IRAS observations of AGN candidates at low flux levels

Details IRAS observations of AGN candidates at low flux levels IRAS observations of AGN candidates at low flux levels

May 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987nascp2466..693d&link_type=abstract

Star formation in galaxies, Proceedings of a conference at the California Institute of Technology, Pasadena, California, June 16

Astronomy and Astrophysics

Astronomy

Active Galactic Nuclei, Faint Objects, Galactic Evolution, Point Sources, Radiant Flux Density, Star Formation, Infrared Astronomy, Infrared Astronomy Satellite, Infrared Spectra, Red Shift, Seyfert Galaxies, Stellar Color

Scientific paper

IRAS additional observations were used to obtain a sample of point sources at much fainter flux levels than hitherto available through the IRAS Point Source Catalogue. This sample is being used to compile an incomplete but representative catalogue of faint IRAS candidate Active Galactic Nuclei (AGNs) and to study the evolution of the infrared bright galaxies. Ground based follow up observations (optical spectroscopy) are mainly hampered by identification confusion.

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