J/ApJ/832/126ivo://CDS.VizieR/J/ApJ/832/126doi:10.26093/cds/vizier.18320126CDSStark D.V.Kannappan S.J.Eckert K.D.Florez J.Hall K.R.Watson L.C.,Hoversten E.A.Burchett J.N.Guynn D.T.Baker A.D.Moffett A.J.,Berlind A.A.Norris M.A.Haynes M.P.Giovanelli R.Leroy A.K.,Pisano D.J.Wei L.H.Gonzalez R.E.Calderon V.F.2018-09-14T13:12:42Z2017-03-31T12:44:57ZCDS support team

CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France

cds-question@unistra.frgalaxiesspectroscopystellar-massessurveysradio-astronomyWe present the HI mass inventory for the REsolved Spectroscopy Of a Local VolumE (RESOLVE) survey, a volume-limited, multi-wavelength census of >1500 z=0 galaxies spanning diverse environments and complete in baryonic mass down to dwarfs of ~10^9^M_{sun}_. This first 21cm data release provides robust detections or strong upper limits (1.4M_HI_<5%-10% of stellar mass M*) for ~94% of RESOLVE. We examine global atomic gas-to-stellar mass ratios (G/S) in relation to galaxy environment using several metrics: group dark matter halo mass M_h_, central/satellite designation, relative mass density of the cosmic web, and distance to the nearest massive group. We find that at fixed M*, satellites have decreasing G/S with increasing M_h_ starting clearly at M_h_~10^12^M_{sun}_, suggesting the presence of starvation and/or stripping mechanisms associated with halo gas heating in intermediate-mass groups. The analogous relationship for centrals is uncertain because halo abundance matching builds in relationships between central G/S, stellar mass, and halo mass, which depend on the integrated group property used as a proxy for halo mass (stellar or baryonic mass). On larger scales G/S trends are less sensitive to the abundance matching method. At fixed M_h_<=10^12^M_{sun}_, the fraction of gas-poor centrals increases with large-scale structure density. In overdense regions, we identify a rare population of gas-poor centrals in low-mass (M_h_<10^11.4^M_{sun}_) halos primarily located within ~1.5x the virial radius of more massive (M_h_>10^12^M_{sun}_) halos, suggesting that gas stripping and/or starvation may be induced by interactions with larger halos or the surrounding cosmic web. We find that the detailed relationship between G/S and environment varies when we examine different subvolumes of RESOLVE independently, which we suggest may be a signature of assembly bias.2016ApJ...832..126Shttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/832/126CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toV/139 : The SDSS Photometric Catalog, Release 9 (Adelman-McCarthy+, 2012)VII/259 : 6dF galaxy survey final redshift release (Jones+, 2009)VIII/77 : HI spectral properties of galaxies (Springob+, 2005)VII/250 : The 2dF Galaxy Redshift Survey (2dFGRS) (2dFGRS Team, 1998-2003)J/ApJ/824/124 : Galaxy stellar and baryonic mass functions (Eckert+, 2016)J/A+A/596/A14 : Group catalogues of the local universe (Saulder+, 2016)J/ApJS/223/20 : SDSS-DR8 galaxies classified by WND-CHARM (Kuminski+, 2016)J/ApJ/812/89 : Environmental COntext (ECO) catalog (Moffett+, 2015)J/ApJ/810/166 : RESOLVE survey photometry catalog (Eckert+, 2015)J/MNRAS/436/34 : GALEX Arecibo SDSS survey. Final release (Catinella+, 2013)J/ApJ/777/42 : Kinematic and HI data for the NFGS (Kannappan+, 2013)J/ApJ/776/71 : ZENS: gal. in groups along the cosmic web. I (Carollo+, 2013)J/ApJ/769/82 : H_2_ masses in a broad sample of galaxies (Stark+, 2013)J/AJ/144/16 : Optical & HI properties of galaxies in voids (Kreckel+, 2012)J/AJ/142/170 : ALFALFA survey: {alpha}.40 HI source catalog (Haynes+, 2011)J/ApJ/733/74 : GALEX - SDSS properties of local galaxies (Lemonias+, 2011)J/MNRAS/413/971 : Galaxy And Mass Assembly (GAMA) DR1 (Driver+, 2011)J/ApJS/167/1 : Galaxy groups and clusters from SDSS (Berlind+, 2006)J/A+A/417/421 : WSRT wide-field HI survey. II. (Braun+, 2004)J/AJ/119/32 : Survey of galaxies within nearby voids. II (Grogin+, 2000)J/AJ/117/2039 : Sc galaxies I photometry, 21cm data (Haynes+, 1999)http://resolve.astro.unc.edu/ : RESOLVE home pagehttp://www.sdss3.org/ : SDSS-III home pagehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/832/126https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/832/126http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/832/126https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/832/126https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/832/126http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/832/126GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/ApJ/832/126/table1 (REsolved Spectroscopy Of a Local VolumE (RESOLVE) 21cm catalog; from erratum published in 2017, ApJ, 851, 153)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/832/126/table1?https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/832/126/table1?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/832/126/table1?GETtext/xml+votable180.050000true0.01343-1.112890.005555555555555556Cone search capability for table J/ApJ/832/126/table2 (RESOLVE environment metrics)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/832/126/table2?https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/832/126/table2?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/832/126/table2?GETtext/xml+votable180.050000true1.14670.84860.0055555555555555564/1648 1728 5/4441 4442 4454 4458 4501 4502 4505 4517 4518 4693 4694 4697 4713 6507 6509 6510 6511 6551 6557 6558 6567 6571 6572 6574 6575 6579 6584 6596 6598 6600 6601 6747 6751 6763 6766 6769 6771 6777 6807 6815 6828 6829 6831 6833 6835 6849 6920 6/2 4096 4097 4098 4103 4104 4108 4109 4110 4129 4132 4134 8200 8201 8203 8206 8208 8227 8228 8230 8231 8234 17406 17407 17661 17662 17663 17727 17743 17745 17746 17747 17748 17749 17750 17753 17754 17755 17761 17762 17763 17772 17773 17774 17776 17777 17778 17784 17805 17806 17807 17809 17811 17812 17814 17815 17820 17821 17822 17827 17828 17829 17830 17838 17840 17841 17856 17857 17858 17981 17982 17983 17997 17998 17999 18001 18002 18003 18012 18013 18014 18017 18018 18019 18024 18027 18028 18029 18032 18033 18061 18063 18066 18076 18077 18078 18081 18082 18083 18084 18086 18087 18089 18090 18091 18094 18096 18097 18098 18112 18113 18114 18176 18177 18178 18686 18765 18767 18769 18771 18780 18782 18787 18792 18796 18798 18800 18801 18802 18835 18838 18839 18840 18842 18844 18845 18850 18856 18858 18859 18864 18865 18866 18880 18882 19021 19022 19023 19027 19028 19029 19032 19035 19044 19045 19056 19200 19201 19456 25942 25945 25958 25970 25974 25975 25977 25981 26006 26010 26012 26014 26015 26023 26025 26026 26027 26032 26033 26035 26050 26051 26057 26059 26060 26063 26064 26073 26080 26082 26083 26084 26085 26087 26089 26090 26096 26197 26198 26199 26203 26215 26217 26221 26222 26223 26224 26225 26227 26237 26238 26239 26261 26262 26263 26265 26266 26267 26277 26278 26279 26281 26282 26283 26292 26304 26305 26306 26308 26309 26312 26320 26321 26323 26324 26325 26326 26340 26346 26388 26389 26390 26396 26408 26409 26410 26432 26965 26969 26970 26971 26975 26981 26982 26983 26986 26987 26992 26993 26994 26996 26997 26998 27001 27002 27003 27030 27031 27033 27035 27037 27039 27046 27047 27049 27051 27056 27059 27068 27070 27071 27072 27073 27075 27082 27088 27089 27090 27092 27093 27094 27096 27097 27106 27107 27112 27113 27114 27221 27222 27223 27225 27226 27227 27237 27239 27241 27242 27243 27244 27245 27246 27248 27249 27251 27253 27254 27256 27257 27259 27286 27287 27291 27292 27293 27294 27301 27303 27305 27307 27310 27311 27328 27329 27330 27337 27338 27339 27344 27345 27348 27349 27350 27352 27353 27355 27360 27361 27362 27364 27366 27368 27369 27392 27393 27394 27401 27404 27405 27407 27408 27409 27413 27414 27417 27425 27428 27429 27665 27668 27669 27672 27674 27684 27685 27686 27689 27690 27691 31403 31412 31420 31421 31423 31434 31438 31439 31459 31460 31461 31462 31464 31466 36862https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/832/126?format=asciiRadiodefaultJ/ApJ/832/126/table1REsolved Spectroscopy Of a Local VolumE (RESOLVE) 21cm catalog; from erratum published in 2017, ApJ, 851, 153recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNameRESOLVE designation (rfNNNN or rsNNNN)meta.id;meta.maincharprimaryEnvmeta.ref.urlintnullableRAJ2000Galaxy Right Ascension (J2000)degpos.eq.ra;meta.mainDEJ2000Galaxy Declination (J2000)degpos.eq.dec;meta.mainTelTelescope used for observation (1)instr.setupcharF21[0.01/17.5] Total 21cm fluxJy.km/sphot.flux.density;em.radio.750-1500MHzfloate_F21[0.01/9]? Uncertainty on F21Jy.km/sstat.errorfloatnullablerms[0.1/8.4] RMS noise of spectrum assuming 10km/s channelsmJyinstr.det.noisefloatLimFlag indicating upper limit on F21 (1=upper limit; 692 instances)meta.codeintConfFlag indicating 21cm emission likely confused (1=confused; 251 instances)meta.code.error;phys.emissMeasureintF21c[0.01/12.3]? Total 21cm flux after correction for confusionJy.km/sphot.flux.density;em.radio.750-1500MHzfloatnullablee_F21c[0.01/0.4]? Statistical uncertainty on total 21cm flux after correction for confusionJy.km/sstat.errorfloatnullables_F21c[0.01/11]? Additional systematic uncertainty on total 21cm flux after correction for confusionJy.km/sstat.error.sys;phot.flux.density;em.radio.750-1500MHzfloatnullableMode[0/3]? Method used to correct 21cm flux for confusion and determine the additional systematic uncertainty (2)phot.flux;em.radio.750-1500MHzintnullableSloanDisplay the online SDSS data for the nearest objectmeta.ref.urlcharSimbadSimbad column added by the CDSmeta.ref.urlcharJ/ApJ/832/126/table2RESOLVE environment metricsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNameRESOLVE designation (1)meta.id;meta.maincharF21meta.ref.urlintnullableID-s[10001/16319]? Group dark matter halo ID, stellar mass-limited sample (2)meta.id;src.sampleintnullableMass-s[11/14.3]? Group dark matter halo mass, log, stellar mass-limited samplelog(solMass)phys.massfloatnullableID-b[20001/26603]? Group dark matter halo ID, baryonic mass-limited sample (2)meta.id;src.sampleintnullableMass-b[10/14.1]? Group dark matter halo mass, log, baryonic mass-limited samplelog(solMass)phys.massfloatnullableDen-s[9/14.5]? Large-scale structure density, log, stellar mass-limited sample groups, uncorrected for edge-effectslog(solMass.Mpc**-2)phys.densityfloatnullableDenc-s[9.6/14.5]? Large-scale structure density, log, stellar mass-limited sample groups, corrected for edge-effectslog(solMass.Mpc**-2)phys.densityfloatnullableDen-b[8/14.1]? Large-scale structure density, log, baryonic mass-limited sample groups, uncorrected for edge-effectslog(solMass.Mpc**-2)phys.densityfloatnullableDenc-b[9.5/14.1]? Large-scale structure density, log, baryonic mass-limited sample groups, corrected for edge-effectslog(solMass.Mpc**-2)phys.densityfloatnullableDist-s[0.2/62.5]? Projected distance to nearest M_h>10^12^ halo, stellar mass-limited sample groups (3)(4)pos.distancefloatnullablef_Dist-sReliability Flag for dist-s (5)meta.codeintDist-b[0.03/63.3]? Projected distance to nearest M_h>10^12^ halo, baryonic mass-limited sample groups (4)(3)pos.distancefloatnullablef_Dist-bReliability Flag for dist-b (5)meta.codeintSimbadSimbad column added by the CDSmeta.ref.urlchar_RAPositions from Eckert+, 2015, J/ApJ/810/166 (right ascension part)degpos.eq.ra;meta.main_DEPositions from Eckert+, 2015, J/ApJ/810/166 (declination part)degpos.eq.dec;meta.main