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CASIMIR, The Caltech airborne submillimeter interstellar medium investigations receiver

Edgar, Michael L. and Karpov, Alexandre and Lin, Sean and Miller, David and Radford, Simon J. E. and Zmuidzinas, Jonas (2008) CASIMIR, The Caltech airborne submillimeter interstellar medium investigations receiver. In: Millimeter and Submillimeter Detectors and Instrumentation for Astronomy IV. Proceedings of SPIE. No.7020. Society of Photo-optical Instrumentation Engineers (SPIE) , Bellingham, WA, Art. No. 702012. ISBN 9780819472304. https://resolver.caltech.edu/CaltechAUTHORS:20180802-142536503

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Abstract

CASIMIR, the Caltech Airborne Submillimeter Interstellar Medium Investigations Receiver is a multiband, far infrared and submillimeter, high resolution, heterodyne spectrometer under development for SOFIA. It is a first generation, PI class instrument. CASIMIR is designed for detailed, high sensitivity observations of warm (100 K) interstellar gas both in external galaxies and Galactic sources, including molecular clouds, circumstellar envelopes, and protostellar cores. Combining the 2.5 m SOFIA mirror with state of the art superconducting mixers, will give CASIMIR unprecedented sensitivity. Initially, CASIMIR will have two bands, at 1000 and 1250 GHz, and a further three bands, 550, 750, 1400 GHz, will be added soon after. Any four bands will be available on each flight. The availability of multiple bands during each flight will allow for efficient use of flight time. For example, searches for weak lines from rare species in bright sources can be carried out on the same flight with observations of abundant species in faint or distant objects.


Item Type:Book Section
Related URLs:
URLURL TypeDescription
https://doi.org/10.1117/12.790121DOIArticle
ORCID:
AuthorORCID
Miller, David0000-0001-6099-0614
Additional Information:© 2008 Society of Photo-Optical Instrumentation Engineers (SPIE). Various subsystems of the CASIMIR instrument have been or continue to be developed by a number of people at several institutions: H. G. Le Duc, Micro Devices Lab, JPL (mixer fabrication), N. R., M. R. Haas, NASA Ames (optics), the Kosma I/O Team, U. of Köln and S. W. Colgan, NASA Ames (software). The development of CASIMIR is supported by NASA/USRA SOFIA Instrument Development Fund.
Funders:
Funding AgencyGrant Number
NASAUNSPECIFIED
Universities Space Research AssociationUNSPECIFIED
Subject Keywords:heterodyne, spectrometer, FIR/submm, SOFIA
Series Name:Proceedings of SPIE
Issue or Number:7020
Record Number:CaltechAUTHORS:20180802-142536503
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20180802-142536503
Official Citation:Michael L. Edgar, Alexandre Karpov, Sean Lin, David Miller, Simon J. E. Radford, Jonas Zmuidzinas, "CASIMIR, The Caltech airborne submillimeter interstellar medium investigations receiver", Proc. SPIE 7020, Millimeter and Submillimeter Detectors and Instrumentation for Astronomy IV, 702012 (19 July 2008); doi: 10.1117/12.790121; https://doi.org/10.1117/12.790121
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:88529
Collection:CaltechAUTHORS
Deposited By: George Porter
Deposited On:02 Aug 2018 22:01
Last Modified:03 Oct 2019 20:07

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