The Dark Energy Survey and operations: Years 4 and 5

H. T. Diehl; E. Neilsen; R. A. Gruendl; T. M.C. Abbott; S. Allam; O. Alvarez; J. Annis; E. Balbinot; S. Bhargava; K. Bechtol; G. M. Bernstein; R. Bhatawdekar; S. Bocquet; D. Brout; R. Capasso; R. Cawthon; C. Chang; E. Cook; C. J. Conselice; J. Cruz; C. D’Andrea; L. Da Costa; R. Das; D. L. DePoy; A. Drlica-Wagner; A. Elliott; S. W. Everett; J. Frieman; A. Fausti Neto; A. Ferté; I. Friswell; K. E. Furnell; L. Gelman; D. W. Gerdes; M. S.S. Gill; D. A. Goldstein; D. Gruen; D. J. Gulledge; S. Hamilton; D. Hollowood; K. Honscheid; D. J. James; M. D. Johnson; M. W.G. Johnson; S. Kent; R. Kessler; G. Khullar; E. Kovacs; A. Kremin; R. Kron; N. Kuropatkin; J. Lasker; A. Lathrop; T. S. Li; M. Manera; M. March; J. L. Marshall; M. Medford; F. Menanteau; I. Mohammed; M. R. Monroy; B. Moraes; E. P. Morganson; J. Muir; M. Murphy; B. Nord; A. B. Pace; A. Palmese; Y. Park; F. Paz-Chinchón; M. E.S. Pereira; D. Petravick; A. A. Plazas; J. Poh; T. Prochaska; K. Reil; A. K. Romer; A. Roodman; M. Sako; M. Sauseda; D. Scolnic; L. F. Secco; I. Sevilla-Noarbe; N. Shipp; J. A. Smith; M. Soares-Santos; B. Soergel; A. Stebbins; K. T. Story; K. Stringer; F. Tarsitano; B. Thomas; D. L. Tucker; A. K. Vivas; A. R. Walker; M. Y. Wang; C. Weaverdyck; N. Weaverdyck; W. Wester; C. F. Wethers; R. Wilkinson; H. Y. Wu; B. Yanny; A. Zenteno; Y. Zhang

doi:10.1117/12.2312113

The Dark Energy Survey and operations: Years 4 and 5

H. T. Diehl, E. Neilsen, R. A. Gruendl, T. M.C. Abbott, S. Allam, O. Alvarez, J. Annis, E. Balbinot, S. Bhargava, K. Bechtol, G. M. Bernstein, R. Bhatawdekar, S. Bocquet, D. Brout, R. Capasso, R. Cawthon, C. Chang, E. Cook, C. J. Conselice, J. CruzC. D’Andrea, L. Da Costa, R. Das, D. L. DePoy, A. Drlica-Wagner, A. Elliott, S. W. Everett, J. Frieman, A. Fausti Neto, A. Ferté, I. Friswell, K. E. Furnell, L. Gelman, D. W. Gerdes, M. S.S. Gill, D. A. Goldstein, D. Gruen, D. J. Gulledge, S. Hamilton, D. Hollowood, K. Honscheid, D. J. James, M. D. Johnson, M. W.G. Johnson, S. Kent, R. Kessler, G. Khullar, E. Kovacs, A. Kremin, R. Kron, N. Kuropatkin, J. Lasker, A. Lathrop, T. S. Li, M. Manera, M. March, J. L. Marshall, M. Medford, F. Menanteau, I. Mohammed, M. R. Monroy, B. Moraes, E. P. Morganson, J. Muir, M. Murphy, B. Nord, A. B. Pace, A. Palmese, Y. Park, F. Paz-Chinchón, M. E.S. Pereira, D. Petravick, A. A. Plazas, J. Poh, T. Prochaska, K. Reil, A. K. Romer, A. Roodman, M. Sako, M. Sauseda, D. Scolnic, L. F. Secco, I. Sevilla-Noarbe, N. Shipp, J. A. Smith, M. Soares-Santos, B. Soergel, A. Stebbins, K. T. Story, K. Stringer, F. Tarsitano, B. Thomas, D. L. Tucker, A. K. Vivas, A. R. Walker, M. Y. Wang, C. Weaverdyck, N. Weaverdyck, W. Wester, C. F. Wethers, R. Wilkinson, H. Y. Wu, B. Yanny, A. Zenteno, Y. Zhang

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

10 Scopus citations

Abstract

The Dark Energy Survey (DES) is an operating 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 has completed its third observing season out of a nominal five. This paper describes DES “Year 4” (Y4) and “Year 5” (Y5), the survey strategy, an outline of the survey operations procedures, the efficiency of operations and the causes of lost observing time. It provides details about the quality of these two-season's data, a summary of the overall status, and plans for the final survey season.

Original language	English (US)
Title of host publication	Observatory Operations
Subtitle of host publication	Strategies, Processes, and Systems VII
Editors	Robert L. Seaman, Alison B. Peck, Chris R. Benn
Publisher	SPIE
ISBN (Electronic)	9781510619616
DOIs	https://doi.org/10.1117/12.2312113
State	Published - 2018
Externally published	Yes
Event	Observatory Operations: Strategies, Processes, and Systems VII 2018 - Austin, United States Duration: Jun 11 2018 → Jun 15 2018

Publication series

Name	Proceedings of SPIE - The International Society for Optical Engineering
Volume	10704
ISSN (Print)	0277-786X
ISSN (Electronic)	1996-756X

Conference

Conference	Observatory Operations: Strategies, Processes, and Systems VII 2018
Country/Territory	United States
City	Austin
Period	6/11/18 → 6/15/18

Bibliographical note

Publisher Copyright:
© 2018 SPIE

Keywords

CTIO
Cosmology
Dark Energy Camera
Dark Energy Survey
Operations

Publisher link

10.1117/12.2312113

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Cite this

Diehl, H. T., Neilsen, E., Gruendl, R. A., Abbott, T. M. C., Allam, S., Alvarez, O., Annis, J., Balbinot, E., Bhargava, S., Bechtol, K., Bernstein, G. M., Bhatawdekar, R., Bocquet, S., Brout, D., Capasso, R., Cawthon, R., Chang, C., Cook, E., Conselice, C. J., ... Zhang, Y. (2018). The Dark Energy Survey and operations: Years 4 and 5. In R. L. Seaman, A. B. Peck, & C. R. Benn (Eds.), Observatory Operations: Strategies, Processes, and Systems VII Article 107040D (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 10704). SPIE. https://doi.org/10.1117/12.2312113

The Dark Energy Survey and operations: Years 4 and 5. / Diehl, H. T.; Neilsen, E.; Gruendl, R. A. et al.
Observatory Operations: Strategies, Processes, and Systems VII. ed. / Robert L. Seaman; Alison B. Peck; Chris R. Benn. SPIE, 2018. 107040D (Proceedings of SPIE - The International Society for Optical Engineering; Vol. 10704).

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

Diehl, HT, Neilsen, E, Gruendl, RA, Abbott, TMC, Allam, S, Alvarez, O, Annis, J, Balbinot, E, Bhargava, S, Bechtol, K, Bernstein, GM, Bhatawdekar, R, Bocquet, S, Brout, D, Capasso, R, Cawthon, R, Chang, C, Cook, E, Conselice, CJ, Cruz, J, D’Andrea, C, Da Costa, L, Das, R, DePoy, DL, Drlica-Wagner, A, Elliott, A, Everett, SW, Frieman, J, Fausti Neto, A, Ferté, A, Friswell, I, Furnell, KE, Gelman, L, Gerdes, DW, Gill, MSS, Goldstein, DA, Gruen, D, Gulledge, DJ, Hamilton, S, Hollowood, D, Honscheid, K, James, DJ, Johnson, MD, Johnson, MWG, Kent, S, Kessler, R, Khullar, G, Kovacs, E, Kremin, A, Kron, R, Kuropatkin, N, Lasker, J, Lathrop, A, Li, TS, Manera, M, March, M, Marshall, JL, Medford, M, Menanteau, F, Mohammed, I, Monroy, MR, Moraes, B, Morganson, EP, Muir, J, Murphy, M, Nord, B, Pace, AB, Palmese, A, Park, Y, Paz-Chinchón, F, Pereira, MES, Petravick, D, Plazas, AA, Poh, J, Prochaska, T, Reil, K, Romer, AK, Roodman, A, Sako, M, Sauseda, M, Scolnic, D, Secco, LF, Sevilla-Noarbe, I, Shipp, N, Smith, JA, Soares-Santos, M, Soergel, B, Stebbins, A, Story, KT, Stringer, K, Tarsitano, F, Thomas, B, Tucker, DL, Vivas, AK, Walker, AR, Wang, MY, Weaverdyck, C, Weaverdyck, N, Wester, W, Wethers, CF, Wilkinson, R, Wu, HY, Yanny, B, Zenteno, A & Zhang, Y 2018, The Dark Energy Survey and operations: Years 4 and 5. in RL Seaman, AB Peck & CR Benn (eds), Observatory Operations: Strategies, Processes, and Systems VII., 107040D, Proceedings of SPIE - The International Society for Optical Engineering, vol. 10704, SPIE, Observatory Operations: Strategies, Processes, and Systems VII 2018, Austin, United States, 6/11/18. https://doi.org/10.1117/12.2312113

@inproceedings{1b3ec3ada4884514a1410c446ba21c13,

title = "The Dark Energy Survey and operations: Years 4 and 5",

abstract = "The Dark Energy Survey (DES) is an operating 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 has completed its third observing season out of a nominal five. This paper describes DES “Year 4” (Y4) and “Year 5” (Y5), the survey strategy, an outline of the survey operations procedures, the efficiency of operations and the causes of lost observing time. It provides details about the quality of these two-season's data, a summary of the overall status, and plans for the final survey season.",

keywords = "CTIO, Cosmology, Dark Energy Camera, Dark Energy Survey, Operations",

author = "Diehl, {H. T.} and E. Neilsen and Gruendl, {R. A.} and Abbott, {T. M.C.} and S. Allam and O. Alvarez and J. Annis and E. Balbinot and S. Bhargava and K. Bechtol and Bernstein, {G. M.} and R. Bhatawdekar and S. Bocquet and D. Brout and R. Capasso and R. Cawthon and C. Chang and E. Cook and Conselice, {C. J.} and J. Cruz and C. D{\textquoteright}Andrea and {Da Costa}, L. and R. Das and DePoy, {D. L.} and A. Drlica-Wagner and A. Elliott and Everett, {S. W.} and J. Frieman and {Fausti Neto}, A. and A. Fert{\'e} and I. Friswell and Furnell, {K. E.} and L. Gelman and Gerdes, {D. W.} and Gill, {M. S.S.} and Goldstein, {D. A.} and D. Gruen and Gulledge, {D. J.} and S. Hamilton and D. Hollowood and K. Honscheid and James, {D. J.} and Johnson, {M. D.} and Johnson, {M. W.G.} and S. Kent and R. Kessler and G. Khullar and E. Kovacs and A. Kremin and R. Kron and N. Kuropatkin and J. Lasker and A. Lathrop and Li, {T. S.} and M. Manera and M. March and Marshall, {J. L.} and M. Medford and F. Menanteau and I. Mohammed and Monroy, {M. R.} and B. Moraes and Morganson, {E. P.} and J. Muir and M. Murphy and B. Nord and Pace, {A. B.} and A. Palmese and Y. Park and F. Paz-Chinch{\'o}n and Pereira, {M. E.S.} and D. Petravick and Plazas, {A. A.} and J. Poh and T. Prochaska and K. Reil and Romer, {A. K.} and A. Roodman and M. Sako and M. Sauseda and D. Scolnic and Secco, {L. F.} and I. Sevilla-Noarbe and N. Shipp and Smith, {J. A.} and M. Soares-Santos and B. Soergel and A. Stebbins and Story, {K. T.} and K. Stringer and F. Tarsitano and B. Thomas and Tucker, {D. L.} and Vivas, {A. K.} and Walker, {A. R.} and Wang, {M. Y.} and C. Weaverdyck and N. Weaverdyck and W. Wester and Wethers, {C. F.} and R. Wilkinson and Wu, {H. Y.} and B. Yanny and A. Zenteno and Y. Zhang",

note = "Publisher Copyright: {\textcopyright} 2018 SPIE; Observatory Operations: Strategies, Processes, and Systems VII 2018 ; Conference date: 11-06-2018 Through 15-06-2018",

year = "2018",

doi = "10.1117/12.2312113",

language = "English (US)",

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

publisher = "SPIE",

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

booktitle = "Observatory Operations",

address = "United States",

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TY - GEN

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T2 - Observatory Operations: Strategies, Processes, and Systems VII 2018

AU - Diehl, H. T.

AU - Neilsen, E.

AU - Gruendl, R. A.

AU - Abbott, T. M.C.

AU - Allam, S.

AU - Alvarez, O.

AU - Annis, J.

AU - Balbinot, E.

AU - Bhargava, S.

AU - Bechtol, K.

AU - Bernstein, G. M.

AU - Bhatawdekar, R.

AU - Bocquet, S.

AU - Brout, D.

AU - Capasso, R.

AU - Cawthon, R.

AU - Chang, C.

AU - Cook, E.

AU - Conselice, C. J.

AU - Cruz, J.

AU - D’Andrea, C.

AU - Da Costa, L.

AU - Das, R.

AU - DePoy, D. L.

AU - Drlica-Wagner, A.

AU - Elliott, A.

AU - Everett, S. W.

AU - Frieman, J.

AU - Fausti Neto, A.

AU - Ferté, A.

AU - Friswell, I.

AU - Furnell, K. E.

AU - Gelman, L.

AU - Gerdes, D. W.

AU - Gill, M. S.S.

AU - Goldstein, D. A.

AU - Gruen, D.

AU - Gulledge, D. J.

AU - Hamilton, S.

AU - Hollowood, D.

AU - Honscheid, K.

AU - James, D. J.

AU - Johnson, M. D.

AU - Johnson, M. W.G.

AU - Kent, S.

AU - Kessler, R.

AU - Khullar, G.

AU - Kovacs, E.

AU - Kremin, A.

AU - Kron, R.

AU - Kuropatkin, N.

AU - Lasker, J.

AU - Lathrop, A.

AU - Li, T. S.

AU - Manera, M.

AU - March, M.

AU - Marshall, J. L.

AU - Medford, M.

AU - Menanteau, F.

AU - Mohammed, I.

AU - Monroy, M. R.

AU - Moraes, B.

AU - Morganson, E. P.

AU - Muir, J.

AU - Murphy, M.

AU - Nord, B.

AU - Pace, A. B.

AU - Palmese, A.

AU - Park, Y.

AU - Paz-Chinchón, F.

AU - Pereira, M. E.S.

AU - Petravick, D.

AU - Plazas, A. A.

AU - Poh, J.

AU - Prochaska, T.

AU - Reil, K.

AU - Romer, A. K.

AU - Roodman, A.

AU - Sako, M.

AU - Sauseda, M.

AU - Scolnic, D.

AU - Secco, L. F.

AU - Sevilla-Noarbe, I.

AU - Shipp, N.

AU - Smith, J. A.

AU - Soares-Santos, M.

AU - Soergel, B.

AU - Stebbins, A.

AU - Story, K. T.

AU - Stringer, K.

AU - Tarsitano, F.

AU - Thomas, B.

AU - Tucker, D. L.

AU - Vivas, A. K.

AU - Walker, A. R.

AU - Wang, M. Y.

AU - Weaverdyck, C.

AU - Weaverdyck, N.

AU - Wester, W.

AU - Wethers, C. F.

AU - Wilkinson, R.

AU - Wu, H. Y.

AU - Yanny, B.

AU - Zenteno, A.

AU - Zhang, Y.

PY - 2018

Y1 - 2018

N2 - The Dark Energy Survey (DES) is an operating 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 has completed its third observing season out of a nominal five. This paper describes DES “Year 4” (Y4) and “Year 5” (Y5), the survey strategy, an outline of the survey operations procedures, the efficiency of operations and the causes of lost observing time. It provides details about the quality of these two-season's data, a summary of the overall status, and plans for the final survey season.

AB - The Dark Energy Survey (DES) is an operating 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 has completed its third observing season out of a nominal five. This paper describes DES “Year 4” (Y4) and “Year 5” (Y5), the survey strategy, an outline of the survey operations procedures, the efficiency of operations and the causes of lost observing time. It provides details about the quality of these two-season's data, a summary of the overall status, and plans for the final survey season.

KW - CTIO

KW - Cosmology

KW - Dark Energy Camera

KW - Dark Energy Survey

KW - Operations

UR - http://www.scopus.com/inward/record.url?scp=85050820310&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=85050820310&partnerID=8YFLogxK

U2 - 10.1117/12.2312113

DO - 10.1117/12.2312113

M3 - Conference contribution

AN - SCOPUS:85050820310

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

BT - Observatory Operations

A2 - Seaman, Robert L.

A2 - Peck, Alison B.

A2 - Benn, Chris R.

PB - SPIE

Y2 - 11 June 2018 through 15 June 2018

ER -

The Dark Energy Survey and operations: Years 4 and 5

Abstract

Publication series

Conference

Bibliographical note

Keywords

Publisher link

Find It

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