J/ApJS/276/59ivo://CDS.VizieR/J/ApJS/276/59doi:10.26093/cds/vizier/bb-8m-1vCDSSwaters R.A.Andersen D.R.Bershady M.A.Martinsson T.P.K.Scholz P.,Verheijen M.A.W.Westfall K.B.2026-08-03T07:26:13Z2026-02-09T08:40:46ZCDS support team

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

cds-question@unistra.frgalaxiescatalogsvisible-astronomyspectroscopyinfrared-photometryabsolute-magnitudeextinctiongalaxy-kinematicsline-intensitiesWe present H{alpha}-region integral-field spectroscopy for 137 low-inclination, intermediate to late-type galaxies. Spectroscopic data, obtained with SparsePak and the Bench Spectrograph on the WIYN 3.5m telescope, span 6475-6880 {AA} with an instrumental resolution of 13km/s ({sigma}). The spectral range includes H{alpha} and [NII]{lambda}{lambda}6548,6584 for every source, and in most cases includes [SII]{lambda}{lambda}6717,6731. We present and publicly release 18288 calibrated spectra and visually inspected Gaussian line fits to the H{alpha} emission. Most measurements yield a signal-to-noise ratio above 5 in integrated H{alpha} line flux, adequate to derive reliable line centroids and widths. Second kinematic components are required to adequately describe the emission-line profile in 15% of reliable data. The H{alpha} velocity dispersion distribution peaks at 18km/s, modestly increasing with H{alpha} surface brightness, reaching 20km/s at {Sigma}H{alpha}=10^40^erg/s/kpc^2^. Lower-flux secondary components, when present, have widths of ~50km/s. These results agree well with previous echelle measurements of nearby galaxies. Velocity-field analysis yields kinematic inclinations, with a sample mean of 26{deg}. Large kinematic asymmetries systematically affect kinematic inclination estimates in a small fraction of our sample. When deviations from circular motion are below 10% of the projected velocity, kinematic inclinations are consistent, within errors, to estimates from inverting the Tully-Fisher relation. This confirms previous disk-submaximality estimates for galaxies with regular kinematics based on inclinations derived from inverting the Tully-Fisher relation.2025ApJS..276...59Shttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/276/59CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toII/183 : UBVRI Photometric Standards (Landolt 1992)VII/233 : 2MASS All-Sky Extended Source Catalog (XSC) (IPAC/UMass, 2003-2006)J/AJ/114/2402 : Rotation curves of early-type galaxies (Courteau+, 1997)J/ApJ/533/744 : Calibration of the Tully-Fischer relation (Tully+, 2000)J/A+A/370/765 : HI synthesis observations in UMa cluster (Verheijen+, 2001)J/A+A/390/863 : CCD R Photometry of WHISP Dwarf Galaxies (Swaters, 2002)J/ApJS/166/505 : H{alpha} photometry of face-on galaxies (Andersen+, 2006)J/MNRAS/390/466 : GHASP: H{alpha} data cubes for 97 galaxies (Epinat+, 2008)J/ApJ/716/198 : The DiskMass survey. I. (Bershady+, 2010)J/MNRAS/401/2113 : GHASP: H{alpha} data cubes for 153 galaxies (Epinat+, 2010)J/MNRAS/465/123 : SAMI Galaxy Survey asymmetries (Bloom+, 2017)J/MNRAS/495/2265 : Veloc. dispersions in star-forming galaxies (Varidel+, 2020)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJS/276/59https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJS/276/59http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJS/276/59https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJS/276/59https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJS/276/59http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJS/276/59GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/ApJS/276/59/sample (Halpha velocity field parameters (Table 3) and photometric data and inverse Tully-Fisher inclinations (Table 4))https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJS/276/59/sample?https://vizier.iucaa.in/viz-bin/conesearch/J/ApJS/276/59/sample?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJS/276/59/sample?GETtext/xml+votable180.050000true0.95366287.47871470.0055555555555555566/43 528 556 957 2051 2142 2243 2257 2355 4446 4654 4731 4740 4825 4842 5096 5200 5341 5370 5975 5980 6011 6116 6353 6411 6483 6561 6637 7403 7576 7601 7672 7896 7898 7980 8064 8088 8287 8363 8558 8640 8642 9004 9098 9133 9368 9382 9471 9658 9794 9893-9894 9998 10171 10395 10469 10565 10589 10594 10682 10735 10781 10802 10895 10901 10987 11069 11118 11240 11306 11387 11693 11726 11772 11801 13381 13385 15260 17717 17727 17901 17912 18046 18229 18271 18394 18800 19273 19481 19510 19614 19746 19749 19978 19980 19983 19996 20008 20060 20140 20309 20318 22945 22956 23297 25996 26389 26584 27285 27650 27719 27763 27871 28054 28191 28201 28218 28237 28279 28416 28447 28579 28671 32669 45050https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJS/276/59?format=asciiOpticalInfrareddefaultJ/ApJS/276/59/sampleHalpha velocity field parameters (Table 3) and photometric data and inverse Tully-Fisher inclinations (Table 4)Arc[0.016/0.8]? Asymmetry measure, A_RC_, defined in Section 5.3src.morph.paramfloatnullableNoteNote (s) (3)meta.notecharSimbadSimbad column added by the CDSmeta.ref.urlcharNEDNED column added by the CDSmeta.ref.urlcharLEDAmeta.ref.urlcharKmag[8.62/11.93] 2MASS K band magnitude (4)magphot.mag;em.IR.Kfloate_Kmag[0.01/0.23] Uncertainty on the Kmagmagstat.error;phot.mag;em.IR.KfloatDist[1.8/181.4] Distance (5)Mpcpos.distancefloatrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintUGC[16/12808] UGC galaxy identifiermeta.id;meta.mainintprimaryNobsNumber of Halpha measurements for this galaxy (link to Table 7)meta.numberintnullableN[25/393] Numbermeta.numberintsigMod[0/16.1] Extra error term, {sigma}_mod_ (see Equation 6)km/sstat.errorfloatinc[14.5/47.5]? Inclinationdegsrc.orbital.inclinationfloatnullablee_inc[0.8/15]? inc uncertaintydegstat.error;src.orbital.inclinationfloatnullablef_incFlag on inc (1)meta.codecharphi0[8/374.1] Position angle of the major axis, {phi}_0_degpos.posAngfloate_phi0[0.2/8] phi0 uncertaintydegstat.error;pos.posAngfloatVrot[6.6/211] Asymptotic rotation speed, V_rot_km/sphys.veloc.rotatfloate_Vrot[0.4/12.2] Vrot uncertaintykm/sstat.error;phys.veloc.rotatfloathrot[0.1/38]? Rotation scale, h_rot_arcsecinstr.scalefloatnullablee_hrot[0/5.1]? hrot uncertaintyarcsecstat.error;instr.scalefloatnullablef_hrotFlag on hrot (2)meta.codecharVsys[224.8/12794] Systemic velocitykm/sphys.velocfloate_Vsys[0.3/4] Vsys uncertaintykm/sstat.error;phys.velocfloatAphi[0.015/0.4] Asymetry measure, A_{phi}_, defined in Section 5.3src.morph.paramfloate_Dist[2.5/2.5] Dist uncertaintyMpcstat.error;pos.distancefloatAk[-0.03/0.06] K-band extinctionmagphys.absorption;em.IR.KfloatKcor[-0.1/0.01] K-correctionmagarith.factor;phot.magfloatKMag[-26.07/-16.09] Absolute K band magnitudemagphys.magAbs;em.IR.Kfloate_KMag[0.02/1.95] KMag uncertaintymagstat.error;phys.magAbs;em.IR.KfloatiiTF[1.8/90] Inverse Tully-Fisher inclination, i_iTF_degsrc.orbital.inclinationfloate_iiTF[0/4.3] iiTF uncertaintydegstat.error;src.orbital.inclinationfloat_RARight Ascension (J2000) from SIMBAD (not part of the original data)degpos.eq.ra;meta.main_DEDeclination (J2000) from SIMBAD (not part of the original data)degpos.eq.dec;meta.mainJ/ApJS/276/59/table7H{alpha} data table for individual fiber measurementsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintUGC[16/12808] UGC galaxy identifiermeta.id;meta.mainintRRun code (1)meta.id;obscharN[1/5] Night during the observing runmeta.noteintP[1/4] SparsePak pointingobs.fieldintA[1/82] SparsePak fiber apertureinstr.fovintC[1/9] Fitting code (2)meta.codeintoRA[-70.5/38.7] East-West offset of fiber aperture (3)arcsecpos.eq.ra;arith.difffloatoDE[-47/62.5] North-South offset of fiber aperture (3)arcsecpos.eq.dec;arith.difffloatEWg[-0.2/1167]? H{alpha} emission equivalent width from sum of Gaussian line parameters1e-10mspect.line.eqWidthfloatnullableEWsum[-0.2/29060]? H{alpha} emission equivalent width from zeroth moment of line emission1e-10mspect.line.eqWidthfloatnullablelogmuN[-16.6/-13] Log H{alpha} narrow component surface-brightness (flux within the 4.7" diameter fiber aperture); in erg/s/cm^2^/arcsec^2^log(mW.m**-2.arcsec**-2)phot.mag.sbfloate_logmuN[0/73] Uncertainty in logmuNlog(mW.m**-2.arcsec**-2)stat.error;phot.mag.sbfloatVelN[-382/348] Narrow component velocity relative to kinematic model galaxy barycenterkm/sphys.veloc;arith.difffloate_VelN[0/5579] Uncertainty in VelNkm/sstat.error;phys.veloc;arith.difffloatsigmaN[2.9/142] Narrow component velocity dispersionkm/sphys.veloc.dispersionfloate_sigmaN[0/999] Uncertainty in sigmaNkm/sstat.error;phys.veloc.dispersionfloatlogmuB[-99/-13]? Log H{alpha} broad component surface-brightness; in erg/s/cm^2^/arcsec^2^log(mW.m**-2.arcsec**-2)phot.mag.sbfloatnullablee_logmuB[0/13.4]? Uncertainty in logmuBlog(mW.m**-2.arcsec**-2)stat.error;phot.mag.sbfloatnullableVelB[-487/340]? Broad component velocity relative to the kinematic model galaxy barycenterkm/sphys.veloc;arith.difffloatnullablee_VelB[0/1174]? Uncertainty in VelBkm/sstat.error;phys.veloc;arith.difffloatnullablesigmaB[0/888]? Broad component velocity dispersionkm/sphys.veloc.dispersionfloatnullablee_sigmaB[0/999]? Uncertainty in sigmaBkm/sstat.error;phys.veloc.dispersionfloatnullable