Deep Imaging of Extended Optical Structure around the Quasar 4C37.43

Details Deep Imaging of Extended Optical Structure around the Quasar 4C37.43 Deep Imaging of Extended Optical Structure around the Quasar 4C37.43

Jul 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996hst..prop.6490s&link_type=abstract

HST Proposal ID #6490

Physics

Hst Proposal Id #6490 Agn

Scientific paper

Essentially all imaging of low-redshift QSO host galaxies in Cycle 4 and Cycle 5 programs has been of a survey nature, with relatively short exposures on a large number of objects. Particularly in view of the uncertainties and questions that have arisen as a result of these survey programs, we feel that it is essential to carry out deep imaging of a few critical fields in bandpasses matched to the objects' spectral properties. We propose here such observations of 4C37.43 Specifically, we will obtain {1} deep WFC images in a continuum band between [O III] Lambda5007 and HAlpha, {2} PC images, in the same band, with exposures calculated to avoid saturation on the quasar, to give good resolution of the immediate nuclear environment, and {3} deep narrow-band {linear ramp filter} images, centered on O III Lambda5007. 4C37.43 has the most luminous extended emission region of any low-redshift QSO.

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