J/A+A/596/A60ivo://CDS.VizieR/J/A+A/596/A60doi:10.26093/cds/vizier.35960060CDSButcher Z.Schneider S.van Driel W.Lehnert M.Minchin R.2018-08-31T09:02:21Z2016-11-30T08:59:14ZCDS support team

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

cds-question@unistra.frgalaxiesphotometryspectroscopyradio-astronomyh-i-line-emissionWe obtained Arecibo HI line follow-up observations of 154 of the 2600 galaxies in the Nancay Interstellar Baryons Legacy Extragalactic Survey (NIBLES) sample. These observations are on average four times more sensitive than the original observations at the Nancay Radio Telescope. The main goal of this survey is to characterize the underlying HI properties of the NIBLES galaxies which were undetected or marginally detected at Nancay. Of the Nancay non-detections, 85% were either clearly or marginally detected at Arecibo, while 89% of the Nancay marginal detections were clearly detected. Based on the statistics of the detections relative to g-i color and r-band luminosity (Lr) distribution among our Arecibo observations, we anticipate ~60% of our 867 Nancay non-detections and marginal detections could be detected at the sensitivity of our Arecibo observations. Follow-up observations of our low luminosity (Lr<10^8.5^L_{sun}_) blue sources indicate that they have, on average, more concentrated stellar mass distributions than the Nancay detections in the same luminosity range, suggesting we may be probing galaxies with intrinsically different properties. These follow-up observations enable us to probe HI mass fractions, log(MHI/M*) 0.5dex and 1dex lower, on average, than the NIBLES and ALFALFA surveys respectively.2016A&A...596A..60Bhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/596/A60CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toJ/A+A/595/A118 : NIBLES. I. The Nancay HI survey (van Driel+, 2016)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/596/A60https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/596/A60http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/596/A60https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/596/A60https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/596/A60http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/596/A60GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/A+A/596/A60/table4 (Basic optical and HI data - comparison of Arecibo and Nancay detections)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/596/A60/table4?https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/596/A60/table4?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/596/A60/table4?GETtext/xml+votable180.050000true5.202514.22438890.005555555555555556Cone search capability for table J/A+A/596/A60/table5 (Basic optical and HI data - Arecibo detected galaxies not included in the final Nancay sample)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/596/A60/table5?https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/596/A60/table5?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/596/A60/table5?GETtext/xml+votable180.050000true20.26229170.85147220.005555555555555556Cone search capability for table J/A+A/596/A60/table1 (Basic optical and HI data - Arecibo detections of Nancay non-detections and marginals)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/596/A60/table1?https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/596/A60/table1?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/596/A60/table1?GETtext/xml+votable180.050000true2.6062514.28972220.005555555555555556Cone search capability for table J/A+A/596/A60/table2 (Basic optical and HI data - Arecibo marginal detections of Nancay non-detections)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/596/A60/table2?https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/596/A60/table2?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/596/A60/table2?GETtext/xml+votable180.050000true46.24150.95391670.005555555555555556Cone search capability for table J/A+A/596/A60/table3 (Marginal and confused Nancay detections are flagged with an M and K respectively)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/596/A60/table3?https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/596/A60/table3?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/596/A60/table3?GETtext/xml+votable180.050000true143.511666710.10869440.0055555555555555566/0 553 4125 4182 4188 4197 4224 4228 4323 4334 4354 4471 4599 4718 4767 4803 4806 4826 4840 4869 4914 4942 4986 5016 5022 5066 5147 5158 5190 5200-5201 5295 5396 5633 5641 6363 8283 8362-8363 8382 8394 8545 8683 8936 9118 9184 9186 9760 9772 10308 10350 10417 10522 10773 12379 12381 12391 12405 12408 12551 12553 12555-12556 12568 17750 18013 18850-18851 18859 19022 19042 19047 19049 19054 19097 19108 19115 19117 19121 19387 19401-19402 19667 19669-19671 19987 21853 23211 25967 25977 25979 26074 26091 26222 26288 26451 26453 26459 26472 26495 26584 26596 27079 27135 27257 27426 27431 27485 27509 27525 27554 27556 27571 27606 27608 27657 27666 27680 27727 27856 27896 28035 28165 28180 28284 28293-28294 28304 28458 28477 28567 28576 28585 28596 28618 31399 31420 31440 31735https://cdsarc.cds.unistra.fr/viz-bin/moc/J/A+A/596/A60?format=asciiRadiodefaultJ/A+A/596/A60/table4Basic optical and HI data - comparison of Arecibo and Nancay detectionsSimbadNameSimbad column added by the CDSmeta.idcharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintspShow the spectrummeta.ref.urlcharSourceSource numbermeta.idintn_Source[CDKR3 ] Note (G1)meta.notecharRAJ2000Right ascension (J2000)pos.eq.ra;meta.mainDEJ2000Declination (J2000)pos.eq.dec;meta.mainNameCommon name, other than SDSSmeta.id;meta.maincharVoptOptical heliocentric radial velocity (cz)km/sspect.dopplerVeloc.opt;pos.heliocentricinte_Voptrms uncertainty on Voptkm/sstat.errorintg-zg-z integrated colour index of the galaxy using SDSS model magnitudes, corrected for Galactic extinction, following Schlegel et al. (1998ApJ...500..525S)magphot.colorfloatgMAGIntegrated absolute g magnitude, corrected for Galactic extinction, following Schlegel et al. (1998ApJ...500..525S)magphys.magAbsfloatlogM*? Total median stellar mass estimatelog(solMass)phys.massfloatnullablelogsSFR? Specific star formation rate, or SFR/M*log(yr**-1)meta.idfloatnullablermsAOArecibo rms noise level value of HI spectramJyinstr.det.noisefloatrmsNRTNancay rms noise level value of HI spectramJyinstr.det.noisefloatVHIAOArecibo heliocentric radial velocity (cz) of the center of the HI line profilekm/sspect.dopplerVeloc;pos.heliocentricinte_VHIAOrms uncertainty on VHIAOkm/sstat.errorintVHINRTNancay heliocentric radial velocity (cz) of the center of the HI line profilekm/sspect.dopplerVeloc;pos.heliocentricinte_VHINRTrms uncertainty on VHINRTkm/sstat.errorintW50AOArecibo velocity width measured at 50% of the HI profile peak level, uncorrected for galaxy inclinationkm/sspect.line.widthintW50NRTNancay velocity width measured at 50% of the HI profile peak level, uncorrected for galaxy inclinationkm/sspect.line.widthintFHIAOArecibo integrated HI line fluxJy.km/sphot.flux.density;em.line.HI;spect.linefloate_FHIAOrms uncertainty on FHIAOJy.km/sstat.errorfloatFHINRTNancay integrated HI line fluxJy.km/sphot.flux.density;em.line.HI;spect.linefloate_FHINRTrms uncertainty on FHINRTJy.km/sstat.errorfloatS/NAOArecibo signal-to-noise ratio (G2)stat.snrfloatS/NNRTNancay signal-to-noise ratio (G2)stat.snrfloatlogMHIAOArecibo total HI masslog(solMass)phys.massfloatlogMHINRTNancay total HI masslog(solMass)phys.massfloatspectrumDisplay the spectrum filemeta.ref.urlcharNEDNED column added by the CDSmeta.ref.urlcharJ/A+A/596/A60/table5Basic optical and HI data - Arecibo detected galaxies not included in the final Nancay sampleSimbadNameSimbad column added by the CDSmeta.idcharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintspShow the spectrummeta.ref.urlcharSourceSource numbermeta.idintn_Source[MDK ] Note (G1)meta.notecharRAJ2000Right ascension (J2000)pos.eq.ra;meta.mainDEJ2000Declination (J2000)pos.eq.dec;meta.mainNameCommon name, other than SDSSmeta.id;meta.maincharVoptOptical heliocentric radial velocity (cz)km/sspect.dopplerVeloc.opt;pos.heliocentricinte_Voptrms uncertainty on Voptkm/sstat.errorintg-zg-z integrated colour index of the galaxy using SDSS model magnitudes, corrected for Galactic extinction, following Schlegel et al. (1998ApJ...500..525S)magphot.colorfloatgMAGIntegrated absolute g magnitude, corrected for Galactic extinction, following Schlegel et al. (1998ApJ...500..525S)magphys.magAbsfloatlogM*? Total median stellar mass estimatelog(solMass)phys.massfloatnullablelogsSFR? Specific star formation rate, or SFR/M*log(yr**-1)meta.idfloatnullablermsrms noise level value of HI spectramJyinstr.det.noisefloatVHI? Heliocentric radial velocity (cz) of the center of the HI line profilekm/sspect.dopplerVeloc;pos.heliocentricintnullablee_VHI? rms uncertainty on VHIkm/sstat.errorintnullableW50? Velocity width measured at 50% of the HI profile peak level, uncorrected for galaxy inclinationkm/sspect.line.widthintnullableW20? Velocity width measured at 20% of the HI profile peak level, uncorrected for galaxy inclinationkm/sspect.line.widthintnullableFHI? Integrated HI line fluJy.km/sphot.flux;em.line.HI;spect.linefloatnullablee_FHI? rms uncertainty on FHIJy.km/sstat.errorfloatnullableSNRPeak signal-to-noise ratio (3)stat.snr;stat.maxfloatS/N? Signal-to-noise ratio determined taking into account the line width (G2)stat.snr;spect.line.widthfloatnullablel_logMHILimit flag on logMHImeta.code.errorcharlogMHIHI masslog(solMass)phys.massfloatl_logMHI/M*Limit flag on logMHI/M*meta.code.errorcharlogMHI/M*? HI to stellar mass ratiophys.mass;arith.ratiofloatnullablespectrumDisplay the spectrum filemeta.ref.urlcharNEDNED column added by the CDSmeta.ref.urlcharJ/A+A/596/A60/table1Basic optical and HI data - Arecibo detections of Nancay non-detections and marginalsSimbadNameSimbad column added by the CDSmeta.idcharSNRPeak signal-to-noise ratio (3)stat.snr;stat.maxfloatSourceSource numbermeta.idintrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintspShow the spectrummeta.ref.urlcharn_Source[MDK ] Note (G1)meta.notecharRAJ2000Right ascension (J2000)pos.eq.ra;meta.mainDEJ2000Declination (J2000)pos.eq.dec;meta.mainNameCommon name, other than SDSSmeta.id;meta.maincharVoptOptical heliocentric radial velocity (cz)km/sspect.dopplerVeloc.opt;pos.heliocentricinte_Voptrms uncertainty on Voptkm/sstat.errorintg-zg-z integrated colour index of the galaxy using SDSS model magnitudes, corrected for Galactic extinction, following Schlegel et al. (1998ApJ...500..525S)magphot.colorfloatgMAGIntegrated absolute g magnitude, corrected for Galactic extinction, following Schlegel et al. (1998ApJ...500..525S)magphys.magAbsfloatlogM*? Total median stellar mass estimatelog(solMass)phys.massfloatnullablelogsSFR? Specific star formation rate, or SFR/M*log(yr**-1)meta.idfloatnullablermsrms noise level value of HI spectramJyinstr.det.noisefloatVHI? Heliocentric radial velocity (cz) of the center of the HI line profilekm/sspect.dopplerVeloc;pos.heliocentricintnullablee_VHI? rms uncertainty on VHIkm/sstat.errorintnullableW50? Velocity width measured at 50% of the HI profile peak level, uncorrected for galaxy inclinationkm/sspect.line.widthintnullableW20? Velocity width measured at 20% of the HI profile peak level, uncorrected for galaxy inclinationkm/sspect.line.widthintnullableFHI? Integrated HI line fluJy.km/sphot.flux;em.line.HI;spect.linefloatnullablee_FHI? rms uncertainty on FHIJy.km/sstat.errorfloatnullableS/N? Signal-to-noise ratio determined taking into account the line width (G2)stat.snr;spect.line.widthfloatnullablel_logMHILimit flag on logMHImeta.code.errorcharlogMHIHI masslog(solMass)phys.massfloatl_logMHI/M*Limit flag on logMHI/M*meta.code.errorcharlogMHI/M*? HI to stellar mass ratiophys.mass;arith.ratiofloatnullablespectrumDisplay the spectrum filemeta.ref.urlcharNEDNED column added by the CDSmeta.ref.urlcharJ/A+A/596/A60/table2Basic optical and HI data - Arecibo marginal detections of Nancay non-detectionsSimbadNameSimbad column added by the CDSmeta.idcharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintspShow the spectrummeta.ref.urlcharSourceSource numbermeta.idintn_Source[MDK ] Note (G1)meta.notecharRAJ2000Right ascension (J2000)pos.eq.ra;meta.mainDEJ2000Declination (J2000)pos.eq.dec;meta.mainNameCommon name, other than SDSSmeta.id;meta.maincharVoptOptical heliocentric radial velocity (cz)km/sspect.dopplerVeloc.opt;pos.heliocentricinte_Voptrms uncertainty on Voptkm/sstat.errorintg-zg-z integrated colour index of the galaxy using SDSS model magnitudes, corrected for Galactic extinction, following Schlegel et al. (1998ApJ...500..525S)magphot.colorfloatgMAGIntegrated absolute g magnitude, corrected for Galactic extinction, following Schlegel et al. (1998ApJ...500..525S)magphys.magAbsfloatlogM*? Total median stellar mass estimatelog(solMass)phys.massfloatnullablelogsSFR? Specific star formation rate, or SFR/M*log(yr**-1)meta.idfloatnullablermsrms noise level value of HI spectramJyinstr.det.noisefloatVHI? Heliocentric radial velocity (cz) of the center of the HI line profilekm/sspect.dopplerVeloc;pos.heliocentricintnullablee_VHI? rms uncertainty on VHIkm/sstat.errorintnullableW50? Velocity width measured at 50% of the HI profile peak level, uncorrected for galaxy inclinationkm/sspect.line.widthintnullableW20? Velocity width measured at 20% of the HI profile peak level, uncorrected for galaxy inclinationkm/sspect.line.widthintnullableFHI? Integrated HI line fluJy.km/sphot.flux;em.line.HI;spect.linefloatnullablee_FHI? rms uncertainty on FHIJy.km/sstat.errorfloatnullableSNRPeak signal-to-noise ratio (3)stat.snr;stat.maxfloatS/N? Signal-to-noise ratio determined taking into account the line width (G2)stat.snr;spect.line.widthfloatnullablel_logMHILimit flag on logMHImeta.code.errorcharlogMHIHI masslog(solMass)phys.massfloatl_logMHI/M*Limit flag on logMHI/M*meta.code.errorcharlogMHI/M*? HI to stellar mass ratiophys.mass;arith.ratiofloatnullablespectrumDisplay the spectrum filemeta.ref.urlcharNEDNED column added by the CDSmeta.ref.urlcharJ/A+A/596/A60/table3Marginal and confused Nancay detections are flagged with an M and K respectivelySimbadNameSimbad column added by the CDSmeta.idcharlogM*? Total median stellar mass estimatelog(solMass)phys.massfloatnullableVoptOptical heliocentric radial velocity (cz)km/sspect.dopplerVeloc.opt;pos.heliocentricintrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintSourceSource numbermeta.idintn_Source[MDK ] Note (G1)meta.notecharRAJ2000Right ascension (J2000)pos.eq.ra;meta.mainDEJ2000Declination (J2000)pos.eq.dec;meta.mainNameCommon name, other than SDSSmeta.id;meta.mainchare_Voptrms uncertainty on Voptkm/sstat.errorintg-zg-z integrated colour index of the galaxy using SDSS model magnitudes, corrected for Galactic extinction, following Schlegel et al. (1998ApJ...500..525S)magphot.colorfloatgMAGIntegrated absolute g magnitude, corrected for Galactic extinction, following Schlegel et al. (1998ApJ...500..525S)magphys.magAbsfloatlogsSFR? Specific star formation rate, or SFR/M*log(yr**-1)meta.idfloatnullablermsrms noise level value of HI spectramJyinstr.det.noisefloatVHI? Heliocentric radial velocity (cz) of the center of the HI line profilekm/sspect.dopplerVeloc;pos.heliocentricintnullablee_VHI? rms uncertainty on VHIkm/sstat.errorintnullableW50? Velocity width measured at 50% of the HI profile peak level, uncorrected for galaxy inclinationkm/sspect.line.widthintnullableW20? Velocity width measured at 20% of the HI profile peak level, uncorrected for galaxy inclinationkm/sspect.line.widthintnullableFHI? Integrated HI line fluJy.km/sphot.flux;em.line.HI;spect.linefloatnullablee_FHI? rms uncertainty on FHIJy.km/sstat.errorfloatnullableSNRPeak signal-to-noise ratio (3)stat.snr;stat.maxfloatS/N? Signal-to-noise ratio determined taking into account the line width (G2)stat.snr;spect.line.widthfloatnullablel_logMHILimit flag on logMHImeta.code.errorcharlogMHIHI masslog(solMass)phys.massfloatl_logMHI/M*Limit flag on logMHI/M*meta.code.errorcharlogMHI/M*? HI to stellar mass ratiophys.mass;arith.ratiofloatnullablespectrumDisplay the spectrum filemeta.ref.urlcharNEDNED column added by the CDSmeta.ref.urlchar