STIS02: CCD Functional for SMOV3a

Details STIS02: CCD Functional for SMOV3a STIS02: CCD Functional for SMOV3a

Jul 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999hst..prop.8502g&link_type=abstract

HST Proposal ID #8502

Computer Science

Performance

Hst Proposal Id #8502

Scientific paper

This activity measures the baseline performance and commandability of the CCD subsystem. Only primary amplifier D is used. Bias, Dark, and Flat Field exposures are taken in order to measure read noise, dark current, CTE, and gain. Numerous bias frames are taken to permit construction of "superbias" frames in which the effects of read noise have been rendered negligible. Dark exposures are made outside the SAA. Full frame and binned observations are made, with binning factors of 1 x 1 and 2 x 2. Finally, tungsten lamp exposures are taken through narrow slits to confirm the slit positions in the current database after SM3a. All exposures are internals. Bias frames and flats through all Amps were added as a test of the read noise.

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