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:
Target dimension:
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
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)
Help Xmatch is

 
Standard Original
Query by Constraints constraints help applied on Columns (Output Order: + - )
ShowSortJoin tables
more join
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
Adapt form
Display your selection only Reset to default columns
usage  Display UCD1+    UCD1  
elapse time 0