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CCD News (1Mar96) (from CTIO, NOAO Newsletter No. 45, March 1996) The Loral 1K CCD was successfully used for a month-long block (14 November-13 December) with the 1.5-m spectrograph, and has allowed us to retire definitely the small EEV CCD previously used for this application. With this upgrade, we are now scheduling a total of six CCDs (four Tek's and two Loral's). The two Loral CCDs are dedicated: the 3K (3072 x 1024) is in an Air Schmidt camera, which is used with the 4-m spectrographs (R-C, Echelle, Argus), while the 1K (1200 x 800) is used only with the 1.5-m spectrograph. Two of the four Tek (SITe) 2048 x 2048 CCDs are normally dedicated to imaging, the Tek/STIS 2K at the Schmidt and the Tek 2K #3 at the 0.9-m. Tek 2K #4 is used for imaging at the 4-m and 1.5-m, with the 4-m Echelle long camera, and with the 1.5-m bench echelle, while the Tek 1K (1024 x 1024) is used with the Rutgers Fabry-Perot (RFP) Interferometer and for some 1.5-m imaging applications. Very recently we purchased another SITe 2K, from SITE's year-end half-price (!) sale. This is a grade 1 CCD with two amplifiers operative, and is intended for use in a new spectrograph camera that will be used with the fiber spectrograph Argus and eventually with Hydra. In the meantime, we will install the new CCD in a direct dewar; its availability will ease the job of scheduling. The RFP will likely use a Tek 2K in future, since read noise is lower than for our Tek 1K, even though the large format is not needed. The Tek 1K should be scheduled only infrequently. Here is a brief summary of the CCDs presently scheduled. Visit the CCD section via WWW to find out further information, or contact the under-signed. CCD Type Pix N RON QE (%) 0.3 0.4 0.6 0.8 0.9 Tek 2K #3 B 24 4 2-4 20 60 75 60 35 Tek 2K #4 B 24 4 2-4 20 60 75 60 35 Tek/STIS 2K F 21 4 2-4 20 18 40 35 14 Tek 1K B 24 4 2-4 0 35 70 60 35 Loral 3K B 15 1 7-9 70 75 90 75 40 Loral 1K B 15 2 7-9 20 60 95 80 50 Type: B = back-illuminated, F = front-illuminated + Metachrome. Pix: Pixel size in um. N: Number of operative amplifiers. The Tek 2K's are normally read out using all amplifiers, typical read time is 30-40 seconds depending on gain setting. RON: Read noise (e- rms) for the typical range of gains used. QE: Wavelengths are in m. The Loral CCDs are UV-flooded, there is some concern at present that the QE of the Loral 3K CCD in the UV may not be as high as stated. Alistair Walker
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