Monochromatic PSF in the red

Details Monochromatic PSF in the red Monochromatic PSF in the red

Jul 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004hst..prop10720r&link_type=abstract

HST Proposal ID #10720

Physics

Hst Proposal Id #10720

Scientific paper

This is a request to use 1 orbit, the last in Cycle 13 of the ACS calibration contingency pool, to characterize the monochromatic PSF in the red. For programs which need to do careful photometry in the F850lp filter this is sorely needed. The problem is that f850lp contains a superposition of monochromatic PSFs in the region where its shape is changing rapidly. A catalog of monochromatic PSFs would be useful to produce the appropriate superposition seen in f850lp. The idea is this program is to use the ramp filters, FR853N, FR931N, FR1016N to step a bright star every 200 Angstroms or so, using the dither box pattern at each wavelength. The measurements can be done in a single orbit and are best done soon {in 3 gyro mode if possible}.

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