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Mid-infrared selection of AGN

Martin Haas·Ralf Siebenmorgen·Christian Leipski·Stephan Ott·Barbara Cunow·Helmut Meusinger·Sven Mueller·Rolf Chini·Norbert Schartel
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Abstract

Since a large fraction of active galactic nuclei (AGN) is missed in common UV-excess surveys and is even hard to find in radio, near-IR and X-ray surveys, we have used a new AGN selection technique which is expected to be not affected by extinction. Within the scientific verification of the ISOCAM Parallel Survey at 6.7 micron we have discovered objects with exceptional mid-infrared (MIR) emission. They are essentially not detected on IRAS-ADDSCANs and only very few of them show up in the NVSS and FIRST radio surveys. Various colour criteria of the 6.7 micron data with 2MASS and optical wavebands show that the sources reach more extreme IR colours than the sources in the Hubble Deep Field-South and the ELAIS survey. The comparison with known object types suggests that we have found AGN with a pronounced MIR emission, probably due to circum-nuclear dust. First results from optical spectroscopy of ten candidates corroborate this interpretation showing four AGN, two reddened LINER and four extremely reddened emission-line galaxies with MIR/FIR flux ratios higher than for known pure starburst galaxies. The results will make a significant contribution to the debate on the entire AGN population.

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Martin Haas, Ralf Siebenmorgen, Christian Leipski, Stephan Ott, Barbara Cunow, Helmut Meusinger, Sven Mueller, Rolf Chini, Norbert Schartel. 2004-04-15. Mid-infrared selection of AGN. https://doi.org/10.1051/0004-6361%3A20040143

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