Abstract
We present results from daily radio continuum observations of the Boötes field as part of the PiGHz Sky Survey (PiGSS). These results are part of a systematic and unbiased campaign to characterize variable and transient sources in the radio sky. The observations include 78 individual epochs distributed over five months at a radio frequency of 3.1GHz with a median rms image noise in each epoch of 2.8mJy. We produce five monthly images with a median rms of 0.6mJy. No transient radio sources are detected in the daily or monthly images. At 15mJy, we set an upper limit (2σ) to the surface density of one-day radio transients at 0.025 deg-2. At 5mJy, we set an upper limit (2σ) to the surface density of one-month radio transients at 0.18 deg-2. We also produce light curves for 425 sources and explore the variability properties of these sources. Approximately 20% of the sources exhibit some variability on daily and monthly timescales. The maximum rms fractional modulations on the one-day and one-month timescales for sources brighter than 10mJy are 2 and 0.5, respectively. The probability of a daily fluctuation for all sources and all epochs by a factor of 10 is less than 10-4. We compare the radio to mid-infrared variability for sources in the field and find no correlation. Finally, we apply the statistics of transient and variable populations to constrain models for a variety of source classes. © 2011 The American Astronomical Society. All rights reserved.
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Bower, G. C., Whysong, D., Blair, S., Croft, S., Keating, G., Law, C., … Wright, M. C. H. (2011, October 1). The Allen telescope array PiGHz sky survey II. daily and monthly monitoring for transients and variability in the Boötes field. Astrophysical Journal. Institute of Physics Publishing. https://doi.org/10.1088/0004-637X/739/2/76
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