========================================================================== J/A+A/439/1137 PHOENIX model chromospheres of M dwarfs (Fuhrmeister+, 2005) The following files can be converted to FITS (extension .fit .fgz or .fiZ) stars.dat table1.dat ========================================================================== Query from: http://vizier.u-strasbg.fr/viz-bin/VizieR?-source=J/A+A/439/1137 ==========================================================================
drwxr-xr-x 13 cats archive 4096 Jan 29 2012 [Up] drwxr-xr-x 2 cats archive 4096 May 12 09:57 [TAR file] -rw-r--r-- 1 cats archive 480 Sep 8 2005 .message -r--r--r-- 1 cats archive 5168 Sep 8 2005 ReadMe -rw-r--r-- 1 cats archive 297 Sep 19 2007 +footg5.gif -rw-r--r-- 1 cats archive 2402 Mar 5 2008 +footg8.gif -r--r--r-- 1 cats archive 1342 Aug 25 2005 stars.dat [txt] [txt.gz] [fits] [fits.gz] [html] -r--r--r-- 1 cats archive 188814 May 20 2005 table1.dat [txt] [txt.gz] [fits] [fits.gz] [html]
Beginning of ReadMe : 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 6680AA). 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.