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J/A+AS/129/41 Fe I line shifts in the Sun (Allende Prieto+ 1998)
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Fe I line shifts in the optical spectrum of the Sun
Allende Prieto C., Garcia Lopez R.J.
<Astron. Astrophys. Suppl. Ser. 129, 41 (1998)>
=1998A&AS..129...41A (SIMBAD/NED BibCode)
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ADC_Keywords: Sun ; Atomic physics
Keywords: convection - atlases - Sun: photosphere - stars: atmospheres
Description:
Central wavelengths measured in the FTS disc-centre spectrum, in the
FTS flux spectrum, rest wavelengths, excitation potentials, transition
probabilities (log(gfs)) and line equivalent widths at the centre of
the disc when available (from Moore et al. 1966 (The Solar Spectrum
2935{AA} to 8770{AA}, National Bureau of Standards Monograph 61) and
compiled by A. D. Wittmann, private communication). An asterisk in the
equivalent width means that the line has a blend.
File Summary:
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FileName Lrecl Records Explanations
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ReadMe 80 . This file
table1.dat 46 1446 Caption of the table
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See also:
J/A+AS/102/269 : Lab. and solar Highly-excited levels of Fe I (Nave+ 1993)
J/ApJS/94/221 : New multiplet table for FeI (Nave+, 1994)
Byte-by-byte Description of file: table1.dat
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Bytes Format Units Label Explanations
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1- 9 F9.4 0.1nm Int. Central Waveleng. in the disc-centre spectrum
11- 19 F9.4 0.1nm Flux Central Wavelengths in the flux spectrum
21- 29 F9.4 0.1nm Lab Central Wavelengths at rest
(Nave et al., 1994, Cat. <J/ApJS/94/221>)
31- 34 F4.2 eV EP Excitation potential (Thevenin,
1989A&AS...77..137T, 1990A&AS...82..179T)
36- 40 F5.2 --- log(gf) ? Transition probabilities
(Nave et al. 1994, Cat. <J/ApJS/94/221>)
42- 45 I4 mA EW ? Equivalent widths (disc centre)
46 A1 --- n_EW Note on line (1)
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Note (1): *: The line is Known to be blended
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Acknowledgements: Carlos Allende Prieto <callende@ll.iac.es>
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(End) Patricia Bauer [CDS] 18-Sep-1997