J/A+A/429/115ivo://CDS.VizieR/J/A+A/429/115doi:10.26093/cds/vizier.34290115CDSNoeske K.G.Papaderos P.Cairos L.M.Fricke K.J.2017-10-13T15:41:29Z2005-03-05T09:06:43ZCDS support team

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

cds-question@unistra.frgalaxiesphotometryinfrared-photometryThis paper is part of a series of publications which present a systematic study of Blue Compact Dwarf (BCD) Galaxies in the near infrared (NIR). Compared to the visible light, NIR data allow a better separation of the starburst emission from the light distribution of the old stellar low-surface brightness (LSB) host galaxy. We analyze deep NIR broad band images of a sample of 11 BCDs, observed with the Calar Alto 3.6m telescope. This work enlarges the samples presented in preceding papers of this study (Noeske et al., 2003A&A...410..481N, Cairos et al., 2003ApJ...593..312C) by BCDs of the most common morphological type, displaying a regular elliptical LSB host galaxy. The data presented here allow the detection and quantitative study of the extended stellar LSB host galaxy in all sample BCDs.2005A&A...429..115Nhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/429/115CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/429/115https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/429/115http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/429/115https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/429/115https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/429/115http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/429/115GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/A+A/429/115/table1 (Sample galaxies)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/429/115/table1?https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/429/115/table1?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/429/115/table1?GETtext/xml+votable180.050000true345.74708316.605250.0055555555555555566/38 602 7926 9954 10472 10970 16016 17614 20015 20065 26592https://cdsarc.cds.unistra.fr/viz-bin/moc/J/A+A/429/115?format=asciiOpticalInfrareddefaultJ/A+A/429/115/table1Sample galaxiesNameNamecharprimaryRAJ2000Right ascension (J2000)pos.eq.ra;meta.mainrecnoRecord number assigned by the VizieR team. Should Not be used for identification.intClassClassification (1)charDEJ2000Declination (J2000)pos.eq.dec;meta.maintJExposition tine in J bandsinttHExposition tine in H bandsinttK'Exposition tine in K' bandsintBMAGAbsolute B magnitudemagfloatr_BMAGReference for BMAG (2)charABAbsorption in B bandmgfloatDistDistanceMpcfloatr_DistReference for Dist (2)charFWHMFinal FWHMarcsecfloatONamesOther namescharSimbadSimbad column added by the CDScharNEDSimbad column added by the CDScharJ/A+A/429/115/table2*Structural properties of the dwarfsb? b parameter for eq. 2 (1)floatnullableNameGalaxy namecharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.intq? q parameter for eq. 2 (1)floatnullableNote[*] * Objects for which the LSB component was modelled by a pure exponential, SuBr(R*)=SuBr_E,0_ + 1.0857(R*/alpha)charn_Name[fg] Note on Name (2)charBandFilter (J, H, K')charn_Band[dieh ] Note on Band (3)charSuBrE,0? Extrapolated central surface brightness in the band (5)mag.arcsec**-2floatnullablee_SuBrE,0? rms uncertainty on SuBrE,0 (5)mag.arcsec**-2floatnullablealpha? Exponential scale length, alpha (1)kpcfloatnullablee_alpha? rms uncertainty on alphakpcfloatnullablemLSB? Total apparent magnitude of the LSB component, computed by extrapolating the fitted model to R*={infinity}magfloatnullablePiso? Radial extent of the star-forming component, at an isophotal level iso (4)kpcfloatnullablemPiso? Encircled magnitude of the star-forming component, at an isophotal level iso (4)magfloatnullableEiso? Radial extent of the underlying stellar LSB component, at an isophotal level iso (4)kpcfloatnullablemEiso? Encircled magnitude of the underlying stellar LSB component, at an isophotal level iso (4)magfloatnullablemSBPMagnitude from surface brightness profile (SBP) integration out to the last data pointmagfloatmtotTotal magnitude from aperture measurements (5)magfloate_mtotrms uncertainty on mtot (5)magfloatreffEffective radius, enclosing 50% of the SPP's fluxkpcfloatr80Radius, enclosing 80% of the SPP's fluxkpcfloatetaSBPFormal Sersic exponent for the whole SBPfloatsigmaJ, H, K' calibration uncertainty for each galaxy (5)magfloat