activity
20042026
most citedThe Infrared Astronomical Mission AKARI

842 citations · 4.2k across the 82 of their papers we have counts for

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astro-ph.EP2019★ 1 cited

Mid-infrared spectroscopy of zodiacal emission with AKARI/IRC

Aoi Takahashi, Takafumi Ootsubo, Hideo Matsuhara +3

Interplanetary dust (IPD) is thought to be recently supplied from asteroids and comets. Grain properties of the IPD can give us the information about the environment in the proto-s…

astro-ph.EP2018★ 30 cited

Subaru/HiCIAO imaging of LkH 330 - multi-band detection of the gap and spiral-like structures

Taichi Uyama, Jun Hashimoto, Takayuki Muto +56

We present - and -bands observations of the LkH 330 disk with a multi-band detection of the large gap and spiral-like structures. The morphology of the outer disk…

astro-ph.EP2015★ 24 cited

High-resolution 25 μm imaging of the disks around Herbig Ae/Be stars

M. Honda, K. Maaskant, Y. K. Okamoto +12

We imaged circumstellar disks around 22 Herbig Ae/Be stars at 25 μm using Subaru/COMICS and Gemini/T-ReCS. Our sample consists of equal numbers of objects belonging to the two cate…

astro-ph.EP2013★ 19 cited

Low-Resolution Spectrum of the Zodiacal Light with AKARI InfraRed Camera

Kohji Tsumura, Toshio Matsumoto, Shuji Matsuura +3

We present the near- and mid-infrared zodiacal light spectrum obtained with the AKARI Infra-Red Camera (IRC). A catalog of 278 spectra of the diffuse sky covering a wide range of G…

astro-ph.EP2012★ 104 cited

Mid-IR imaging of the transitional disk of HD169142: Measuring the size of the gap

M. Honda, Koen Maaskant, Y. K. Okamoto +14

The disk around the Herbig Ae star HD\,169142 was imaged and resolved at 18.8 and 24.5\,m using Subaru/COMICS. We interpret the observations using a 2D radiative transfer model…

astro-ph.EP2010★ 15 cited

Pre-transitional disk nature of the AB Aur disk

M. Honda, A. K. Inoue, Y. K. Okamoto +12

The disk around AB Aur was imaged and resolved at 24.6\,m using the Cooled Mid-Infrared Camera and Spectrometer on the 8.2m Subaru Telescope. The gaussian full-width at half-max…