Exploring the OIII, X-ray and IR Luminosities of Nearby AGN

Details Exploring the OIII, X-ray and IR Luminosities of Nearby AGN Exploring the OIII, X-ray and IR Luminosities of Nearby AGN

Jan 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aas...21541103c&link_type=abstract

American Astronomical Society, AAS Meeting #215, #411.03; Bulletin of the American Astronomical Society, Vol. 42, p.240

Astronomy and Astrophysics

Astronomy

Scientific paper

We have gathered archival data from the NASA/IPAC Extragalactic Database for a total of 264 nearby Active Galactic Nuclei (AGN), including OIII, IR and X-ray luminosities (see McKernan et al. 2009) Of the 264 AGN only 89 have detected OIII in NED. Our goal is to look for correlations between OIII, IR and X-ray luminosities for AGN in our sample. We are looking at OIII because it has been used as an indicator of AGN activity. This is a continuation of work by Mckernan et al. 2009.

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