VizieR

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

Simple TargetList Of TargetsFast Xmatch with large catalogs or Simbad
Target Name (resolved by Sesame) or Position:
 Target dimension:
NB: The epoch used for the query is the original epoch of the table(s)Radius Box size

  
J/A+AS/146/103
  CaII H&K to CaII IRT echelle spectra (Montes+, 2000)
ReadMe+ftp
2000A&AS..146..103M
Similar Catalogs
Post annotation 		img(gal)
1.J/A+AS/146/103/stars(c)Star positions (from Simbad) (16 rows)
2.J/A+AS/146/103/table3Hα line measures in the observed and subtracted spectra (56 rows)
3.J/A+AS/146/103/table5Hβ line measurements in the observed and subtracted spectra (36 rows)
4.J/A+AS/146/103/table6CaII H&K and Hε lines measures in the observed and subtracted spectra (35 rows)
5.J/A+AS/146/103/table7CaII IRT lines measures in the observed and subtracted spectra (58 rows)

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)Name (char) (i) Star name (meta.id;meta.main)
  (1)RAJ2000 "h:m:s" (i) Right ascension (J2000.0) (pos.eq.ra;meta.main)
  (1)DEJ2000 "d:m:s" (i) Declination (J2000.0) (pos.eq.dec;meta.main)
  (2+3+4+5)Obs (char) Telescope and observation run (Note G1)   (meta.code;obs)
  (2+3+4+5)phi  (n) [0/1[ Orbital phase (time.phase)
  (2+3+4+5)E (char) [HCTP] Type of emission (Note G2)   (src.class)
  (2)SH  (n) Relative contribution of the hot component to the total continuum (stat.param)
  (2)SC  (n) Relative contribution of the cool component to the total continuum (stat.param)
  (2)Halpha (char) [AEF] Observed Hα profile: A: absorption, E: emission, F: totally filled-in by emission (spect.index;em.line.Halpha)
  (2+3)Wobs 0.1nm (n) Full width at half maximum in the observed spectrum (spect.line.width)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (2+3)Rc  Residual intensity in the observed spectrum (Rc=Fc/Fcont) (phot.count;em.opt)
  (2+3)EWobs 0.1nm (n) Equivalent width in the observed spectrum (spect.line.eqWidth)
  (2+3)Wsub 0.1nm (n) Full width at half maximum in the subtracted spectrum (spect.line.width)
  (2+3)Int  (n) Peak emission intensity in the subtracted spectrum (spect.line.intensity)
  (2+3)EWSub 0.1nm Excess Hα emission equivalent width in the subtracted spectrum (Note 1)   (spect.line.eqWidth)
  (2)logFS(Ha) [10mW/m2/nm]Absolute flux at the stellar surface (phot.flux)
  (3)EW(Ha)/EW(Hb)  (n) Ratio of excess emission EW in the Hα and Hβ lines (phot.flux;arith.ratio)
  (3)E(Ha)/E(Hb)  (n) Corrected ratio of excess emission (Note 2)   (phot.flux;arith.ratio)
  (4)EW(K)r 0.1nm CaII K equivalent width obtained by reconstruction of the absorption line profile (spect.line.eqWidth)
  (4)EW(H)r 0.1nm CaII H equivalent width obtained by reconstruction of the absorption line profile (spect.line.eqWidth)
  (4)EW(He)r 0.1nm (n) Hε equivalent width obtained by reconstruction of the absorption line profile (spect.line.eqWidth)
  (4)EW(K)s 0.1nm CaII K equivalent width using spectral subtraction technique (Note 1)   (spect.line.eqWidth)
  (4)EW(H)s 0.1nm CaII H equivalent width using spectral subtraction technique (Note 1)   (spect.line.eqWidth)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (4)EW(He)s 0.1nm (n) Hε equivalent width using spectral subtraction technique (Note 1)   (spect.line.eqWidth)
  (4)logF(K) [10mW/m2/nm]CaII K surface flux (Note 2)   (phot.flux)
  (4)logF(H) [10mW/m2/nm]CaII H surface flux (Note 2)   (phot.flux)
  (4)logF(He) [10mW/m2/nm](n) Hε surface flux (Note 2)   (phot.flux)
  (5)EW(8498)r 0.1nm (n) λ8498 equivalent width obtained by absorption line profile reconstruction (spect.line.eqWidth)
  (5)EW(8542)r 0.1nm (n) λ8542 equivalent width obtained by absorption line profile reconstruction (spect.line.eqWidth)
  (5)EW(8662)r 0.1nm (n) λ8662 equivalent width obtained by absorption line profile reconstruction (spect.line.eqWidth)
  (5)EW(8498)s 0.1nm (n) λ8498 equivalent width using spectral subtraction technique (Note 1)   (spect.line.eqWidth)
  (5)EW(8542)s 0.1nm (n) λ8542 equivalent width using spectral subtraction technique (Note 1)   (spect.line.eqWidth)
  (5)EW(8662)s 0.1nm (n) λ8662 equivalent width using spectral subtraction technique (Note 1)   (spect.line.eqWidth)
  (5)EW(8582)/EW(8498)  (n) Ratio of excess emission EW (Note 2)   (phot.flux;arith.ratio)
  (5)logF(8498) [10mW/m2/nm](n) λ8498 surface flux (Note 3)   (phot.flux)
  (5)logF(8542) [10mW/m2/nm](n) λ8542 surface flux (Note 3)   (phot.flux)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (5)logF(8662) [10mW/m2/nm](n) λ8662 surface flux (Note 3)   (phot.flux)

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