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摘要
We present the results of a 5 GHz survey with the Very Large Array (VLA) and the expanded VLA, designed to search for short-lived (less than or similar to 1 day) transients and to characterize the variability of radio sources at milli-Jansky levels. A total sky area of 2.66 deg(2), spread over 141 fields at low Galactic latitudes (b congruent to 6-8 deg), was observed 16 times with a cadence that was chosen to sample timescales of days, months, and years. Most of the data were reduced, analyzed, and searched for transients in near real-time. Interesting candidates were followed up using visible light telescopes (typical delays of 1-2 hr) and the X-ray Telescope on board the Swift satellite. The final processing of the data revealed a single possible transient with a peak flux density of f(nu) congruent to 2.4 mJy. This implies a transient's sky surface density of kappa(f(nu) > 1.8mJy) = 0.039(-0.032,-0.038)(+0.13,+0.18) deg(-2) (1 sigma, 2 sigma confidence errors). This areal density is roughly consistent with the sky surface density of transients from the Bower et al. survey extrapolated to 1.8 mJy. Our observed transient areal density is consistent with a neutron star's origin for these events. Furthermore, we use the data to measure the source variability on timescales of days to years, and we present the variability structure function of 5 GHz sources. The mean structure function shows a fast increase on approximate to 1 day timescale, followed by a slower increase on timescales of up to 10 days. On timescales between 10 and 60 days, the structure function is roughly constant. We find that greater than or similar to 30% of the unresolved sources brighter than 1.8 mJy are variables at the >4 sigma confidence level, presumably mainly due to refractive scintillation.
- 出版日期2011-10-20
