MIRIS observation of near-infrared diffuse Galactic light

• Published in: Publications of the Astronomical Society of Japan 2018-08, Vol.70 (4)
• Main Authors: Onishi, Yosuke, Sano, Kei, Matsuura, Shuji, Jeong, Woong-Seob, Pyo, Jeonghyun, Kim, Il-Jong, Seo, Hyun Jong, Han, Wonyong, Lee, DaeHee, Moon, Bongkon, Park, Wonkee, Park, Younsik, Kim, MinGyu, Matsumoto, Toshio, Matsuhara, Hideo, Nakagawa, Takao, Tsumura, Kohji, Shirahata, Mai, Arai, Toshiaki, Ienaka, Nobuyuki
• Format: Article
• Language: English
• ISSN: 0004-6264; 2053-051X
• DOI: 10.1093/pasj/psy070

We report near-infrared (IR) observations of high Galactic latitude clouds to investigate diffuse Galactic light (DGL), which is starlight scattered by interstellar dust grains. The observations were performed at 1.1 and 1.6 μm with a wide-field camera instrument, the Multi-purpose Infra-Red Imaging System (MIRIS) onboard the Korean satellite STSAT-3. The DGL brightness is measured by correlating the near-IR images with a far-IR 100 μm map of interstellar dust thermal emission. The wide-field observation of DGL provides the most accurate DGL measurement achieved to-date. We also find a linear correlation between optical and near-IR DGL in the MBM32 field. To study interstellar dust properties in MBM32, we adopt recent dust models with and without μm-sized very large grains and predict the DGL spectra, taking into account the reddening effect of the interstellar radiation field. The result shows that the observed color of the near-IR DGL is closer to the model spectra without very large grains. This may imply that dust growth in the observed MBM32 field is not active owing to the low density of its interstellar medium.