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• W3105505723 startingPage "97" @default.
• W3105505723 abstract "We measure the environmental dependence, where environment is defined by the distance to the third nearest neighbor, of multiple galaxy properties inside the Environmental COntext (ECO) catalog. We focus primarily on void galaxies, which we define as the $10 %$ of galaxies having the lowest local density. We compare the properties of void and non-void galaxies: baryonic mass, color, fractional stellar mass growth rate (FSMGR), morphology, and gas-to-stellar-mass ratio (estimated from a combination of HI data and photometric gas fractions calibrated with the RESOLVE survey). Our void galaxies typically have lower baryonic masses than galaxies in denser environments, and they display the properties expected of a lower mass population: they have more late-types, are bluer, have higher FSMGR, and are more gas rich. We control for baryonic mass and investigate the extent to which void galaxies are different at fixed mass. Void galaxies are bluer, more gas-rich, and more star forming at fixed mass than non-void galaxies, which is a possible signature of galaxy assembly bias. Furthermore, we show that these trends persist even at fixed mass and morphology, and we find that voids host a distinct population of early-types that are bluer and more star-forming than the typical red and quenched early-types. In addition to these empirical observational results, we also present theoretical results from mock catalogs with built-in galaxy assembly bias. We show that a simple matching of galaxy properties to (sub)halo properties, such as mass and age, can recover the observed environmental trends in ECO galaxies." @default.
• W3105505723 created "2020-11-23" @default.
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• W3105505723 date "2021-01-01" @default.
• W3105505723 modified "2023-10-12" @default.
• W3105505723 title "Void Galaxies Follow a Distinct Evolutionary Path in the Environmental COntext Catalog" @default.
• W3105505723 cites W1613735089 @default.
• W3105505723 cites W1751039464 @default.
• W3105505723 cites W1896841992 @default.
• W3105505723 cites W1948610287 @default.
• W3105505723 cites W1965779302 @default.
• W3105505723 cites W1979503956 @default.
• W3105505723 cites W1980407824 @default.
• W3105505723 cites W1981855749 @default.
• W3105505723 cites W1987399761 @default.
• W3105505723 cites W1987522415 @default.
• W3105505723 cites W1996879250 @default.
• W3105505723 cites W1999702339 @default.
• W3105505723 cites W2000444334 @default.
• W3105505723 cites W2002142654 @default.
• W3105505723 cites W2004372001 @default.
• W3105505723 cites W2021966030 @default.
• W3105505723 cites W2023351067 @default.
• W3105505723 cites W2023873184 @default.
• W3105505723 cites W2029910311 @default.
• W3105505723 cites W2038434077 @default.
• W3105505723 cites W2039047466 @default.
• W3105505723 cites W2041545130 @default.
• W3105505723 cites W2042179541 @default.
• W3105505723 cites W2045674582 @default.
• W3105505723 cites W2050340293 @default.
• W3105505723 cites W2051707349 @default.
• W3105505723 cites W2053201549 @default.
• W3105505723 cites W2055327934 @default.
• W3105505723 cites W2058685713 @default.
• W3105505723 cites W2061231038 @default.
• W3105505723 cites W2065353414 @default.
• W3105505723 cites W2069685156 @default.
• W3105505723 cites W2070820850 @default.
• W3105505723 cites W2071734029 @default.
• W3105505723 cites W2072271826 @default.
• W3105505723 cites W2077054687 @default.
• W3105505723 cites W2083609951 @default.
• W3105505723 cites W2087432755 @default.
• W3105505723 cites W2089729354 @default.
• W3105505723 cites W2093052816 @default.
• W3105505723 cites W2113768579 @default.
• W3105505723 cites W2116757101 @default.
• W3105505723 cites W2127193056 @default.
• W3105505723 cites W2128372566 @default.
• W3105505723 cites W2131472136 @default.
• W3105505723 cites W2134209509 @default.
• W3105505723 cites W2140834585 @default.
• W3105505723 cites W2153037851 @default.
• W3105505723 cites W2157917411 @default.
• W3105505723 cites W2168182511 @default.
• W3105505723 cites W2170689655 @default.
• W3105505723 cites W2337188492 @default.
• W3105505723 cites W2469036835 @default.
• W3105505723 cites W2545020124 @default.
• W3105505723 cites W2545641380 @default.
• W3105505723 cites W2609256388 @default.
• W3105505723 cites W2612406039 @default.
• W3105505723 cites W2616323325 @default.
• W3105505723 cites W2902704612 @default.
• W3105505723 cites W3098804119 @default.
• W3105505723 cites W3098844796 @default.
• W3105505723 cites W3100987161 @default.
• W3105505723 cites W3101752698 @default.
• W3105505723 cites W3102678289 @default.
• W3105505723 cites W3102941904 @default.
• W3105505723 cites W3103145119 @default.
• W3105505723 cites W3103395327 @default.
• W3105505723 cites W3104579003 @default.
• W3105505723 cites W3104609245 @default.
• W3105505723 cites W3105014804 @default.
• W3105505723 cites W3105190296 @default.
• W3105505723 cites W3105363723 @default.
• W3105505723 cites W3105631369 @default.
• W3105505723 cites W3105905443 @default.
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• W3105505723 cites W3122687038 @default.
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• W3105505723 doi "https://doi.org/10.3847/1538-4357/abca9f" @default.
• W3105505723 hasPublicationYear "2021" @default.
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