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J/MNRAS/521/1292
  Omega/WINGS clusters/fields galaxies (Perez-Millan+, 2023)
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2023MNRAS.521.1292P
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1.J/MNRAS/521/1292/tablec1(c)*Basic properties of the WINGS/OmegaWINGS clusters sample (Note) (76 rows)
2.J/MNRAS/521/1292/cluster(c)Astrometrics and physical properties as ages, masses and SFRs of WINGS cluster galaxies (9278 rows)
3.J/MNRAS/521/1292/field(c)Astrometrics and physical properties as ages, masses and SFRs of WINGS field galaxies (1572 rows)
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Simple ConstraintList Of Constraints
 
Query by Constraints constraints help applied on Columns (Output Order: + - )
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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)Cluster (char) Cluster field name (meta.id;meta.main)
  (1)Cava (char) Display the WINGS spectroscopy of 48 galaxy clusters of Cava et al. 2009A&A...495..707C, Cat. J/A+A/495/707 (meta.ref.url)
  (1)Varela (char) Display the WINGS: Deep optical phot. of 77 nearby clusters of Varela et al. 2009A&A...497..667V, Cat. J/A+A/497/667 (meta.ref.url)
   (ALL)Gullieuszik15 (char) Display OmegaWINGS BV photometry of galaxy clusters of Gullieuszik et al. 2015A&A...581A..41G, Cat. J/A+A/581/A41 (meta.ref.url)
   (ALL)Moretti (char) Display OmegaWINGS local clusters of galaxies redshifts od Moretti et al. 2017A&A...599A..81M, Cat. J/A+A/599/A81 (meta.ref.url)
  (1)Biviano (char) Display Properties of the sample of clusters of Biviano et al. 2017A&A...607A..81B, Cat. J/A+A/607/A81 (meta.ref.url)
  (1)Gullieuszik20 (char) Display GASP cluster data of Gullieuszik et al. 2020ApJ...899...13G, Cat. J/ApJ/899/13 (meta.ref.url)
  (1)z  The mean redshift (src.redshift)
  (1+2)sigma km/s (n) The velocity dispersion from data Biviano et al. (2017A&A...607A..81B, Cat. J/A+A/607/A81) and Gullieuszik et al. (2020ApJ...899...13G, Cat. J/ApJ/899/13) (phys.veloc.dispersion)
  (1+2)R200 Mpc (n) The virial radius (phys.size.radius)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (1+2)logLX [10-7W] (n) The X-ray luminosity taken from the ROSAT All-Sky Survey (phys.luminosity;em.X-ray)
  (1)Wings (char) Flag to indicates if the cluster was observed in spectroscopy with WINGS (meta.code)
  (1)OWings (char) Flag to indicates if the cluster was observed in spectroscopy with Omega Wings (meta.code)
  (1)Sinopsis (char) Flag to whether WINGS/OmegaWINGS spectra have sufficient signal-to-noise ratio to run the sinopsis code (meta.code)
  (1)SimbadName (char) (n)Designation understandable by the Simbad data-base (meta.id)
  (1)_RA deg (i) Right Ascension (J2000) from SIMBAD (not part of the original data) (pos.eq.ra;meta.main)
  (1)_DE deg (i) Declination (J2000) from SIMBAD (not part of the original data) (pos.eq.dec;meta.main)
  (2+3)WINGS (char) WINGS identifier designation as WINGSJHHMMSS.ss+DDMMSS.s (WINGS_ID) (meta.id;meta.main)
  (2+3)RAJ2000 deg (i) Right ascension (J2000) (RAJ2000) (pos.eq.ra;meta.main)
  (2+3)DEJ2000 deg (i) Declination (J2000) (DECJ2000) (pos.eq.dec;meta.main)
  (2+3)zgal  Redshift of the galaxies (z_gal) (src.redshift)
  (2+3)DL Mpc Distance luminosity (Lum_dist) (pos.distance)
  (2+3)rChi  Reduced chi squared of the SINOPSIS model spectral profile fit (redchi) (stat.fit.chi2;spect.line.profile;meta.modelled)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (2+3)AVy mag Extinction of the youngest stellar populations as age <=2*10^7 yr (Av_y) (phys.absorption)
  (2+3)Av mag Average extinction value for all the stellar populations (Av) (phys.absorption;stat.mean)
  (2+3)SFR1 Msun/yr SFR in first age-bin 0-19.95 Myr as described in section 3 were selected based on the presence and intensity of stellar population features (SFR1) (Note G1)   (phys.SFR)
  (2+3)SFR2 Msun/yr SFR in second age-bin 19.95-571.5 Myr as described in section 3 were selected based on the presence and intensity of stellar population features (SFR2) (Note G1)   (phys.SFR)
  (2+3)SFR3 Msun/yr SFR in third age-bin from 0.5715-5.754 Gyr as described in section 3 were selected based on the presence and intensity of stellar population features (SFR3) (Note G1)   (phys.SFR)
  (2+3)SFR4 Msun/yr SFR in fourth age-bin from 5.754-tu Gyr as described in sect. 3 were selected based on the presence and intensity of stellar population features (SFR4) (Note G1)   (phys.SFR)
  (2+3)M*a3 Msun Stellar mass, calculated according to definition n.3 of the SFR3, normalized to aperture magnitude or spectrum (AMass3) (phys.mass)
  (2+3)TotM*3 Msun Total stellar mass calculated according to definition n.3 of the SFR3 (TotMass3) (phys.mass)
  (2+3)M*a2 Msun Stellar mass, calculated according to definition n.2 of the SFR2, normalized to aperture magnitude or spectrum (AMass2) (phys.mass)
  (2+3)TotM*2 Msun Total stellar mass calculated according to definition n.2 of the SFR2 (TotMass2) (phys.mass)
  (2+3)M*a1 Msun Stellar mass, calculated according to definition n.1 of the SFR1, normalized to aperture magnitude or spectrum (AMass1) (phys.mass)
  (2+3)TotM*1 Msun Total stellar mass calculated according to definition n.1 of the SFR1 (TotMass1) (phys.mass)
  (2+3)logAgelwV [yr] Logarithm of the luminosity-weighted age in V-band (lVwage) (time.age)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (2+3)logAgemw [yr] Logarithm of the mass-weighted age (mwage) (time.age)
  (2+3)Hb 0.1nm The H{Beta} index (Hb) (spect.index;em.line.Hbeta)
  (2+3)Ha 0.1nm The H{alpha} index (Ha) (spect.index;em.line.Halpha)
  (2+3)D4000  The D4000 4000Å break index (D4000) (spect.index)
  (2+3)Dn4000  The Dn4000 spectral indicator (Dn4000) (spect.index)
  (2+3)SNR  Signal to noise ratio (SNR) (stat.snr)
  (2+3)BfibMag mag Absolute magnitude with fiber aperture in B-band (ABSBfib) (phot.mag)
  (2+3)VfibMag mag Absolute magnitude with fiber aperture in V-band (ABSVfib) (phot.mag)
  (2+3)Vmag mag Apparent magnitude with automatic aperture in V-band (Vauto) (phot.mag;em.opt.V)
  (2+3)Vfibmag mag Apparent magnitude with fiber aperture in V-band (V_fib) (phot.mag;em.opt.V)
  (2+3)Bmag mag Apparent magnitude with automatic aperture in B-band (Bauto) (phot.mag;em.opt.B)
  (2+3)Bfibmag mag Apparent magnitude with fiber aperture in B-band (B_fib) (phot.mag;em.opt.B)
  (2+3)VtotMag mag Total absolute magnitude in V-band (ABSVtot) (phot.mag)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (2+3)BtotMag mag Total absolute magnitude in B-band (ABSBtot) (phot.mag)
  (2)zcl  Redshift of the cluster (z_cl) (src.redshift;pos.heliocentric)
  (2)RXproj Mpc The clustercentric distance radius is calculated in projection to the centre of the cluster in the X-ray emission (RXproj) (pos.distance)
  (2)Morph (char) Flag for cluster morphology of neighbour galaxies as early and late types (neigh_morph) (meta.code)
  (2)RRv  The cluster RRv quantity (RRv) (stat.param)
  (2+3)Simbad (char) ask the Simbad data-base about this object (meta.ref.url)

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