@inproceedings{oai:jaxa.repo.nii.ac.jp:00005295,
 author = {Gehrels, Neil},
 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 Swift mission has great synergy with MAXI. Operating together, the two missions will provide sensitive sky monitoring in both the soft and hard X-ray bands. Swift will also provide follow-up observations for sources detected by MAXI. This paper describes the non-GRB capabilities and science of Swift. The mission is made up of the BAT wide-field hard X-ray instrument and the XRT and UVOT focusing narrow-field X-ray and UV-optical telescopes. The BAT continuously observes the hard X-ray sky performing a sensitive survey in the 15 - 350 keV range. It is nearly uniform across the sky and is not affected by absorption for Compton-thin sources. At a sensitivity of 10(exp -11) ergs cm(exp -2) s(exp -1), it was detected ca. 580 sources in 22 months. The XRT performs observations in the 0.2 - 10 keV range of select source fields during GRB and non-GRB pointings. Sensitivities achieved are in the 10(exp -15) to 10(exp -14) erg cm(exp -2) range. The UVOT observes UV and optical fields to a sensitivity of ac. 23 magnitude. Valuable data are obtained from Target of Opportunity observations of transients. To date more that 500 such TOOs have been performed. This paper summarizes the non-GRB capabilities and science of Swift., Physical characteristics: Original contains color illustrations, 資料番号: AA0064306056, レポート番号: JAXA-SP-08-014E},
 pages = {282--286},
 publisher = {宇宙航空研究開発機構, Japan Aerospace Exploration Agency (JAXA)},
 title = {Non-GRB sources observed with Swift},
 volume = {JAXA-SP-08-014E},
 year = {2009}
}