Ienaka, NKawara, KimiakiMatsuoka, YSameshima, HOyabu, STsujimoto, TakujiPeterson, Bruce2015-12-130004-637Xhttp://hdl.handle.net/1885/74340We have conducted B-, g-, V-, and R-band imaging in a 45′ × 40′ field containing part of the high Galactic latitude translucent cloud MBM32, and correlated the intensity of diffuse optical light S ν(λ) with that of 100 μm emission S ν(100 μm). AAuthor/s retain copyrightKeywords: diffuse radiation; dust, extinction; infrared: ISM; ISM: clouds; ISM: individual objects (MBM32); scattering201310.1088/0004-637X/767/1/802016-02-24