arXiv · astro-ph/0003387
Submillimeter and Far-InfraRed Experiment (SAFIRE): A PI class instrument for SOFIA
Abstract
SAFIRE is a versatile imaging Fabry-Perot spectrograph covering 145 to 655 microns, with spectral resolving powers ranging over 5-10,000. Selected as a "PI" instrument for the airborne Stratospheric Observatory for Infrared Astronomy (SOFIA), SAFIRE will apply two-dimensional pop-up bolometer arrays to provide background-limited imaging spectrometry. Superconducting transition edge bolometers and SQUID multiplexers are being developed for these detectors. SAFIRE is expected to be a "First Light" instrument, useable during the initial SOFIA operations. Although a PI instrument rather than a "Facility Class" science instrument, it will be highly integrated with the standard SOFIA planning, observation, and data analysis tools.
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R. A. Shafer, S. H. Moseley, Jr., P. A. R. Ade, D. J. Benford, G. Bjoraker, E. Dwek, D. A. Neufeld, F. Pajot, T. G. Phillips, G. J. Stacey. 2000-03-24. Submillimeter and Far-InfraRed Experiment (SAFIRE): A PI class instrument for SOFIA. https://doi.org/10.1117/12.389126
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