VizieR

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

VizieR

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J/MNRAS/522/3439
  AGNs Optical/MIR time series analysis properties (Chen+, 2023)
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2023MNRAS.522.3439C
Similar Catalogs
Post annotation 		img(gal)
1.J/MNRAS/522/3439/table1(c)The sample of reverberation mapped AGNs selected from literature and their physical properties (101 rows)
2.J/MNRAS/522/3439/table3Optical and MIR photometric light curves for our selected AGNs sample based on work in sect. 2.2 (50028 rows)
3.J/MNRAS/522/3439/table4*Results of time lag measurements for W1 and W2 bands time series (Note) (92 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)Name (char) (i) AGN name designation (Name) (meta.id;meta.main)
  (1+3)n_Name (char) Note on AGNs (Note 1)   (meta.note)
  (1)T4 (char) Indicates data in table4 (meta.ref.url)
  (1)RAJ2000 "h:m:s" (i) Right ascension (J2000) (pos.eq.ra;meta.main)
  (1)DEJ2000 "d:m:s" (i) Declination (J2000) (pos.eq.dec;meta.main)
  (1)z  Redshift (z) (src.redshift)
  (1)Vmag mag Apparent magnitude in V-band (V) (Note 2)   (phot.mag;em.opt.V)
  (1)W1mag mag Apparent magnitude in W1-band (W1) (Note 2)   (phot.mag;em.IR.3-4um)
  (1)W2mag mag Apparent magnitude in W2-band (W2) (Note 2)   (phot.mag;em.IR.4-8um)
  (1)SNRv  Signal to noise ratio in V band (S/NV) (stat.snr)

ALL cols		    
 (i)indexed column
  (1)SNRw1  Signal to noise ratio in W1 band (S/NW1) (stat.snr)
  (1)SNRw2  Signal to noise ratio in W2 band (S/NW2) (stat.snr)
  (1)Type (char) The subclasses of intermediate Seyfert galaxies (Type) (Note 3)   (src.class)
  (1)tauHbeta d The time lag of the H{beta} line ({tau}_H{beta}) (time.interval)
  (1)e_tauHbeta d Lower uncertainties of tau_Hbeta (err{tau}_H{beta}) (stat.error)
  (1)E_tauHbeta d Upper uncertainties of tau_Hbeta (Err{tau}_H{beta}) (stat.error;stat.max)
  (1)log(MBH) [Msun] Black hole mass (logM./M{sun}) (phys.mass)
  (1)e_log(MBH) [Msun] Lower uncertainties of log (MBH) (errlogM./M{sun}) (stat.error)
  (1)E_log(MBH) [Msun] Upper uncertainties of log (MBH) (ErrlogM./M{sun}) (stat.error;stat.max)
  (1)logL5100 [10-7W] Optical luminosity at 5100 Å (logL5100) (phys.luminosity;em.opt)
  (1)e_logL5100 [10-7W] Uncertainties of logL5100 (errlogL5100) (stat.error)
  (1)dM/dt  Dimensionless accretion rates (Mdot) (phys.mass.loss)
  (1)e_dM/dt  Lower uncertainties of dM/dt (errMdot) (stat.error)

ALL cols		    
 (i)indexed column
  (1)E_dM/dt  Upper uncertainties of dM/dt (ErrMdot) (stat.error;stat.max)
  (1)r_Name (char) Reference literature of the AGN (Ref.) (Note 4)   (meta.ref;pos.frame)
  (1)T3 (char) Link to table3.dat data (meta.ref.url)
  (1)SimbadName (char) (n)Designation understandable by the Simbad data-base (meta.id)
  (2)MJD d (i) Modified julian date of observation JD-2452000 from photometry (JD) (time.epoch)
  (2)Flux 10-17W/m2/nmFlux density from photometry (Flux) (phot.flux.density)
  (2)e_Flux 10-17W/m2/nmUncertainty of Flux (errFlux) (stat.error;phot.flux)
  (2)Filter (char) Filter name (Filter) (Note 2)   (meta.id;instr.filter)
  (2)Survey (char) Survey name (Survey) (Note 3)   (meta.id)
  (2)MJDc d (n) Modified julian date of observation JD-2452000 from combined photometry (JD_combined) (time.epoch)
  (2)Fluxc 10-17W/m2/nm(n) Flux density from combined photometry (Flux_combined) (phot.flux.density)
  (2)e_Fluxc 10-17W/m2/nm(n) Uncertainty of Fluxc (errFlux_combined) (stat.error)
  (3)rmaxW1ICCF  For the ICCF method we determine the lag as the centroid of the ICCF above 80 % of the peak as rmax of the W1 WISE band (rmaxW1ICCF) (stat.param)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (3)tauW1ICCF d Time lag computed with W1 WISE at 2.6-3.4 µm and ICCF method (tauW1ICCF) (time.interval)
  (3)e_tauW1ICCF d Lower uncertainty of tauW1ICCF (errtauW1ICCF) (stat.error)
  (3)E_tauW1ICCF d Upper uncertainty of tauW1ICCF (ErrtauW1ICCF) (stat.error;stat.max)
  (3)rmaxW2ICCF  For the ICCF method we determine the lag as the centroid of the ICCF above 80% of the peak as rmax of the W2 WISE band (rmaxW2ICCF) (stat.param)
  (3)tauW2ICCF d Time lag computed with W2 WISE at 3.5-4.6 µm and ICCF method (tauW2ICCF) (time.interval)
  (3)e_tauW2ICCF d Lower uncertainty of tauW2ICCF (errtauW2ICCF) (stat.error)
  (3)E_tauW2ICCF d Upper uncertainty of tauW2ICCF (ErrtauW2ICCF) (stat.error;stat.max)
  (3)tauW1MICA d Time lag computed with W1 WISE at 2.6-3.4 µm and MICA method (tauW1MICA) (Note 2)   (time.interval)
  (3)e_tauW1MICA d Lower uncertainty of tauW1MICA (errtauW1MICA) (stat.error)
  (3)E_tauW1MICA d Upper uncertainty of tauW1MICA (ErrtauW1MICA) (stat.error;stat.max)
  (3)tauW2MICA d Time lag computed with W2 WISE at 3.5-4.6 µm and MICA method (tauW2MICA) (Note 2)   (time.interval)
  (3)e_tauW2MICA d Lower uncertainty of tauW2MICA (errtauW2MICA) (stat.error)
  (3)E_tauW2MICA d Upper uncertainty of tauW2MICA (ErrtauW2MICA) (stat.error;stat.max)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (3)tauW1zcorMICA d Time lag computed with W1 WISE at 2.6-3.4 µm and MICA method which adds a redshift corrected MICA lag (tauW1zcor_MICA) (time.interval)
  (3)e_tauW1zcorMICA d Lower uncertainty of tauW1zcorMICA (errtauW1zcorMICA) (stat.error)
  (3)E_tauW1zcorMICA d Upper uncertainty of tauW1zcorMICA (ErrtauW1zcorMICA) (stat.error;stat.max)
  (3)tauW2zcorMICA d Time lag computed with W2 WISE at 3.5-4.6 µm and MICA method which adds a redshift corrected MICA lag (tauW2zcor_MICA) (time.interval)
  (3)e_tauW2zcorMICA d Lower uncertainty of tauW2zcorMICA (errtauW2zcorMICA) (stat.error)
  (3)E_tauW2zcorMICA d Upper uncertainty of tauW2zcorMICA (ErrtauW2zcorMICA) (stat.error;stat.max)
  (3)log(taud) [d] The logarithm of damped time-scale parameters (logtau_d) (Note 3)   (time.scale)
  (3)e_log(taud) [d] Lower uncertainty of log(taud) (errlogtau_d) (stat.error)
  (3)E_log(taud) [d] Upper uncertainty of log(taud) (Errlogtau_d) (stat.error;stat.max)
  (3)logSigmad [-] The variability amplitudes at long time-scale (logSigma_d) (Note 3)   (phot.mag;arith.ratio)
  (3)e_logSigmad [-] Lower uncertainty of logSigmad (errlogSigma_d) (stat.error)
  (3)E_logSigmad [-] Upper uncertainty of logSigmad (ErrlogSigma_d) (stat.error;stat.max)
  (3)SigmaMICAW1 d Gaussian MICA width in W1 WISE band (SigmaMICAW1) (stat.param)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (3)e_SigmaMICAW1 d Lower uncertainty of SigmaMICAW1 (errSigmaMICAW1) (stat.error)
  (3)E_SigmaMICAW1 d Upper uncertainty of SigmaMICAW1 (ErrSigmaMICAW1) (stat.error;stat.max)
  (3)SigmaMICAW2 d Gaussian MICA width in W2 WISE band (SigmaMICAW2) (stat.param)
  (3)e_SigmaMICAW2 d Lower uncertainty of SigmaMICAW2 (errSigmaMICAW2) (stat.error)
  (3)E_SigmaMICAW2 d Upper uncertainty of SigmaMICAW2 (ErrSigmaMICAW2) (stat.error;stat.max)

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