==========================================================================
III/27A Abundances of late G/K dwarfs in solar neighborhood (Taylor, 1970)
The following files can be converted to FITS (extension .fit or fit.gz)
raw_data.dat blocking.dat
==========================================================================
Query from: http://vizier.cds.unistra.fr/viz-bin/VizieR?-source=III/27A
==========================================================================
drwxr-xr-x 259 cats archive 8192 Dec 5 19:00 [Up]
drwxr-xr-x 2 cats archive 4096 Jan 13 2023 [TAR file]
-rw-r--r-- 1 cats archive 477 Dec 19 2022 .message
-r--r--r-- 1 cats archive 5338 Feb 14 2016 ReadMe
-rw-r--r-- 1 cats archive 624 Feb 14 2016 +footg5.gif
-rw-r--r-- 1 cats archive 5131 Feb 14 2016 +footg8.gif
-r--r--r-- 1 cats archive 20093 Feb 14 2016 blocking.dat [txt] [txt.gz] [fits] [fits.gz] [html]
-r--r--r-- 1 cats archive 47544 Feb 14 2016 raw_data.dat [txt] [txt.gz] [fits] [fits.gz] [html]
Beginning of ReadMe :III/27A Abundances of late G/K dwarfs in solar neighborhood (Taylor, 1970)
================================================================================
Scanner abundance studies II. Late G and K dwarfs in the solar neighborhood
Taylor B.J.
<Astrophys. J. Suppl. Ser. 22, 177-248 (1970)>
=1970ApJS...22..177T
=2016yCat.3027....0T
================================================================================
ADC_Keywords: Abundances; Stars, late-type; Stars, dwarfs; Spectrophotometry
Description:
In this investigation, a technique developed by Spinrad and Taylor for
obtaining metal abundances of late-type stars, and used by them in an
earlier investigation of evolved stars (see Cat. II/47), is applied to
field dwarfs in the solar vicinity and to the Hyades. The colors
determined from photoelectric spectrum-scanner observations are listed
in the "raw_data.dat" file; the derived blocking factors are given in
the "blocking.dat" file. These results were published as the Table 5
of the paper.