STIS-24 NUV MAMA Spectroscopic Image Quality

Physics

Scientific paper

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Scientific paper

A point source will be placed at three locations along the 52X0.1 aperture to measure alignment of the slit with telescope offsets. First an exposure will be recorded through the 52X2 aperture. Then at the nominal center of the 52X0.1 aperture, a pattern of seven exposures will be taken spaced at 0.1 arcsec intervals centered on the aperture with Perpendicular to Slit pattern. The pattern done three times, on the nominal aperture center and offset to 2 arcsecs above aperture center {the 52X0.1D1 position} and 2 arcseconds below aperture center.;

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