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J/A+A/549/A63 GMASS photometry (Kurk+, 2013)
The following files can be converted to FITS (extension .fit or fit.gz)
tablea1.dat
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Query from: http://vizier.cds.unistra.fr/viz-bin/VizieR?-source=J/A+A/549/A63
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drwxr-xr-x 5 cats archive 4096 Jan 12 2023 [TAR file]
-rw-r--r-- 1 cats archive 463 Dec 19 2022 .message
-r--r--r-- 1 cats archive 7104 May 26 2013 ReadMe
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-rw-r--r-- 1 cats archive 2295 Feb 2 2015 +footg8.gif
drwxr-xr-x 2 cats archive 12288 Oct 19 2012 fits
-r--r--r-- 1 cats archive 30280 Dec 20 2012 tablea1.dat [txt] [txt.gz] [fits] [fits.gz] [html]
Beginning of ReadMe :J/A+A/549/A63 GMASS photometry (Kurk+, 2013)
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GMASS ultradeep spectroscopy of galaxies at z 2.
VII. Sample selection and spectroscopy.
Kurk J., Cimatti A., Daddi E., Mignoli M., Pozzetti L., Dickinson M.,
Bolzonella M., Zamorani G., Cassata P., Rodighiero G., Franceschini A.,
Renzini A., Rosati P., Halliday C., Berta S.
<Astron. Astrophys. 549, A63 (2013)>
=2013A&A...549A..63K
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ADC_Keywords: Galaxies, photometry ; Redshifts ; Spectroscopy
Keywords: galaxies: distances and redshifts - galaxies: evolution -
galaxies: formation - galaxies: fundamental parameters -
galaxies: high-redshift
Abstract:
We designed a spectroscopic observing campaign of a sample of both
massive, quiescent and star-forming galaxies at z>1.4, called Galaxy
Mass Assembly ultra-deep Spectroscopic Survey (GMASS). To determine
redshifts and physical properties, such as metallicity, dust content,
dynamical masses, and star formation history, we performed ultra-deep
spectroscopy with the red-sensitive optical spectrograph FORS2 at the
VLT. Our sample consists of objects, within the CDFS/GOODS area,
detected at 4.5 micron, to be sensitive to stellar mass rather than
star formation intensity. The spectroscopic targets were selected with
a photometric redshift constraint (z>1.4) and magnitude constraints
(B(AB)<26, I(AB)<26.5), which should ensure that these are faint,
distant, and fairly massive galaxies. Up to 30 hours of spectroscopy
of 174 spectroscopic targets and 70 additional objects enabled us to
determine 210 redshifts, of which 145 are at z>1.4. We publicly
release the redshifts and reduced spectra.
Description:
Properties of objects observed in the GMASS masks, including the GMASS
identification number, coordinates, photometry in four bands,
redshifts determined from spectroscopy, average S/N per pixel in
spectrum, photometric normalisation factor to obtain imaging flux,
sample of which the target is part and mask(s) in which the target was
observed.