@inproceedings{oai:jaxa.repo.nii.ac.jp:00003040,
 author = {川良, 公明 and 佐野, 圭 and 家中, 信幸 and 松岡, 良樹 and 鮫島, 寛明 and 大薮, 進喜 and Kawara, Kimiaki and Sano, Kei and Ienaka, Nobuyuki and Matsuoka, Yoshiki and Sameshima, Hiroaki and Oyabu, Shinki},
 book = {宇宙航空研究開発機構特別資料, JAXA Special Publication: Proceedings of the SPICA Science Conference from Exoplanets to Distant Galaxies: SPICA's New Window on the Cool Universe},
 month = {Mar},
 note = {SPICA Science Conference from Exoplanets to Distant Galaxies: SPICA's New Window on the Cool Universe (June 18-21, 2013. Ito Hall, the University of Tokyo), Bunkyou-ku, Tokyo, Japan, We have conducted multi-color optical imaging toward a high-Galactic cloud, and correlated the intensity of diffuse optical light to the 100 micrometers intensity S(100 micrometers). A X(exp 2)-minimum technique was employed to fit a linear function of S(100 micrometers) to the observed correlation and derive the slope parameter of the best fit-function delta(DGL)/delta(100 micrometers). Combining our slope values and published ones, we show that the slope parameter values vary from cloud to cloud. Because the slope parameter decreases as S(100 micrometers) increases, we suggest that a non-linear DGL model including a negative quadratic term of S(100 micrometers) be fitted to the observed correlation., 形態: カラー図版あり, Physical characteristics: Original contains color illustrations, 資料番号: AA1730027063, レポート番号: JAXA-SP-17-010E},
 pages = {289--291},
 publisher = {宇宙航空研究開発機構(JAXA), Japan Aerospace Exploration Agency (JAXA)},
 title = {Diffuse Galactic Light in a Field of Translucent Cloud MBM32 at High Galactic Latitude},
 volume = {JAXA-SP-17-010E},
 year = {2018}
}