An untriggered search for optical bursts

被引:15
作者
Kehoe, R
Akerlof, C
Balsano, R
Bloch, J
Casperson, D
Fletcher, S
Gisler, G
Lee, B
Marshall, S
McKay, T
Rykoff, E
Smith, D
Vestrand, T
Wren, J
机构
[1] Univ Michigan, Dept Phys, Randall Lab, Ann Arbor, MI 48109 USA
[2] Michigan State Univ, Dept Phys & Astron, E Lansing, MI 48824 USA
[3] Los Alamos Natl Lab, Div NIS2, Los Alamos, NM 87545 USA
[4] Fermilab Natl Accelerator Lab, Batavia, IL 60510 USA
[5] Lawrence Livermore Natl Lab, IGPP Div, Livermore, CA 94550 USA
基金
美国国家科学基金会;
关键词
gamma rays : bursts; gamma rays : observations; ISM : jets and outflows; methods : data analysis; stars : variables : other;
D O I
10.1086/342231
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present an untriggered search for optical bursts with the Robotic Optical Transient Search Experiment (ROTSE-I) telephoto array. Observations were taken that monitor an effective 256 deg(2) field continuously over 125 hr to m(ROTSE) = 15.7. The uniquely large field, moderate limiting magnitude, and fast cadence of 10 minutes permit transient searches in a new region of sensitivity. Our search reveals no candidate events. To quantify this result, we simulate potential optical bursts with peak magnitude m(p) at t = 10 s, which fade as f = (t/t(0))(alphat), where alpha(t) < 0. Simple estimates based on observational evidence indicate that a search of this sensitivity begins to probe the possible region occupied by gamma-ray burst ( GRB) orphan afterglows. Our observing protocol and image sensitivity result in a broad region of high detection efficiency for light curves to the bright and slowly varying side of a boundary running from [alpha(t), m(p)] = [-2.0, 6.0] to [-0.3, 13.2]. Within this region, the integrated rate of brief optical bursts is less than 1.1 x10(-8) s(-1) deg(-2). At similar to 22 times the observed GRB rate from BATSE, this suggests a limit on theta(opt)/theta(gamma)less than or similar to 5, where theta(opt) and theta(gamma) are the optical and gamma-ray collimation angles, respectively. Several effects might explain the absence of optical bursts, and a search of the kind described here but more sensitive by about 4 mag should offer a more definitive probe.
引用
收藏
页码:845 / 852
页数:8
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