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J/A+A/412/495       Equivalent widths for 6 RS CVn systems     (Morel+, 2003)

The photospheric abundances of active binaries. II. Atmospheric parameters and abundance patterns for 6 single-lined RS CVn systems. Morel T., Micela G., Favata F., Katz D., Pillitteri I. <Astron. Astrophys., 412, 495-512 (2003)> =2003A&A...412..495M
ADC_Keywords: Stars, variable ; Equivalent widths Keywords: stars: fundamental parameters - stars: abundances Abstract: Photospheric parameters and abundances are presented for a sample of single-lined chromospherically active binaries from a differential LTE analysis of high-resolution spectra. Abundances have been derived for 13 chemical species, including several key elements such as Li, Mg, and Ca. Description: The spectra were acquired in January 2000 at the ESO 1.52-m telescope (La Silla, Chile) with the fiber-fed, cross-dispersed echelle spectrograph FEROS in the object+sky configuration. The atomic data have been calibrated using a high S/N moonlight spectrum extracted from the archive of the first FEROS commissioning period (fall 1998). File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file stars.dat 39 6 Stars studied tablea1.dat 68 95 Calibrated atomic data and EW measurements.
Byte-by-byte Description of file: stars.dat
Bytes Format Units Label Explanations
1- 9 A9 --- HD Name of the star 12- 15 I4 pc Dist Heliocentric distance 17- 22 F6.3 mag (B-V)0 Unreddened Johnson V magnitude 25- 29 F5.2 [Sun] [Fe/H] Metallicity of the star 31- 35 I5 K Teff Effective temperature from Fe excitation 37- 39 I3 K e_Teff Mean error on Teff
Byte-by-byte Description of file: tablea1.dat
Bytes Format Units Label Explanations
1- 5 A5 --- Ion Ion designation 7- 10 F4.2 [Sun] epsSolar Kurucz solar abundance (logarithmic scale, H=12) 12- 19 F8.3 0.1nm Lambda Wavelength 21- 25 F5.3 eV EP Excitation potential 27- 32 F6.3 [---] loggf Calibrated log(gf)-value 34- 38 F5.1 0.1pm EWHD10909 ? EWs for UV For (HD 10909) (1) 40- 44 F5.1 0.1pm EWHD72688 ? EWs for VX Pyx (HD 72688) (1) 46- 50 F5.1 0.1pm EWHD83442 ? EWs for IN Vel (HD 83442) (1) 52- 56 F5.1 0.1pm EWHD113816 ? EWs for IS Vir (HD 113816) (1) 58- 62 F5.1 0.1pm EWHD118238 ? EWs for V764 Cen (HD 118238) (1) 64- 68 F5.1 0.1pm EWHD119285 ? EWs for V851 Cen (HD 119285) (1)
Note (1): A blank indicates that the EW was not reliably measurable for one of the following reasons: the line was affected by telluric features or cosmetic defaults (e.g., cosmic rays), the line was significantly van der Walls broadened, or the Gaussian fit was judged unsatisfactory.
Acknowledgements: Thierry Morel
(End) Patricia Bauer [CDS] 02-Dec-2003
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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