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/491/3606
  Effects of metallicity on HMXB formation (Ponnada+, 2020)
ReadMe+ftp
2020MNRAS.491.3606P
Similar Catalogs
Post annotation 		img(gal)
1.J/MNRAS/491/3606/tablea1(c)BCDs including the Brorby et al. (2014MNRAS.441.2346B) and NED sample (46 rows)
2.J/MNRAS/491/3606/tablea2X-ray source photometry (46 rows)
3.J/MNRAS/491/3606/tablea3UV measurements and SFRs (46 rows)

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)Name (char) Galaxy name (meta.id;meta.main)
  (1)ID  ObsID from Chandra (meta.id)
  (1)12+log(O/H) [-] Oxygen abundance 12+log(O/H) (phys.abund)
  (1)r_12+log(O/H) (char) Reference for 12+log(O/H) (Note 1)   (meta.ref;pos.frame)
  (1)RAJ2000 "h:m:s" (i) Right ascension (J2000) (pos.eq.ra;meta.main)
  (1)DEJ2000 "d:m:s" (i) Declination (J2000) (pos.eq.dec;meta.main)
  (1)Exptime ks Chandra exposure time (time.duration;obs.exposure)
  (1)Dist Mpc Distance (pos.distance)
  (1)SimbadName (char) (n)Designation understandable by the Simbad data-base (meta.id)
  (2)f_Name (char) [*] Flag on Name (Note 1)   (meta.code)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (2)nH 10+20cm-2Column density obtained using the Colden tool (phys.columnDensity)
  (2)R25 arcsec R25 taken from HyperLeda and modified as described in Section 3 (phys.angSize;src)
  (2)R25HL arcsec Major axis radius at the 25B-mag/arcsec2 from HyperLeda (R25=D25/2) (phys.angSize;src)
  (2)PA deg [] Position angle from HyperLEDA (pos.posAng)
  (2)NsupLmin  Number of observed sources within the D25 ellipse with luminosity greater than Lmin (meta.number)
  (2)Nbkg  Number of expected background sources within the D25 ellipse, as determined by logN-logS curves of Georgakakis et al. (2008MNRAS.388.1205G) (meta.number)
  (2)Lmin 10+31W Luminosity limit calculated for the 0.5-8.0keV energy band (phys.luminosity;em.X-ray)
  (3)E(B-V) mag Extinction obtained using the Infrared Science Archive (IRSA) tool DUST (phot.color.excess)
  (3)CRFUV ct/s Count rate in the FUV band of GALEX observations (phot.count;em.UV)
  (3)LFUV 10+19W/HzLuminosity in the FUV band, 1350-1750Å (phys.luminosity;em.UV)
  (3)SFRFUV 10-3Msun/yrStar formation rate as determined by the Hunter et al. (2010AJ....139..447H) method (phys.SFR)
  (3)CRNUV ct/s Count Rate in the NUV band of GALEX, 1750-2800Å (phot.count;em.UV)
  (3)SFRNUV 10-3Msun/yrStar formation rate in the NUV (phys.SFR)
  (3)SFRIR 10-3Msun/yr(n) Star formation rate in the IR via Spitzer images (Brorby et al. 2014MNRAS.441.2346B) (phys.SFR)

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