SMOV3a STIS BEA Science {1999 Dec 16-18 launch}

Details SMOV3a STIS BEA Science {1999 Dec 16-18 launch} SMOV3a STIS BEA Science {1999 Dec 16-18 launch}

Jul 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999hst..prop.8530g&link_type=abstract

HST Proposal ID #8530

Astronomy and Astrophysics

Astronomy

Hst Proposal Id #8530

Scientific paper

Use SMOV3a Bright Earth Avoidance time period for science exposures with the STIS CCD. Various kinds of targets are observed: {1} Nearby late-type irregular galaxies {deep 50CCD & F28X50LP images}, reaching 1 mag beyond the RGB peak magnitude. {2} Interacting galaxies {50CCD & F28X50LP images, typically reaching the turn-over absolute magnitude of globular cluster systems}. {3} Deep slitless G750L spectroscopy of an empty, high Galactic latitude field. {4} The region around 2 powerful Radio Galaxies: One at z 1.06 and one at z 1.25, to test the suggested powerful radio galaxy-cluster connection at medium redshift. The proprietary period of the data will only last until after the January 2000 meeting of the American Astronomical Society, when the first post-SM3a HST images will be released to the public.

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