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

  Stellar Content of LH 9 and 10 in the LMC (Parker+ 1992)
Post annotation
1.J/AJ/103/1205/starsAll stars with UBV photometry with their bolometric magnitudes and effective temperatures which were not listed in the original tables (tables 10 to 12). (795 rows)

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)
  Star (char) (i) Star number (Note 1)   (;meta.main)
  RA2000 "h:m:s" (i) Right ascension (2000) (pos.eq.ra;meta.main)
  DE2000 "d:m:s" (i) Declination (2000) (pos.eq.dec;meta.main)
  Xpos pix X position (Note 2)   (pos.cartesian.x;instr.det)
  Ypos pix Y position (Note 2)   (pos.cartesian.y;instr.det)
  Vmag mag V magnitude (phot.mag;em.opt.V)
  B-V mag B-V colour index (phot.color;em.opt.B;em.opt.V)
  U-B mag U-B colour index (phot.color;em.opt.U;em.opt.B)
  Q mag (U-B)-0.72(B-V) (phot.color.reddFree)
  E(B-V) mag Color excess calculated from Q or spectral type or mean reddening as discussed in Section 3.1 of the article. (phot.color.excess)
  Mv mag Absolute V magnitude=V-Rv*E(B-V)-DM where Rv=3.1, and the distance modulus DM=18.3 mag (phys.magAbs;em.opt)
  log(Teff) [K] log10 of the effective temperature: is calculated from Q or (B-V)0 as discussed in Section 3.2 of the article. (phys.temperature.effective)
  Mbol mag Bolometric magnitude=Mv+BC, where BC is calculated from Teff as discussed in Section 3.2 of the article. (phot.mag.bol)
  Sp (char) Spectral type and luminosity class as determined from spectroscopic observations (Note 3)   (src.spType)
  Comments (char) Comments (Note 4)   (meta.note)

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