AKARI Infrared Camera Observations of the 3.3 μm PAH Feature in Swift/BAT AGNs

Angel Castro,Takamitsu Miyaji, Mai Shirahata, Kohei Ichikawa, Shinki Oyabu, David M. Clark, Masatoshi Imanishi, Takao Nakagawa, Yoshihiro Ueda 1Instituto de Astronomia, Universidad Nacional Autonoma de Mexico (UNAM), Ensenada, Baja California, Mexico (mailing address: PO Box 439027, San Diego, CA 92143-9027, USA) 2University of California, San Diego, Center for Astrophysics and Space Sciences, 9500 Gilman Drive, La Jolla, CA 92093-0424, USA 3National Astronomical Observatory of Japan (NAOJ), 2-21-1 Osawa, Mitaka, Tokyo 181-8588, Japan 4Institute of Space and Astronautical Science (ISAS), Japan Aerospace Exploration Agency (JAXA), 3-1-1 Yoshino-dai, Chuo-ku, Sagamihara 252-5210 5Department of Astronomy, Kyoto University, Kitashirakawa-Oiwake-cho, Sakyo-ku, Kyoto 606-8502 6Graduate School of Science, Nagoya University, Furo-cho, Chikusa-ku, Nagoya, Aichi 464-8602, Japan 7Subaru Telescope, 650 North Aohoku Place, Hilo, Hawaii, 96720, USA acastro@astrosen.unam.mx