HS1543+5921 - a Bright QSO Behind SBS1543+593

Details HS1543+5921 - a Bright QSO Behind SBS1543+593 HS1543+5921 - a Bright QSO Behind SBS1543+593

Jul 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000hst..prop.8485j&link_type=abstract

HST Proposal ID #8485

Physics

Hst Proposal Id #8485

Scientific paper

To determine its flux in the NUV and FUV, we will observe the QSO HS1543+5921 {z = 0.807} for 1 orbit with STIS in the G140L and G230L modes. This QSO is potentially very interesting since it is directly behind the extended spiral galaxy SBS1543+593 at z = 0.009. However, its ultraviolet flux is currently unknown, and it could be severely depressed by an intervening absorption system between the redshift of the galaxy and the redshift of the QSO. This observation will enable a more reliable assessment of whether or not this QSO is well-suited for future UV spectroscopy with HST.

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