A Survey for Transient Astronomical Radio Emission at 611 MHz
arXiv:astro-ph/0304260 · doi:10.1086/375568
Abstract
We have constructed and operated the Survey for Transient Astronomical Radio Emission (STARE) to detect transient astronomical radio emission at 611 MHz originating from the sky over the northeastern United States. The system is sensitive to transient events on timescales of 0.125 s to a few minutes, with a typical zenith flux density detection threshold of approximately 27 kJy. During 18 months of around-the-clock observing with three geographically separated instruments, we detected a total of 4,318,486 radio bursts. 99.9% of these events were rejected as locally generated interference, determined by requiring the simultaneous observation of an event at all three sites for it to be identified as having an astronomical origin. The remaining 3,898 events have been found to be associated with 99 solar radio bursts. These results demonstrate the remarkably effective RFI rejection achieved by a coincidence technique using precision timing (such as GPS clocks) at geographically separated sites. The non-detection of extra-solar bursting or flaring radio sources has improved the flux density sensitivity and timescale sensitivity limits set by several similar experiments in the 1970s. We discuss the consequences of these limits for the immediate solar neighborhood and the discovery of previously unknown classes of sources. We also discuss other possible uses for the large collection of 611 MHz monitoring data assembled by STARE.
arXiv comment24 pages, 6 figures; to appear in PASP
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- The Dynamic Radio Sky
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- STARE2: Detecting Fast Radio Bursts in the Milky Way
- Surveying the Dynamic Radio Sky with the Long Wavelength Demonstrator Array
- Searching for giga-Jansky fast radio bursts from the Milky Way with a global array of low-cost radio receivers
- The discovery and significance of fast radio bursts
- Short-duration Radio Bursts with Apparent Extragalactic Dispersion
- Astropulse: A Search for Microsecond Transient Radio Signals Using Distributed Computing. I. Methodology
- Strategies for the Detection of ET Probes Within Our Own Solar System