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VII/228 Las Campanas Infrared Survey (Chen+, 2001-2002)
The following files can be converted to FITS (extension .fit .fgz or .fiZ)
table2.dat table6.dat table7.dat
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Query from: http://vizier.cds.unistra.fr/viz-bin/VizieR?-source=VII/228
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-rw-r--r-- 1 cats archive 3057 Mar 5 2008 +footg8.gif
-r--r--r-- 1 cats archive 2304137 Jul 25 2002 cdfs.dat.gz [txt] [txt.gz] [fits] [fits.gz] [html]
-r--r--r-- 1 cats archive 2195282 Jul 25 2002 hdfs.dat.gz [txt] [txt.gz] [fits] [fits.gz] [html]
-r--r--r-- 1 cats archive 1608 Jul 25 2002 obslog.dat [txt] [txt.gz] [fits] [fits.gz] [html]
Beginning of ReadMe :VII/228 Las Campanas Infrared Survey (Chen+, 2001-2002)
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The Las Campanas Infrared Survey.
I. Early-type galaxy progenitors beyond z=1.
Chen H.-W., McCarthy P.J., Marzke R.O., Wilson J., Carlberg R.G.,
Firth A.E., Persson S.E., Sabbey C.N., Lewis J.R., McMahon R.G., Lahav O.,
Ellis R.S., Martini P., Abraham R.G., Oemler A., Murphy D.C.,
Somerville R.S., Beckett M.G., MacKay C.D.
<Astrophys. J. 560, L131 (2001)>
=2001ApJ...560L.131M
II. Photometric redshifts, comparison with models and clustering evolution.
<Mon. Not. R. Astron. Soc. 332, 617 (2002)>
=2002MNRAS.332..617F
III. The H-band imaging survey and the near-infrared and optical photometric
catalogs
<Astrophys. J. 570, 54 (2002)>
=2002ApJ...570...54C
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ADC_Keywords: Surveys ; Galaxies, IR ; Photometry, UBVRI ; Photometry, infrared
Keywords: catalogs - cosmology: observations - galaxies: evolution -
galaxies: high-redshift - infrared: galaxies - surveys
Abstract:
The Las Campanas Infrared Survey, based on broadband optical and
near-infrared photometry, is designed to robustly identify a
statistically significant and representative sample of evolved
galaxies at redshifts z>1. We have completed an H-band imaging survey
over 1.1deg^2^ of sky in six separate fields. The average 5sigma
detection limit in a 4" diameter aperture is H 20.8. Here we describe
the design of the survey, the observation strategies, data-reduction
techniques, and object identification procedures. We present sample
near-infrared and optical photometric catalogs for objects identified
in two survey fields. The optical images of the Hubble Deep Field-South
region obtained from the literature reach 5sigma detection
thresholds in a 4" diameter aperture of U 24.6, B 26.1, V 25.6,
R 25.1, and I 24.2mag. The optical images of the Chandra Deep
Field-South region obtained from our own observations reach 5 sigma
detection thresholds in a 4" diameter aperture of V 26.8, R 26.2,
I 25.3, and z' 23.7mag. We perform object detection in all bandpasses
and identify> 54000 galaxies over 1408 arcmin^2^ of sky in the two
fields. Of these galaxies, 14000 are detected in the H band and 2000
have the colors of evolved galaxies, I-H > 3, at z> 1.