A SEARCH FOR RADIO TRANSIENTS IN VERY LARGE ARRAY ARCHIVAL IMAGES OF THE 3C 286 FIELD

被引:35
作者
Bower, Geoffrey C. [1 ,2 ]
Saul, Destry [3 ]
机构
[1] Univ Calif Berkeley, Radio Astron Lab, Berkeley, CA 94720 USA
[2] Univ Calif Berkeley, Dept Astron, Berkeley, CA 94720 USA
[3] Columbia Univ, Dept Phys, New York, NY 10027 USA
基金
美国国家科学基金会;
关键词
radio continuum: galaxies; radio continuum: general; radio continuum: stars; surveys; GAMMA-RAY BURSTS; AFTERGLOWS; CATALOG; SKY;
D O I
10.1088/2041-8205/728/1/L14
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present a search for radio transients (RTs) in the field of the bright radio source 3C 286 using archival observations from the Very Large Array (VLA). These observations span 23 years and include 1852 epochs at 1.4 GHz in the C and D configurations. We find no transients in the field. The sensitivity of the observations is limited by dynamic range effects in the images. At large flux densities (>0.2 Jy), single-epoch observations provide a strong limit on the transient surface density. At flux densities near the dynamic range threshold, we use the requirement that transient sources must appear in consecutive epochs to be confirmed as real. This sets the sensitivity at low flux densities to transient durations of tau similar to 1 day, while tau > 1 minute for high flux densities. At 70 mJy, we find a 2 sigma limit on the surface density Sigma < 3 x 10(-3) deg(-2). At 3 Jy, we find a 2 sigma limit Sigma < 9 x 10(-4) deg(-2). A future systematic search of the VLA archives can provide one to two orders of magnitude more sensitivity to RTs.
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