1. The Dark Energy Survey and operations: Year 1
- Author
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Douglas L. Tucker, Alex Drlica-Wagner, Emma Beynon, S. Serrano, T. Rigby, Richard Kessler, J. Annis, Huan Lin, Tim Eifler, Matthew P. Wiesner, E. Buckley-Geer, Felipe Menanteau, H. Wilcox, E. Suchyta, K. Patton, Tenglin Li, Elisabeth Krause, Ann Elliott, Ricard Casas, H. H. Head, Jennifer L. Marshall, M. Carter, Andrea Kunder, Y. Zhang, Eric H. Neilsen, Allyn Smith, Alistair R. Walker, Peter Nugent, Robert Connon Smith, Daniel Gruen, Maayane T. Soumagnac, Marcelle Soares-Santos, L. Baruah, Erin Sheldon, R. D. Kennedy, A. Papadopoulos, Robert C. Nichol, T. M. C. Abbott, Brian Nord, T. Kacprzac, Joshua A. Frieman, C. Cuhna, R. Das, Jennifer E. Helsby, E. Sanchez Alvaro, R. Covarrubias, W. C. Wester, A. Bermeo, A. Roodman, M. W. G. Johnson, Gary Bernstein, Brian Yanny, Kara Hoffman, A. K. Romer, Jiangang Hao, Robert Armstrong, Paul Martini, D. W. Gerdes, A. Fausti Neto, Richard G. Kron, M. March, J. P. Dietrich, H. T. Diehl, D. James, K. Honscheid, Robert Williams, Peter Melchior, Niall MacCrann, James Etherington, M. Gelman, Juan Estrada, L. N. da Costa, B. Flaugher, C. B. D'Andrea, Ricardo L. C. Ogando, Claudio Bruderer, P. Rooney, J. Katsaros, Lyndsay Old, Kevin Reil, H. M. Spinka, H. Campbell, A. Pujol, Alex G. Kim, S. E. Kuhlmann, L. Clerkin, Darren L. DePoy, Don Petravick, Robert A. Gruendl, R. Poulton, Steve Kent, A. A. Plazas, and Diego Capozzi
- Subjects
Telescope ,Physics ,Galaxy groups and clusters ,Observatory ,law ,Dark energy ,Astronomy ,Baryon acoustic oscillations ,Astrophysics ,Cosmology ,Galaxy cluster ,Weak gravitational lensing ,law.invention - 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.
- Published
- 2014
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