@inproceedings{oai:jaxa.repo.nii.ac.jp:00005108,
 author = {Urata, Yuji and Huang, K.Y. and Tsai, M. F. and Tang, C.H. and Shen, C.S. and Lin, Y.J and Taiwan PS1TCS team},
 book = {宇宙航空研究開発機構特別資料:, JAXA Special Publication: The Energetic Cosmos; from Suzaku to ASTRO-H},
 month = {Feb},
 note = {The 3rd Suzaku international Conference "Energetic Cosmos : from Suzaku to ASTRO-H" (June 29-July 2, 2009. Grand Park Otaru Hotel), Otaru, Hokkaido Japan, Pan-STARRS (the Panoramic Survey Telescope And Rapid Response System) will be able to scan the visible sky to approximately 23rd magnitude in less than one week. This unique combination of sensitivity and field of view will open many new possibilities in time-domain astronomy and address a wide range of astrophysical problems in the Solar System, the Galaxy, and the Universe. NCU, Taiwan is one of the member of Pan-STARRS Science Consortium (PS1SC). We are working on (1) GRBs (both triggered and orphan events), (2) new type transients, and (3) cross matching of high energy transients detected by Swfit, Fermi, MAXI etc. The cross matching of MAXI and Pan-STARRS transient is one of the standard project of Pan-STARRS (PIs Y.Urata and K.Y. Huang). The main aspects of this cross-identification are (1) Supernova Shock-break out such as SN2008D / XRF090105, (2) Optical identification of X-ray flash., Meeting sponsors: The University of Tokyo, The Institute of Physical and Chemical Research, The Japan Society for the Promotion of Science, 資料番号: AA0064574176, レポート番号: JAXA-SP-09-008E},
 pages = {448--449},
 publisher = {宇宙航空研究開発機構, Japan Aerospace Exploration Agency (JAXA)},
 title = {Optical time domain whole sky survey and Transient/Monitoring science NCU's Pan-STARRS transient cross matching},
 volume = {JAXA-SP-09-008E},
 year = {2010}
}