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J/MNRAS/380/986 Ultraviolet galaxies catalog (Burgarella+, 2007)
The following files can be converted to FITS (extension .fit .fgz or .fiZ)
table1.dat table3.dat
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Query from: http://vizier.cds.unistra.fr/viz-bin/VizieR?-source=J/MNRAS/380/986
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-r--r--r-- 1 cats archive 6095 Mar 1 2008 ReadMe
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-rw-r--r-- 1 cats archive 2977 Mar 5 2008 +footg8.gif
-r--r--r-- 1 cats archive 1215608 Jan 5 2008 table1.dat.gz [txt] [txt.gz] [fits] [fits.gz] [html]
-r--r--r-- 1 cats archive 31222 Jan 5 2008 table3.dat [txt] [txt.gz] [fits] [fits.gz] [html]
Beginning of ReadMe :J/MNRAS/380/986 Lyman-break galaxies from GALEX (Burgarella+, 2007)
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Lyman break galaxies at z 1 and the evolution of dust attenuation in
star-forming galaxies with redshift.
Burgarella D., Le Floc'h E., Takeuchi T.T., Huang J.S., Buat V.,
Rieke G.H., Tyler K.D.
<Mon. Not. R. Astron. Soc., 380, 986-998 (2007)>
=2007MNRAS.380..986B
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ADC_Keywords: Galaxies, UV-excess ; Ultraviolet ; Redshifts
Keywords: galaxies: evolution - galaxies: starburst - infrared: galaxies -
ultraviolet: galaxies
Abstract:
Ultraviolet (UV) galaxies have been selected from the Galaxy Evolution
Explorer deep imaging survey. The presence of a far-UV (FUV) drop-out
in their spectral energy distributions (SEDs) proved to be a very
complete (83.3 per cent) but not very efficient (21.4 per cent) tool
for identifying Lyman break galaxies (LBGs) at z 1. In this paper,
we explore the physical properties of these galaxies and how they
contribute to the total star formation rate (SFR).