Asymmetric sub-reflectors for spherical antennas and interferometric observations with an FPGA-based correlator

Hiroshi Takeuchi*, Masaya Kuniyoshi, Tsuneaki Daishido, Kuniyuki Asuma, Nobuo Matsumura, Kazuhiro Takefuji, Kotaro Niinuma, Hajime Ichikawa, Riki Okubo, Akihiro Sawano, Naoya Yoshimura, Fumiyuki Fujii, Keiju Mizuno, Yukinori Akamine

*この研究の対応する著者

    研究成果: Article査読

    16 被引用数 (Scopus)

    抄録

    The Nasu Radio Interferometer, consisting of eight equally spaced, 20-m diameter fixed spherical antennas, was developed for the purpose of surveying unknown variable radio sources at 1.4GHz. An asymmetrical Gregorian sub-reflector was designed and installed on each antenna for the purpose of correcting aberrations caused by the spherical reflector. The total collecting area is 2512 m2 and the field-of-view of each antenna is 0.°6 × 0.°6. In survey observations a spatial-fast Fourier-transform (FFT)-type multi-beam system will be used. We report on the design of spherical reflectors and a digital back-end system, the basic principle of spatial-FFT image forming, and a result of interferometric observations with an FPGA-based digital correlator.

    本文言語English
    ページ(範囲)815-820
    ページ数6
    ジャーナルPublications of the Astronomical Society of Japan
    57
    5
    出版ステータスPublished - 2005

    ASJC Scopus subject areas

    • 天文学と天体物理学
    • 宇宙惑星科学

    フィンガープリント

    「Asymmetric sub-reflectors for spherical antennas and interferometric observations with an FPGA-based correlator」の研究トピックを掘り下げます。これらがまとまってユニークなフィンガープリントを構成します。

    引用スタイル