VizieR

CfA VizieR . ADAC VizieR . Cambridge (UK) VizieR . IUCAA VizieR . INASAN VizieR .

VizieR

  
J/AJ/156/78
  44 validated planets from K2 Campaign 10 (Livingston+, 2018)
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2018AJ....156...78L
Similar Catalogs
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)

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)
  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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