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DESIVAST: A Catalog of Low-Redshift Voids using Data from the DESI DR1 Bright Galaxy Survey

Hernan RinconRochester US. BenZviRochester UKelly A. DouglassRochester UDahlia VeyratRochester UJ. AguilarLBNL, BerkeleyS. AhlenBoston UDavide BianchiMylan (Switzerland)David BrooksUniversity Coll. LondonT. ClaybaughLBNL, BerkeleyShaun ColeDurham U., ICCAxel de la MacorraUNAM, MexicoP. DoelUniversity Coll. LondonAndreu Font-RiberaBarcelona, IFAEJ. E. Forero-RomeroE. GaztañagaICE, BellaterraSatya Gontcho A GontchoLBNL, BerkeleyG. GutiérrezFermilabKlaus HonscheidChicago U., KICPCullan HowlettQueensland US. JuneauNatl. Solar Observ., TucsonR. KehoeSouthern Methodist US. E. KoposovCambridge UAndrew LambertLBNL, BerkeleyMartin LandriauLBNL, BerkeleyL. Le GuillouLPNHE, ParisAaron MeisnerNatl. Solar Observ., TucsonR. MiquelInstitut Català de Ciències del ClimaJohn MoustakasSiena Coll., LoudonvilleGustavo NizGuanajuato UWill J. PercivalRegional Municipality of WaterlooFrancisco PradaGranada U., Theor. Phys. AstrophysIgnasi Pérez-RàfolsBarcelona, Polytechnic UGraziano RossiSejong UE. SánchezCentro de Investigaciones Energéticas, Medioambientales y TecnológicasM. SchubnellU. Michigan, Ann ArborHee‐Jong SeoDavid SprayberryNatl. Solar Observ., TucsonG. TarléMichigan UBenjamin Alan WeaverNatl. Solar Observ., TucsonH. ZouBeijing Observ
arXiv (Cornell University)repository2024en
ABI

Annotatsiya

We present three separate void catalogs created using a volume-limited sample of the DESI Year 1 Bright Galaxy Survey. We use the algorithms VoidFinder and V2 to construct void catalogs out to a redshift of z=0.24. We obtain 1,461 interior voids with VoidFinder, 420 with V2 using REVOLVER pruning, and 295 with V2 using VIDE pruning. Comparing our catalog with an overlapping SDSS void catalog, we find generally consistent void properties but significant differences in the void volume overlap, which we attribute to differences in the galaxy selection and survey masks. These catalogs are suitable for studying the variation in galaxy properties with cosmic environment and for cosmological studies.

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