J/A+A/617/A33ivo://CDS.VizieR/J/A+A/617/A33doi:10.26093/cds/vizier.36170033CDSAndreani P.Boselli A.Ciesla L.Vio R.Cortese L.Buat V.Miyamoto Y.2018-09-28T11:55:20Z2018-09-19T08:20:36ZCDS support team

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

cds-question@unistra.frgalaxiesinfrared-photometryWe discuss the results of the relationships between the K-band and stellar mass, far-infrared luminosities, star formation rate, dust and gas masses of nearby galaxies computing the bivariate K-band Luminosity Function (BLF) and bivariate K-band Mass Function (BMF) of the Herschel Reference Survey (HRS), a volume-limited sample with full wavelength coverage. We derive the BLFs and BMFs from the K-band and stellar mass, far-infrared luminosities, star formation rate, dust and gas masses cumulative distributions using a copula method which is outlined in detail. The use of the bivariate computed taking into account the upper limits allows us to derive on a more solid statistical ground the relationship between the observed physical quantities. The analysis shows that the behaviour of the morphological (optically selected) subsamples is quite different. A statistically meaningful result can be obtained over the whole HRS sample only from the relationship between the K-band and the stellar mass, while for the remaining physical quantities (dust and gas masses, far-IR luminosity and star formation rate), the analysis is distinct for late-type (LT) and early-type galaxies (ETG). However, the number of ETGs is small to perform a robust statistical analysis, and in most of the case results are discussed only for the LTG subsample. The Luminosity and Mass Functions (LFs, MFs) of LTGs are generally dependent on the K-band and the various dependencies are discussed in detail. We are able to derive the corresponding LFs and MFs and compare them with those computed with other samples. Our statistical analysis allows us to characterise the HRS, that, although non homogeneously selected and partially biased towards low IR luminosities, may be considered as representative of the local LT galaxy population.2018A&A...617A..33Ahttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/617/A33CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toJ/PASP/122/261 : Herschel Reference Survey Sample (Boselli+, 2010)J/A+A/528/A107 : GALEX Ultraviolet Virgo Cluster Survey GUViCS (Boselli+ 2011)J/A+A/543/A161 : Submillimetre obs. of 323 HRS nearby galaxies (Ciesla+, 2012)J/A+A/550/A114 : Integrated spectroscopy of HRS galaxies (Boselli+, 2013)J/MNRAS/440/942 : 100 and 160um fluxes of nearby galaxies (Cortese+, 2014)J/A+A/579/A102 : H{alpha} imaging of Herschel Reference Survey (Boselli+ 2015)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/617/A33https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/617/A33http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/617/A33https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/617/A33https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/617/A33http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/617/A33GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/A+A/617/A33/table1 (Logarithmic values of the luminosities, masses and the star formation rates of the Herschel Reference Sample)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/617/A33/table1?https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/617/A33/table1?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/617/A33/table1?GETtext/xml+votable180.050000true154.415220822.80995280.0055555555555555565/6928 6941 6965 6984-6985 6/4439 5124-5125 5152 5164 5172 5181-5183 5190 5196 5198 5200 5241 5244 5247 5332 5336 5342 5440 5629 5966-5967 5975-5978 5981-5982 5999 6001 6011 6037 6082 6087 6103 8235 8320 8330 8359 10454 10475 10592 10632 10672 10684 10845 10990 11010 11074 11435 11789 25575 25581 25599 25775 25788 25790 25966 25980 25997 26055 26065 26068 26072 26088 26090-26091 26119 26125 26128 26139 26148 26157 26161 26166 26174-26175 26210 26214 26217 26222-26223 26260 26265 26271 26285 26294 26301-26303 26307-26309 26311 26313 26316-26318 26320 26323 26330-26331 26336 26338 26340 26343-26344 26346-26347 26349 26351 26361-26363 26365 26377 26388 26432 26472 26528 26530 26537 26542 27079 27130 27603 27606 27653-27654 27716 27718-27719 27724-27725 27727-27728 27730-27731 27734-27736 27738-27739 27741 27743 27750 27757-27758 27761 27763 27772-27773 27814 27823 27841 27853 27855 27857 27889 27907-27909 27913-27918 27922 27926 27931 27934 27944-27945 27947-27949 27955 28032-28033 28035 28037-28039 28041 28054 28056 28123 28126 28141-28142 28162 28170 28191 28201 28208 28213 28220-28221 28234 28258 28264 28294 28299-28300 28304 28348 28404 28416 28491 28508 28529 28538 28643 28651https://cdsarc.cds.unistra.fr/viz-bin/moc/J/A+A/617/A33?format=asciiInfrareddefaultJ/A+A/617/A33/table1Logarithmic values of the luminosities, masses and the star formation rates of the Herschel Reference SamplerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintHRSHRS name, [BEC2010] HRS NNN in simbadmeta.id;meta.mainintlogLHa? Halpha luminosity (erg/s)log(mW.m**-2)phys.luminosity;em.line.HalphafloatnullablelogLKK-band luminositylog(solLum)phys.luminosity;em.IRfloatlogLIRIR luminositylog(solLum)phys.luminosity;em.IRfloatlogMdustDust masslog(solMass)phys.massfloatlogMstellar? Stellar masslog(solMass)phys.massfloatnullablelogMHI? Atomic hydrogen masslog(solMass)phys.massfloatnullablelogMH2? Molecular hydrogen masslog(solMass)phys.massfloatnullableSFRStar Formation RatesolMass/yrphys.SFRdoubleSimbadSimbad column added by the CDSmeta.ref.urlchar_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.main