 cites W2171801427 @default.
- W3098623648 cites W2176131481 @default.
- W3098623648 cites W2182776375 @default.
- W3098623648 cites W2237502840 @default.
- W3098623648 cites W2953003216 @default.
- W3098623648 cites W3098079486 @default.
- W3098623648 cites W3099050667 @default.
- W3098623648 cites W3099155372 @default.
- W3098623648 cites W3099263125 @default.
- W3098623648 cites W3099432089 @default.
- W3098623648 cites W3099532125 @default.
- W3098623648 cites W3099984547 @default.
- W3098623648 cites W3100522481 @default.
- W3098623648 cites W3100780824 @default.
- W3098623648 cites W3101072469 @default.
- W3098623648 cites W3101366286 @default.
- W3098623648 cites W3102274475 @default.
- W3098623648 cites W3102443279 @default.
- W3098623648 cites W3103782874 @default.