Observing Elliptical Galaxies with IPCS

Details Observing Elliptical Galaxies with IPCS Observing Elliptical Galaxies with IPCS

Mar 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980msngr..20....8u&link_type=abstract

The Messenger, No.20, P. 8, 1980

Physics

Scientific paper

The Image Photon Counting System (IPCS) developed in the early 1970's at University College London by Dr. A. Boksenberg and collaborators (A. Boksenberg, 1972 in Auxiliary Instrumentation for Large Telescapes, proceedings of ESO/CERN Conference, p. 295; A. Boksenberg and D. E. Burgess, 1972 in Adv. in Electronics and Electron Physics, 33B p. 285) is a two-dimensional detector. It has been used on the ESO 3.6-m telescope at La Silla to observe spectrographically a variety of faint astronomical objects: extended objects, in particular regions of galaxies outside the nucleus, nebulosities associated with active nuclei, etc., and star-like objects such as quasars or halo stars.

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