@inproceedings{oai:jaxa.repo.nii.ac.jp:00005306,
 author = {吉田, 篤正 and 中川, 友進 and Takahashi, I. and Uehara, T. and Yamazaki, O. and Shiraki, T. and Kojima, T. and Yoshida, Atsumasa and Nakagawa, Yujin E.},
 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), In order to observe the early optical afterglows of GRBs, we have developed and operated the automatic telescope Aoyama Gakuin University Robotic Optical Monitor for Astrophysical objects (AROMA). It currently consists of amateur-oriented astronomical instruments to conduct immediate and automatic follow-up observations and analyses of the GRB optical afterglows. In order to expand the scope of AROMA, a development of an observation system using multiple digital single-lens reflex cameras (AROMA-W) is underway. The new function of AROMA can achieve simultaneous observations in multiple optical bands with a wide field of view. The software which analyzes massive amounts of imaging data automatically was also under development. Finally we aim at discoveries of the optical transients by monitoring all the stars which are visible in an AROMA-W view. We report a developmental status of AROMA-W and a possibility of the simultaneous observation to the X-ray transients (e.g., X-ray nova, Supernova) discovered with MAXI., 資料番号: AA0064306067, レポート番号: JAXA-SP-08-014E},
 pages = {348--353},
 publisher = {宇宙航空研究開発機構, Japan Aerospace Exploration Agency (JAXA)},
 title = {Possible coordinate observations by MAXI and the AROMA wide-field optical monitor},
 volume = {JAXA-SP-08-014E},
 year = {2009}
}