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J/A+A/413/285       Spectroscopic atlas of o Per 3826-4882Å (Gulliver+, 2004)

A spectroscopic atlas of o Pegasi (A1 IV) λλ3826-4882. Gulliver A.F., Adelman S.J., Friesen T.P. <Astron. Astrophys. 413, 285 (2004)> =2004A&A...413..285G
ADC_Keywords: Stars, early-type ; Spectroscopy Keywords: atlases - stars: early-type - stars: individual: o Pegasi - stars: chemically peculiar Abstract: We present a spectroscopic atlas of the sharp-lined, hot metallic-line star o Pegasi (A1 IV) based on spectrograms obtained with the long camera of the 1.22-m telescope of the Dominion Astrophysical Observatory using a Reticon detector. For 3826-4882 the inverse dispersion is 2.4Å/mm with a resolution of 0.072Å. At the continuum the mean signal-to-noise ratio is 800. The wavelengths in the laboratory frame, the equivalent widths, and the identifications of the various spectral features are given. The stellar and synthetic spectra with their corresponding line identifications can be examined at . Objects: ----------------------------------------- RA (2000) DE Designation(s) ----------------------------------------- 22 41 45.4 +29 18 27 omi Peg ----------------------------------------- File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table2.dat 141 1760 Line measurements of ο Pegasi
See also: J/A+A/400/1043 : Spectroscopic atlas of Deneb 3826-5212Å (Albayrak+, 2003) Byte-by-byte Description of file: table2.dat
Bytes Format Units Label Explanations
1 A1 --- Blend [bre] b: blue, r: red 4- 8 F5.1 0.1pm EW ? Equivalent Width 10- 14 F5.3 --- Depth ? The line depth as a fraction of the continuum height 16- 19 F4.2 0.1nm FWHM ? Full width at half maximum 21- 28 F8.3 0.1nm lambda Laboratory wavelength 29 A1 --- Link [a-r] Flag for common line identification (1) 32-141 A110 --- ID Line Identifications, separated by comma (2)
Note (1): When the line identification is associated to 2 lambda, a letter links the two lines, i.e. b 3.5 0.018 0.18 3849.352a ] Fe II(KX)3849.418(p) r 64.7 0.350 0.17 3849.552a ] Fe II(KX)3849.418(p) The bracket indicates that an identified line may be contributing to two measured stellar features Note (2): Line identification, in the form Ion(Multiplet Number) wavelength in Angstroms(laboratory intensity) i.e., in the Fe I(45)3841.0480(80r), Fe I is atomic species, (45) is multiplet number, 3841.0480 is the laboratory wavelength, (80r) is intensity.
History: Copied at
(End) Patricia Vannier [CDS] 06-Jul-2004
The document above follows the rules of the Standard Description for Astronomical Catalogues.From this documentation it is possible to generate f77 program to load files into arrays or line by line

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