VizieR

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

VizieR

Simple TargetList Of TargetsFast Xmatch with large catalogs or Simbad
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J/MNRAS/516/2080
  Variability of {delta} Scuti stars with TESS LC (Barac+, 2022)
ReadMe+ftp
2022MNRAS.516.2080B
Similar Catalogs
Post annotation 		img(gal)
1.J/MNRAS/516/2080/table1(c)Compilation of 62 stars identified as non-{delta} Sct stars (62 rows)
2.J/MNRAS/516/2080/table2(c)Properties of {delta} Sct stars in our sample (372 rows)
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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)
   (ALL)HD  (n) HD designation number as HD NNNNNN (HD) (meta.id.assoc)
   (ALL)Name (char) Star name (Name) (meta.id)
   (ALL)TIC  TIC number identifier (TIC) (meta.id;meta.main)
   (ALL)r_Name  (n) [0/1] Flag indicates reference (R2000) (Note 1)   (meta.ref;pos.frame)
   (ALL)R2000/C2013 (char) Display R2000 or C2013 catalogs data (meta.ref.url)
   (ALL)Simbad (char) ask the Simbad data-base about this object (meta.ref.url)
   (ALL)_RA deg (i) Right Ascension (J2000) from SIMBAD (not part of the original data) (pos.eq.ra;meta.main)
   (ALL)_DE deg (i) Declination (J2000) from SIMBAD (not part of the original data) (pos.eq.dec;meta.main)
  (2)fcat 1/d (n) Published dominant frequency from previous references (fcat) (em.freq;src.var)
  (2)f1 1/d Frequency of the dominant frequency measured with our TESS light curves (f1) (em.freq;src.var)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (2)a1 10-12 Amplitude of the dominant frequency measured with our TESS light curves (a1) (src.var.amplitude)
  (2)Dist pc (n) Star distance based on values from GaiaDR3 (Gaia Collaboration Cat. I/355) and computed as explianed in section 4 P-L relation (dist) (pos.distance)
  (2)e_Dist pc (n) Mean uncertainty of Dist (e_dist) (stat.error)
  (2)AV mag Interstellar dust extinction calculated by fitting the star SED (AV) (Note 2)   (phys.absorption;meta.modelled)
  (2)e_AV mag Mean uncertainty of AV (e_AV) (stat.error)
  (2)VMag  Absolute V-band magnitude related to period, distance, parallax and AV values as equations 1, 3 and 4 of the section 4 P-L relation show (MV) (phys.magAbs;em.opt.V;meta.modelled)
  (2)e_VMag  Mean uncertainty of VMag (e_MV) (stat.error)

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