A catalogue of the Chandra Deep Field South with multi-colour classification and photometric redshifts from COMBO-17

被引:366
|
作者
Wolf, C
Meisenheimer, K
Kleinheinrich, A
Borch, A
Dye, S
Gray, A
Wisotzki, L
Bell, EF
Rix, HW
Cimatti, A
Hasinger, G
Szokoly, G
机构
[1] Univ Oxford, Dept Phys, Oxford OX1 3RH, England
[2] Max Planck Inst Astron, D-69117 Heidelberg, Germany
[3] Univ London Imperial Coll Sci Technol & Med, Blackett Lab, Astrophys Grp, London, England
[4] Univ Nottingham, Sch Phys & Astron, Nottingham NG7 2RD, England
[5] Astrophys Inst Potsdam, D-14482 Potsdam, Germany
[6] Osserv Astrofis Arcetri, INAF, I-50125 Florence, Italy
[7] Max Planck Inst Extraterr Phys, D-85741 Garching, Germany
关键词
catalogs; surveys; techniques : photometric; methods : observational; galaxies : general;
D O I
10.1051/0004-6361:20040525
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present the COMBO-17 object catalogue of the Chandra Deep Field South for public use, covering a field which is 31.'5 x 30' in size. This catalogue lists astrometry, photometry in 17 passbands from 350 to 930 nm, and ground-based morphological data for 63 501 objects. The catalogue also contains multi-colour classification into the categories Star, Galaxy and Quasar as well as photometric redshifts. We include restframe luminosities in Johnson, SDSS and Bessell passbands and estimated errors. The redshifts are most reliable at R<24, where the sample contains approximately 100 quasars, 1000 stars and 10 000 galaxies. We use nearly 1000 spectroscopically identified objects in conjunction with detailed simulations to characterize the performance of COMBO-17. We show that the selection of quasars, more generally type-1 AGN, is nearly complete and minimally contaminated at z=[0.5, 5] for luminosities above M-B=-21.7. Their photometric redshifts are accurate to roughly 5000 km s(-1). Galaxy redshifts are accurate to 1% in delta(z)/(1+z) at R<21. They degrade in quality for progressively fainter galaxies, reaching accuracies of 2% for galaxies with Rsimilar to22 and of 10% for galaxies with R>24. The selection of stars is complete to Rsimilar to23, and deeper for M stars. We also present an updated discussion of our classification technique with maps of survey completeness, and discuss possible failures of the statistical classification in the faint regime at Rgreater than or similar to24.
引用
收藏
页码:913 / 936
页数:24
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