Relationship Between Black Hole Mass and Their Infrared Brightness to Synchrotron Radio Emission Ratio

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The objective of this proposal is to see whether there is a correlation between the central black hole masses of nearby AGN and the ratio of their radio to infrared flux. Spitzer will image the AGN in the 3.6 to 8um range and that will be compared to data gathered by the GAVRT students in the S and X radio bands. Once the data is in hand a comparison can be made of the thermal processes generating the IR and the non-thermal processes generating the radio, and whether the ratio of the thermal to the non-thermal is related to the masses of the black holes.

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