Sat Observation: Nucleus of a Nearby Normal Galaxy

Details Sat Observation: Nucleus of a Nearby Normal Galaxy Sat Observation: Nucleus of a Nearby Normal Galaxy

Jul 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990hst..prop.3009w&link_type=abstract

HST Proposal ID #3009

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Hst Proposal Id #3009

Scientific paper

Direct images of the nucleus of a nearby early-type galaxy NGC 7457 will be used to assess the utility of WFPC images for deconvolution and other image processing techniques. The galaxy will be imaged with the F555W and F785LP filters. The PSF must be measured once per WF/PC SAT "campaign" or if the mirror position has changed or more than 7 days have passed since the last calibration.

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