J/MNRAS/390/466ivo://CDS.VizieR/J/MNRAS/390/466doi:10.26093/cds/vizier.73900466CDSEpinat B.Amram P.Marcelin M.2024-07-07T20:17:08Z2010-04-27T12:16:44ZCDS support team

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

cds-question@unistra.frgalaxiescatalogsradial-velocitygalaxy-classification-systemsThe Gassendi HAlpha survey of SPirals survey (GHASP) consists of 3D H{alpha} data cubes for 203 spiral and irregular galaxies, covering a large range in morphological types and absolute magnitudes, for kinematics analysis. It is the largest sample of Fabry-Perot data published up to now. In order to provide an homogenous sample, reduced and analysed using the same procedure, we present in this paper the new reduction and analysis for a set of 97 galaxies already published in previous papers but now using the new data reduction procedure adopted for the whole sample. The GHASP survey is now achieved and the whole sample is reduced using the adaptive binning techniques based on Voronoi tessellations. We have derived H{alpha} data cubes from which are computed H{alpha} maps, radial velocity fields as well as residual velocity fields, position-velocity diagrams, rotation curves and kinematical parameters for almost all galaxies. The rotation curves, the kinematical parameters and their uncertainties are computed homogeneously using the new method based on the power spectrum of the residual velocity field. This paper provides the kinematical parameters for the whole sample. For the first time, the integrated H{alpha} profiles have been computed and are presented for the whole sample. The total H{alpha} fluxes deduced from these profiles have been used in order to provide a flux calibration for the 203 GHASP galaxies. This paper confirms the conclusions already drawn from half the sample concerning (i) the increased accuracy of position angles measurements using kinematical data, (ii) the difficulty to have robust determinations of both morphological and kinematical inclinations in particular for low-inclination galaxies and (iii) the very good agreement between the Tully-Fisher relationship derived from our data and previous determinations found in the literature.2008MNRAS.390..466Ehttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/390/466CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toJ/MNRAS/388/500 : GHASP: H{alpha} data cubes for 108 galaxies (Epinat+, 2008)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/390/466https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/390/466http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/390/466https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/390/466https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/390/466http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/MNRAS/390/466GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/MNRAS/390/466/galaxies (Galaxy parameters, model and calibration)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/390/466/galaxies?https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/390/466/galaxies?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/390/466/galaxies?GETtext/xml+votable180.050000true0.11666717.2191670.0055555555555555566/700 816 896 909 922 932-933 955 1892 2013 2121 2155 2254 2320 2347 2359 2363 2372 2380 2382 2400 2564 2687 3085 3389 3446 3516 3860 3910 4149 4469 4471 4599 4719 4820 5080 5096 5142 5174 5200 5241 5244 5306 5309 5329 5545 5581 5584 5596 5636 5639 5710 5814 5982 6034 6204 6216 6337 6411 6448 6519 6604-6605 6609 6619 6623 6649 6780 6948 7110 7137 7303 7584 7604 7659 7726 7799 7808 7878 7915 7957 8010-8011 8106 8113 8169 8173 8225 8458 9149 9277 9437 9855 9869 10014 10490 10601 10628 10674 10711 10723 10799 10841 10900-10901 10911-10912 10935 11127 11140 11227 11306 11371 11389 11392 11434 11446 11448 11460 11566 11582 11639 11681 11696 11724 11726 11738 11750 11772 11789 11800 12025 12047 12122 12619 13130 13162 13391 13472 13489 13510-13511 13516 13609 13611 13668 13944 13948 14033 14777 14935 15068 15161 15197 15551 15592 15981 16050 16098 16114 16120 16194 17905 18011 19708 20000 20254 20270 23872 23921 26068 26331 26983 27090 27331 27351 27606 27654 27955 28053 28208 28251 28496 28535 28612 28631 30529 32729https://cdsarc.cds.unistra.fr/viz-bin/moc/J/MNRAS/390/466?format=asciiOpticaldefaultJ/MNRAS/390/466/galaxiesGalaxy parameters, model and calibrationrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintn_NameSimbad column added by the CDSmeta.ref.urlcharNameGalaxy namemeta.id;meta.maincharprimaryrotplot the rotation curvemeta.ref.urlcharTMorphological type from the de Vaucouleurs classification (de Vaucouleurs 1979, VII/155) in HyperLeda data basesrc.morph.typefloate_Trms uncertainty on T Typestat.errorfloatMTypeMorphological type from HyperLeda data basesrc.morph.typecharDistDistance (5)Mpcpos.distance;pos.heliocentricfloatr_DistReference for Distance (6)meta.ref;pos.framecharBMAG? Absolute B magnitude from Dist and apparent corrected B magnitude (HyperLeda)magphot.mag;em.opt.Bfloatnullableb/aAxis ratio from HyperLedaphys.angSize;arith.ratiofloate_b/arms uncertainty on b/astat.errorfloatiInclination derived from the axis ratio (arccos(b/a))degphys.angSizeinte_irms uncertainty on idegstat.errorintD25Isophotal radius at the limiting surface brightness of 25 Bmag/arcsec^2^, in arcsec (7)arcsecphys.angSizeinte_D25rms uncertainty on D25arcsecstat.errorintD25kpcIsophotal radius at the limiting surface brightness of 25 Bmag/arcsec^2^, in kpc (7)kpcpos.distancefloate_D25kpcrms uncertainty on D25kpckpcstat.errorfloatr_D25[*] an asterisk (*) indicates that the galaxy is larger than GHASP field of viewmeta.ref;pos.framecharVmax? Maximum velocitykm/sspect.dopplerVeloc;pos.heliocentricintnullablee_Vmax? rms uncertainty on Vmaxkm/sstat.errorintnullablen_Vmax[PV ] PV = Vmax from Position-Velocity diagram (from fit of velocity field otherwise)meta.notecharf_Vmax[1/4]? Vmax reached (8)meta.codeintnullableHI[VW] VLA or WHISP datameta.id;instr.obstycharr_HIReferences for aperture synthesis HI data (9)meta.ref;pos.framecharVsysLSystemic velocity found in HyperLeda data basekm/sphys.velocinte_VsysLrms uncertainty on VsysLkm/sstat.errorintVsys? Systemic velocity deduced from our velocity field analysiskm/sphys.velocintnullablee_Vsys? rms uncertainty on Vsyskm/sstat.errorintnullableiMMorphological inclination from HyperLeda (Paturel et al., 1997, Cat. VII/237)degsrc.morphinte_iMrms uncertainty on iMdegstat.errorintiK? Inclination deduced from the analysis of our velocity fielddegsrc.orbital.inclinationintnullablee_iK? rms uncertainty on iKdegstat.errorintnullablen_iK[*] * for fixed value (3)meta.notecharPA1? Morphological position angledegpos.posAngintnullabler_PA1[M] Reference for PA1 (4)meta.ref;pos.framecharPA2? Morphological position angledegpos.posAngintnullabler_PA2[Ha ] Reference for PA2 (4)meta.ref;pos.framecharPA3? Morphological position angledegpos.posAngintnullabler_PA3[M Pa Va] Reference for PA3 (4)meta.ref;pos.framecharPA4? Morphological position angledegpos.posAngintnullabler_PA4[Ha M Ni Pa] Reference for PA4 (4)meta.ref;pos.framecharPA? Morphological position angledegpos.posAngintnullabler_PA[Ha M Ni Pa A Sp] Reference for PA (4)meta.ref;pos.framechare_PA? rms uncertainty on PAdegstat.errorintnullablePA-FP? Position angle deduced from our velocity fielddegpos.posAngintnullablen_PA-FP[a] a indicates that the position angle refers to the approaching sidemeta.notechare_PA-FP? rms uncertainty on PA-FPdegstat.errorintnullablef_PA-FP[*] * for PA that have been fixed equal to morphological valuemeta.codecharl_VresLimit flag on Vresmeta.code.errorcharVres? Mean residual velocity on the whole velocity fieldm/sstat.fit.residual;phys.veloc;stat.meanfloatnullablesigres? Residual velocity dispersion on the whole velocity fieldkm/sstat.fit.residual;phys.velocintnullablechi2? Reduced {chi}^2^ of the modelstat.fit.chi2floatnullableSimbadDetails from SIMBAD databasemeta.ref.urlcharNEDSimbad column added by the CDScharLEDASimbad column added by the CDScharUGC? UGC numbermeta.idintnullablem_UGC[c] Multiplicity index on UGCmeta.code.multipcharNGC? NGC numbermeta.idintnullablem_NGC[A] Multiplicity index on NGCmeta.code.multipcharRAJ2000Right ascension (J2000) (1)pos.eq.ra;meta.mainDEJ2000Declination (J2000) (1)pos.eq.dec;meta.mainExpTimeExposure timestime.duration;obs.exposureintScalePixel scale (arcsec/pix)arcsecinstr.scalefloatl_Flux[>= ] Limit flag on Fluxmeta.code.error;phot.fluxcharFlux? Integrated H{alpha} flux deduced from the comparison with James et al. (2004, Cat. J/A+A/414/23) data (2)1e-16W.m**-2phot.flux;em.line.Halphafloatnullablee_Flux? rms uncertainty on Flux1e-16W.m**-2stat.error;phot.fluxfloatnullablePapPublication papersmeta.bibcharJ/MNRAS/390/466/tablefRotation curves for 82 galaxiesrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNameGalaxy namemeta.id;meta.maincharrGalactic radius, in kpckpcphys.size.radius;pos.galacticfloate_rDispersion around the galactic radius in kpckpcstat.errorfloatr2Galactic radius, in arcsecarcsecphys.size.radiusfloate_r2Dispersion around the galactic radius in arcsecarcsecstat.errorfloatVrotRotation velocitykm/sphys.veloc.rotatinte_VrotDispersion on the rotation velocitykm/sstat.errorintNbinsNumber of velocity binsmeta.numberintSide[ar] Receding - r - or approaching - a - sidemeta.codechar