VizieR

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

VizieR

Simple TargetList Of TargetsFast Xmatch with large catalogs or Simbad
Target Name (resolved by Sesame) or Position:
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NB: The epoch used for the query is the original epoch of the table(s)Radius Box size

  
J/ApJS/244/40
  A3COSMOS. I. ALMA continuum photometry catalogs (Liu+, 2019) Query images/fits /fits
ReadMe+ftp
2019ApJS..244...40L
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image/fits
image
Post annotation 		img(gal)
1.J/ApJS/244/40/blind(c)The "blind"-extraction photometry catalog; all sources with S/N_peak>5.40 in the ALMA continuum data (see Section 2.2) (original column names in green)[image/fits]
image
(1134 rows)
2.J/ApJS/244/40/prior(c)The "prior"-fitting photometry catalog; known sources in deep optical/near-infrared/radio catalogs which have S/N_peak>4.35 in the ALMA continuum data (see Section 2.4) (original column names in green) (1277 rows)
3.J/ApJS/244/40/catalog(c)*A3COSMOS final galaxy catalog (see Section 4) (original column names in green) (Note) (669 rows)
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Simple ConstraintList Of Constraints
 
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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)RAJ2000 deg (i) Right ascension of the ALMA emission (J2000) (pos.eq.ra;meta.main)
   (ALL)DEJ2000 deg (i) Declination of the ALMA emission (J2000) (pos.eq.dec;meta.main)
  (1+2)Fluxc mJy [0.04/52.4] The fitted total flux with Gaussian source models, corrected for flux bias and PBA (Total_flux_pbcor) (phot.flux.density;em.radio)
  (1+2)e_Fluxc mJy [0.01/6.2] Fluxc uncertainty (E_Total_flux_pbcor) (Note G1)   (stat.error)
  (1+2)s_Fluxc mJy [0.009/5] Fluxc error but estimated from our own simulation statistics (E_Total_flux_sim_pbcor) (stat.error;phot.flux.density)
  (1+2)Pbcor   [0.2/1] Primary beam attenuation (PBA) factor (instr.param)
  (1+2)Beam arcsec [8.6/64.6] ALMA 12m antenna's primary beam FWHM size at the observing frequency (Primary_beam) (phys.angSize;em.radio.20-100MHz;instr.beam)
  (1+2)FPk mJy/beam [0.02/27.6] Fitted ALMA continuum emission's peak flux, uncorrected for PBA (Peak_flux) (phot.flux.density;em.radio)
  (1+2)rms mJy/beam [0.005/1.8] Pixel rms noise in the continuum image (RMS_noise) (stat.stdev;instr.det.noise;instr.pixel)
  (1+2)Freq GHz [90.2/671.5] Observing frequency, i.e., the center frequency of all collapsed spectral windows (Obs_frequency) (em.freq)

ALL cols		    
 (i)indexed column
  (1+2)lambda um [446.4/3323.7] Observing wavelength =(2.99792458x105)/Freq (Obs_wavelength) (em.wl)
  (1+2)FWHMa arcsec [0.1/3.9] Synthesized beam's major-axis FWHM size (Maj_beam) (phys.angSize.smajAxis)
  (1+2)FWHMb arcsec [0.09/2.6] Synthesized beam's minor axis FWHM size (Min_beam) (phys.angSize;instr.beam)
  (1+2)PA deg [-90/90] Synthesized beam's position angle; zero means to the north (PA_beam) (pos.posAng;instr.beam)
  (1+2)fits (char) Download the FITS file (meta.ref.url)
  (1+2)FileName (char) Name of the image FITS file in subdirectory fits (Image_file) (meta.id;meta.fits)
  (1)Mult (char) [MS] Flag= S (or M) means that the source is fitted with single (or multiple) Gaussian component(s) (Flag_multi) (meta.code.error;pos.cartesian.y;meta.modelled)
  (1+2)Flag   [0/1] 0=reliable flux (Flag_inconsistent_flux) (Note G2)   (meta.code.error)
  (2)R (char) Display the star formation data for this robust galaxy (link to the final catalog) (meta.ref.url)
   (2+3)ID  (i) A3COSMOS master catalog identification number (Note G3)   (meta.id;meta.main)
  (2)OID  ID number in "Ref" (ID_PriorCat) (meta.id.cross)
  (2)Ref (char) The reference of the prior catalog in which the source is first included (Ref_ID_PriorCat) (Note 1)   (meta.ref;pos.frame;meta.table)
  (2)Chi2   [0.01/48.2] The reduced χ2 of galfit prior source fitting, measured from the residual image for each source with an aperture of 1.0" in diameter (Galfit_reduced_chi_square) (stat.fit)

ALL cols		    
 (i)indexed column
  (2)Bound   [0/1] Flag=1 means that the fitted source major-axis FWHM size reaches the upper boundary of 3.0" and should be used with caution (Flag_size_upper_boundary) (meta.code)
  (2)CPA   [0/1] Unreliable counterpart outlier flag; see Section 4.2 (Flag_outlier_CPA) (meta.code)
  (2)SED   [0/1] SED-excess outlier flag; see Section 4.4 (Flag_outlier_SED) (meta.code)
  (2)SMUVS  (n)Display data from Ashby+, 2018, J/ApJS/237/39 within 0.5" (meta.ref.url)
  (2)L16 (char) Display the COSMOS2015 data (Laigle+, 2016, J/ApJS/224/24) for this source (meta.ref.url)
  (3)z   [0.3/7.3] SED best-fit redshift from the list of prior redshifts (src.redshift)
  (3)f_z (char) p: photometric or s: spectroscopic (meta.code)
  (3)q_z  (n) [1/212] Quality flag "Qz" for dzLiu or S17 (meta.code.qual;src.redshift)
  (3)r_z (char) Reference for z (Note 1)   (meta.ref;pos.frame)
  (3)zPrior (char) Prior redshifts in the literature (z_prior) (src.redshift;pos.heliocentric)
  (3)r_zPrior (char) References of zPrior (Ref_z_prior) (Note 2)   (meta.ref;pos.frame)
  (3)Mstar Msun [2.7e+9/8.4e+12] Stellar mass from our SED fitting (M_star) (Note 3)   (phys.mass)
  (3)Ldust Lsun [9.3e+10/3.9e+13] Infrared 8-1000u luminosity from dust (L_dust) (Note 3)   (phys.luminosity;em.IR)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (3)SFR Msun/yr [9.3/3890.5] SFR integrated from SFH (Note 3)   (phys.SFR)
  (3)sSFR Gyr-1 [0.1/35] Specific SFR from SFH; SFR/Mstarx109 (phys.SFR)
  (3)SimbadName (char) (n)Designation understandable by the Simbad data-base (meta.id)

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