Star Formation in Galaxies at 0<z<1.6

Details Star Formation in Galaxies at 0<z<1.6 Star Formation in Galaxies at 0<z<1.6

Jul 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999hst..prop.8380g&link_type=abstract

HST Proposal ID #8380

Mathematics

Logic

Hst Proposal Id #8380 Distant Galaxies

Scientific paper

The installation of STIS on HST has allowed two-dimensional optical and ultraviolet slitless spectroscopy of faint objects from space for the first time. The STIS Parallel Survey {SPS} routinely obtains broad band images and slitless spectra of random fields in parallel with HST observations using other instruments. The SPS is designed to study a wide variety of astrophysical phenomena, including the rate of star formation in galaxies and detection of emission-line galaxies at intermediate to high redshift. We have presented the first results of the SPS in Gardner et al {1998}, which demonstrated the capability of STIS slitless spectroscopy to detect and identify emission-line galaxies. The redshift range of 0.0

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