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  Abundances of φ Her (Zavala+, 2007)
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1.J/ApJ/655/1046/table2Astrometric solutions for φ Her (25 rows)
2.J/ApJ/655/1046/table7Abundances of φ Her including new lines (196 rows)
3.J/ApJ/655/1046/table8Comparison of derived and solar abundances (log N/H) (33 rows)

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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)
  (1)ObsY yr Julian Year of NPOI observation (time.epoch;obs)
  (1)rho mas Fitted binary separation (pos.angDistance;meta.modelled)
  (1)theta deg Fitted binary position angle (pos.posAng;meta.modelled)
  (1)errMaj mas Semimajor axis of error ellipse (phys.angSize.smajAxis;pos.errorEllipse)
  (1)errMin mas Semiminor axis of error ellipse (phys.angSize.sminAxis;pos.errorEllipse)
  (1)errPA deg Position angle of error ellipse (pos.posAng;pos.errorEllipse)
  (1)Crho mas Calculated binary separation (pos.angDistance;meta.modelled)
  (1)Ctheta deg Calculated binary position angle (pos.posAng;meta.modelled)
  (1)(O-C)rho mas Binary separation (O-C) value (pos.angDistance;
  (1)(O-C)theta deg Binary position angle (O-C) value (pos.posAng;

ALL cols
 (i)indexed column
  (2+3)Ion (char) Species name (Note 1)   (;meta.main)
  (2)Mult (char) Muliplet identification (Note 2)   (phys.atmol.level)
  (2)lambda 0.1nm (n) Laboratory wavelength in Angstroms (em.wl)
  (2)log(gf) [-] (n) Log of the gf value (stat.value;phys.absorption.coeff)
  (2)r_log(gf) (char) Reference for log(gf) (Note 3)   (meta.ref;pos.frame)
  (2)EW 0.1pm (n) Observed equivalent width in milliAngstroms (spect.line.eqWidth)
  (2)logN/NT [-] (n) Log of the derived number abundance (phys.abund)
  (3)AAbd [-] (n) Adelman et al. (2001, Cat. J/A+A/367/597) φ Her A abundance (phys.abund)
  (3)e_AAbd [-] (n) Uncertainty in AAbd (stat.error)
  (3)ATP [-] This paper's φ Her A abundance (phys.abund)
  (3)e_ATP [-] (n) Uncertainty in ATP (Note 2)   (stat.error)
  (3)n_ATP  (n) Number of lines used in ATP (meta.note)
  (3)Sun [-] Solar abundance (Note 3)   (phys.abund)

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