Calibration update of the COMBO-17 CDFS catalogue
arXiv:0809.2066 · doi:10.1051/0004-6361:200810954
Abstract
We present an update to the photometric calibration of the COMBO-17 catalogue on the Extended Chandra Deep Field South, which is now consistent with the GaBoDS and MUSYC catalogues. As a result, photometric redshifts become slightly more accurate, with <0.01 rms and little bias in the delta_z/(1+z) of galaxies with R<21 and of QSOs with R<24. With increasing photon noise the rms of galaxies reaches 0.02 for R<23 and 0.035 at R~23.5. Consequences for the rest-frame colours of galaxies at z<1 are discussed.
A&A research note, resubmitted 02 Oct 2008, 4 pages in print format
References in corpus (1)
Cited by in corpus (13)
- The Multiwavelength Survey by Yale-Chile (MUSYC): Deep Medium-Band optical imaging and high quality 32-band photometric redshifts in the ECDF-S
- Clumpy Galaxies in GOODS and GEMS: Massive Analogs of Local Dwarf Irregulars
- Charting the evolution of the ages and metallicities of massive galaxies since z=0.7
- A Public, K-Selected, Optical-to-Near-Infrared Catalog of the Extended Chandra Deep Field South (ECDFS) from the MUltiwavelength Survey by Yale-Chile (MUSYC)
- A joint analysis of BLAST 250--500um and LABOCA 870um observations in the Extended Chandra Deep Field South
- The Advanced Camera for Surveys General Catalog: Structural Parameters for Approximately Half a Million Galaxies
- The Chandra Deep Fields: Lifting the Veil on Distant Active Galactic Nuclei and X-Ray Emitting Galaxies
- A search for variable and transient radio sources in the extended Chandra Deep Field South at 5.5 GHz
- The environmental dependence of the structure of galactic discs in STAGES S0 galaxies: implications for S0 formation
- Quasi-stellar objects in the ALHAMBRA survey. I. Photometric redshift accuracy based on a 23 optical-NIR filter photometry
- ELDAR, a new method to identify AGN in multi-filter surveys: the ALHAMBRA test-case
- The 2-degree Field Lensing Survey: photometric redshifts from a large new training sample to r<19.5
- The XMM Deep Survey in the CDF-S VII. UV catalogue of the Optical Monitor observations