VizieR

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VizieR

  
J/A+A/470/317
  UV spectra of the central star of Sh 2-216 (Rauch+, 2007)
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2007A&A...470..317R
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The additional tables contain observed an synthetic spectra of LS V +46 21:
– FUSE spectrum (table A2) and a comparison with the model described in the paper; (list of FUSE spectra from the FUSE log B/fuse)
– HST/STIS spectrum (table A3) and a comparison with the model described in the paper; (list of HST/STIS spectra from the HST log B/hst)
– synthetic spectra in the wavelength ranges λλ 1144-1730Å (table A3) and 910-1190Å (table A4)
Post annotation 		  
1.J/A+A/470/317/tablea1Positions of identified lines in the FUSE (Fig. A1) and STIS (Fig. A2) spectra of LS V +46 21, the white dwarf central star of Sh 2-216 (2607 rows)

Simple ConstraintList Of Constraints
 
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)
  Line (char) Line identification (ion) (meta.id;spect.line)
  n_Line (char) Photospheric (ph) or interstellar (is) origin (meta.note)
  lambdaObs 0.1nm Observed spectrum is shifted to the stellar rest wavelength, the given wavelength is the NIST wavelength (em.wl.effective)
  lambdaLab 0.1nm (n) Rest wavelength of interstellar lines (em.wl)

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