CCD PSF and LP Filter Curve Calibration

Details CCD PSF and LP Filter Curve Calibration CCD PSF and LP Filter Curve Calibration

Jul 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001hst..prop.8924p&link_type=abstract

HST Proposal ID #8924

Physics

Hst Proposal Id #8924

Scientific paper

To tie dow the wavelength dependence of the CCD imaging sensitivity, it is necessary to have good photometric imaging data in both 50CCD and F28X50LP for stars of a variety of colors for which the spectral energy distribution is known with great accuracy. To fill in a color gap in the data that meets these requirements, we will obtain STIS spectra of a late F star for which we already have extensive imaging data, and also will obtain both spectra and deep dithered CCD images of an early K star.

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