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II/47 Scanner Abundance in late-type evolved stars (Spinrad+ 1969)
The following files can be converted to FITS (extension .fit .fgz or .fiZ)
stars.dat color.dat ircol.dat block.dat
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Query from: http://vizier.cds.unistra.fr/viz-bin/VizieR?-source=II/47
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-r--r--r-- 1 cats archive 8019 Dec 7 2006 ReadMe
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-rw-r--r-- 1 cats archive 4543 Mar 5 2008 +footg8.gif
-r--r--r-- 1 cats archive 16259 Apr 23 2002 block.dat [txt] [txt.gz] [fits] [fits.gz] [html]
-r--r--r-- 1 cats archive 28625 Apr 25 2002 color.dat [txt] [txt.gz] [fits] [fits.gz] [html]
-r--r--r-- 1 cats archive 4118 May 10 2002 ircol.dat [txt] [txt.gz] [fits] [fits.gz] [html]
-r--r--r-- 1 cats archive 15202 Apr 25 2002 stars.dat [txt] [txt.gz] [fits] [fits.gz] [html]
Beginning of ReadMe :II/47 Scanner Abundance in late-type evolved stars (Spinrad+ 1969)
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Scanner abundance studies. I. An investigation of super-metallicity
in late-type evolved stars.
Spinrad H., Taylor B.J.
<Astrophys. J., 157, 1279 (1969)>
=1969ApJ...157.1279S
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ADC_Keywords: Abundances; Colors; Stars, late-type; Spectrophotometry
Description:
Abundance parameters have been derived from scanner observations of
229 stars. Observations were made with the Wampler photoelectric
spectrum scanner (Wampler, 1966) on Lick Observatory's Crossley and
120inch telescopes. Data reductions were performed at UC Berkeley on
the IBM 7094 computer using programs by L.V. Kuhi and B.J. Taylor. The
method of reduction and the photometric standard system are described
by Spinrad and Taylor (1969AJ.....72..320S). The file "color.dat"
(tables 5 and 6 in the publication) gives colors between 3880 and
7400AA for program stars and survey stars, normalized so that
I(5360)=1000. The file "block.dat" gives the blocking fractions for
program stars.