==========================================================================
J/AN/320/105 Spectrophotometry in LMC (Oestreicher+ 1999)
The following files can be converted to FITS (extension .fit or fit.gz)
targets.dat
==========================================================================
Query from: http://vizier.cds.unistra.fr/viz-bin/VizieR?-source=J/AN/320/105
==========================================================================
drwxr-xr-x 3 cats root 63 Aug 5 2013 [Up]
drwxr-xr-x 5 cats root 324 Jan 12 2023 [TAR file]
-rw-r--r-- 1 cats archive 458 Dec 19 2022 .message
-r--r--r-- 1 cats archive 4862 Aug 28 2013 ReadMe
-rw-r--r-- 1 cats archive 257 Aug 28 2013 +footg5.gif
-rw-r--r-- 1 cats archive 2154 Aug 28 2013 +footg8.gif
drwxr-xr-x 2 cats archive 4096 Aug 5 2013 sp
-r--r--r-- 1 cats archive 3402 Aug 5 2013 targets.dat [txt] [txt.gz] [fits] [fits.gz] [html]
Beginning of ReadMe :J/AN/320/105 Spectrophotometry of 26 supergiants in the LMC (Oestreicher+ 1999)
================================================================================
Red supergiants in the LMC - III: luminous F and G stars.
Oestreicher M.O., Schmidt-Kaler T.
<Astron. Nachrichten 320.105 (1999)>
=1999AN....320..105O
================================================================================
ADC_Keywords: Spectrophotometry ; Stars, supergiant ; Magellanic Clouds
Description:
New spectrophotometric data for 3 galactic and 23 LMC F to G
supergiants are presented. The wavelength range of the spectra is 3400
to 6400AA, the resolution about 10AA. The mean transformational
error of the fluxes is 0.03mag. The S/N ratio is about 100 and 30 for
galactic and LMC stars, respectively. Details about the reduction one
may found in Oestreicher & Schmidt-Kaler (1998MNRAS.299..625O) and
Malyuto et al. (1997MNRAS.286..500M). The fluxes are given in
magnitudes according to the system of Hayes & Latham
(1975ApJ...197..593H). For each star an ASCII file is given with the
name of the first identifier. In the first column the wavelength, in
the second column the flux is given.