Imaging and Spectrophotometry of NGC1566

Details Imaging and Spectrophotometry of NGC1566 Imaging and Spectrophotometry of NGC1566

Jul 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990hst..prop.3050f&link_type=abstract

HST Proposal ID #3050

Computer Science

Hst Proposal Id #3050 Quasars &Amp, Agn

Scientific paper

Narrow band [O III] 5007A, nearby offband, and UV continuum PC images will be used to resolve the narrow and broad line regions. These data will test the ability to resolve the narrow regions of Seyfert 1 galaxies in the vicinity of a bright unresolved nucleus. Small aperture FOS spectra of the nucleus will be used to determine how well the emission from the broad line region can be separated from the narrow line region given the degraded spatial resolution. The spectra will be compared to published ground-based (optical) and IUE (ultraviolet) spectrophhotometry of the nucleus.

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