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Star Formation and AGN Activity in Galaxies Classified Using the 1.6 µm Bump and PAH Features at z = 0.4-2
DOI: 10.1093/pasj/64.4.70 Bibcode: 2012PASJ...64...70H

Goto, Tomotsugu; Oyabu, Shinki; Ohyama, Youichi +17 more

We studied the star-formation and AGN activity of massive galaxies in the redshift range $ z$ $ =$ 0.4-2, which were detected in a deep survey field using the AKARI InfraRed (IR) astronomic…

2012 Publications of the Astronomical Society of Japan
AKARI 33
Multi-Wavelength Photometric and Polarimetric Observations of the Outburst of 3C 454.3 in 2009 December
DOI: 10.1093/pasj/64.3.58 Bibcode: 2012PASJ...64...58S

Fukazawa, Yasushi; Sakon, Itsuki; Sasada, Mahito +11 more

In 2009 December, the bright blazar 3C 454.3 exhibited a strong outburst in the optical, X-ray, and gamma-ray regions. We performed photometric and polarimetric monitoring of this outburst in the optical and near-infrared bands with TRISPEC and HOWPol attached to the Kanata telescope. We also observed this outburst in the infrared band with AKARI,…

2012 Publications of the Astronomical Society of Japan
AKARI 18
Processing of Polycyclic Aromatic Hydrocarbons in Molecular-Loop Regions near the Galactic Center Revealed by AKARI
DOI: 10.1093/pasj/64.2.25 Bibcode: 2012PASJ...64...25K

Oyabu, Shinki; Onaka, Takashi; Yamagishi, Mitsuyoshi +7 more

We present an AKARI mid-infrared diffuse map of an area of about 4° × 3° near the Galactic center in the 9 µm band. The band intensity is mostly attributed to aromatic hydrocarbon infrared emissions of carbonaceous grains at wavelengths of 6.2, 7,7, 8.6, and 11.3 µm. We detected 9 µm emission structures extending from the Galacti…

2012 Publications of the Astronomical Society of Japan
AKARI 12
Slow-Scan Observations with the Infrared Camera (IRC) aboard AKARI
DOI: 10.1093/pasj/64.6.126 Bibcode: 2012PASJ...64..126T

Oyabu, Shinki; Yamamura, Issei; Takita, Satoshi +6 more

We present the characterization and calibration of the slow-scan observation mode of the Infrared Camera (IRC) aboard AKARI. The IRC Slow-scan observations were operated at the S9W (9µm) and L18W (18µm) bands. We developed a toolkit for data reduction of the IRC Slow-scan observations. We introduced a "self-pointing reconstruction" met…

2012 Publications of the Astronomical Society of Japan
AKARI 7