========================================================================== III/201 Pulkovo Spectrophotometric Catalog (Alekseeva+ 1997) The following files can be converted to FITS (extension .fit .fgz or .fiZ) stars.dat notes.dat ========================================================================== Query from: http://vizier.cds.unistra.fr/viz-bin/VizieR?-source=III/201 ==========================================================================
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Beginning of ReadMe : III/201 Pulkovo Spectrophotometric Catalog (Alekseeva+ 1997) ================================================================================ The Pulkovo spectrophotometric catalog of bright stars in the range from 320 to 1080nm Alekseeva G.A., Arkharov A.A. , Galkin V.D. , Hagen-Thorn E.I., Nikanorova I.N., Novikov V.V., Novopashenny V.B., Pakhomov V.P., Ruban E.V., Shchegolev D.E. <Baltic Astron. 5, 603 (1996); 6, 481 (1997)> =1996BaltA...5..603A =1997BaltA...6..481A ================================================================================ ADC_Keywords: Spectrophotometry ; Stars, bright Abstract: A spectrophotometric catalog is presented, combining results of numerous observations by Pulkovo astronomers at different observing sites. The catalog consists of three parts: the first contains the data of 602 stars in the spectral range 320-735 nm with a resolution 5 nm; the second one contains 285 stars in the spectral range of 500-1080 nm with resolution10 nm and the third one contains 278 stars combined from the preceding catalogs in spectral range 320-1080 nm with resolution 10 nm. The data are presented in the absolute energy units W/mm, with step of 2.5 nm and with an accuracy no more than 1.5 - 2.0%. Description: A complete list of the observed stars is given in Table 4. The following information about the stars is given: HR and HD numbers, the Bayer's name, the number of independent scans of the spectrum (short-/long-wavelength range), equatorial coordinates for 2000.0, spectral type from the 1982 version of the BS catalog, magnitude V and color index B-V from the same source. Information on binarity and variability is given in the remarks following Table 4. For the visual binaries, the separation and m are taken also from the BS . For the variables, variability type and magnitudes at the maximum and minimum light and the period are from the General Catalog of Variable Stars (Kholopov et al. 1985-1990) and its three Supplements (Inf. Bull. Var. Stars Nos. 2681, 3058, and 3323). The final energy distribution data in the range 320-1080 nm with a step 2.5 nm, expressed in W/m2/m (or 10^-6^arg/cm^2^/s/nm in cgs) given in Tables 5, 5a and 6. Tables 5 contains the combined data covering the wavelengths 320-1080 nm and Table 5a is for the stars having data only in the 500-1080 nm range. All the data are for the same effective spectral broadening, 10 nm. The data covering only the wavelengths 320-735 nm (with effective spectral broadening of 5 nm) are presented in Table 6.