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J/AJ/156/78
  44 validated planets from K2 Campaign 10 (Livingston+, 2018)
Post annotation
  
1.J/AJ/156/78/vespaIndividual false positive scenario likelihoods computed by vespa (table 7) and additional constraints to vespa (table 8) (72 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)
  EPIC (char) EPIC number (EPIC NNNNNNNNN.NN) (meta.id;meta.main)
  L-beb   [0/0.0006] Likelihood that the signal is due to a background eclipsing binary, at the measured period (stat.likelihood)
  L-beb-Px2   [0/0.0014] Likelihood that the signal is due to a background eclipsing binary, at twice the measured period (stat.likelihood)
  L-eb (char) [9.4e-114/0.0029] Likelihood that the signal is due to an eclipsing binary, at the measured period (stat.likelihood)
  L-eb-Px2   [1.4e-16/0.00039] Likelihood that the signal is due to an eclipsing binary, at twice the measured period (stat.likelihood)
  L-heb (char) [7.7e-224/1.9e-05] Likelihood that the signal is due to a hierarchical star system with an eclipsing component, at the measured period (stat.likelihood)
  L-heb-Px2 (char) [1.4e-102/1e-05] Likelihood that the signal is due to a hierarchical star system with an eclipsing component, at twice the measured period (stat.likelihood)
  L-pl   [0.00017/7.5] Likelihood that the signal is due to a planet (stat.likelihood)
  FPP   [9.5e-15/0.64] False Positive Probability (stat.fit.goodness)
  MaxRad arcsec [6.4/32.6] Maximum radius (the angular size of the photometric aperture) (phys.angSize;src)
  Thresh   [1e-05/0.003] Secondary eclipse threshold (the maximum secondary eclipse depth allowed by the light curve) (phot.mag;stat.min)

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