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Redshift estimation from low-resolution prism SEDs with an NGST MOS
Harry I. Teplitz, Eliot Malumuth, Bruce E. Woodgate +8
We discuss the utility of a low resolution prism as a component of a Multi-Object Spectrometer for NASA's proposed Next Generation Space Telescope (NGST). Low resolution prism spec…
Submillimeter and Far-InfraRed Experiment (SAFIRE): A PI class instrument for SOFIA
R. A. Shafer, S. H. Moseley, P. A. R. Ade +7
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 airb…
Calibrating Array Detectors
D. J. Fixsen, S. H. Moseley, R. G. Arendt
The development of sensitive large format imaging arrays for the infrared promises to provide revolutionary capabilities for space astronomy. For example, the Infrared Array Camera…
Dithering Strategies for Efficient Self-Calibration of Imaging Arrays
Richard G. Arendt, D. J. Fixsen, S. Harvey Moseley
With high sensitivity imaging arrays, accurate calibration is essential to achieve the limits of detection of space observatories. One can simultaneously extract information about…