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J/A+A/329/721       Sensitivity indicators of Fraunhofer lines  (Shenimova 1998)

Sensitivity indicators of Fraunhofer lines Sheminova V. A. <Astron. Astrophys. 329, 721 (1998)> =1998A&A...329..721S (SIMBAD/NED BibCode)
ADC_Keywords: Sun ; Stars, atmospheres Keywords: Sun: atmosphere - Sun: photosphere Abstract: The results of calculations of the sensitivity indicators to the temperature, as well as the average geometrical heights of localization of the effective response to the temperature variations are presented for the central line depths, for the line depths on half-width, and for the equivalent widths of the 604 Fe I and 58 Fe II absorption lines. This list of unblended solar lines in the range of the wavelengths 401.0-901.0nm contains the maximum of lines suitable for the analysis of the fine structure of the line profiles and primarily for study of the line asymmetries. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table1 71 604 The Fe I lines table2 71 58 The Fe II lines
Byte-by-byte Description of file: table1 table2
Bytes Format Units Label Explanations
1- 7 F7.3 nm lambda ]401,902[+= Wavelength 9- 12 F4.2 eV EP Lower-level excitation potential 14- 19 F6.3 --- log(gf) Calculated oscillator strength 21- 25 F5.3 --- Robs Observed central line depth 27- 32 F6.3 pm EWcal Calculated equivalent width 34- 37 F4.0 km H(R) Heights (central line depths) 39- 42 F4.0 km H(0.5R) Heights (line depths on half-widths) 44- 47 F4.0 km H(EW) Heights (equivalent widths) 49- 55 F7.3 --- I(R) Indicators (central line depths) 57- 63 F7.3 --- I(0.5R) Indicators (line depths on half-widths) 65- 71 F7.3 --- I(EW) Indicators (equivalent widths)
Acknowledgements: Valentina A. Sheminova
(End) Sheminova [Main Astronomical Observatory of Ukrainian NAS] 07-May-1997
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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