@article{oai:jaxa.repo.nii.ac.jp:00036688,
 author = {Woong-Seob, JEONG and Soojong, PAK and Hyung, Mok  Lee and Sam, KIM and Mikako, MATSUURA and Takao, NAKAGAWA and Issei, YAMAMURA and Hiroshi, MURAKAMI and Shuji, MATSUURA and Mitsunobu, KAWADA and Hidehiro, KANEDA and Hiroshi, SHIBAI},
 journal = {The Institute of Space and Astronautical Science report. S.P. : Mid- and Far-Infrared Astronomy and Future Space Mission},
 month = {Dec},
 note = {The Far-Infrared Surveyor (FIS) is one of the on-board instruments on the ASTRO-Fsatellite, which will be launched in early 2004. The first a half year of its mission period of 500days is dedicated to an all sky survey in four bands between 50 and 200μm. On the basis of thepresent hardware specfications and configurations of the FIS, we have written a computer programto simulate the FIS. The program can be used to evaluate the performance of the instrument aswell as to produce input for the data reduction system. In this paper, we describe the currentstatus of the program. As an example of the usage of the simulation program, we present theexpected observing data for three different detector sampling rates. The functions which shouldbe implemented into the program, in the future, are enumerated., 資料番号: SA4597881000},
 pages = {297--304},
 title = {Simulations of Observations with the Far-Infrared Surveyor: Design Overview and Current Status},
 volume = {14},
 year = {2000}
}