VizieR

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

VizieR

  
J/MNRAS/483/2282
  p-mode-dominated subdwarf B pulsators in binaries (Reed+, 2019)
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2019MNRAS.483.2282R
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1.J/MNRAS/483/2282/table4p-mode frequencies detected for PG 0048+091 (188 rows)
2.J/MNRAS/483/2282/table5g-mode frequencies detected for PG 0048+091 (18 rows)
3.J/MNRAS/483/2282/table6Lorentzian widths and power (Hi) fitted to observations for PG 0048+091 (8 rows)
4.J/MNRAS/483/2282/table7p-mode frequencies detected for PG 1315-123 (46 rows)
5.J/MNRAS/483/2282/table8g-mode frequencies detected for PG 1315-123 (16 rows)
6.J/MNRAS/483/2282/table9Lorentzian widths fitted to observations of PG 1315-123 (4 rows)

Simple ConstraintList Of Constraints
 
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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+2+4+5)ID (char) p-mode frequency identifier (meta.id;meta.main)
   (ALL)Freq uHz p-mode frequencies detected for PG 0048+091 (em.freq)
  (1+2+4+5)e_Freq uHz (n) Error on Freq (stat.error)
  (1+4)Stoc (char) In this column, 'stochastic' indicates there is a broad excess of power (meta.code)
  (1+2+4+5)Amp 10-3 (n) Amplitude (in ppt) (src.var.amplitude)
  (1+2+4+5)S/N  (n) Signal to noise ratio (stat.snr)
  (1+2)mode (char) Mode of degree and azimuthal order (l,m) (stat.fit.param)
  (1)f2004/5 (char) Closest frequency from Reed et al. (2007ApJ...664..518R) (em.freq)
  (2+5)Period s Period (time.period)
  (2+5)e_Period s Error on Period (stat.error;time.period)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (2+5)n  (n) Relative radial indices (stat.fit.param)
  (2+5)Dev  (n) Deviation from the asymptotic sequence (stat.fit.param)
  (3)LW1 uHz Lorentzian width form the power spectra fit (src.var.amplitude)
  (3)LW2 uHz (n) Second Lorentzian width form the power spectra fit (src.var.amplitude)
  (3)Hi1 10-6 Power form the power spectra fit (in ppt2) (stat.fit.param)
  (3)Hi2 10-6 (n) Second Power form the power spectra fit (in ppt2) (stat.fit.param)
  (4)mode  (n) Mode of degree and azimuthal order (l,m) (stat.fit.param)
  (5)m  (n) Azimuthal order, if a multiplet (Note 1)   (stat.fit.param)
  (6)LW uHz Lorentzian width form the power spectra fit (src.var.amplitude)
  (6)Hi  Power form the power spectra fit (in ppt2) (stat.fit.param)

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