The Sloan Digital Sky Survey photometric camera

被引：1516

作者：

Gunn, JE

Carr, M

Rockosi, C

Sekiguchi, M

Berry, K

Elms, B

de Haas, E

Ivezic, Z

Knapp, G

Lupton, R

Pauls, G

Simcoe, R

Hirsch, R

Sanford, D

Wang, S

York, D

Harris, F

Annis, J

Bartozek, L

Boroski, W

Bakken, J

Haldeman, M

Kent, S

Holm, S

Holmgren, D

Petravick, D

Prosapio, A

Rechenmacher, R

Doi, M

Fukugita, M

Shimasaku, K

Okada, N

Hull, C

Siegmund, W

Mannery, E

Blouke, M

Heidtman, D

Schneider, D

Lucinio, R

Brinkman, J

机构：

[1] Princeton Univ, Dept Astrophys Sci, Princeton, NJ 08544 USA

[2] Princeton Univ Observ, Princeton, NJ 08544 USA

[3] Univ Chicago, Ctr Astron & Astrophys, Chicago, IL 60637 USA

[4] USN Observ, Flagstaff, AZ 86002 USA

[5] Fermi Natl Accelerator Lab, Batavia, IL 60510 USA

[6] Univ Tokyo, Sch Sci, Dept Astron, Bunkyo Ku, Tokyo 113, Japan

[7] Natl Astron Observ, Tokyo 181, Japan

[8] Univ Washington, Dept Astron, Seattle, WA 98195 USA

[9] Sci Imaging Technol Inc, Beaverton, OR USA

[10] Penn State Univ, Dept Astron & Astrophys, Davey Lab 525, University Pk, PA 16802 USA

[11] Apache Point Observ, Sunspot, NM 88349 USA

来源：

ASTRONOMICAL JOURNAL | 1998年 / 116卷 / 06期

关键词：

astrometry; atlases; catalogs; cosmology : observations; instrumentation : detectors; instrumentation : photometers; surveys;

D O I：

10.1086/300645

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We have constructed a large-format mosaic CCD camera for the Sloan Digital Sky Survey. The camera consists of two arrays, a photometric array that uses 30 2048 x 2048 SITe/Tektroniu CCDs (24 mu m pixels) with an effective imaging area of 720 cm(2) and an astrometric array that uses 24 400 x 2048 CCDs with the same pixel size, which will allow us to tie bright astrometric standard stars to the objects imaged in the photometric camera. The instrument will be used to carry out photometry essentially simultaneously in five color bands spanning the range accessible to silicon detectors on the ground in the time-delay-and-integrate (TDI) scanning mode. The photometric detectors are arrayed in the focal plane in six columns of five chips each such that two scans cover a filled stripe 2." 5 wide. This paper presents engineering and technical details of the camera.

引用

页码：3040 / 3081

页数：42

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