2008
DOI: 10.1117/12.790053
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Characterization of DECam focal plane detectors

Abstract: DECam is a 520 Mpix, 3 square-deg FOV imager being built for the Blanco 4m Telescope at CTIO. This facility instrument will be used for the "Dark Energy Survey" of the southern galactic cap. DECam has chosen 250 µm thick CCDs, developed at LBNL, with good QE in the near IR for the focal plane. In this work we present the characterization of these detectors done by the DES team, and compare it to the DECam technical requirements. The results demonstrate that the detectors satisfy the needs for instrument.

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Cited by 23 publications
(32 citation statements)
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“…The readout system utilized in these experiments was originally developed for the DECAM project (Dark Energy Camera, [11]) at Fermilab [15,16], that was modified to handle the skipper technology. The CCD, placed in an aluminium dewar and run at 143 • K to diminish dark current generation, was tested at one of the Fermilab's laboratories.…”
Section: Resultsmentioning
confidence: 99%
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“…The readout system utilized in these experiments was originally developed for the DECAM project (Dark Energy Camera, [11]) at Fermilab [15,16], that was modified to handle the skipper technology. The CCD, placed in an aluminium dewar and run at 143 • K to diminish dark current generation, was tested at one of the Fermilab's laboratories.…”
Section: Resultsmentioning
confidence: 99%
“…The vertical and horizontal charge transfer inefficiency measured for several detectors fabricated on high resistivity silicon was found to be less than 1 × 10 −6 [15]. The pixel in the last row and column in the array is the one that experiment the major charge loss; other pixels in the array are less affected because less transfers are needed to displace its charge to the output stage.…”
Section: Fig 15mentioning
confidence: 94%
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“…The measurements were made with the CCD working at approximately 135 K to avoid any spurious generation of charge. At this temperature the dark current contribution is less than a 1e-/pixel/hour and has a negligible effect on the alpha detection [38]. Figure 2 shows an image obtained by exposing the CCD active surface to different ionizing radiations.…”
Section: Introductionmentioning
confidence: 99%