A Deep Multicolor Survey I. Imaging Observations and Catalog of Stellar Objects
arXiv:astro-ph/9512051 · doi:10.1086/192297
Abstract
We have used the KPNO 4-meter Mayall telescope to image 0.83 square degrees of sky in six fields at high galactic latitude in six filters spanning 3000-10000Å to magnitude limits ranging from 22.1 to 23.8. We have assembled a catalog of 21,375 stellar objects detected in the fields for use primarily in conducting a multicolor search for quasars. This paper describes the data reduction techniques used on the CCD data, the methods used to construct the stellar object catalog, and the simulations performed to understand its completeness and contamination.
To Appear in ApJ Supplement, 1996. 168k uuencoded gunzipped tarred tex file (requires aas2pp4.sty and tighten.sty) and 4 PostScript figures. Also available at http://astro.as.arizona.edu/~pathall/astro.html#preprints
Cited by in corpus (12)
- Star counts in the Galaxy. Simulating from very deep to very shallow photometric surveys with the TRILEGAL code
- Early galaxy evolution from deep wide field star counts. II. First estimate of the thick disc mass function
- A Deep Multicolor Survey. VI. Near-Infrared Observations, Selection Effects, and Number Counts
- A CCD Study of High Latitude Galactic Structure: Testing the Model Parameters
- An Optical/Near-Infrared Study of Radio-Loud Quasar Environments I. Methods and z=1-2 Observations
- A Deep Multicolor Survey. VII. Extremely Red Objects and Galaxy Formation
- A Deep Multicolor Survey. IV. The Electronic Stellar Catalog
- Luminosity Functions And Evolution Of Blue Galaxies In A Deep Multicolor CCD Field Survey
- A Deep Multicolor Survey V: The M Dwarf Luminosity Function
- Active Galactic Nuclei in the CNOC2 Field Galaxy Redshift Survey
- An Optical Multicolor System For Measuring Galaxy Redshifts And Spectral Types
- Radio-Quiet Quasars in the Direction of the Northern Hubble Deep Field