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J/ApJ/697/1369 GOODS Ks-selected multiwavelength compilations (Bundy+, 2009)
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Beginning of ReadMe :J/ApJ/697/1369 GOODS Ks-selected multiwavelength compilations (Bundy+, 2009)
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The greater impact of mergers on the growth of massive galaxies:
implications for mass assembly and evolution since z = 1.
Bundy K., Fukugita M., Ellis R.S., Targett T.A., Belli S., Kodama T.
<Astrophys. J., 697, 1369-1383 (2009)>
=2009ApJ...697.1369B
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ADC_Keywords: Surveys ; Galaxies, photometry
Keywords: galaxies: evolution - galaxies: formation - galaxies: interactions
Abstract:
Ks-selected multiwavelength compilations in GOODS.
Description:
We obtained Ks-band observations using MOIRCS on the Subaru Telescope
during two nights in 2006 April. Each MOIRCS pointing is imaged onto
two overlapping detectors, giving a total field of view that is
roughly 4' by 7'. Our observations consisted of eight tiled pointings
arranged with some overlap in order to cover the entire GOODS-N
region. The MOIRCS Ks-band 80% completeness depth varies across the
GOODS-N field from Ks=23.5 to Ks=24.0 with an average of Ks 23.8. In
GOODS-S, JHKs imaging was obtained by an ESO/GOODS project using ISAAC
on the VLT at the ESO Paranal Observatory. The survey details and data
reduction are described in J. Retzlaff (2009, in prep.). The final
version 2.0 reduced and calibrated images are publicly available on
the ESO website and, for the Ks-band are similar in quality to our
MOIRCS data in GOODS-N.
We constructed our Ks-selected sample in GOODS-N by combining the
detections in all of the MOIRCS images into a single source list.
Because we designed the field layout so that the pointings overlap,
duplicate sources must be removed from this list. We matched this
Ks-band source list to a number of publicly available catalogs in
GOODS-N. We then cross-referenced our Ks-band sample to several
spectroscopic redshift catalogs.
In GOODS-S, a source catalog based on the ISAAC data was constructed
with the same methods used for building the MOIRCS catalog in GOODS-N.
Matching to the version 1.1 GOODS-S z-selected ACS catalog was also
carried out in a similar fashion. The Ks-selected ISAAC catalog was
correlated to source catalogs obtained from the ISAAC J and H-bands
(JH photometry was not obtained in GOODS-N). The final ISAAC
Ks-selected catalog in GOODS-S contains 9043 unique sources over
160arcmin^2^.