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The Dark Energy Camera

Journal Article · · Astron.J.
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  1. Fermilab
  2. Ohio State U., CCAPP; Ohio State U.
  3. Cerro-Tololo InterAmerican Obs.
  4. University Coll. London
  5. Barcelona, IFAE
  6. Ohio State U.
  7. Pennsylvania U.
  8. Carnegie Inst. Observ.
  9. Michigan U.
  10. Madrid, CIEMAT
  11. Barcelona, IEEC
  12. Rio de Janeiro Observ.
  13. Texas A-M
  14. LBL, Berkeley
  15. Fermilab; Chicago U., KICP
  16. Chicago U., KICP
  17. Illinois U., Urbana
  18. Australian Astron. Observ.
  19. Argonne
  20. SLAC
  21. Barcelona, IFAE; ICREA, Barcelona
  22. Portsmouth U., ICG
  23. Brookhaven; Caltech
  24. KIPAC, Menlo Park; SLAC
The Dark Energy Camera is a new imager with a 2.2-degree diameter field of view mounted at the prime focus of the Victor M. Blanco 4-meter telescope on Cerro Tololo near La Serena, Chile. The camera was designed and constructed by the Dark Energy Survey Collaboration, and meets or exceeds the stringent requirements designed for the wide-field and supernova surveys for which the collaboration uses it. The camera consists of a five element optical corrector, seven filters, a shutter with a 60 cm aperture, and a CCD focal plane of 250 micron thick fully-depleted CCDs cooled inside a vacuum Dewar. The 570 Mpixel focal plane comprises 62 2kx4k CCDs for imaging and 12 2kx2k CCDs for guiding and focus. The CCDs have 15 microns x15 microns pixels with a plate scale of 0.263 arc sec per pixel. A hexapod system provides state-of-the-art focus and alignment capability. The camera is read out in 20 seconds with 6-9 electrons readout noise. This paper provides a technical description of the camera's engineering, construction, installation, and current status.
Research Organization:
Argonne National Laboratory (ANL), Argonne, IL (United States); Australian Astron. Observ.; Barcelona, IEEC; Barcelona, IFAE; Brookhaven National Laboratory (BNL), Upton, NY (United States); Caltech; Carnegie Inst. Observ.; Cerro-Tololo InterAmerican Obs.; Chicago U., KICP; Fermi National Accelerator Laboratory (FNAL), Batavia, IL (United States); ICREA, Barcelona; Illinois U., Urbana; Lawrence Berkeley National Laboratory (LBNL), Berkeley, CA (United States); Madrid, CIEMAT; Michigan U.; Ohio State U.; Ohio State U., CCAPP; Pennsylvania U.; Portsmouth U., ICG; Rio de Janeiro Observ.; SLAC National Accelerator Laboratory (SLAC), Menlo Park, CA (United States); Texas A-M; University Coll. London
Sponsoring Organization:
US Department of Energy; USDOE Office of Science (SC), High Energy Physics (HEP)
Contributing Organization:
The DES Collaboration
Grant/Contract Number:
AC02-07CH11359; AC02-76SF00515
OSTI ID:
1212751
Alternate ID(s):
OSTI ID: 22520108
OSTI ID: 1258494
OSTI ID: 2530171
Report Number(s):
FERMILAB-PUB-15-121-PPD; oai:inspirehep.net:1359376; arXiv:1504.02900
Journal Information:
Astron.J., Journal Name: Astron.J. Vol. 150
Country of Publication:
United States
Language:
English

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