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The Ohio State University College of Mathematical & Physical Sciences Department of Astronomy |
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OSMOS (Ohio State MultiObject Spectrograph) is a wide field imager and multiobject spectrograph under construction for the 2.4m Hiltner telescope at the MDM Observatory. OSMOS employs an all-refractive, zero-deviation design to produce a plate scale of 0.3"/pixel and a 20' diameter FOV onto the MDM 4k detector system. Slits will be laser cut into spherical, NicAlloy masks that match the 2.4m focal surface. Up to 50 to 100 slitlets should be feasible. In addition, numerous long slit options will be available. The initial complement of dispersing elements will include a very low resolution triple prism and a high-efficiency, low-resolution VPH grism (the details are still TBD). The disperser wheel has sufficient space for mounting up to five dispersing elements and potential users interested in other dispersers should contact Paul Martini. The planned completion date for OSMOS is the end of 2009 with commissioning in early 2010.
Nov 6, 2009: The OSMOS enclosure design is complete and ordered. The parts are expected by the end of December.
May 8, 2009: The OSMOS collimator and camera lens barrels have arrived!
February 27, 2009: The OSMOS collimator and camera lens barrels have been completed. Acceptance testing at Coastal Optical Systems is scheduled for mid March.
January 27, 2009: The OSMOS triple prism disperser arrived today from Coastal Optical Systems. Follow the links for an image of the prism and a demonstration of zero deviation.
December 19, 2008: Assembly and testing of the double filter wheel was completed today with the lab electronics. Follow the link to a recent picture of the filter wheels and slit wheel.
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Updated: 2010 January 28 [pm]