GaBoDS: The Garching-Bonn Deep Survey - IV. Methods for the image reduction of multi-chip cameras demonstrated on data from the ESO wide-field imager

被引:232
作者
Erben, T
Schirmer, M
Dietrich, JP
Cordes, O
Haberzettl, L
Hetterscheidt, M
Hildebrandt, H
Schmithuesen, O
Schneider, P
Simon, P
Deul, E
Hooks, RN
Kaiser, N
Radovich, M
Benoist, C
Nonino, M
Olsen, LF
Prandoni, I
Wichmann, R
Zaggia, S
Bomans, D
Dettmar, RJ
Miralles, JM
机构
[1] Univ Bonn, IAEF, D-53121 Bonn, Germany
[2] Isaac Newton Grp Telescopes, Santa Cruz de La Palma 38700, Tenerife, Spain
[3] Ruhr Univ Bochum, Inst Astron, D-44780 Bochum, Germany
[4] Leiden Observ, NL-2300 RA Leiden, Netherlands
[5] European So Observ, Space Telescope European Coordinating Facil, D-85748 Garching, Germany
[6] Univ Hawaii, Inst Astron, Honolulu, HI 96822 USA
[7] Osserv Astron Capodimonte, INAF, I-80131 Naples, Italy
[8] Observ Cote Azur, CNRS, Lab Cassiopee, F-06304 Nice, France
[9] Osserv Astron Trieste, INAF, I-34131 Trieste, Italy
[10] Copenhagen Univ Observ, DK-2100 Copenhagen, Denmark
[11] INAF, Inst Radioastron, I-40129 Bologna, Italy
[12] Univ Hamburg, D-21029 Hamburg, Germany
[13] European So Observ, D-85748 Garching, Germany
关键词
methods : data analysis; techniques : image processing;
D O I
10.1002/asna.200510396
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present our image processing system for the reduction of optical imaging data from multi-chip cameras. In the framework of the Garching Bonn Deep Survey (GaBoDS; Schirmer et al. 2003) consisting of about 20 square degrees of high-quality data from WFI@MPG/ESO 2.2m, our group developed an imaging pipeline for the homogeneous and efficient processing of this large data set. Having weak gravitational lensing as the main science driver, our algorithms are optimised to produce deep co-added mosaics from individual exposures obtained from empty field observations. However, the modular design of our pipeline allows an easy adaption to different scientific applications. Our system has already been ported to a large variety of optical instruments and its products have been used in various scientific contexts. In this paper we give a thorough description of the algorithms used and a careful evaluation of the accuracies reached. This concerns the removal of the instrumental signature, the astrometric alignment, photometric calibration and the characterisation of final co-added mosaics. In addition we give a more general overview on the image reduction process and comment on observing strategies where they have significant influence on the data quality.
引用
收藏
页码:432 / 464
页数:33
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