Index of /~bessell/FTP/Allbrow
Name Last modified Size Description
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dbs00184b.fits 13-Jul-2007 09:13 1.2M
dbs184bc.fits 13-Jul-2007 09:12 2.1M
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jun2006bluedbs.log 12-Jul-2007 11:29 14K
jun_glcl2006.log 12-Jul-2007 11:29 4.5K
sp184bd.fits 13-Jul-2007 09:42 17K
sp206bd.fits 13-Jul-2007 09:51 17K
sp208bd.fits 13-Jul-2007 10:01 17K
sp210bd.fits 13-Jul-2007 10:05 17K
sp211_2bd.fits 13-Jul-2007 10:13 17K
sp214bd.fits 13-Jul-2007 10:15 17K
sp215_6bd.fits 13-Jul-2007 10:22 17K
sp217bd.fits 13-Jul-2007 10:24 17K
sp514bd.fits 13-Jul-2007 10:30 17K
sp515bd.fits 13-Jul-2007 10:33 17K
sp536bd.fits 13-Jul-2007 10:40 17K
sp537bd.fits 13-Jul-2007 10:42 17K
sp538bd.fits 13-Jul-2007 10:44 17K
sp539bd.fits 13-Jul-2007 10:46 17K
sp540bd.fits 13-Jul-2007 10:47 17K
sp541bd.fits 13-Jul-2007 10:49 17K
sp542bd.fits 13-Jul-2007 10:52 17K
sp561bd.fits 13-Jul-2007 10:52 17K
sp562bd.fits 13-Jul-2007 10:55 17K
sp563bd.fits 13-Jul-2007 10:57 17K
sp564bd.fits 13-Jul-2007 12:14 17K
sp565bd.fits 13-Jul-2007 12:14 17K
sp566bd.fits 13-Jul-2007 11:04 17K
sp567bd.fits 13-Jul-2007 11:06 17K
sp568bd.fits 13-Jul-2007 11:08 17K
sp569bd.fits 13-Jul-2007 11:10 17K
sp570bd.fits 13-Jul-2007 11:11 17K
sp571bd.fits 13-Jul-2007 11:12 17K
sp572bd.fits 13-Jul-2007 11:14 17K
There are two logfiles here. One has all the observed objects, the other
has the clusters. I have included a few halo stars, dwarfs or turnoff stars
for comparison.
The spectra have been divided through by spectra of EG131 (a continuous
white dwarf) to take out the gross instrument response and to straighten out
the continuum (see the attached paper BJpaper2.pdf).