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J/A+A/366/1003  8500-8750Å high resolution spectroscopy. III. (Munari+, 2001)

High resolution spectroscopy over 8500-8750Å for GAIA. III. A library of synthetic spectra for 7750<Teff<50000K Castelli F., Munari U. <Astron. Astrophys. 366, 1003 (2001)> =2001A&A...366.1003C
ADC_Keywords: Models, atmosphere ; Spectroscopy Keywords: atlases - surveys - stars: fundamental parameters Abstract: In this paper we complete the library of synthetic spectra for the range 7650-8750Å, which includes the 8500-8750Å interval currently base-lined for the spectroscopic observations by GAIA, candidate ESA Cornerstone 5 mission. As for Paper II (Munari & Castelli, Cat. J/A+AS/141/141), the spectra are based on Kurucz's codes and line data. The explored metallicity, gravity and temperature ranges are -2.5≤[Z/Z]≤+0.5, 4.5≤logg≤2.0 and 7750≤Teff≤50000K, respectively. The 698 new spectra are computed at the same λ/Δλ=20000 resolving power of the observed spectra given in Paper I (Munari & Castelli, Cat. J/A+AS/137/521) (131 standard stars mapping the MKK spectral classification system) and the 254 synthetic spectra of Paper II (characterized by Teff≤7500K). File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file tables.dat 80 645 Main absorption lines in the interval 8490-8750Å for different spectra of solar metallicity (tables 2, 3 and 4 of the paper)
See also: J/A+AS/137/521 : 8500-8750Å high resolution spectroscopy (Munari+, 1999) J/A+AS/141/141 : 8500-8750Å high resolution spectroscopy (Munari+, 2000) Byte-by-byte Description of file: tables.dat
Bytes Format Units Label Explanations
1- 8 F8.3 0.1nm lambda Wavelength 10 I1 --- n_lambda [1/5]? Number of components of unresolved blends 12- 17 A6 --- Ion Identification 18- 21 I4 --- Mult ? Multiplet number 23- 27 F5.2 eV EP Excitation potential of the lower level in eV 29- 38 F10.3 cm-1 EP2 Excitation potential of the lower level in cm-1 40- 45 F6.3 --- loggf Oscillator strength 47- 51 A5 --- r_loggf Source of loggf (1) 53- 57 I5 K Teff Effective temperature 59- 61 F3.1 [cm/s2] logg Surface gravity 63- 67 F5.3 --- RCI Residual central intensity for Teff and logg
Note (1): Reference for loggf BWL: Black et al. 1972ApJ...177..567B FMW: Fuhr et al. 1988, Cat. VI/72 FT: Friedrich and Trefftz, 1969, MPI-PAE/Astro, 29 GUESS: guessed value K88: Kurucz 1988, Trans. IAU, XXB, McNally M. (ed.). Kluwer, p. 168 K: unpublished and given in the Kurucz's line lists on CD-ROMs KP: Kurucz and Peytremann 1975, Cat. VI/10 M: Murphy 1968ApJ...153..301M MC: McEachran and Cohen, 1971, JQSRT 11, 1819 NBS: Wiese et al. 1966, NSRDS-NBS 4
Acknowledgements: Ulisse Munari
(End) Patricia Bauer [CDS] 04-Jan-2001
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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