The dark energy survey and operations: Year 1

H. T. Diehl; T. M.C. Abbott; J. Annis; R. Armstrong; L. Baruah; A. Bermeo; G. Bernstein; E. Beynon; C. Bruderer; E. J. Buckley-Geer; H. Campbell; D. Capozzi; M. Carter; R. Casas; L. Clerkin; R. Covarrubias; C. Cuhna; C. D'Andrea; L. Da Costa; R. Das; D. L. Depoy; J. Dietrich; A. Drlica-Wagner; A. Elliott; T. Eifler; J. Estrada; J. Etherington; B. L. Flaugher; J. Frieman; A. Fausti Neto; M. Gelman; D. Gerdes; D. Gruen; R. Gruendl; J. Hao; H. Head; J. Helsby; K. Hoffman; K. Honscheid; D. James; M. Johnson; T. Kacprzac; J. Katsaros; R. Kennedy; S. Kent; R. Kessler; A. Kim; E. Krause; R. Kron; S. Kuhlmann; A. Kunder; T. Li; H. Lin; N. Maccrann; M. March; J. Marshall; E. Neilsen; P. Nugent; P. Martini; P. Melchior; F. Menanteau; R. C. Nichol; B. Nord; R. Ogando; L. Old; A. Papadopoulos; K. Patton; D. Petravick; A. A. Plazas; R. Poulton; A. Pujol; K. Reil; T. Rigby; A. Romer; A. Roodman; P. Rooney; E. Sanchez Alvaro; S. Serrano; E. Sheldon; A. Smith; R. C. Smith; M. Soares-Santos; M. Soumagnac; H. Spinka; E. Suchyta; D. Tucker; A. R. Walker; W. Wester; M. Wiesner; H. Wilcox; R. Williams; B. Yanny; Y. Y. Zhang

doi:10.1117/12.2056982

The dark energy survey and operations: Year 1

H. T. Diehl, T. M.C. Abbott, J. Annis, R. Armstrong, L. Baruah, A. Bermeo, G. Bernstein, E. Beynon, C. Bruderer, E. J. Buckley-Geer, H. Campbell, D. Capozzi, M. Carter, R. Casas, L. Clerkin, R. Covarrubias, C. Cuhna, C. D'Andrea, L. Da Costa, R. DasD. L. Depoy, J. Dietrich, A. Drlica-Wagner, A. Elliott, T. Eifler, J. Estrada, J. Etherington, B. L. Flaugher, J. Frieman, A. Fausti Neto, M. Gelman, D. Gerdes, D. Gruen, R. Gruendl, J. Hao, H. Head, J. Helsby, K. Hoffman, K. Honscheid, D. James, M. Johnson, T. Kacprzac, J. Katsaros, R. Kennedy, S. Kent, R. Kessler, A. Kim, E. Krause, R. Kron, S. Kuhlmann, A. Kunder, T. Li, H. Lin, N. Maccrann, M. March, J. Marshall, E. Neilsen, P. Nugent, P. Martini, P. Melchior, F. Menanteau, R. C. Nichol, B. Nord, R. Ogando, L. Old, A. Papadopoulos, K. Patton, D. Petravick, A. A. Plazas, R. Poulton, A. Pujol, K. Reil, T. Rigby, A. Romer, A. Roodman, P. Rooney, E. Sanchez Alvaro, S. Serrano, E. Sheldon, A. Smith, R. C. Smith, M. Soares-Santos, M. Soumagnac, H. Spinka, E. Suchyta, D. Tucker, A. R. Walker, W. Wester, M. Wiesner, H. Wilcox, R. Williams, B. Yanny, Y. Y. Zhang

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

Abstract

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.

Original language	English (US)
Title of host publication	Observatory Operations
Subtitle of host publication	Strategies, Processes, and Systems V
Editors	Alison B. Peck, Chris R. Benn, Robert L. Seaman
Publisher	SPIE
ISBN (Electronic)	9780819496171
DOIs	https://doi.org/10.1117/12.2056982
State	Published - 2014
Event	Observatory Operations: Strategies, Processes, and Systems V - Montreal, Canada Duration: Jun 25 2014 → Jun 27 2014

Publication series

Name	Proceedings of SPIE - The International Society for Optical Engineering
Volume	9149
ISSN (Print)	0277-786X
ISSN (Electronic)	1996-756X

Other

Other	Observatory Operations: Strategies, Processes, and Systems V
Country/Territory	Canada
City	Montreal
Period	6/25/14 → 6/27/14

Keywords

CTIO
Cosmology
Dark Energy Camera
Dark Energy Survey
Operations

ASJC Scopus subject areas

Electronic, Optical and Magnetic Materials
Condensed Matter Physics
Computer Science Applications
Applied Mathematics
Electrical and Electronic Engineering

Online availability

10.1117/12.2056982

Library availability

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Cite this

Diehl, H. T., Abbott, T. M. C., Annis, J., Armstrong, R., Baruah, L., Bermeo, A., Bernstein, G., Beynon, E., Bruderer, C., Buckley-Geer, E. J., Campbell, H., Capozzi, D., Carter, M., Casas, R., Clerkin, L., Covarrubias, R., Cuhna, C., D'Andrea, C., Da Costa, L., ... Zhang, Y. Y. (2014). The dark energy survey and operations: Year 1. In A. B. Peck, C. R. Benn, & R. L. Seaman (Eds.), Observatory Operations: Strategies, Processes, and Systems V Article 91490V (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 9149). SPIE. https://doi.org/10.1117/12.2056982

The dark energy survey and operations: Year 1. / Diehl, H. T.; Abbott, T. M.C.; Annis, J. et al.
Observatory Operations: Strategies, Processes, and Systems V. ed. / Alison B. Peck; Chris R. Benn; Robert L. Seaman. SPIE, 2014. 91490V (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 9149).

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution

Diehl, HT, Abbott, TMC, Annis, J, Armstrong, R, Baruah, L, Bermeo, A, Bernstein, G, Beynon, E, Bruderer, C, Buckley-Geer, EJ, Campbell, H, Capozzi, D, Carter, M, Casas, R, Clerkin, L, Covarrubias, R, Cuhna, C, D'Andrea, C, Da Costa, L, Das, R, Depoy, DL, Dietrich, J, Drlica-Wagner, A, Elliott, A, Eifler, T, Estrada, J, Etherington, J, Flaugher, BL, Frieman, J, Fausti Neto, A, Gelman, M, Gerdes, D, Gruen, D, Gruendl, R, Hao, J, Head, H, Helsby, J, Hoffman, K, Honscheid, K, James, D, Johnson, M, Kacprzac, T, Katsaros, J, Kennedy, R, Kent, S, Kessler, R, Kim, A, Krause, E, Kron, R, Kuhlmann, S, Kunder, A, Li, T, Lin, H, Maccrann, N, March, M, Marshall, J, Neilsen, E, Nugent, P, Martini, P, Melchior, P, Menanteau, F, Nichol, RC, Nord, B, Ogando, R, Old, L, Papadopoulos, A, Patton, K, Petravick, D, Plazas, AA, Poulton, R, Pujol, A, Reil, K, Rigby, T, Romer, A, Roodman, A, Rooney, P, Sanchez Alvaro, E, Serrano, S, Sheldon, E, Smith, A, Smith, RC, Soares-Santos, M, Soumagnac, M, Spinka, H, Suchyta, E, Tucker, D, Walker, AR, Wester, W, Wiesner, M, Wilcox, H, Williams, R, Yanny, B & Zhang, YY 2014, The dark energy survey and operations: Year 1. in AB Peck, CR Benn & RL Seaman (eds), Observatory Operations: Strategies, Processes, and Systems V., 91490V, Proceedings of SPIE - The International Society for Optical Engineering, vol. 9149, SPIE, Observatory Operations: Strategies, Processes, and Systems V, Montreal, Canada, 6/25/14. https://doi.org/10.1117/12.2056982

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abstract = "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.",

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note = "Publisher Copyright: {\textcopyright} 2014 SPIE.; Observatory Operations: Strategies, Processes, and Systems V ; Conference date: 25-06-2014 Through 27-06-2014",

year = "2014",

doi = "10.1117/12.2056982",

language = "English (US)",

series = "Proceedings of SPIE - The International Society for Optical Engineering",

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editor = "Peck, {Alison B.} and Benn, {Chris R.} and Seaman, {Robert L.}",

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TY - GEN

T1 - The dark energy survey and operations

T2 - Observatory Operations: Strategies, Processes, and Systems V

AU - Diehl, H. T.

AU - Abbott, T. M.C.

AU - Annis, J.

AU - Armstrong, R.

AU - Baruah, L.

AU - Bermeo, A.

AU - Bernstein, G.

AU - Beynon, E.

AU - Bruderer, C.

AU - Buckley-Geer, E. J.

AU - Campbell, H.

AU - Capozzi, D.

AU - Carter, M.

AU - Casas, R.

AU - Clerkin, L.

AU - Covarrubias, R.

AU - Cuhna, C.

AU - D'Andrea, C.

AU - Da Costa, L.

AU - Das, R.

AU - Depoy, D. L.

AU - Dietrich, J.

AU - Drlica-Wagner, A.

AU - Elliott, A.

AU - Eifler, T.

AU - Estrada, J.

AU - Etherington, J.

AU - Flaugher, B. L.

AU - Frieman, J.

AU - Fausti Neto, A.

AU - Gelman, M.

AU - Gerdes, D.

AU - Gruen, D.

AU - Gruendl, R.

AU - Hao, J.

AU - Head, H.

AU - Helsby, J.

AU - Hoffman, K.

AU - Honscheid, K.

AU - James, D.

AU - Johnson, M.

AU - Kacprzac, T.

AU - Katsaros, J.

AU - Kennedy, R.

AU - Kent, S.

AU - Kessler, R.

AU - Kim, A.

AU - Krause, E.

AU - Kron, R.

AU - Kuhlmann, S.

AU - Kunder, A.

AU - Li, T.

AU - Lin, H.

AU - Maccrann, N.

AU - March, M.

AU - Marshall, J.

AU - Neilsen, E.

AU - Nugent, P.

AU - Martini, P.

AU - Melchior, P.

AU - Menanteau, F.

AU - Nichol, R. C.

AU - Nord, B.

AU - Ogando, R.

AU - Old, L.

AU - Papadopoulos, A.

AU - Patton, K.

AU - Petravick, D.

AU - Plazas, A. A.

AU - Poulton, R.

AU - Pujol, A.

AU - Reil, K.

AU - Rigby, T.

AU - Romer, A.

AU - Roodman, A.

AU - Rooney, P.

AU - Sanchez Alvaro, E.

AU - Serrano, S.

AU - Sheldon, E.

AU - Smith, A.

AU - Smith, R. C.

AU - Soares-Santos, M.

AU - Soumagnac, M.

AU - Spinka, H.

AU - Suchyta, E.

AU - Tucker, D.

AU - Walker, A. R.

AU - Wester, W.

AU - Wiesner, M.

AU - Wilcox, H.

AU - Williams, R.

AU - Yanny, B.

AU - Zhang, Y. Y.

PY - 2014

Y1 - 2014

N2 - 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.

AB - 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.

KW - CTIO

KW - Cosmology

KW - Dark Energy Camera

KW - Dark Energy Survey

KW - Operations

UR - http://www.scopus.com/inward/record.url?scp=84922620752&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=84922620752&partnerID=8YFLogxK

U2 - 10.1117/12.2056982

DO - 10.1117/12.2056982

M3 - Conference contribution

AN - SCOPUS:84922620752

T3 - Proceedings of SPIE - The International Society for Optical Engineering

BT - Observatory Operations

A2 - Peck, Alison B.

A2 - Benn, Chris R.

A2 - Seaman, Robert L.

PB - SPIE

Y2 - 25 June 2014 through 27 June 2014

ER -

The dark energy survey and operations: Year 1

Abstract

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