@inproceedings{oai:jaxa.repo.nii.ac.jp:00005297,
 author = {Reimer, Olaf},
 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), Since VHE gamma-ray observations made during the H.E.S.S. Galactic Plane Survey revealed for the first time the existence of dozens of extreme particle accelerators in our Galaxy, source identification became a crucial aspect in ground-based high-energy gamma-ray astronomy. Whereas the general problem resembles that of the unidentified EGRET sources, a low-threshold imaging Cherenkov telescope array's superior angular resolution and resulting imaging capability against a drastically reduced diffuse component enables different identification techniques. Given that IC photons at TeV energies originate from seed photons at keV energies, the wide field X-ray imaging capabilities and high duty cycle of the MAXI mission will provide contemporaneous X-ray observations to essentially all VHE gamma-ray observations to come, and might ultimately help to characterize the underlying particle population of these extreme Galactic gamma-ray emitter. Most particular, the so far sparsely probed domain of time dependent high-energy characteristics offered from all-sky monitoring by MAXI will add new perspectives to the exploration of VHE gamma-ray sources., Physical characteristics: Original contains color illustrations, 資料番号: AA0064306058, レポート番号: JAXA-SP-08-014E},
 pages = {294--299},
 publisher = {宇宙航空研究開発機構, Japan Aerospace Exploration Agency (JAXA)},
 title = {The challenge of identifying Galactic TeV sources},
 volume = {JAXA-SP-08-014E},
 year = {2009}
}