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Simple TargetList Of TargetsFast Xmatch with large catalogs or Simbad
Target Name (resolved by Sesame) or Position:
 Target dimension:
NB: The epoch used for the query is the original epoch of the table(s)Radius Box size

  
J/ApJS/256/43
  O-rich and C-rich AGB stars in our Galaxy (Suh, 2021)
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2021ApJS..256...43S
Similar Catalogs
Post annotation 		img(gal)
1.J/ApJS/256/43/table9(c)O-rich asymptotic giant branch (AGB) stars based on IRAS PSC (OAGB-IRAS) (5908 rows)
2.J/ApJS/256/43/table10(c)C-rich AGB stars based on IRAS PSC (CAGB-IRAS) (3596 rows)
3.J/ApJS/256/43/table11(c)O-rich asymptotic giant branch (AGB) stars based on AllWISE (OAGB-WISE) (5301 rows)
4.J/ApJS/256/43/table12(c)C-rich AGB stars based on AllWISE (CAGB-WISE) (3576 rows)
5.J/ApJS/256/43/table13OAGB-IRAS objects with obtained variation parameters from WISE light curves (885 rows)
6.J/ApJS/256/43/table14CAGB-IRAS objects with obtained variation parameters from WISE light curves (141 rows)
7.J/ApJS/256/43/table15OAGB-WISE objects with obtained variation parameters from WISE light curves (2468 rows)
8.J/ApJS/256/43/table16CAGB-WISE objects with obtained variation parameters from WISE light curves (216 rows)

Simple ConstraintList Of Constraints
 
Query by Constraints constraints help applied on Columns (Output Order: + - )
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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+5)OI-N  (i) [1/5908] OAGB-IRAS running sequence number (meta.id;meta.main)
   (ALL)Ref (char) Supgroup identifier (Note 1)   (meta.bib)
  (1+2+5+6)IRAS (char) IRAS PSC identifier (HHMMm+DDMM; B1950) (meta.id)
  (1+2+3+4)AKARIP (char) AKARI PSC identifier (HHMMSSs+DDMMSS, J2000; <AKARI-IRC-V1 JHHMMSSs+DDMMSS> in Simbad) (meta.id.cross)
  (1+2)AKARIB (char) AKARI BSC identifier (HHMMSSs+DDMMSS, J2000; <AKARI-FIS-V1 JHHMMSSs+DDMMSS> in Simbad) (meta.id.cross)
  (1+2+3+4)RAJ2000 deg (i) Best Right Ascension in decimal degrees (J2000) (pos.eq.ra;meta.main)
  (1+2+3+4)DEJ2000 deg (i) Best Declination in decimal degrees (J2000) (pos.eq.dec;meta.main)
  (1+2)BPos (char) Best position source (Note 2)   (meta.note)
  (1+2+3+4)WISEA (char) ALLWISE identifier (JHHMMSS.ss+DDMMSS.s) (meta.id.cross)
  (1+2)SpType (char) Kwok+ 1997, J/ApJS/112/557 spectral type (src.spType)

ALL cols		    
 (i)indexed column
  (1+2)LRS (char) Kwok+ 1997, J/ApJS/112/557 IRAS LRS type (meta.note)
  (1+2+3+4)AName (char) AAVSO identifier (meta.id.cross)
   (ALL)AType (char) AAVSO variable type (src.class)
   (ALL)APer d (n) [0.06/2052.2] AAVSO period (time.period)
  (1)OH (char) A OH maser detection? (See Section 5.2) (meta.code)
  (1)SiO (char) A SiO maser detection? (See Section 5.2) (meta.code)
  (1)Var (char) Display variation parameters obtained from WISE LCs (link to Table 13) (meta.ref.url)
  (1+2+3+4)GCat  (n)Display data from Messineo+, 2018, J/A+A/619/A35 ; Soszynski+, 2013, J/AcA/63/21 and Stroh+, 2019, J/ApJS/244/25 (meta.ref.url)
  (1+2+3+4)Simbad (char) ask the Simbad data-base about this object (meta.ref.url)
  (2+6)CI-N   [1/3596] CAGB-IRAS running sequence number (meta.id;meta.main)
  (2+3+4)Var  (n)Display variation parameters obtained from WISE LCs (link to Table 14) (meta.ref.url)
  (3+7)OW-N   [1/5301] OAGB-WISE running sequence number (meta.id;meta.main)
  (3+4)recStar   [0/232397] Record number / Star number (meta.record)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (3+4)2MASS (char) 2MASS identifier (HHMMSSss+DDMMSSss; J2000) (meta.id.cross)
  (3+4)MSX6C (char) MSX identifier (GLLL.llll+BB.bbbb) (meta.id.cross)
  (4+8)CW-N   [1/3576] CAGB-WISE running sequence number (meta.id;meta.main)
  (5+6)EP d (n) [51.7/3079.2] Expected period (Note 1)   (time.period)
  (5+6+7+8)G-W1(P) d (n) [52.6/2290.1] Good period derived from WISE W1 light curve (time.period)
  (5+6+7+8)G-W1(A) mag (n) [0.06/2.11] Good amplitude derived from WISE W1 light curve (src.var.amplitude)
  (5+6+7+8)G-W1(R2)  (n) [0.6/0.98] Good R2 derived from WISE W1 light curve (stat.fit.param)
  (5+6+7+8)GM-W1(P) d (n) [163.82/1699.1] Good selected period derived from WISE W1 light curve for an object known as a Mira variable with period (time.period)
  (5+6+7+8)GM-W1(A) mag (n) [0.2/1.5] Good amplitude derived from WISE W1 light curve for an object known as a Mira variable with period (src.var.amplitude)
  (5+6+7+8)GM-W1(R2)  (n) [0.3/0.97] Good R2 derived from WISE W1 light curve for an object known as a Mira variable with period (stat.fit.param)
  (5+6)GN-W1(P) d (n) [72.27/2290.05] Good selected period derived from WISE W1 light curve for an object with unknown period or known as a non-Mira variable (time.period)
  (5+6)GN-W1(A) mag (n) [0.05/1.8] Good amplitude derived from WISE W1 light curve for an object with unknown period or known as a non-Mira variable (src.var.amplitude)
  (5+6)GN-W1(R2)  (n) [0.04/0.98] Good R2 derived from WISE W1 light curve for an object with unknown period or known as a non-Mira variable (stat.fit.param)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (5+6+7+8)G-W2(P) d (n) [56/2263] Good period derived from WISE W2 light curve (time.period)
  (5+6+7+8)G-W2(A) mag (n) [0.07/4.92] Good amplitude derived from WISE W2 light curve (src.var.amplitude)
  (5+6+7+8)G-W2(R2)  (n) [0.6/0.98] Good R2 derived from WISE W2 light curve (stat.fit.param)
  (5+6+7+8)GM-W2(P) d (n) [157.34/1778.2] Good selected period derived from WISE W2 light curve for an object known as a Mira variable with period (time.period)
  (5+6+7+8)GM-W2(A) mag (n) [0.099/2.2] Good amplitude derived from WISE W2 light curve for an object known as a Mira variable with period (src.var.amplitude)
  (5+6+7+8)GM-W2(R2)  (n) [-0.23/0.94] Good R2 derived from WISE W2 light curve for an object known as a Mira variable with period (stat.fit.param)
  (5+6)GN-W2(P) d (n) [72.4/2263] Good selected period derived from WISE W2 light curve for an object with unknown period or known as a non-Mira variable (time.period)
  (5+6)GN-W2(A) mag (n) [0.07/2.2] Good amplitude derived from WISE W2 light curve for an object with unknown period or known as a non-Mira variable (src.var.amplitude)
  (5+6)GN-W2(R2)  (n) [-0.2/0.97] Good R2 derived from WISE W2 light curve for an object with unknown period or known as a non-Mira variable (stat.fit.param)

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