VizieR

CfA VizieR . ADAC VizieR . Cambridge (UK) VizieR . IUCAA VizieR . INASAN VizieR .

VizieR

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J/MNRAS/462/2878
  SFR & AGN in most luminous local universe LINERs (Povic+, 2016)
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2016MNRAS.462.2878P
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Post annotation 		img(gal)
1.J/MNRAS/462/2878/table1(c)Summary of observations (42 rows)
2.J/MNRAS/462/2878/table2Summary of FIR observations with Herschel and IRAS (16 rows)
3.J/MNRAS/462/2878/table3Dn4000 and Hδ measurements (42 rows)
4.J/MNRAS/462/2878/table4The best stellar population mixture found by STARLIGHT (41 rows)
5.J/MNRAS/462/2878/table5Properties of strong emission lines (42 rows)
6.J/MNRAS/462/2878/table6Properties of extinction corrected strong emission lines (40 rows)
7.J/MNRAS/462/2878/table7AGN contribution measured through L(Hα) and STARLIGHT SFRs (obtained from young stellar populations) (40 rows)
8.J/MNRAS/462/2878/table8SFRs and AGN luminosities (42 rows)

Simple ConstraintList Of Constraints
 
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Column  Constraint Explain   (UCD)
  (ALL)recno  Record number assigned by the VizieR team. Should Not be used for identification. (meta.record)
   (ALL)ID (char) MLLINER identification (meta.id;meta.main)
  (1+3+4+5+6)n_ID (char) [*! ] Note (Note G1)   (meta.note)
  (1)RAJ2000 deg (i) Right ascension (J2000) (pos.eq.ra;meta.main)
  (1)DEJ2000 deg (i) Declination (J2000) (pos.eq.dec;meta.main)
  (1)z  Redshift, from SDSS public catalogues (src.redshift)
  (1)m6500 mag AB continuum magnitude at 6500Å (phot.mag;spect.continuum)
  (1)Morph (char) Visual morphological classification (Note 1)   (meta.note)
  (1)Date "Y:M:D" (n)Date of observation (time.epoch)
  (1)Seeing arcsec (n) Average FWHM of the seeing (instr.obsty.seeing;stat.mean)
  (1)PA deg (n) []? Slit position angle, orientated along the major axis (pos.posAng)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (1)n_PA (char) [PA ] PA means that the parallactic angle was used (meta.note)
  (1)Texpb (char) s Total exposure time in blue parts in seconds (time.duration;obs.exposure;em.opt.B)
  (1)Texpr (char) s Total exposure time in red parts in seconds (time.duration;obs.exposure;em.opt.R)
  (1)Areanuc arcsec+2 (n) Area covered with our 'nuclear' extraction (Note 2)   (phys.area)
  (1)IRdata (char) [1,2 ] Availability of Herschel (1) and IRAS (2) data (meta.code)
  (2)F70 Jy (n) FIR flux in the 70um Herschel/PACS band (phot.flux.density;em.IR.30-60um)
  (2)e_F70 Jy (n) FIR flux in the 70um Herschel/PACS band (stat.error)
  (2)F160 Jy (n) FIR flux in the 160um Herschel/PACS band (phot.flux.density;em.mm.1500-3000GHz)
  (2)e_F160 Jy (n) FIR flux in the 160um Herschel/PACS band (stat.error)
  (2)F60 Jy (n) IRAS FIR flux in 60um band (phot.flux.density;em.IR.30-60um)
  (2)q_F60  (n) Quality flag on F60 (Note 1)   (meta.code.qual)
  (2)F100 Jy (n) IRAS FIR flux in 100um band (phot.flux.density;em.IR.60-100um)
  (2)q_F100  (n) Quality flag on F100 (Note 1)   (meta.code.qual)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (3)Dn4000  (n) Strength of 4000Å break (spect.index)
  (3)e_Dn4000  (n) rms uncertainty on Dn4000 (stat.error)
  (3)Hd  (n) Balmer absorption-line index Hδ (spect.index)
  (4)adev  Goodness of the fit (see the text) (stat.fit.goodness)
  (4)S/N  Measured S/N ratio (see Section 4.2) (stat.snr)
  (4+6)AV mag (n) Extinction in V band (phys.absorption;em.opt.V)
  (4)M* 10+10MsunCurrent mass in stars (phys.mass)
  (4)M*ini 10+10MsunInitial mass in stars (phys.mass)
  (4)stpop1 % Fraction of young stars with age[yr]≤108 (meta.number)
  (4)stpop2 % Fraction of intermediate stars with 108<age[yr]≤109 (meta.number)
  (4)stpop3 % Fraction of old stars with age[yr]>109 (meta.number)
  (4)logtmean yr Mean age (time.age;stat.mean)
  (5+6)[OII]  (n) Flux of [OII]3272 in Hα flux unit (phot.flux;arith.ratio)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (5+6)e_[OII]  (n) rms uncertainty on [OII] (stat.error)
  (5)Hb  (n) Flux of Hβ in Hα flux unit (meta.unit;phot.flux;em.line.Hbeta)
  (5)e_Hb  (n) rms uncertainty on Hb (stat.error)
  (5+6)[OIII]1  (n) Flux of [OIII]4959 in Hα flux unit (phot.flux;arith.ratio)
  (5+6)e_[OIII]1  (n) rms uncertainty on [OIII]1 (stat.error)
  (5+6)[OIII]2  Flux of [OIII]5007 in Hα flux unit (phot.flux;arith.ratio)
  (5+6)e_[OIII]2  rms uncertainty on [OIII]2 (stat.error)
  (5+6)[OI]  (n) Flux of [OI]6300 in Hα flux unit (phot.flux;arith.ratio)
  (5+6)e_[OI]  (n) rms uncertainty on [OI] (stat.error)
  (5+6)[NII]1  (n) Flux of [NII]6548 in Hα flux unit (phot.flux;arith.ratio)
  (5+6)e_[NII]1  (n) rms uncertainty on [NII]1 (stat.error)
  (5+6)[NII]2  Flux of [NII]6584 in Hα flux unit (phot.flux;arith.ratio)
  (5+6)e_[NII]2  rms uncertainty on [NII]2 (stat.error)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (5+6)[SII]1  (n) Flux of [SII]6716 in Hα flux unit (phot.flux;arith.ratio)
  (5+6)e_[SII]1  (n) rms uncertainty on [SII]1 (stat.error)
  (5+6)[SII]2  (n) Flux of [SII]6731 in Hα flux unit (phot.flux;arith.ratio)
  (5+6)e_[SII]2  (n) rms uncertainty on [SII]2 (stat.error)
  (5+6)FHa 10-19mW/m2Hα flux (phot.flux;em.line.Halpha)
  (5+6)e_FHa 10-19mW/m2rms uncertainty on FHA (stat.error)
  (5)EWHa 0.1nm Hα equivalent width (Note 1)   (spect.line.eqWidth;em.line.Halpha)
  (6)LHa 10+33W Hα luminosity (phys.luminosity;em.line.Halpha)
  (6)e_LHa 10+33W rms uncertainty on LHA (stat.error)
  (7)L(Ha)test 10+33W Hα luminosity obtained from the STARLIGHT SFRs correspondent only to young stellar populations (phys.luminosity;em.line.Halpha)
  (7)AGNcont % Approximation of AGN contribution to Hα luminosity (stat.fit.param)
  (8)SFR1  SFR measured through the starlight best-fitting model using only young (age<108) stars (phys.SFR)
  (8)SFR2  SFR measured through the starlight best-fitting model using young and intermediate (age<109) stars (phys.SFR)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (8)SFRtot  Total SFR obtained from the best-fitting model (phys.SFR)
  (8)e_SFRtot  rms uncertainty on SFRtot (stat.error)
  (8)SFRtotsc  Total SFR obtained from the best-fitting model scaled to the entire galaxy (phys.SFR)
  (8)e_SFRtotsc  rms uncertainty on SFRtotsc (stat.error)
  (8)SFRDn  (n) SFR measured using the Dn4000 index (phys.SFR)
  (8)e_SFRDn  (n) rms uncertainty on SFRDn4000 (stat.error)
  (8)SFRDnsc  (n) SFR measured using the Dn4000 index scaled to the entire galaxy (phys.SFR)
  (8)e_SFRDnsc  (n) rms uncertainty on SFRDn4000sc (stat.error)
  (8)SFRPACS  (n) SFRs measured through Herschel/PACS data (phys.SFR)
  (8)e_SFRPACS  (n) rms uncertainty on SFRPACS (stat.error)
  (8)SFRIRAS  (n) SFRs measured through IRAS FIR data (phys.SFR)
  (8)e_SFRIRAS  (n) rms uncertainty on SFRIRAS (stat.error)
  (8)logLAGN [10-7W] (n) AGN luminosity, measured through Hα and [OIII]5007 extinction corrected emission lines (phys.luminosity)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (8)e_logLAGN [10-7W] (n) rms uncertainty on logLAGN (stat.error)
  (8)logMtot [Msun] (n) Total stellar mass, measured by MPA-JHU team using SDSS DR7 data (phys.mass)
  (8)logMBH [Msun] (n) Black hole mass measured for galaxies classified as E (phys.mass)
  (8)n_logMBH (char) [*] * for B13 that is classified as S (meta.note)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
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