FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W1948610287> ?p ?o ?g. }

• W1948610287 endingPage "3050" @default.
• W1948610287 startingPage "3041" @default.
• W1948610287 abstract "Using the sample presented in Pan:2011, we analyse the photometric properties of 88,794 void galaxies and compare them to galaxies in higher density environments with the same absolute magnitude distribution. In Pan et al. (2011), we found a total of 1054 dynamically distinct voids in the SDSS with radius larger than 10h^-1 Mpc. The voids are underdense, with delta rho/rho < -0.9 in their centers. Here we study the photometric properties of these void galaxies. We look at the u - r colours as an indication of star formation activity and the inverse concentration index as an indication of galaxy type. We find that void galaxies are statistically bluer than galaxies found in higher density environments with the same magnitude distribution. We examine the colours of the galaxies as a function of magnitude, and we fit each colour distribution with a double-Gaussian model for the red and blue subpopulations. As we move from bright to dwarf galaxies, the population of red galaxies steadily decreases and the fraction of blue galaxies increases in both voids and walls, however the fraction of blue galaxies in the voids is always higher and bluer than in the walls. We also split the void and wall galaxies into samples depending on galaxy type. We find that late type void galaxies are bluer than late type wall galaxies and the same holds for early galaxies. We also find that early type, dwarf void galaxies are blue in colour. We also study the properties of void galaxies as a function of their distance from the center of the void. We find very little variation in the properties, such as magnitude, colour and type, of void galaxies as a function of their location in the void. The only exception is that the dwarf void galaxies may live closer to the center. The centers of voids have very similar density contrast and hence all void galaxies live in very similar density environments (ABRIDGED)" @default.
• W1948610287 created "2016-06-24" @default.
• W1948610287 creator A5049177150 @default.
• W1948610287 creator A5050636305 @default.
• W1948610287 creator A5072255876 @default.
• W1948610287 date "2012-10-17" @default.
• W1948610287 modified "2023-09-27" @default.
• W1948610287 title "Photometric properties of void galaxies in the Sloan Digital Sky Survey Data Release 7" @default.
• W1948610287 cites W109761076 @default.
• W1948610287 cites W1509549320 @default.
• W1948610287 cites W1788569890 @default.
• W1948610287 cites W1964280853 @default.
• W1948610287 cites W1966609605 @default.
• W1948610287 cites W1966876239 @default.
• W1948610287 cites W1966926356 @default.
• W1948610287 cites W1967368622 @default.
• W1948610287 cites W1969395888 @default.
• W1948610287 cites W1978875836 @default.
• W1948610287 cites W1979742375 @default.
• W1948610287 cites W1998130311 @default.
• W1948610287 cites W2000821703 @default.
• W1948610287 cites W2002569490 @default.
• W1948610287 cites W2004372001 @default.
• W1948610287 cites W2019372364 @default.
• W1948610287 cites W2021545503 @default.
• W1948610287 cites W2021966030 @default.
• W1948610287 cites W2026619221 @default.
• W1948610287 cites W2032327414 @default.
• W1948610287 cites W2035320096 @default.
• W1948610287 cites W2036311035 @default.
• W1948610287 cites W2039989896 @default.
• W1948610287 cites W2040405503 @default.
• W1948610287 cites W2041545130 @default.
• W1948610287 cites W2046397236 @default.
• W1948610287 cites W2049757954 @default.
• W1948610287 cites W2055327934 @default.
• W1948610287 cites W2070121531 @default.
• W1948610287 cites W2070308719 @default.
• W1948610287 cites W2080657868 @default.
• W1948610287 cites W2086769041 @default.
• W1948610287 cites W2092571324 @default.
• W1948610287 cites W2103263072 @default.
• W1948610287 cites W2104403548 @default.
• W1948610287 cites W2109510044 @default.
• W1948610287 cites W2119969282 @default.
• W1948610287 cites W2124199755 @default.
• W1948610287 cites W2131480207 @default.
• W1948610287 cites W2150195330 @default.
• W1948610287 cites W2150331774 @default.
• W1948610287 cites W2153037851 @default.
• W1948610287 cites W2153690020 @default.
• W1948610287 cites W2154263420 @default.
• W1948610287 cites W2157917411 @default.
• W1948610287 cites W2158639540 @default.
• W1948610287 cites W2166393334 @default.
• W1948610287 cites W2167389038 @default.
• W1948610287 cites W2168182511 @default.
• W1948610287 cites W3101136340 @default.
• W1948610287 cites W3101335975 @default.
• W1948610287 cites W3101463758 @default.
• W1948610287 cites W3101752698 @default.
• W1948610287 cites W3102031721 @default.
• W1948610287 cites W3102941904 @default.
• W1948610287 cites W3104413800 @default.
• W1948610287 cites W3104453257 @default.
• W1948610287 cites W3105054341 @default.
• W1948610287 cites W3105363723 @default.
• W1948610287 cites W3122227674 @default.
• W1948610287 cites W3125927684 @default.
• W1948610287 cites W3125986925 @default.
• W1948610287 cites W4292310541 @default.
• W1948610287 doi "https://doi.org/10.1111/j.1365-2966.2012.21943.x" @default.
• W1948610287 hasPublicationYear "2012" @default.
• W1948610287 type Work @default.
• W1948610287 sameAs 1948610287 @default.
• W1948610287 citedByCount "71" @default.
• W1948610287 countsByYear W19486102872013 @default.
• W1948610287 countsByYear W19486102872014 @default.
• W1948610287 countsByYear W19486102872015 @default.
• W1948610287 countsByYear W19486102872016 @default.
• W1948610287 countsByYear W19486102872017 @default.
• W1948610287 countsByYear W19486102872018 @default.
• W1948610287 countsByYear W19486102872019 @default.
• W1948610287 countsByYear W19486102872020 @default.
• W1948610287 countsByYear W19486102872021 @default.
• W1948610287 countsByYear W19486102872022 @default.
• W1948610287 countsByYear W19486102872023 @default.
• W1948610287 crossrefType "journal-article" @default.
• W1948610287 hasAuthorship W1948610287A5049177150 @default.
• W1948610287 hasAuthorship W1948610287A5050636305 @default.
• W1948610287 hasAuthorship W1948610287A5072255876 @default.
• W1948610287 hasBestOaLocation W19486102871 @default.
• W1948610287 hasConcept C121332964 @default.
• W1948610287 hasConcept C1276947 @default.
• W1948610287 hasConcept C134122466 @default.
• W1948610287 hasConcept C152268414 @default.
• W1948610287 hasConcept C159985019 @default.
• W1948610287 hasConcept C160147972 @default.

• next