@inproceedings{oai:jaxa.repo.nii.ac.jp:00005251,
 author = {廣井, 和雄 and 上田, 佳宏 and 江口, 智士 and Hiroi, Kazuo and Ueda, Yoshihiro and Eguchi, Satoshi},
 book = {宇宙航空研究開発機構特別資料, JAXA Special Publication: Astrophysics with All-Sky X-Ray observations: 3rd International MAXI Workshop},
 month = {Feb},
 note = {Astrophysics with All-Sky X-Ray observations: 3rd International MAXI Workshop (RIKEN, 10-12 June 2008), The MAXI source catalog will become a unique database of X-ray populations covering the 0.5-30 keV band in all sky. It will contain more than 1,300 AGNs (Ueda et al. 2009), including many new sources. We develop a software program of source detection of faint sources from MAXI/GSC data, where maximum likelihood fit is performed to a projected image by taking into account the image response and background. In this paper, we present our study to estimate the realistic sensitivities and the position accuracy of MAXI based on simulations., 資料番号: AA0064306012, レポート番号: JAXA-SP-08-014E},
 pages = {54--57},
 publisher = {宇宙航空研究開発機構, Japan Aerospace Exploration Agency (JAXA)},
 title = {MAXI catalog: Source detection and sensitivity},
 volume = {JAXA-SP-08-014E},
 year = {2009}
}