FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W3100967345> ?p ?o ?g. }

• W3100967345 endingPage "76" @default.
• W3100967345 startingPage "76" @default.
• W3100967345 abstract "Previous work has demonstrated that at a given stellar mass, quiescent galaxies are more strongly clustered than star-forming galaxies. The contribution to this signal from central, as opposed to satellite, galaxies is not known, which has strong implications for galaxy evolution models. To investigate the contribution from central galaxies, here we present measurements of the clustering of isolated primary (IP) galaxies, used as a proxy for central galaxies, at 0.2 < z < 0.9 with data from the PRIsm MUlti-Object Survey (PRIMUS) galaxy redshift survey. Using a sample of spectroscopic redshifts for ∼60,000 galaxies with covering 5 deg2 on the sky, we define IP galaxies using isolation cuts in spatial proximity and stellar mass of nearby galaxies. We find that at a fixed stellar mass, quiescent IP galaxies are more strongly clustered than star-forming IP galaxies at z ∼ 0.35 (10σ). Using mock galaxy catalogs based on the recent halo occupation models of Behroozi et al. and designed to replicate the parameters of the PRIMUS survey data set, we find that these clustering differences are due in part to quiescent central galaxies being more strongly clustered than star-forming central galaxies. This is consistent with either distinct stellar-to-halo mass relations for quiescent and star-forming central galaxies, and/or central galaxy assembly bias. We additionally use mock catalogs to assess the dependence of both incompleteness and satellite galaxy contamination in the IP galaxy samples on redshift, galaxy type, and stellar mass, and demonstrate how isolation criteria yield biased subsamples of central galaxies via environmental incompleteness, or the preferential exclusion of central galaxies in overdense environments." @default.
• W3100967345 created "2020-11-23" @default.
• W3100967345 creator A5033558209 @default.
• W3100967345 creator A5034370718 @default.
• W3100967345 creator A5063587809 @default.
• W3100967345 creator A5085992419 @default.
• W3100967345 date "2019-10-14" @default.
• W3100967345 modified "2023-09-24" @default.
• W3100967345 title "PRIMUS: Clustering of Star-forming and Quiescent Central Galaxies at 0.2 < <i>z</i> < 0.9" @default.
• W3100967345 cites W1520258040 @default.
• W3100967345 cites W1915403329 @default.
• W3100967345 cites W1931677786 @default.
• W3100967345 cites W1965779302 @default.
• W3100967345 cites W1966926090 @default.
• W3100967345 cites W1969514664 @default.
• W3100967345 cites W1980904486 @default.
• W3100967345 cites W1984743356 @default.
• W3100967345 cites W1996537612 @default.
• W3100967345 cites W1999367759 @default.
• W3100967345 cites W1999702339 @default.
• W3100967345 cites W2006284873 @default.
• W3100967345 cites W2008877686 @default.
• W3100967345 cites W2017605375 @default.
• W3100967345 cites W2023351067 @default.
• W3100967345 cites W2025180048 @default.
• W3100967345 cites W2025634246 @default.
• W3100967345 cites W2029910311 @default.
• W3100967345 cites W2039047466 @default.
• W3100967345 cites W2040393541 @default.
• W3100967345 cites W2042179541 @default.
• W3100967345 cites W2042707894 @default.
• W3100967345 cites W2043685494 @default.
• W3100967345 cites W2054852647 @default.
• W3100967345 cites W2064377583 @default.
• W3100967345 cites W2065975941 @default.
• W3100967345 cites W2073986801 @default.
• W3100967345 cites W2074259895 @default.
• W3100967345 cites W2079825621 @default.
• W3100967345 cites W2094993922 @default.
• W3100967345 cites W2096882371 @default.
• W3100967345 cites W2102519805 @default.
• W3100967345 cites W2121991715 @default.
• W3100967345 cites W2126510815 @default.
• W3100967345 cites W2127888248 @default.
• W3100967345 cites W2135202711 @default.
• W3100967345 cites W2148804397 @default.
• W3100967345 cites W2157544440 @default.
• W3100967345 cites W2158528198 @default.
• W3100967345 cites W2158622701 @default.
• W3100967345 cites W2169910932 @default.
• W3100967345 cites W2197026494 @default.
• W3100967345 cites W2210633397 @default.
• W3100967345 cites W2233433857 @default.
• W3100967345 cites W2463842489 @default.
• W3100967345 cites W2509454543 @default.
• W3100967345 cites W2520788058 @default.
• W3100967345 cites W2530063092 @default.
• W3100967345 cites W2547700289 @default.
• W3100967345 cites W2553718159 @default.
• W3100967345 cites W2612406039 @default.
• W3100967345 cites W2614409774 @default.
• W3100967345 cites W2616836162 @default.
• W3100967345 cites W2626545803 @default.
• W3100967345 cites W2750704704 @default.
• W3100967345 cites W2773012159 @default.
• W3100967345 cites W2809045192 @default.
• W3100967345 cites W2902704612 @default.
• W3100967345 cites W3098356719 @default.
• W3100967345 cites W3098629121 @default.
• W3100967345 cites W3098640821 @default.
• W3100967345 cites W3098804119 @default.
• W3100967345 cites W3099270657 @default.
• W3100967345 cites W3099599559 @default.
• W3100967345 cites W3099871027 @default.
• W3100967345 cites W3100024326 @default.
• W3100967345 cites W3100669571 @default.
• W3100967345 cites W3100987161 @default.
• W3100967345 cites W3101369122 @default.
• W3100967345 cites W3101475602 @default.
• W3100967345 cites W3103018756 @default.
• W3100967345 cites W3103073255 @default.
• W3100967345 cites W3103813867 @default.
• W3100967345 cites W3104013352 @default.
• W3100967345 cites W3104579003 @default.
• W3100967345 cites W3104639138 @default.
• W3100967345 cites W3104952135 @default.
• W3100967345 cites W3105014804 @default.
• W3100967345 cites W3105733428 @default.
• W3100967345 cites W3106072945 @default.
• W3100967345 cites W3106456019 @default.
• W3100967345 cites W3121623664 @default.
• W3100967345 cites W3124120495 @default.
• W3100967345 cites W4293088723 @default.
• W3100967345 doi "https://doi.org/10.3847/1538-4357/ab3b5d" @default.
• W3100967345 hasPublicationYear "2019" @default.
• W3100967345 type Work @default.
• W3100967345 sameAs 3100967345 @default.
• W3100967345 citedByCount "6" @default.

• next