The on-orbit optical performance of STIS

Details The on-orbit optical performance of STIS The on-orbit optical performance of STIS

Jan 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997hstc.work...18b&link_type=abstract

The 1997 HST Calibration Workshop with a New Generation of Instruments, p. 18

Computer Science

Performance

3

Calibrating, Hubble Space Telescope, Spectrographs, Orbital Servicing, Instrument Errors, Imaging Spectrometers, Spacecraft Instruments, Multi-Anode Microchannel Arrays, Onboard Equipment, Near Infrared Radiation, Ultraviolet Radiation, Charge Coupled Devices, Spectral Resolution, Echelle Gratings, Optical Correction Procedure, Alignment, Infrared Detectors, Spatial Resolution, Cameras, Stellar Spectrophotometry

Scientific paper

The Space Telescope Imaging Spectrograph (STIS) is a versatile, general purpose instrument installed aboard the Hubble Space Telescope in February, 1997. During the following Servicing Mission Orbital Verification (SMOV) period, STIS has been made operational and aligned, and initial checkout and calibration completed. The overall optical performance goals have largely been achieved and a summary of these results is presented.

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