Possible coordinate observations by MAXI and the AROMA wide-field optical monitor

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説明

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

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詳細情報 詳細情報について

  • CRID
    1050011086285859968
  • NII論文ID
    120006828775
  • NII書誌ID
    AA11984031
  • ISSN
    1349113X
  • Web Site
    http://id.nii.ac.jp/1696/00005300/
  • 本文言語コード
    en
  • 資料種別
    conference paper
  • データソース種別
    • IRDB
    • CiNii Articles

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