Initial FUSE Results on Active Galactic Nuclei

Details Initial FUSE Results on Active Galactic Nuclei Initial FUSE Results on Active Galactic Nuclei

Dec 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999aas...195.0617k&link_type=abstract

American Astronomical Society, 195th AAS Meeting, #06.17; Bulletin of the American Astronomical Society, Vol. 31, p.1376

Astronomy and Astrophysics

Astronomy

Scientific paper

The excellent throughput and low background rates of FUSE enable observations of many dozens of AGN at wavelengths shortward of 1200 Angstroms. Early FUSE observations of AGN include ESO141--G55, PG0052+251, PG0804+761, VII Zw 118, H1821+64, Mrk 352, Mrk 876, and HS 1700+64. In contemporaneous observing programs, we are also obtaining longer-wavelength UV spectra with HST/STIS covering 1150--3200 Angstroms, and ground-based spectra from the atmospheric limit to 1 μ m, for many of the FUSE program objects. We will discuss the intrinsic properties of the observed AGN and show sample spectral energy distributions covering the 912--10,000 Angstroms observed wavelength range. This work is supported by NASA contract NAS5-32985.

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