Reliability of radio transients detected in the nasu sky survey

Takahiro Aoki, Tai Tanaka, Kotaro Niinuma, Kazuhiro Takefuji, Sumiko Kida, Ryota Nakao, Naomi Nomura, Kentaro Sugisawa, Tsuneaki Daishido

    研究成果: Article査読

    3 被引用数 (Scopus)

    抄録

    This article reports on the reliability of 11 radio transients detected in the Nasu sky survey. We derived false detection rates and evaluated the statistical significance of each transient source. A single source, labeled WJN J1443+3439, was statistically significant at the 10-5 significance level; the other 10 sources were insignificant. On the basis of this single detection, the sky surface density of live radio transients was estimated to be 2+9 -1.9 × 10-6 deg-2 at a flux density above 3 Jy and a frequency of 1.42 GHz. Since this result is comparable with other survey results and known transients, WJN J1443+3439 could not be excluded. The sky surface density supported a power-law distribution of source count versus flux density. For transient events, the power-law exponent was approximately-3/2. These results are expected to assist radio variable/transient surveys in next-generation facilities such as the Square Kilometre Array.

    本文言語English
    論文番号10
    ジャーナルAstrophysical Journal
    781
    1
    DOI
    出版ステータスPublished - 2014 1 20

    ASJC Scopus subject areas

    • Space and Planetary Science
    • Astronomy and Astrophysics

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