Observations of extrasolar planets by the transit method

DOI

Bibliographic Information

Other Title
  • トランジット法による系外惑星観測

Description

We have observed the extrasolar planets by transit method. The method is to observe light intensity when a planet is crossing in front of the star. However, the errors of light intensity were large, so that we could not find the information of extraplanets such as orbital parameters. In the paper, we clarify the reason of large error and report the new method to reduce the error.

Journal

Details 詳細情報について

  • CRID
    1390001205558558080
  • NII Article ID
    130004636058
  • DOI
    10.14909/jsps.2006f.0.134.0
  • Data Source
    • JaLC
    • CiNii Articles
  • Abstract License Flag
    Disallowed

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