The K20 survey. III. Photometric and spectroscopic properties of the sample
arXiv:astro-ph/0206168 · doi:10.1051/0004-6361:20020861
Abstract
The K20 survey is an ESO VLT optical and near-infrared spectroscopic survey aimed at obtaining spectral information and redshifts of a complete sample of about 550 objects to K_s\leq20.0 over two independent fields with a total area of 52 arcmin^2. In this paper we discuss the scientific motivation of such a survey, we describe the photometric and spectroscopic properties of the sample, and we release the -band photometric catalog. Extensive simulations showed that the sample is photometrically highly complete to K_s=20. The observed galaxy counts and the R-K_s color distribution are consistent with literature results. We observed spectroscopically 94% of the sample, reaching a spectroscopic redshift identification completeness of 92% to K_s\leq20.0 for the observed targets, and of 87% for the whole sample (i.e. counting also the unobserved targets). Deep spectroscopy was complemented with multi-band deep imaging in order to derive tested and reliable photometric redshifts for the galaxies lacking spectroscopic redshifts. The results show a very good agreement between the spectroscopic and the photometric redshifts with <z_{spe}-z_{phot}>=0.01 and with a dispersion of σ_{Δz}=0.09. Using both the spectroscopic and the photometric redshifts, we reached an overall redshift completeness of about 98%. The size of the sample, the redshift completeness, the availability of high quality photometric redshifts and multicolor spectral energy distributions make the K20 survey database one of the most complete samples available to date for constraining the currently competing scenarios of galaxy formation and for a variety of other galaxy evolution studies.
arXiv comment13 pages, 10 figures, to appear in Astronomy & Astrophysics
References in corpus (37)
- Maps of Dust IR Emission for Use in Estimation of Reddening and CMBR Foregrounds
- Hierarchical Galaxy Formation
- New Insight on Galaxy Formation and Evolution from Keck Spectroscopy of the Hawaii Deep Fields
- The Star Formation History of Field Galaxies
- The 2dF Galaxy Redshift Survey: Near Infrared Galaxy Luminosity Functions
- The Nature of High-Redshift Galaxies
- First Results from the X-ray and Optical Survey of the Chandra Deep Field South
- The K-Band Galaxy Luminosity Function
- Evolution of the Hubble Sequence in Hierarchical Models for Galaxy Formation
- The Ages of Elliptical Galaxies in a Merger Model
- Caltech Faint Galaxy Redshift Survey X: A Redshift Survey in the Region of the Hubble Deep Field North
- The K20 survey. I. Disentangling old and dusty star-forming galaxies in the ERO population
- The CANADA-FRANCE REDSHIFT SURVEY I: Introduction to the Survey, Photometric Catalogs and Surface Brightness Selection Effects
- The K-band luminosity function at z=1: a powerful constraint on galaxy formation theory
- Photometric redshifts and selection of high redshift galaxies in the NTT and Hubble Deep Fields
- Quantitative Morphology of Galaxies in the Hubble Deep Field
- The Hawaii K-Band Galaxy Survey. II. Bright K-band Imaging
- Subaru Deep Survey I. Near-Infrared Observations
- A wide-field K-band survey - I. Galaxy counts in B, V, I and K
- Colors and K-Band Counts of Extremely Faint Field Galaxies
- An imaging K-band survey - I: The catalogue, star and galaxy counts
- A K-band Selected Photometric Redshift Catalog in the HDF-S: Sampling the Rest-Frame V-Band to z=3
- Deep near-IR observations of the Chandra Deep Field and of the HDF-South - Color and Number Counts
- The Near-Infrared Number Counts and Luminosity Functions of Local Galaxies
- The Spatial Clustering of Distant, z~1, Early-Type Galaxies
- The K20 survey. II. The Different Spatial Clustering of z~1 Old and Dusty Star-Forming EROs
- K-Band Galaxy Counts in the South Galactic Pole Region
- Caltech Faint Galaxy Redshift Survey VIII: Analysis for the Field J0053+1234
- Caltech Faint Galaxy Redshift Survey VII: Data Analysis Techniques and Redshifts in the Field J0053+1234
- A Deep Multicolor Survey. VI. Near-Infrared Observations, Selection Effects, and Number Counts
- Systematic Biases in Galaxy Luminosity Functions
- The Munich Near-Infrared Cluster Survey (MUNICS) - Number density evolution of massive field galaxies to z ~ 1.2 as derived from the K-band selected survey
- High redshift evolution of optically and IR-selected galaxies: a comparison with CDM scenarios
- The ESO K'-band Galaxy Survey - Galaxy Counts
- A Massive Disk Galaxy at z=1.34
- An Optical/Near-Infrared Study of Radio-Loud Quasar Environments I. Methods and z=1-2 Observations
- Early-type Galaxies in the Hubble Deep Field. The <mu_e>-r_e relation and the lack of large galaxies at high redshift
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