STIS-23 FUV MAMA Image Quality

Details STIS-23 FUV MAMA Image Quality STIS-23 FUV MAMA Image Quality

Jul 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008hst..prop11393g&link_type=abstract

HST Proposal ID #11393. Cycle 17

Physics

Scientific paper

This proposal will measure the FUV spectroscopic PSF along the length of a long slit. It will do this by observing a point source with the 52X0.1 aperture and the G140L grating, using a five-point centered Perpendicular-to-Slit dither pattern with 0.1 arcsec spacing to measure centering of the target. This seven-point pattern will be done at three different positions along the length of the aperture, including both the nominal centered aperture position and the D1 aperture position, which is located at a position of low FUV dark current. A single centered exposure will also be taken through the photometric 52X2 aperture to provide a reference for estimating the small slit throughput. Sufficient targets will be provided to allow this test to be executed at any time during the BEA period..;

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