The Dark Energy Survey and Operations: Year 1

被引:39
作者
Diehl, H. T. [1 ]
Abbott, T. M. C. [2 ]
Annis, J. [1 ]
Armstrong, R. [3 ]
Baruah, L. [4 ]
Bermeo, A. [4 ]
Bernstein, G. [3 ]
Beynon, E. [5 ]
Bruderer, C. [6 ]
Buckley-Geer, E. J. [1 ]
Campbell, H. [5 ]
Capozzi, D. [5 ]
Carter, M. [4 ]
Casas, R. [7 ]
Clerkin, L. [8 ]
Covarrubias, R. [9 ,18 ]
Cuhna, C.
D'Andrea, C. [5 ]
da Costa, L. [11 ]
Das, R.
DePoy, D. L.
Dietrich, J. [14 ,15 ]
Drlica-Wagner, A. [1 ]
Elliott, A.
Eifler, T. [3 ]
Estrada, J. [1 ]
Etherington, J. [3 ,5 ]
Flaugher, B. L. [1 ]
Frieman, J. [1 ]
Fausti Neto, A. [11 ]
Gelman, M. [9 ]
Gerdes, D. [12 ]
Gruen, D. [17 ]
Gruendl, R. [9 ,18 ,24 ]
Hao, J. [1 ]
Head, H. [19 ]
Helsby, J. [20 ]
Hoffman, K. [7 ]
Honscheid, K. [16 ]
James, D. [2 ]
Johnson, M. [9 ,18 ]
Kacprzac, T. [8 ]
Katsaros, J.
Kennedy, R. [4 ]
Kent, S. [1 ]
Kessler, R. [20 ]
Kim, A. [21 ]
Krause, E. [3 ]
Kron, R. [1 ]
Kuhlmann, S. [22 ]
机构
[1] Fermilab Natl Accelerator Lab, POB 500, Batavia, IL 60510 USA
[2] Natl Opt Astron Observ, Cerro Tololo Inter Amer Observ, La Serena, Chile
[3] Univ Penn, Dept Phys & Astron, Philadelphia, PA 19104 USA
[4] Dept Phys & Astron, Sussex, England
[5] Univ Portsmouth, Inst Cosmol & Gravitat, Portsmouth PO1 3FX, Hants, England
[6] Swiss Fed Inst Technol, Inst Astron, Dept Phys, CH-8093 Zurich, Switzerland
[7] IEEC, CSIC, ICE, E-08193 Barcelona, Spain
[8] UCL, Dept Phys & Astron, London WC1E 6BT, England
[9] Natl Ctr Supercomp Applicat, Urbana, IL 61801 USA
[10] Stanford Univ, Kavli Inst Particle Astrophys & Cosmol, Stanford, CA 94305 USA
[11] Lab Interinstituc & Astronomia, BR-20921400 Janeiro, RJ, Brazil
[12] Univ Michigan, Dept Phys, Ann Arbor, MI 48109 USA
[13] Texas A&M Univ, Inst Fuindamental Phys & Astron, Dept Phys & Astron, College Stn, TX 77843 USA
[14] Univ Observ Munich, D-81679 Munich, Germany
[15] Excellence Cluster Univ, D-85748 Garching, Germany
[16] Ohio State Univ, Dept Phys, Columbus, OH 43210 USA
[17] Max Planck Inst Extraterr Phys, D-85748 Garching, Germany
[18] Univ Illinois, Dept Astron, Urbana, IL 61801 USA
[19] Austin Peay State Univ, Dept Phys & Astron, Clarksville, TN 37044 USA
[20] Univ Chicago, Kavli Inst Cosmol Phys, Chicago, IL 60637 USA
[21] Lawrence Berkeley Natl Lab, Berkeley, CA 94720 USA
[22] Argonne Natl Lab, Argonne, IL 60439 USA
[23] Univ Manchester, Manchester M13 9PL, Lancs, England
[24] Ohio State Univ, Ctr Cosmol & Astro Particle Phys, Columbus, OH 43210 USA
[25] Observ Nac, BR-20921400 Janeiro, RJ, Brazil
[26] Univ Park, Cripps Ctr Astron & Particle Theory, Nottingham NG7 2RD, England
来源
OBSERVATORY OPERATIONS: STRATEGIES, PROCESSES, AND SYSTEMS V | 2014年 / 9149卷
基金
美国国家科学基金会; 英国科学技术设施理事会;
关键词
Cosmology; Dark Energy Survey; Dark Energy Camera; Operations; CTIO; COMPRESSION;
D O I
10.1117/12.2056982
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The Dark Energy Survey (DES) is a next generation optical survey aimed at understanding the accelerating expansion of the universe using four complementary methods: weak gravitational lensing, galaxy cluster counts, baryon acoustic oscillations, and Type Ia supernovae. To perform the 5000 sq-degree wide field and 30 sq-degree supernova surveys, the DES Collaboration built the Dark Energy Camera (DECam), a 3 square-degree, 570-Megapixel CCD camera that was installed at the prime focus of the Blanco 4-meter telescope at the Cerro Tololo Inter-American Observatory (CTIO). DES started its first observing season on August 31, 2013 and observed for 105 nights through mid-February 2014. This paper describes DES "Year 1" (Y1), the strategy and goals for the first year's data, provides an outline of the operations procedures, lists the efficiency of survey operations and the causes of lost observing time, provides details about the quality of the first year's data, and hints at the "Year 2" plan and outlook.
引用
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页数:15
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