The on-orbit performance of the STIS detectors

Details The on-orbit performance of the STIS detectors The on-orbit performance of the STIS detectors

Jan 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997hstc.work....8k&link_type=abstract

The 1997 HST Calibration Workshop with a New Generation of Instruments, p. 8

Computer Science

Performance

1

Hubble Space Telescope, Multi-Anode Microchannel Arrays, Charge Coupled Devices, Spectrographs, Spectroscopy, Infrared Detectors, Spacecraft Instruments, Imaging Spectrometers, Data Processing, Orbital Servicing, Performance

Scientific paper

The Space Telescope Imaging Spectrograph (STIS), successfully installed into the Hubble Space Telescope in February 1997, achieves its advances over the first-generation HST spectrographs primarily through the use of modern large-format, two-dimensional array detectors. The performance of the STIS detectors, two Multi-Anode Microchannel Arrays (MAMAS) and one CCD, has been evaluated on-orbit as part of the Servicing Mission Orbital Verification (SMOV) program. All three detectors are functioning well. We report highlights of the results to date here.

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