ESO Imaging Survey I. Description of the survey, data reduction and reliability of the data

被引:69
作者
Nonino, M
Bertin, E
da Costa, L
Deul, E
Erben, T
Olsen, L
Prandoni, I
Scodeggio, M
Wicenec, A
Wichmann, R
Benoist, C
Freudling, W
Guarnieri, MD
Hook, I
Hook, R
Mendez, R
Savaglio, S
Silva, D
Slijkhuis, R
机构
[1] European So Observ, D-85748 Garching, Germany
[2] Osservatorio Astron Trieste, I-31144 Trieste, Italy
[3] Leiden Observ, NL-2300 RA Leiden, Netherlands
[4] Inst Astrophys, F-75014 Paris, France
[5] Max Planck Inst Astrophys, D-85748 Garching, Germany
[6] Astron Observ, DK-2100 Copenhagen, Denmark
[7] CNR, Ist Radioastron, I-40129 Bologna, Italy
[8] Landessternwarte Konigstuhl, D-69117 Heidelberg, Germany
[9] Observ Paris, DAEC, F-92195 Meudon, France
[10] Space Telescope European Coordinating Facil, D-85748 Garching, Germany
[11] Osservatorio Astron Pino Torinese, I-10025 Pino Torinese, Italy
[12] Cerro Tololo Interamer Observ, La Serena, Chile
[13] ESO La Silla Observ, La Silla, Chile
来源
ASTRONOMY & ASTROPHYSICS SUPPLEMENT SERIES | 1999年 / 137卷 / 01期
关键词
surveys; stars : statistics; galaxies : statistics;
D O I
10.1051/aas:1999473
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
This paper presents the first data evaluation of the ESO Imaging Survey (EIS), a public survey being carried out by ESO and member states, in preparation for the VLT first-light. The survey goals, organization, strategy and observations are discussed and an overview is given of the survey pipeline developed to handle EIS data and produce object catalogs. A report is presented on moderately deep I-band observations obtained in the first of four patches surveyed, covering a region of 3.2 square degrees centered at alpha similar to 22(h)40(m) and delta = -40 degrees. The products available to the community, including pixel maps (with astrometric and photometric calibrations) and the corresponding object catalogs, are also described. In order to evaluate the quality of the data, preliminary estimates are presented for the star and galaxy number counts, and for the angular two-point correlation function obtained from the available data. The present work is meant as a preview of the final release of the EIS data that will become available later this year.
引用
收藏
页码:51 / 74
页数:24
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