J/MNRAS/394/340ivo://CDS.VizieR/J/MNRAS/394/340doi:10.26093/cds/vizier.73940340CDSGarcia-Appadoo D.A.West A.A.Dalcanton J.J.Cortese L.Disney M.J.2024-07-08T20:15:35Z2010-07-25T14:12:08ZCDS support team

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

cds-question@unistra.frgalaxiesphotometryh-i-line-emissionvisible-astronomysloan-photometryWe have used the Parkes Multibeam system and the Sloan Digital Sky Survey to assemble a sample of 195 galaxies selected originally from their HI signature to avoid biases against unevolved or low surface brightness objects. For each source nine intrinsic properties are measured homogeneously, as well as inclination and an optical spectrum. The sample, which should be almost entirely free of either misidentification or confusion, includes a wide diversity of galaxies ranging from inchoate, low surface brightness dwarfs to giant spirals. Despite this diversity there are five clear correlations among their properties. They include a common dynamical mass-to-light ratio within their optical radii, a correlation between surface brightness and luminosity and a common HI surface density. Such correlation should provide strong constrains on models of galaxy formation and evolution.2009MNRAS.394..340Ghttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/394/340CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toVIII/73 : HI Parkes All Sky Survey Catalogue (HIPASS) (Meyer+, 2004)II/294 : The SDSS Photometric Catalog, Release 7 (Adelman-McCarthy+, 2009)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/394/340https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/394/340http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/394/340https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/394/340https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/394/340http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/MNRAS/394/340GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/MNRAS/394/340/essample (Combined table from original tables)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/394/340/essample?https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/394/340/essample?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/394/340/essample?GETtext/xml+votable180.050000true3.65-0.7450.0055555555555555565/6573 7830 6/4105 8195 8198 17745 17747 17753 17755 17761 17767-17768 17776-17777 17818 18004 18006-18007 18012-18013 18024 18028 18032 18061 18066 18069 18081 18793 18800-18802 18837 21845 21858-21859 21864 21911 21970 23144 23204 23208 23210 25565 25581 25588 25591 25594 25599 25855 25918 25935 25958-25960 25970 25972 25974 25979 25999 26037 26044 26061 26063 26159 26168-26169 26174-26175 26178 26182 26185 26191 26194 26208 26211 26217 26222 26231 26234 26237 26241 26254 26260-26261 26265-26268 26270 26277 26279 26282 26287-26288 26290 26301-26302 26304 26306 26309 26317-26318 26320 26323-26324 26329-26331 26337-26338 26371-26372 26377 26388 26411-26412 26500 26946 26955 26960 26962 26979 26992 26997 27005 27028 27034 27052 27055 27058 27062 27064 27068 27071 27074 27079 27090 27098 27106 27120 27199 27246-27247 27253 27259 27279 27285 27328-27329 27331 27333 27340 27347 27368 27406 27426 27434 27650 27654 27656 27670 29973 31352 31400 31406 31424 31426 31436 36734 368632.040811542443644e-19 6.090060298487514e-19https://cdsarc.cds.unistra.fr/viz-bin/moc/J/MNRAS/394/340?format=asciiOpticalRadiodefaultJ/MNRAS/394/340/essampleCombined table from original tablesrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintHIPEQES source name (HHMM+DD, <HIPEQ JHHMM+DD> in Simbad)meta.id;meta.maincharm_HIPEQ[ab] Multiplicity index on HIPEQmeta.code.multipcharRAJ2000Fitted HI right ascension (J2000)pos.eq.ra;meta.mainDEJ2000Fitted HI declination (J2000)pos.eq.dec;meta.mainSpeakHI peak flux densityJyphot.flux.density;em.radio.750-1500MHzfloatSintIntegrated HI flux densityJy.km/sphot.flux.density;em.radio.750-1500MHzfloatVHIHI systematic velocity, Vsys, measured at the 20% level of peak flux densitykm/sstat.error.sysintW20Velocity linewidth, W20, measured at the 20% level of the peak fluxkm/sspect.line.widthintDistDistance (see text for description)Mpcpos.distance;pos.heliocentricfloatlogMHILogarithm of the HI mass, calculated using equation (3) (see text)log(solMass)phys.mass;meta.modelledfloatRAORight ascension of optical position of SDSS-DR2 source (J2000)pos.eq.raDEODeclination of optical position of SDSS-DR2 source (J2000)pos.eq.decumagPetrosian SDSS u magnitude (1)magphot.mag;em.opt.Ufloate_umagrms uncertainty on umagmagstat.error;phot.mag;em.opt.UfloatgmagPetrosian SDSS g magnitude (1)magphot.mag;em.opt.Bfloate_gmagrms uncertainty on gmagmagstat.error;phot.mag;em.opt.BfloatrmagPetrosian SDSS r magnitude (1)magphot.mag;em.opt.Rfloate_rmagrms uncertainty on rmagmagstat.error;phot.mag;em.opt.RfloatimagPetrosian SDSS i magnitude (1)magphot.mag;em.opt.Ifloate_imagrms uncertainty on imagmagstat.error;phot.mag;em.opt.IfloatzmagPetrosian SDSS z magnitude (1)magphot.mag;em.opt.Ifloate_zmagrms uncertainty on zmagmagstat.error;phot.mag;em.opt.IfloatR50g-band semimajor axes that encompass 50% of the total Petrosian fluxarcsecphys.angSize;srcfloate_R50rms uncertainty on PetroR50arcsecstat.errorfloatR90g-band semimajor axes that encompass 90% of the total Petrosian fluxarcsecphys.angSize;srcfloate_R90rms uncertainty on PetroR90arcsecstat.errorfloatDR7Details of the optical source from the SDSS-DR7 (Cat. II/294)meta.ref.urlchar