J/A+A/595/A118ivo://CDS.VizieR/J/A+A/595/A118doi:10.26093/cds/vizier.35950118CDSvan Driel M.Butcher Z.Schneider S.Lehnert M.Minchin R.Blyth S-L.,Chemin L.Hallet N.Joseph T.Kotze P.Kraan-Korteweg R.C.Olofsson H.,Ramatsoku M.2019-02-01T06:58:11Z2016-11-11T15:24:09ZCDS support team

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

cds-question@unistra.frradio-galaxiesh-i-line-emissionvisible-astronomysloan-photometryradial-velocityTo investigate galaxy properties as a function of their total stellar mass, we obtained 21cm HI line observations at the 100-m class Nancay Radio Telescope of 2839 galaxies from the Sloan Digital Sky Survey (SDSS) in the Local Volume (900<cz<12000km/s), dubbed the Nancay Interstellar Baryons Legacy Extragalactic Survey (NIBLES) sample. They were selected evenly over their entire range of absolute SDSS z-band magnitudes (Mz~-13.5 to -24mag), which were used as a proxy for their stellar masses. In this paper, a first, global presentation of the observations and basic results is given; their further analysis will be presented in other papers in this series. The galaxies were originally selected based on their properties, as listed in SDSS DR5. Comparing this photometry to their total HI masses, we noted that, for a few percent, the SDSS magnitudes appeared severely misunderestimated, as confirmed by our re-measurements for selected objects. Although using the later DR9 results eliminated this problem in most cases, 384 still required manual photometric source selection. Usable HI spectra were obtained for 2600 of the galaxies, of which 1733 (67%) were clearly detected and 174 (7%) marginally. The spectra for 241 other observed galaxies could not be used for further analysis owing to problems with either the HI or the SDSS data. We reached the target number of about 150 sources per half-magnitude bin over the Mz range -16.5 to -23mag. Down to -21mag the overall detection rate is rather constant at the ~75% level but it starts to decline steadily towards the 30% level at -23mag. Making regression fits by comparing total HI and stellar masses for our sample, including our conservatively estimated HI upper limits for non-detections, we find the relationship log(MHI/M*)=-0.59log(M*)+5.05, which lies significantly below the relationship found in the MHI/M*-M* plane when only using HI detections.2016A&A...595A.118Vhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/595/A118CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/595/A118https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/595/A118http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/595/A118https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/595/A118https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/595/A118http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/595/A118GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/A+A/595/A118/tablea3 (Basic optical and HI data - non-detected galaxies)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/595/A118/tablea3?https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/595/A118/tablea3?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/595/A118/tablea3?GETtext/xml+votable180.050000true0.199583314.27752780.005555555555555556Cone search capability for table J/A+A/595/A118/tablea5 (Basic optical and HI data - galaxies with V<850km/s not used for further analysis)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/595/A118/tablea5?https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/595/A118/tablea5?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/595/A118/tablea5?GETtext/xml+votable180.050000true46.6950.46952780.005555555555555556Cone search capability for table J/A+A/595/A118/tablea12 (Basic optical and HI data - clearly and marginally detected galaxies (tables A1 and A2 of the paper))https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/595/A118/tablea12?https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/595/A118/tablea12?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/595/A118/tablea12?GETtext/xml+votable180.050000true0.0087515.88169440.0055555555555555565/1201 1254 1349 1357 1407-1409 1495 1501 1527 1563 1642 1685 2621 2648 2656 2659 2795 2950 4309 4389 4697 4960 4998 6486 6913 6917 6943 6978 7008 9182 6/0 552-554 640 4096 4105 4108-4110 4114 4123 4125 4136 4142 4144 4147 4149 4167 4179-4180 4182 4188 4197 4210 4213 4224-4225 4228-4229 4232 4236 4249 4279 4302 4322 4328 4334 4346 4348 4354 4359 4410 4438-4439 4443 4445-4447 4452 4469 4471 4473 4484 4491 4511 4519 4550 4575 4577 4583 4598-4599 4602 4633 4642 4654-4655 4660 4682 4686-4688 4691 4695 4697-4698 4706 4708 4712-4713 4716 4718-4720 4725 4733-4734 4740 4743 4751 4753 4756 4767 4769 4787 4799 4801-4803 4809 4813 4815-4816 4821 4823 4825-4826 4828-4829 4831 4833-4834 4840 4843-4844 4850-4852 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26083 26087-26088 26090-26091 26093 26100 26102 26141 26161 26163 26167-26168 26175 26178 26184 26187 26189 26191 26198 26209 26211 26214 26217 26222-26223 26225-26227 26233-26234 26241 26249 26251 26260 26263-26264 26278 26280 26283-26284 26287-26288 26291 26296-26297 26299-26300 26302 26304 26306-26309 26311-26312 26316-26317 26320-26322 26328 26330 26336 26338 26343-26344 26349 26365 26371 26375 26377 26388-26389 26397 26400 26403-26404 26412 26414 26423-26424 26432 26436 26445-26446 26451 26453 26459 26461 26463 26466 26472 26486 26493-26496 26517-26519 26548 26555 26563 26584 26592 26596 26910 26946 26951-26952 26955 26960 26963 26967 26969-26970 26977-26979 26983 26991-26993 26995 27000-27001 27003 27028 27045 27047 27049 27056 27062 27064 27079 27085 27087 27090-27091 27093 27097 27109-27110 27129 27132 27135 27199 27250 27253 27255 27257 27259 27285 27287 27310-27311 27314-27315 27324 27328 27331 27334 27340 27345 27347-27348 27350 27364-27365 27372 27379 27384 27413 27423 27426-27427 27431 27439 27458 27477 27480 27485 27491 27496 27502 27509-27510 27512-27513 27515 27518 27520 27525 27527-27528 27540 27554-27556 27558 27562 27567 27571 27578 27588 27599 27601 27603-27604 27606 27608 27613 27621 27656-27657 27664 27666 27674 27680 27683 27685 27697 27712 27714 27727 27731 27735-27738 27740-27742 27748-27749 27751 27758-27761 27763 27766-27767 27769-27771 27799-27802 27806 27811-27812 27814 27818-27820 27823 27828 27833 27838 27849 27853 27855-27857 27859 27861-27863 27869 27874-27876 27878 27882-27883 27896 27898 27907-27910 27917-27918 27922 27924 27926 27929 27931 27937-27938 27940 27943 27947-27948 27951 27968 28125 28160 28162 28165 28167-28170 28172 28175 28178 28180-28181 28183 28188 28200-28201 28207-28208 28211 28218 28220 28225-28227 28290-28291 28293-28295 28304 28382 28404-28406 28412 28414 28458 28461 28463 28466 28471 28473 28477 28489 28491 28493 28495 28498 28513 28515 28517 28526 28528 28537 28539 28548 28555 28565 28567 28572 28574 28576 28585 28587 28593-28594 28596 28598-28599 28604 28607-28608 28610 28617-28618 28633 28635 28638-28639 28646 28651 28659 28663 28666 28670 31369 31372-31373 31381-31382 31399 31404 31406-31407 31418 31420 31422 31426 31440 31455 31458 31624 31626 31628-31629 31632 31735 32427 32462 32480 32482 36703 36717 36719 36732-36734 36767 36773 36775 36777-36778 36785 36790 36793 36803 36805-36806 36808-36809 36861 36863 45050 45054-45055 49014 49016 49018-49019 49086 49097 49101 49124 49128 49149-49150https://cdsarc.cds.unistra.fr/viz-bin/moc/J/A+A/595/A118?format=asciiRadioOpticaldefaultJ/A+A/595/A118/tablea3Basic optical and HI data - non-detected galaxiesrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintSourceSource numbermeta.idintFlagFlags regarding the SDSS and NRT datameta.code.errorcharRAJ2000Right ascension (J2000.0)pos.eq.ra;meta.mainDEJ2000Declination (J2000.0)pos.eq.dec;meta.mainNameCommon catalog name, other than the SDSSmeta.idcharVoptOptical heliocentric radial velocity, czkm/sspect.dopplerVeloc.opt;pos.heliocentricinte_Voptrms uncertainty on Voptkm/sstat.errorintg-zSDSS g-z colour index, based on model magnitudesmagphot.colorfloatgMAGSDSS absolute g-band model magnitudemagphys.magAbsfloatlog(M*)? Logarithm of the MEDIAN total stellar mass estimatelog(solMass)phys.massfloatnullablelog(sSFR)? Logarithm of the specific Star Formation Rate, or SFR/M*log(yr**-1)phys.SFRfloatnullablermsrms noise level values of the HI spectramJyinstr.det.noisefloatSNRPeak signal-to-noise ratiostat.snr;stat.maxfloatl_log(MHI)Limit flag on logMHImeta.code.errorcharlog(MHI)HI masslog(solMass)phys.massfloatl_log(MHI/M*)limit flag on logMHI/M*meta.code.errorcharlog(MHI/M*)Logarithm of the ratio of the total HI and stellar massesphys.mass;arith.ratiofloatJ/A+A/595/A118/tablea5Basic optical and HI data - galaxies with V<850km/s not used for further analysisspShow the spectrummeta.ref.urlcharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintSourceInternal source numbermeta.idintFlagFlags regarding the SDSS and NRT datameta.code.errorcharRAJ2000Right ascension (J2000.0)pos.eq.ra;meta.mainDEJ2000Declination (J2000.0)pos.eq.dec;meta.mainNamecommon catalog name, other than the SDSSmeta.idcharVoptOptical heliocentric radial velocity, czkm/sspect.dopplerVeloc.opt;pos.heliocentricinte_VoptUncertainty in Voptkm/sstat.errorintg-r? SDSS g-r band color, based on model magnitudesmagphot.color;em.opt.B;em.opt.RfloatnullablegMAGSDSS absolute g-band model magnitudemagphys.magAbsfloatlog(M*)? Logarithm of the MEDIAN total stellar mass estimatelog(solMass)phys.massfloatnullablelog(sSFR)? Logarithm of the specific Star Formation Rate, or SFR/M*log(yr**-1)phys.SFRfloatnullablermsrms noise level values of the HI spectramJyinstr.det.noisefloatVHIHeliocentric HI radial velocitykm/sspect.dopplerVeloc;em.line.HI;spect.lineinte_VHIUncertainty in VHIkm/sstat.errorintW50HI profile velocity width measured at 50% of the peak levelkm/sspect.line.width;em.line.HIintW20HI profile velocity width measured at 20% of the peak levelkm/sspect.line.width;em.line.HIintFHIIntegrated measured HI line fluxJy.km/sphot.flux.density;em.line.HI;spect.linefloate_FHIUncertainty in FHIJy.km/sstat.errorfloatSNRPeak signal-to-noise ratiostat.snr;stat.maxfloatS/NSignal-to-noise ratio determined taking into account the HI line widthspect.line.width;em.line.HIfloatlog(MHI)Logarithm of the total HI masslog(solMass)phys.massfloatlog(MHI/M*)? 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Logarithm of the ratio of the total HI and stellar massesphys.mass;arith.ratiofloatnullable