VizieR

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

VizieR

  
J/ApJS/243/28
  M-type star magnetic activities from LAMOST & Kepler (Lu+, 2019)
Post annotation
img(gal)
1.J/ApJS/243/28/table5Hα variability of LAMOST M-type stars (5499 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)
  Seq   [1/5499] Sequential running number (meta.id)
  LAMOST (char) LAMOST spectral name (JHHMMSS.ss+DDMMSS.s) (meta.id;meta.main)
  SpT (char) Spectral type (src.spType)
  NObs   [2/21] Number of spectra observed by LAMOST (meta.number)
  Max(EWHa) 0.1nm [0.7/337] Maximum Hα equivalent width (spect.line.eqWidth;stat.max;em.line.Halpha)
  e_Max(EWHa) 0.1nm [0.01/88] Uncertainty in Max(EWHa) (stat.error)
  Min(EWHa) 0.1nm [0.7/192] Minumum Hα equivalent width (spect.line.eqWidth;stat.min;em.line.Halpha)
  e_Min(EWHa) 0.1nm [0.01/25] Uncertainty in Min(EWHa) (stat.error)
  REW   [1/24.2] Ratio, Max(EWHa)/Min(EWHa) (spect.line.intensity;arith.ratio)
  dEW 0.1nm [0/265] Difference, Max(EWHa)-Min(EWHa) (src.var.amplitude)
  e_dEW 0.1nm [0.02/88.5] Uncertainty, dEW (stat.error)
  Var (char) [Yes, No] Is Hα variable? (meta.code)

ALL cols
    
 (i)indexed column
Adapt form
Display your selection only Reset to default columns
usage  Display UCD1+    UCD1  
elapse time 0