Mid-IR spectroscopy of Dwarf Seyfert 1s

Computer Science

Scientific paper

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Scientific paper

We propose to observe the low-resolution IRS spectra of a sample of 10 AGN with the smallest known BH mass: <10^6M_{&sun;}. The mid-IR observation of these intermediate BH mass AGN will provide critical information on AGN evolution, including the formation and evolution of the dusty torus. The dust mass of these AGN compare with that of high BH mass AGN could also give us clue on AGN fueling history. The total observation time is 8.3hrs.

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