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. ((unassigned);phys.veloc.orbital;arith.diff;phys.veloc)
  (1+2+4+5)ID (char) p-mode frequency identifier ((unassigned);phys.veloc.orbital;arith.diff;spect.line.veloc;arith)
   (ALL)Freq uHz p-mode frequencies detected for PG 0048+091 ((unassigned);(unassigned);(unassigned);instr.spect)
  (1+2+4+5)e_Freq uHz (n) Error on Freq ((unassigned);(unassigned);(unassigned);time.age;meta.main)
  (1+4)Stoc (char) In this column, 'stochastic' indicates there is a broad excess of power ((unassigned);phys.veloc.orbital;arith.diff;pos.eq.dec)
  (1+2+4+5)Amp 10-3 (n) Amplitude (in ppt) ((unassigned);(unassigned);(unassigned);pos.supergalactic.lat;meta.main)
  (1+2+4+5)S/N  (n) Signal to noise ratio ((unassigned);(unassigned);(unassigned);meta.abstract;meta.main)
  (1+2)mode (char) Mode of degree and azimuthal order (l,m) ((unassigned);(unassigned);(unassigned);pos.bodyrc.lon;meta.main)
  (1)f2004/5 (char) Closest frequency from Reed et al. (2007ApJ...664..518R) ((unassigned);(unassigned);(unassigned);instr.spect)
  (2+5)Period s Period ((unassigned);(unassigned);(unassigned);phys.dust;meta.main)
  (2+5)e_Period s Error on Period ((unassigned);(unassigned);(unassigned);time.age;phys.electCharge;meta.main)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (2+5)n  (n) Relative radial indices ((unassigned);(unassigned);(unassigned);pos.bodyrc.lon;meta.main)
  (2+5)Dev  (n) Deviation from the asymptotic sequence ((unassigned);(unassigned);(unassigned);pos.bodyrc.lon;meta.main)
  (3)LW1 uHz Lorentzian width form the power spectra fit ((unassigned);(unassigned);(unassigned);pos.supergalactic.lat;meta.main)
  (3)LW2 uHz (n) Second Lorentzian width form the power spectra fit ((unassigned);(unassigned);(unassigned);pos.supergalactic.lat;meta.main)
  (3)Hi1 10-6 Power form the power spectra fit (in ppt2) ((unassigned);(unassigned);(unassigned);pos.bodyrc.lon;meta.main)
  (3)Hi2 10-6 (n) Second Power form the power spectra fit (in ppt2) ((unassigned);phys.veloc.orbital;arith.diff;pos.bodyrc.lon;meta.main)
  (4)mode  (n) Mode of degree and azimuthal order (l,m) ((unassigned);phys.veloc.orbital;arith.diff;pos.bodyrc.lon;meta.main)
  (5)m  (n) Azimuthal order, if a multiplet (Note 1)   ((unassigned);(unassigned);(unassigned);pos.bodyrc.lon;meta.main)
  (6)LW uHz Lorentzian width form the power spectra fit ((unassigned);(unassigned);(unassigned);pos.supergalactic.lat;meta.main)
  (6)Hi  Power form the power spectra fit (in ppt2) ((unassigned);(unassigned);(unassigned);pos.bodyrc.lon;meta.main)

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