Paper
29 June 2006 The Dark Energy Survey instrument design
Author Affiliations +
Abstract
We describe a new project, the Dark Energy Survey (DES), aimed at measuring the dark energy equation of state parameter, w, to a statistical precision of ~5%, with four complementary techniques. The survey will use a new 3 sq. deg. mosaic camera (DECam) mounted at the prime focus of the Blanco 4m telescope at the Cerro-Tololo International Observatory (CTIO). DECam includes a large mosaic camera, a five element optical corrector, four filters (g,r,i,z), and the associated infrastructure for operation in the prime focus cage. The focal plane consists of 62 2K x 4K CCD modules (0.27"/pixel) arranged in a hexagon inscribed within the 2.2 deg. diameter field of view. We plan to use the 250 micron thick fully-depleted CCDs that have been developed at the Lawrence Berkeley National Laboratory (LBNL). At Fermilab, we will establish a packaging factory to produce four-side buttable modules for the LBNL devices, as well as to test and grade the CCDs. R&D is underway and delivery of DECam to CTIO is scheduled for 2009.
© (2006) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
B. Flaugher "The Dark Energy Survey instrument design", Proc. SPIE 6269, Ground-based and Airborne Instrumentation for Astronomy, 62692C (29 June 2006); https://doi.org/10.1117/12.672433
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Cited by 12 scholarly publications.
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KEYWORDS
Charge-coupled devices

Telescopes

Cameras

CCD cameras

Optical filters

Semiconducting wafers

Mirrors

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