@article{oai:mue.repo.nii.ac.jp:00000809,
 author = {FUKUDA, Yoshiyuki and ANZAI, Daisuke and KAMEI, Yuto and Narengerile and OBATA, Akira and MORIYAMA, Shigetaka and HIRAIDE, Katsuki and OGAWA, Izumi and GUNJI, Takahiro and HAYAMI, Ryohei and TSUKADA, Satoru and KUROSAWA, Shunsuke},
 journal = {宮城教育大学紀要, Bulletin of Miyagi University of Education},
 month = {Jan},
 note = {The spectral pulse shape of Cherenkov lights was directly measured by using cosmic muons. The observed decay times for early and late timing were 5.0 and 5.2ns, respectively. They were actually shorter than the time of scintillation lights which were also measured as 9.3ns and 9.2ns, respectively. However we could not see the difference of the rise time between scintillation and Cherenkov lights. This was due to the slow response of our DAQ equipment, photomultiplier and FADC digitizer},
 pages = {183--192},
 title = {Direct measurement of spectral shape of Cherenkov light using cosmic muons},
 volume = {53},
 year = {2019}
}