VizieR

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

  
J/ApJS/256/43
  O-rich and C-rich AGB stars in our Galaxy (Suh, 2021)
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2021ApJS..256...43S
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1.J/ApJS/256/43/table14CAGB-IRAS objects with obtained variation parameters from WISE light curves (141 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)
  CI-N   [6/3590] CAGB-IRAS identifier (see Table 10) (meta.id;meta.main)
  AType (char) AAVSO variable type (src.class)
  APer d (n) [0.29/1060] AAVSO period (time.period)
  EP d (n) [83.5/3990.5] Expected period (Note 1)   (time.period)
  G-W1(P) d (n) [51.5/2185.4] Good period derived from WISE W1 light curve (time.period)
  G-W1(A) mag (n) [0.4/2.9] Good amplitude derived from WISE W1 light curve (src.var.amplitude)
  G-W1(R2)  (n) [0.6/0.96] Good R2 derived from WISE W1 light curve (stat.fit.param)
  GM-W1(P) d (n) [130.29/1018] Good selected period derived from WISE W1 light curve for an object known as a Mira variable with period (time.period)
  GM-W1(A) mag (n) [0.44/2.93] Good amplitude derived from WISE W1 light curve for an object known as a Mira variable with period (src.var.amplitude)
  GM-W1(R2)  (n) [0.2/0.94] Good R2 derived from WISE W1 light curve for an object known as a Mira variable with period (stat.fit.param)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  GN-W1(P) d (n) [90/1183] Good selected period derived from WISE W1 light curve for an object with unknown period or known as a non-Mira variable (time.period)
  GN-W1(A) mag (n) [0.4/2.7] Good amplitude derived from WISE W1 light curve for an object with unknown period or known as a non-Mira variable (src.var.amplitude)
  GN-W1(R2)  (n) [-0.03/0.96] Good R2 derived from WISE W1 light curve for an object with unknown period or known as a non-Mira variable (stat.fit.param)
  G-W2(P) d (n) [52.49/2500] Good period derived from WISE W2 light curve (time.period)
  G-W2(A) mag (n) [0.085/3.4] Good amplitude derived from WISE W2 light curve (src.var.amplitude)
  G-W2(R2)  (n) [0.6/0.96] Good R2 derived from WISE W2 light curve (stat.fit.param)
  GM-W2(P) d (n) [364.9/1002] Good selected period derived from WISE W2 light curve for an object known as a Mira variable with period (time.period)
  GM-W2(A) mag (n) [0.6/7] Good amplitude derived from WISE W2 light curve for an object known as a Mira variable with period (src.var.amplitude)
  GM-W2(R2)  (n) [0.6/0.9] Good R2 derived from WISE W2 light curve for an object known as a Mira variable with period (stat.fit.param)
  GN-W2(P) d (n) [92.28/1191] Good selected period derived from WISE W2 light curve for an object with unknown period or known as a non-Mira variable (time.period)
  GN-W2(A) mag (n) [0.09/3.14] Good amplitude derived from WISE W2 light curve for an object with unknown period or known as a non-Mira variable (src.var.amplitude)
  GN-W2(R2)  (n) [0.048/0.92] Good R2 derived from WISE W2 light curve for an object with unknown period or known as a non-Mira variable (stat.fit.param)
  Ref (char) Supgroup identifier (see Table 10) (meta.bib)
  IRAS (char) IRAS PSC identifier (meta.id)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
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