Physics
Scientific paper
Mar 2008
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008ycat..83820109t&link_type=abstract
VizieR On-line Data Catalog: J/MNRAS/382/109. Originally published in: 2007MNRAS.382..109T
Physics
Galaxies: Photometry, Morphology, Redshifts
Scientific paper
We use the Palomar Observatory Wide-field Infrared (POWIR)/DEEP-2 survey (Davis et al., 2003, SPIE, Vol. 4834, p. 161; Bundy et al., 2006ApJ...651..120B ; Conselice et al., 2007ApJ...660L..55C, 2007MNRAS.381..962C) to define a sample of 831 galaxies with masses larger than 1011h70-2M{sun} located over ~710arcmin2 in the Extended Groth Strip (EGS). This field (63 Hubble Space Telescope tiles) was imaged with the Advanced Camera for Surveys (ACS) in the V band (F606W, 2660s) and I band (F814W, 2100s). Each tile was observed in four exposures that were combined to produce a pixel scale of 0.03arcsec, with a point spread function (PSF) of 0.12arcsec full width half-maximum (FWHM). In addition to the HST data, optical imaging from the CanadaFranceHawaii Telescope 3.6-m telescope in the B, R and I bands taken with the CFH12K camera was used. Integration times for these observations were 1h in B and R, and 2h in I. Limiting magnitudes reached are B=24.5 (AB, 8{sigma}), R=24.2 (AB, 8{sigma}) and I=23.5 (AB, 8{sigma}). The details of the data reduction for this data are provided in Coil et al. (2004ApJ...617..765C).
(1 data file).
Bundy Kevin
Conselice Christopher J.
Cooper Martin C.
Eisenhardt Peter
Ellis Richard S.
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