VizieR

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

VizieR

  
J/A+A/297/391
  T Tauri stars ROSAT survey (Neuhaeuser+, 1995)
Post annotation
img(gal)
1.J/A+A/297/391/table6Statistical significance for classical T Tauri stars (CTTS) and weak-line T Tauri stars (WTTS) being different (19 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)
  Test (char) Test item property (meta.note)
  n_Test (char) Note on Test (Note 1)   (meta.note)
  unit (char) Test item unit (meta.unit)
  CTTSs  Classical T Tauri stars (CTTS) sample size (meta.number)
  CTTSsul  (n) []? Upper limits of the CTTS sample size (meta.number)
  CTTSmn  CTTS mean (src.sample;stat.mean)
  e_CTTSmn  rms uncertainty on CTTS mean (stat.error)
  CTTSmd  (n) []? CTTS median (meta.number)
  WTTSs  Weak-line T Tauri stars (WTTS) sample size (meta.number)
  WTTSsul  (n) []? Upper limits of the WTTS sample size (meta.number)
  WTTSmn  WTTS mean (src.sample;stat.mean)
  e_WTTSmn  rms uncertainty on WTTS mean (stat.error)
  WTTSmd  WTTS median (src.sample;stat.median)
  PrGWpe % Probability for the null hypothesis that CTTS and WTTS distributions are similar according to Gehan's generalized Wilcoxon test for permutation variance (stat.fit.goodness)
  PrGWhy % Probability for the null hypothesis that CTTS and WTTS distributions are similar according to Gehan's generalized Wilcoxon test for hypergeometric variance (stat.fit.goodness)
  PrLogRank  Probability for the null hypothesis that CTTS and WTTS distributions are similar according to the logrank test (c.f. Sec. 5.1.) (stat.fit.goodness)

ALL cols
    
(n) indicates a possible blank or NULL column(i)indexed column
Adapt form
Display your selection only Reset to default columns
usage  Display UCD1+    UCD1  
elapse time 0

Cite/acknowledge VizieR catalogue
Rules of usage of VizieR data

© UDS/CNRS

Contact