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Cosmic voids in Sloan Digital Sky Survey Data Release 7
We study the distribution of cosmic voids and void galaxies using Sloan Digital Sky Survey Data Release 7 (SDSS DR7). Using the VoidFinder algorithm based on the original VoidFinder method devised by El-Ad & Piran and implemented by Hoyle & Vogeley, we identify 1054 statistically significant...
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Published in: | Monthly notices of the Royal Astronomical Society 2012-04, Vol.421 (2), p.926-934 |
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creator | Pan, Danny C. Vogeley, Michael S. Hoyle, Fiona Choi, Yun-Young Park, Changbom |
description | We study the distribution of cosmic voids and void galaxies using Sloan Digital Sky Survey Data Release 7 (SDSS DR7). Using the VoidFinder algorithm based on the original VoidFinder method devised by El-Ad & Piran and implemented by Hoyle & Vogeley, we identify 1054 statistically significant voids in the Northern galactic hemisphere with radii > 10 h
−1 Mpc. The filling factor of voids in the sample volume is 62 per cent. The largest void is just over 30 h
−1 Mpc in effective radius. The median effective radius is 17 h
−1 Mpc. The voids are found to be significantly underdense, with density contrast δ < − 0.85 at the edges of the voids. The radial-density profiles of these voids are similar to predictions of dynamically distinct underdensities in gravitational theory. We find 8046 galaxies brighter than Mr
=− 20.09 within the voids, accounting for 7 per cent of the galaxies. We compare the results of VoidFinder on SDSS DR7 to mock catalogues generated from a smoothed particle hydrodynamics (SPH) halo model simulation as well as other Λ cold dark matter (ΛCDM) simulations and find similar void fractions and void sizes in the data and simulations. This catalogue is made publicly available at http://www.physics.drexel.edu/~pan/VoidCatalog for download. |
doi_str_mv | 10.1111/j.1365-2966.2011.20197.x |
format | article |
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−1 Mpc. The filling factor of voids in the sample volume is 62 per cent. The largest void is just over 30 h
−1 Mpc in effective radius. The median effective radius is 17 h
−1 Mpc. The voids are found to be significantly underdense, with density contrast δ < − 0.85 at the edges of the voids. The radial-density profiles of these voids are similar to predictions of dynamically distinct underdensities in gravitational theory. We find 8046 galaxies brighter than Mr
=− 20.09 within the voids, accounting for 7 per cent of the galaxies. We compare the results of VoidFinder on SDSS DR7 to mock catalogues generated from a smoothed particle hydrodynamics (SPH) halo model simulation as well as other Λ cold dark matter (ΛCDM) simulations and find similar void fractions and void sizes in the data and simulations. This catalogue is made publicly available at http://www.physics.drexel.edu/~pan/VoidCatalog for download.</description><identifier>ISSN: 0035-8711</identifier><identifier>EISSN: 1365-2966</identifier><identifier>DOI: 10.1111/j.1365-2966.2011.20197.x</identifier><language>eng</language><publisher>Oxford, UK: Blackwell Publishing Ltd</publisher><subject>Algorithms ; Astrophysics ; catalogues ; Cosmology ; large‐scale structure of Universe ; Stars & galaxies</subject><ispartof>Monthly notices of the Royal Astronomical Society, 2012-04, Vol.421 (2), p.926-934</ispartof><rights>2012 The Authors Monthly Notices of the Royal Astronomical Society © 2012 RAS 2012</rights><rights>2012 The Authors Monthly Notices of the Royal Astronomical Society © 2012 RAS</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c5347-fd03483f527d9704ca15e8d6d1a30c24e41837c57e41edbf93bcabe6e5073db53</citedby><cites>FETCH-LOGICAL-c5347-fd03483f527d9704ca15e8d6d1a30c24e41837c57e41edbf93bcabe6e5073db53</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>314,780,784,27924,27925</link.rule.ids></links><search><creatorcontrib>Pan, Danny C.</creatorcontrib><creatorcontrib>Vogeley, Michael S.</creatorcontrib><creatorcontrib>Hoyle, Fiona</creatorcontrib><creatorcontrib>Choi, Yun-Young</creatorcontrib><creatorcontrib>Park, Changbom</creatorcontrib><title>Cosmic voids in Sloan Digital Sky Survey Data Release 7</title><title>Monthly notices of the Royal Astronomical Society</title><addtitle>Monthly Notices of the Royal Astronomical Society</addtitle><description>We study the distribution of cosmic voids and void galaxies using Sloan Digital Sky Survey Data Release 7 (SDSS DR7). Using the VoidFinder algorithm based on the original VoidFinder method devised by El-Ad & Piran and implemented by Hoyle & Vogeley, we identify 1054 statistically significant voids in the Northern galactic hemisphere with radii > 10 h
−1 Mpc. The filling factor of voids in the sample volume is 62 per cent. The largest void is just over 30 h
−1 Mpc in effective radius. The median effective radius is 17 h
−1 Mpc. The voids are found to be significantly underdense, with density contrast δ < − 0.85 at the edges of the voids. The radial-density profiles of these voids are similar to predictions of dynamically distinct underdensities in gravitational theory. We find 8046 galaxies brighter than Mr
=− 20.09 within the voids, accounting for 7 per cent of the galaxies. We compare the results of VoidFinder on SDSS DR7 to mock catalogues generated from a smoothed particle hydrodynamics (SPH) halo model simulation as well as other Λ cold dark matter (ΛCDM) simulations and find similar void fractions and void sizes in the data and simulations. This catalogue is made publicly available at http://www.physics.drexel.edu/~pan/VoidCatalog for download.</description><subject>Algorithms</subject><subject>Astrophysics</subject><subject>catalogues</subject><subject>Cosmology</subject><subject>large‐scale structure of Universe</subject><subject>Stars & galaxies</subject><issn>0035-8711</issn><issn>1365-2966</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2012</creationdate><recordtype>article</recordtype><recordid>eNqNkMFLwzAYxYMoOKf_Q_DkpTVpkia9CLI5FabCpueQpqmkds1s1rn-97areFAEc0ge5L33ffwAgBiFuDuXRYhJzIIoieMwQhj3V8LD3QEYfX8cghFChAWCY3wMTrwvEEKURPEI8InzK6vh1tnMQ1vBZelUBaf21W5UCZdvLVw29da0cKo2Ci5MaZQ3kJ-Co1yV3px9vWPwMrt5ntwF86fb-8n1PNCMUB7kGSJUkJxFPEs4olphZkQWZ1gRpCNqKBaEa8Y7YbI0T0iqVWpiwxAnWcrIGFwMvevavTfGb-TKem3KUlXGNV5ihIQgOKG0s57_sBauqatuO5lEgtNYiN4kBpOunfe1yeW6titVt12T7IHKQvbcZM9N9kDlHqjcddGrIfphS9P-OycfHhd72RWQocA16z_iwe-xn_YciJ8</recordid><startdate>201204</startdate><enddate>201204</enddate><creator>Pan, Danny C.</creator><creator>Vogeley, Michael S.</creator><creator>Hoyle, Fiona</creator><creator>Choi, Yun-Young</creator><creator>Park, Changbom</creator><general>Blackwell Publishing Ltd</general><general>Oxford University Press</general><scope>AAYXX</scope><scope>CITATION</scope><scope>8FD</scope><scope>H8D</scope><scope>L7M</scope><scope>7TG</scope><scope>KL.</scope></search><sort><creationdate>201204</creationdate><title>Cosmic voids in Sloan Digital Sky Survey Data Release 7</title><author>Pan, Danny C. ; Vogeley, Michael S. ; Hoyle, Fiona ; Choi, Yun-Young ; Park, Changbom</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c5347-fd03483f527d9704ca15e8d6d1a30c24e41837c57e41edbf93bcabe6e5073db53</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2012</creationdate><topic>Algorithms</topic><topic>Astrophysics</topic><topic>catalogues</topic><topic>Cosmology</topic><topic>large‐scale structure of Universe</topic><topic>Stars & galaxies</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Pan, Danny C.</creatorcontrib><creatorcontrib>Vogeley, Michael S.</creatorcontrib><creatorcontrib>Hoyle, Fiona</creatorcontrib><creatorcontrib>Choi, Yun-Young</creatorcontrib><creatorcontrib>Park, Changbom</creatorcontrib><collection>CrossRef</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Advanced Technologies Database with Aerospace</collection><collection>Meteorological & Geoastrophysical Abstracts</collection><collection>Meteorological & Geoastrophysical Abstracts - Academic</collection><jtitle>Monthly notices of the Royal Astronomical Society</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Pan, Danny C.</au><au>Vogeley, Michael S.</au><au>Hoyle, Fiona</au><au>Choi, Yun-Young</au><au>Park, Changbom</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Cosmic voids in Sloan Digital Sky Survey Data Release 7</atitle><jtitle>Monthly notices of the Royal Astronomical Society</jtitle><stitle>Monthly Notices of the Royal Astronomical Society</stitle><date>2012-04</date><risdate>2012</risdate><volume>421</volume><issue>2</issue><spage>926</spage><epage>934</epage><pages>926-934</pages><issn>0035-8711</issn><eissn>1365-2966</eissn><abstract>We study the distribution of cosmic voids and void galaxies using Sloan Digital Sky Survey Data Release 7 (SDSS DR7). Using the VoidFinder algorithm based on the original VoidFinder method devised by El-Ad & Piran and implemented by Hoyle & Vogeley, we identify 1054 statistically significant voids in the Northern galactic hemisphere with radii > 10 h
−1 Mpc. The filling factor of voids in the sample volume is 62 per cent. The largest void is just over 30 h
−1 Mpc in effective radius. The median effective radius is 17 h
−1 Mpc. The voids are found to be significantly underdense, with density contrast δ < − 0.85 at the edges of the voids. The radial-density profiles of these voids are similar to predictions of dynamically distinct underdensities in gravitational theory. We find 8046 galaxies brighter than Mr
=− 20.09 within the voids, accounting for 7 per cent of the galaxies. We compare the results of VoidFinder on SDSS DR7 to mock catalogues generated from a smoothed particle hydrodynamics (SPH) halo model simulation as well as other Λ cold dark matter (ΛCDM) simulations and find similar void fractions and void sizes in the data and simulations. This catalogue is made publicly available at http://www.physics.drexel.edu/~pan/VoidCatalog for download.</abstract><cop>Oxford, UK</cop><pub>Blackwell Publishing Ltd</pub><doi>10.1111/j.1365-2966.2011.20197.x</doi><tpages>9</tpages><oa>free_for_read</oa></addata></record> |
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subjects | Algorithms Astrophysics catalogues Cosmology large‐scale structure of Universe Stars & galaxies |
title | Cosmic voids in Sloan Digital Sky Survey Data Release 7 |
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