J/MNRAS/462/2878ivo://CDS.VizieR/J/MNRAS/462/2878doi:10.26093/cds/vizier.74622878CDSPovic M.Marquez I.Netzer H.Masegosa J.Nordon R.Perez E.,Schoenell W.2024-08-16T20:18:27Z2018-05-02T14:03:54ZCDS support team

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

cds-question@unistra.fractive-galactic-nucleistar-forming-regionsgalaxy-classification-systemsinfrared-sourcesspectroscopyThis work presents the properties of 42 objects in the group of the most luminous, highest star formation rate (SFR) low-ionization nuclear emission-line regions (LINERs) at z=0.04-0.11. We obtained long-slit spectroscopy of the nuclear regions for all sources, and FIR data (Herschel and IRAS) for 13 of them. We measured emission-line intensities, extinction, stellar populations, stellar masses, ages, active galactic nuclei (AGN) luminosities, and SFRs. We find considerable differences from other low-redshift LINERs, in terms of extinction, and general similarity to star-forming galaxies. We confirm the existence of such luminous LINERs in the local universe, after being previously detected at z~0.3 by Tommasin et al. The median stellar mass of these LINERs corresponds to 6-7x10^10^M_{sun}_ which was found in previous work to correspond to the peak of relative growth rate of stellar populations and therefore for the highest SFRs. Other LINERs although showing similar AGN luminosities have lower SFR. We find that most of these sources have LAGN~LSF suggesting co-evolution of black hole and stellar mass. In general, the fraction of local LINERs on the main sequence of star-forming galaxies is related to their AGN luminosity.2016MNRAS.462.2878Phttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/462/2878CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toII/267 : The SDSS Photometric Catalog, Release 4 (Adelman-McCarthy+, 2006)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/462/2878https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/462/2878http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/462/2878https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/462/2878https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/462/2878http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/MNRAS/462/2878GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/MNRAS/462/2878/table1 (Summary of observations)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/462/2878/table1?https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/462/2878/table1?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/462/2878/table1?GETtext/xml+votable180.050000true47.499331940.299550.0055555555555555566/4173 4783 4813 5052 5668 5991 6469 7187 7211 7524 9366 9876 10700 11024 11094 11233 11473 11591 17515 18070 18544 18951 19115 19432 19684 21847 23196 23212 26019 26080 26161 26296 26307 26976 26984 27503 27663 27671 27758 27931 31421 324159.699422546568423e-22 3.055128279268906e-19https://cdsarc.cds.unistra.fr/viz-bin/moc/J/MNRAS/462/2878?format=asciiOpticalInfrareddefaultJ/MNRAS/462/2878/table1Summary of observationsn_PA[PA ] PA means that the parallactic angle was usedmeta.notecharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintIDMLLINER identificationmeta.id;meta.maincharn_ID[*! ] Note (G1)meta.notecharRAJ2000Right ascension (J2000)degpos.eq.ra;meta.mainDEJ2000Declination (J2000)degpos.eq.dec;meta.mainzRedshift, from SDSS public cataloguessrc.redshiftfloatm6500AB continuum magnitude at 6500{AA}magphot.mag;spect.continuumfloatMorphVisual morphological classification (1)meta.notecharDateDate of observationtime.epochnullableSeeing? Average FWHM of the seeingarcsecinstr.obsty.seeing;stat.meanfloatnullablePA[]? Slit position angle, orientated along the major axisdegpos.posAngintnullableTexpbTotal exposure time in blue parts in secondsstime.duration;obs.exposure;em.opt.BcharTexprTotal exposure time in red parts in secondsstime.duration;obs.exposure;em.opt.RcharAreanuc? Area covered with our 'nuclear' extraction (2)arcsec**2phys.areafloatnullableIRdata[1,2 ] Availability of Herschel (1) and IRAS (2) datameta.codecharJ/MNRAS/462/2878/table2Summary of FIR observations with Herschel and IRASrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintIDMLLINER identificationmeta.id;meta.maincharF70? FIR flux in the 70um Herschel/PACS bandJyphot.flux.density;em.IR.30-60umfloatnullablee_F70? FIR flux in the 70um Herschel/PACS bandJystat.errorfloatnullableF160? FIR flux in the 160um Herschel/PACS bandJyphot.flux.density;em.mm.1500-3000GHzfloatnullablee_F160? FIR flux in the 160um Herschel/PACS bandJystat.errorfloatnullableF60? IRAS FIR flux in 60um bandJyphot.flux.density;em.IR.30-60umfloatnullableq_F60? Quality flag on F60 (1)meta.code.qualintnullableF100? IRAS FIR flux in 100um bandJyphot.flux.density;em.IR.60-100umfloatnullableq_F100? Quality flag on F100 (1)meta.code.qualintnullableJ/MNRAS/462/2878/table3Dn4000 and H{delta} measurementsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintIDMLLINER identificationmeta.id;meta.maincharn_ID[!] Note (G1)meta.notecharDn4000? Strength of 4000{AA} breakspect.indexfloatnullablee_Dn4000? rms uncertainty on Dn4000stat.errorfloatnullableHd? Balmer absorption-line index H{delta}spect.indexfloatnullableJ/MNRAS/462/2878/table4The best stellar population mixture found by STARLIGHTrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintIDMLLINER identificationmeta.id;meta.maincharn_ID[!] Note (G1)meta.notecharadevGoodness of the fit (see the text)stat.fit.goodnessfloatS/NMeasured S/N ratio (see Section 4.2)stat.snrfloatAV? Extinction in V bandmagphys.absorption;em.opt.VfloatnullableM*Current mass in stars1e+10solMassphys.massfloatM*iniInitial mass in stars1e+10solMassphys.massfloatstpop1Fraction of young stars with age[yr]<=10^8^%meta.numberfloatstpop2Fraction of intermediate stars with 10^8^<age[yr]<=10^9^%meta.numberfloatstpop3Fraction of old stars with age[yr]>10^9^%meta.numberfloatlogtmeanMean ageyrtime.age;stat.meanfloatJ/MNRAS/462/2878/table5Properties of strong emission lines[SII]1? Flux of [SII]6716 in H{alpha} flux unitphot.flux;arith.ratiofloatnullablerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintIDMLLINER identificationmeta.id;meta.maincharn_ID[!] Note (G1)meta.notechar[OII]? Flux of [OII]3272 in H{alpha} flux unitphot.flux;arith.ratiofloatnullablee_[OII]? rms uncertainty on [OII]stat.errorfloatnullableHb? Flux of H{beta} in H{alpha} flux unitmeta.unit;phot.flux;em.line.Hbetafloatnullablee_Hb? rms uncertainty on Hbstat.errorfloatnullable[OIII]1? Flux of [OIII]4959 in H{alpha} flux unitphot.flux;arith.ratiofloatnullablee_[OIII]1? rms uncertainty on [OIII]1stat.errorfloatnullable[OIII]2Flux of [OIII]5007 in H{alpha} flux unitphot.flux;arith.ratiofloate_[OIII]2rms uncertainty on [OIII]2stat.errorfloat[OI]? Flux of [OI]6300 in H{alpha} flux unitphot.flux;arith.ratiofloatnullablee_[OI]? rms uncertainty on [OI]stat.errorfloatnullable[NII]1? Flux of [NII]6548 in H{alpha} flux unitphot.flux;arith.ratiofloatnullablee_[NII]1? rms uncertainty on [NII]1stat.errorfloatnullable[NII]2Flux of [NII]6584 in H{alpha} flux unitphot.flux;arith.ratiofloate_[NII]2rms uncertainty on [NII]2stat.errorfloate_[SII]1? rms uncertainty on [SII]1stat.errorfloatnullable[SII]2? Flux of [SII]6731 in H{alpha} flux unitphot.flux;arith.ratiofloatnullablee_[SII]2? rms uncertainty on [SII]2stat.errorfloatnullableFHaH{alpha} flux1e-19mW.m**-2phot.flux;em.line.Halphafloate_FHarms uncertainty on FHA1e-19mW.m**-2stat.errorfloatEWHaH{alpha} equivalent width (1)0.1nmspect.line.eqWidth;em.line.HalphafloatJ/MNRAS/462/2878/table6Properties of extinction corrected strong emission linese_[OIII]2rms uncertainty on [OIII]2stat.errorfloatrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintIDMLLINER identificationmeta.id;meta.maincharn_ID[!] Note (G1)meta.notechar[OII]? Extinction corrected flux of [OII]3272 in H{alpha} flux unitphot.flux;arith.ratiofloatnullablee_[OII]? rms uncertainty on [OII]stat.errorfloatnullable[OIII]1? Extinction corrected flux of [OIII]4959 in H{alpha} flux unitphot.flux;arith.ratiofloatnullablee_[OIII]1? rms uncertainty on [OIII]1stat.errorfloatnullable[OIII]2Extinction corrected flux of [OIII]5007 in H{alpha} flux unitphot.flux;arith.ratiofloat[OI]? Extinction corrected flux of [OI]6300 in H{alpha} flux unitphot.flux;arith.ratiofloatnullablee_[OI]? rms uncertainty on [OI]stat.errorfloatnullable[NII]1? Extinction corrected flux of [NII]6548 in H{alpha} flux unitphot.flux;arith.ratiofloatnullablee_[NII]1? rms uncertainty on [NII]1stat.errorfloatnullable[NII]2Extinction corrected flux of [NII]6584 in H{alpha} flux unitphot.flux;arith.ratiofloate_[NII]2rms uncertainty on [NII]2stat.errorfloat[SII]1? Extinction corrected flux of [SII]6716 in H{alpha} flux unitphot.flux;arith.ratiofloatnullablee_[SII]1? rms uncertainty on [SII]1stat.errorfloatnullable[SII]2? Extinction corrected flux of [SII]6731 in H{alpha} flux unitphot.flux;arith.ratiofloatnullablee_[SII]2? rms uncertainty on [SII]2stat.errorfloatnullableFHaH{alpha} flux1e-19mW.m**-2phot.flux;em.line.Halphafloate_FHarms uncertainty on FHA1e-19mW.m**-2stat.errorfloatLHaH{alpha} luminosity1e+33Wphys.luminosity;em.line.Halphafloate_LHarms uncertainty on LHA1e+33Wstat.errorfloatAVInterstellar extinction parameter in the V bandmagphys.absorption;em.opt.VfloatJ/MNRAS/462/2878/table7AGN contribution measured through L(H{alpha}) and STARLIGHT SFRs (obtained from young stellar populations)recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintIDMLLINER identificationmeta.id;meta.maincharL(Ha)testH{alpha} luminosity obtained from the STARLIGHT SFRs correspondent only to young stellar populations1e+33Wphys.luminosity;em.line.HalphafloatAGNcontApproximation of AGN contribution to H{alpha} luminosity%stat.fit.paramfloatJ/MNRAS/462/2878/table8SFRs and AGN luminositiesrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintIDMLLINER identificationmeta.id;meta.maincharSFR1SFR measured through the starlight best-fitting model using only young (age<10^8^) starsphys.SFRfloatSFR2SFR measured through the starlight best-fitting model using young and intermediate (age<10^9^) starsphys.SFRfloatSFRtotTotal SFR obtained from the best-fitting modelphys.SFRfloate_SFRtotrms uncertainty on SFRtotstat.errorfloatSFRtotscTotal SFR obtained from the best-fitting model scaled to the entire galaxyphys.SFRfloate_SFRtotscrms uncertainty on SFRtotscstat.errorfloatSFRDn? SFR measured using the Dn4000 indexphys.SFRfloatnullablee_SFRDn? rms uncertainty on SFRDn4000stat.errorfloatnullableSFRDnsc? SFR measured using the Dn4000 index scaled to the entire galaxyphys.SFRfloatnullablee_SFRDnsc? rms uncertainty on SFRDn4000scstat.errorfloatnullableSFRPACS? SFRs measured through Herschel/PACS dataphys.SFRfloatnullablee_SFRPACS? rms uncertainty on SFRPACSstat.errorfloatnullableSFRIRAS? SFRs measured through IRAS FIR dataphys.SFRfloatnullablee_SFRIRAS? rms uncertainty on SFRIRASstat.errorfloatnullablelogLAGN? AGN luminosity, measured through H{alpha} and [OIII]5007 extinction corrected emission lineslog(1e-07W)phys.luminosityfloatnullablee_logLAGN? rms uncertainty on logLAGNlog(1e-07W)stat.errorfloatnullablelogMtot? Total stellar mass, measured by MPA-JHU team using SDSS DR7 datalog(solMass)phys.massfloatnullablelogMBH? Black hole mass measured for galaxies classified as Elog(solMass)phys.massfloatnullablen_logMBH[*] * for B13 that is classified as Smeta.notechar