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/MNRAS/516/372
  Radio galaxies and clusters from 150GHz TGSS (Bhukta+, 2022)
ReadMe+ftp
2022MNRAS.516..372B
Similar Catalogs
Post annotation 		img(gal)
1.J/MNRAS/516/372/table1*Sample of our candidate wide-angle tail (WAT) radio sources (Note) (203 rows)

Simple ConstraintList Of Constraints
 
Query by Constraints constraints help applied on Columns (Output Order: + - )
ShowSortColumn  Constraint Explain   (UCD)
  recno  Record number assigned by the VizieR team. Should Not be used for identification. (meta.record)
  ID  Identifier raw number (CatNo) (meta.id)
  T3 (char) Indicates radio sources data in table3 (meta.ref.url)
  Name (char) (i) Name of the radio source as JHHMM±DDMM (Name) (meta.id;meta.main)
  RAJ2000 "h:m:s" (i) Right Ascension of the galaxy core (J2000) (RAcore) (pos.eq.ra;meta.main)
  DEJ2000 "d:m:s" (i) Declination of the galaxy core (J2000) (DECcore) (pos.eq.dec;meta.main)
  Sep arcsec (n) The separation angle between the radio and optical position (Separation) (pos.angDistance)
  Rel  (n) The reliability of the counterpart as described in section 3 ({rho}) (meta.code.qual)
  F150 Jy The total flux density at 150 MHz from TGSS ADR 1 survey (F150) (phot.flux.density;em.radio.100-200MHz)
  F1400 Jy (n) The total flux density at 1400 MHz from NVSS surveys (F1400) (phot.flux.density;em.radio.750-1500MHz)
  alpha  (n) Spectral index between 150 MHz and 1400 MHz fluxes as defined by equation 1 of the section 4.1 (alpha1.40.15) (Note 1)   (spect.index;em.radio.100-200MHz;em.radio.750-1500MHz)
  z  (n) Redshift obtained by photometry or spectroscopy (z) (src.redshift)
  r_z (char) Litterature reference of z (Note 2)   (meta.ref;src.redshift)
  L150 10+25W/Hz(n) Radio luminosity of the galaxy computed with redshift of optical counterpart and/or of the galaxy cluster as described by the equation 3 of the section 4.2 (L150) (phys.luminosity;em.radio.100-200MHz)
  Ref (char) Reference surveys in which the source is presented without identification as tailed radio galaxy (OtherCatalogue) (Note 3)   (meta.ref)

ALL cols		    
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