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Multi-slit Improvements and Other Cryogenic Camera News (1Mar96) (from KPNO, NOAO Newsletter No. 45, March 1996) An option for multi-object spectroscopy at the 4-m telescope has been the Cryogenic Camera or R-C Spectrograph with multi-slit entrance masks. For many years we have been using masks made from photographic film. Cryogenic Camera Grisms Grism No. 650 770 810 730 780-1 780-1 780-2 Order 1 1 1 1 1 2 1 l/mm 400 300 150 300 300 300 300 UDCW*(Angstrom) 4950 5970 6360 8010 9700 4850 7100 Spectral Range 4000 4000 4000 5600 7200 4000 4900 -6900 -8400 -10500 -10400 -10300 -6300 -9700 Resolution 12 15 30 15 15 8 15 (in Angstroms) Angstroms/pixel 3.2 4.3 9.1 4.3 4.3 2.2 4.3 * Undeviated central wavelength We have now developed a new technique using thin etched stainless steel for the mask material. This offers several improvements over the old film method. The chief detraction of the photographic masks was a 10% throughput loss in the film base material. Other problems, now alleviated, were occasional scale errors due to drifts in the film recorder electronics and internal fringing in the film base. All of these deficiencies are now removed with the new blackened metal masks. The only downside factor is cost and lead time. The new masks will cost several hundred dollars for a typical observing run. For most runs, with a reasonable number of masks, KPNO will absorb this cost. If more masks for a run than the norm are requested, the observer may be asked to share the cost. Since an outside vendor is doing the etching, the lead time for receipt of the final mask patterns from the observer will be increased to three weeks. There have been two successful runs using the new material. Photographic masks will no longer be available. Potential users are referred to the manual "Multi-Slits at Kitt Peak" available via anonymous ftp from ftp.noao.edu or from the KPNO Home Page http://www.noao.edu. During recent runs the CryoCam has performed well and the reliability has been excellent. The current chip, a Ford/Loral 800 x 1200 pixel device with 15 um pixel size, offers good cosmetics with a readout noise of ~15e-rms. Past instabilities in the readout noise characteristics have been fixed. Above is a table giving the instrumental specifications for the various grisms. Some grisms can cover more than one harmonic in wavelength and users must choose their order blocking filters with care. Jim De Veny, Buell Jannuzi
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