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Simple TargetList Of TargetsFast Xmatch with large catalogs or Simbad
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J/A+A/703/A294
  Post-RGB binaries and stable mass transfer (Moltzer+, 2025)
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2025A&A...703A.294M
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Post annotation 		img(gal)
1.J/A+A/703/A294/tablec7Estimated orbital periods and post-mass-transfer ages of the post-RGB binary candidate subsamples in the LMC and SMC (75 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)
  Name (char) Identification (JHHMMSS.ss+DDMMSS.s or OGLE-LMC-T2CEP-NNN) (meta.id;meta.main)
  Host (char) [SMC LMC] Host Magellanic Cloud (meta.id.parent)
  Porbmean d (n) Estimated orbital period determined from its luminosity (Note 1)   (time.period)
  f_Porbmean   [0/1] If true (1), the orbital period is a lower limit as the luminosity of the object is larger than the maximum luminosity of the binary models (meta.code)
  Porbmin d (n) Estimated orbital period determined from the lower limit of its luminosity (Note 1)   (time.period)
  Porbmax d (n) Estimated orbital period determined from the upper limit of its luminosity (Note 1)   (time.period)
  f_Porbmax   [0/1] If true (1), the maximum orbital period is a lower limit as the luminosity upper limit of the object is larger than the maximum luminosity of the binary models (meta.code)
  Agemeansol yr Estimated post-mass-transfer age determined from its position in the HRD compared to the solar model grid (time.age)
  f_Agemeansol   [0/1] If true (1), the mean post-mass-transfer age is an upper limit, as the luminosity of the object is larger than the maximum luminosity of the solar model grid (meta.code)
  Ageminsol yr Estimated minimum post-mass-transfer age determined from its position in the HRD compared to the solar model grid (time.age;stat.min)

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(n) indicates a possible blank or NULL column(i)indexed column
  f_Ageminsol   [0/1] If true (1), the minimum post-mass-transfer age is an upper limit, as the luminosity lower limit of the object is larger than the maximum luminosity of the solar model grid (meta.code)
  Agemaxsol yr Estimated maximum post-mass-transfer age determined from its position in the HRD compared to the solar model grid (time.age;stat.max)
  f_Agemaxsol   [0/1] If true (1), the maximum post-mass-transfer age is an upper limit, as the luminosity upper limit of the object is larger than the maximum luminosity of the solar model grid (meta.code)
  Agemeanmp yr Estimated post-mass-transfer age determined from its position in the HRD compared to the metal-poor model grid (time.age)
  f_Agemeanmp   [0/1] If true (1), the mean post-mass-transfer age is an upper limit, as the luminosity of the object is larger than the maximum luminosity of the metal-poor model grid (meta.code)
  Ageminmp yr Estimated minimum post-mass-transfer age determined from its position in the HRD compared to the metal-poor model grid (time.age;stat.min)
  f_Ageminmp   [0/1] If true (1), the minimum post-mass-transfer age is an upper limit, as the luminosity lower limit of the object is larger than the maximum luminosity of the metal-poor model grid (meta.code)
  Agemaxmp yr Estimated maximum post-mass-transfer age determined from its position in the HRD compared to the metal-poor model grid (time.age;stat.max)
  f_Agemaxmp   [0/1] If true (1), the maximum post-mass-transfer age is an upper limit, as the luminosity upper limit of the object is larger than the maximum luminosity of the metal-poor model grid (meta.code)
  _RA deg (i) Positions from Name and Simbad (right ascension part) (pos.eq.ra;meta.main)
  _DE deg (i) Positions from Name and Simbad (declination part) (pos.eq.dec;meta.main)

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