EGRET unidentified source radio observations and performance of receiver gain calibration

Kotaro Niinuma*, Kuniyuki Asuma, Masaya Kuniyoshi, Nobuo Matsumura, Kazuhiro Takefuji, Sumiko Kida, Akihiko Takeuchi, Hajime Ichikawa, Akihiro Sawano, Naoya Yoshimura, Shigehiro Suzuki, Ryosuke Nakamura, Yu Nakayama, Tsuneaki Daishido

*この研究の対応する著者

    研究成果: Article査読

    1 被引用数 (Scopus)

    抄録

    Last year, we have developed the receiver gain calibration system by using Johnson-Nyquist noise, for accuracy flux measurement, because we have been starting radio identification program of transient radio sources, blazars and radio counterpart of The Energetic Gamma Ray Experiment Telescope (EGRET) unidentified γ-ray sources in Waseda Nasu Pulsar Observatory. It is shown that there are a few low correlation data between receiver gain and ambient temperature around receiver for anything troubles of receiver, because we can detect gain and ambient temperature through a day by developed system. Estimated fluctuations of daily data of steady sources decrease by removing low correlation data before analysing. As the result of our analysis by using above system, radio counterpart of EGRET identified source showed fading light-curve for a week.

    本文言語English
    ページ(範囲)223-224
    ページ数2
    ジャーナルJournal of Physics: Conference Series
    31
    1
    DOI
    出版ステータスPublished - 2006 3月 22

    ASJC Scopus subject areas

    • 物理学および天文学一般

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