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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/MNRAS/510/4998
  ATOMS IV Gas clumps properties and SFRs (Zhang+, 2022)
ReadMe+ftp
2022MNRAS.510.4998Z
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Post annotation 		img(gal)
1.J/MNRAS/510/4998/table5Luminosities of ATOMS sources (146 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 source number (ID) (meta.id)
  IRAS (char) IRAS source identifier (IHHMMm±DDMM) (IRAS) (meta.id;meta.main)
  RAJ2000 "h:m:s" (i) Right ascension (J2000) (pos.eq.ra;meta.main)
  DEJ2000 "d:m:s" (i) Declination (J2000) (pos.eq.dec;meta.main)
  D kpc Distance of the source (Distance) (pos.distance)
  RGC kpc Galactocentric distance (RGC) (pos.distance;pos.galactocentric)
  logLbol [Lsun] Logarithm of the bolometric luminosity are calculated from integrating the whole SED (logLbol) (phys.luminosity)
  logL'CS [K.km/s/pc2](n) The molecular carbon monosulfide CS line luminosity from equation 1 of the section 3.3 The Lbol-L'mol scaling relations (logL'CS) (phys.luminosity;phys.mol;em.line)
  logL'HC3N [K.km/s/pc2](n) The molecular cyanoacetylene HC3N line luminosity from equation 1 of the section 3.3 The Lbol-L'mol scaling relations (logL'HC3N) (phys.luminosity;phys.mol;em.line)
  Simbad  ask the Simbad data-base about this object (meta.ref.url)

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