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J/A+A/439/1137     PHOENIX model chromospheres of M dwarfs  (Fuhrmeister+, 2005)

PHOENIX model chromospheres of mid- to late-type M dwarfs. Fuhrmeister B., Schmitt J.H.M.M., Hauschildt P.H. <Astron. Astrophys. 439, 1137 (2005)> =2005A&A...439.1137F
ADC_Keywords: Stars, late-type ; Stars, M-type ; Stars, atmospheres ; Equivalent widths Keywords: stars: activity - stars: late-type - stars: chromospheres Description: We present an extensive identification catalog of chromospheric emission lines in the optical range. The data were obtained with ESO's Kueyen telescope equipped with the UVES spectrograph from March, 13th to 16th in 2002. The instrument was operated in dichroic mode (spectral coverage from 3030 to 3880 and from 4580 to 6680Å). The data for the stars Prox Cen, UV Ceti and LHS 292 were obtained with the same instrument in winter 2000/2001 with a monochroic setup providing only the blue part of the spectrum. We tabulated measured wavelength, equivalent width (EW) and FWHM for every line and star and also provide the rest wavelength from the Moore catalog which was used for identification (Moore 1972). Few lines were identified with the NIST database. The spectra were all corrected for radial velocity besides Kelu-1, DENIS-P J1058.7-1548 and 2MASSI J1315309-264951. DENIS-P J1058.7-1548 has no detected lines, and therefore no data in the table. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file stars.dat 78 24 Star positions, from Simbad table1.dat 82 2577 Catalog of chromospheric emission lines for M dwarfs
See also: J/ApJS/152/261 : Chromospheric Ca II emission in nearby stars (Wright+, 2004) Byte-by-byte Description of file: stars.dat
Bytes Format Units Label Explanations
1- 24 A24 --- Name Star name 31- 32 I2 h RAh Right ascension (J2000) 34- 35 I2 min RAm Right ascension (J2000) 37- 40 F4.1 s RAs Right ascension (J2000) 42 A1 --- DE- Declination sign (J2000) 43- 44 I2 deg DEd Declination (J2000) 46- 47 I2 arcmin DEm Declination (J2000) 49- 50 I2 arcsec DEs Declination (J2000) 52- 78 A27 --- OName Other name
Byte-by-byte Description of file: table1.dat
Bytes Format Units Label Explanations
1- 22 A22 --- Name Name 24- 30 F7.2 0.1nm Lambda ? Measured wavelength 32- 38 F7.3 0.1nm EW ? Equivalent width 40- 43 F4.2 0.1nm FWHM ? FWHM 44 A1 --- n_Lambda Description for the line (1) 45 I1 --- f_Lambda [0/1]? Security flag (2) 47- 54 F8.3 0.1nm LambdaC Comparison wavelength 59- 64 A6 --- Ion Ion code 65- 68 I4 --- Mult ? Multiplet number in Moore catalog 69 A1 --- --- [,] 70- 71 A2 --- Mult2 Additional multiplet number 72 I1 --- f_LambdaC [0/2] Security flag (3) 75- 82 A8 --- Rem Remarks (4)
Note (1): Description for the line as follows: e = the emission core of an absorption line is measured b = line is blended with other lines/decomposed line s = saturated line t = blended with airglow line (decomposed) c = cosmic at position of line Note (2): Security flag as follows: 0 = probable identification in the stars spectrum (e. g. large lineshift, or low amplitude) 1 = secure identification in the stars spectrum Note (3): Security flag as follows: 0 = probable identification of the line 1 = secure identification of the line 2 = only one line of multiplet found/singlet line Note (4): Remarks as follows: (NIST) = line was identified with the help of the NIST database l = fitted with Lorentz profile
Acknowledgements: Birgit Fuhrmeister, bfuhrmeister(at)hs.uni-hamburg.de
(End) Patricia Vannier [CDS] 20-May-2005
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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