Characterization of the H1RG detector for NICFPS instrument

Details Characterization of the H1RG detector for NICFPS instrument Characterization of the H1RG detector for NICFPS instrument

Jul 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006spie.6276e..41b&link_type=abstract

High Energy, Optical, and Infrared Detectors for Astronomy II. Edited by Dorn, David A.; Holland, Andrew D.. Proceedings of th

Astronomy and Astrophysics

Astronomy

Scientific paper

We are presenting the preliminary characterization results of the Rockwell Scientific HgCdTe detector array used in the Near Infrared Camera and Fabry-Perot Spectrograph (NIC-FPS). The detector was fabricated to cover the wavelength range from 0.8 to 2.5 microns and is bonded to a Hawaii-1RG multiplexer. This instrument was designed and built at the University of Colorado in Boulder and is used at the Apache Point Observatory's 3.5 meter telescope.

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