@inproceedings{oai:jaxa.repo.nii.ac.jp:00020516,
 author = {石黒, 正晃 and 猿楽, 祐樹 and 三浦, 直也 and 臼井, 文彦 and 上野, 宗孝 and Chun, Moo-Young and Kwon, Suk Minn and Ishiguro, Masateru and Sarugaku, Yuki and Miura, Naoya and Usui, Fumihiko and Ueno, Munetaka and Chun, Moo-Young and Kwon, Suk Minn},
 book = {第38回月・惑星シンポジウム, Proceedings of the 38th ISAS Lunar and Planetary Symposium},
 month = {Mar},
 note = {Cometary dust trails are composed of large debris ejected from periodic comets. They were first detected in optical wavelength by our group using Kiso 1.05-m Schmidt. The sophisticated data reduction processes as well as the advanced instruments are increasing the total number of trail comets to 15, testifying to the ability of the ground-based observations to achieve the present studies. In this paper, we describe the progress report on the cometary dust trail survey by three ground-based telescopes. In addition, we present the optical color measured under the photometric conditions on Mauna Kea, Hawaii., 資料番号: AA0063350001},
 pages = {1--4},
 publisher = {宇宙航空研究開発機構宇宙科学研究本部, Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA/ISAS)},
 title = {Dark red debris from short-period comets: Summary of dust trail survey and its optical color},
 year = {2006}
}