Sensitive Search For Radio Variables And Transients In The Extended Chandra Deep-Field South

TL;DR

This study analyzed radio variability and searched for transients in the Extended Chandra Deep Field South using VLA data, finding low variability and no transients, indicating a relatively quiet radio sky at 1.4 GHz.

Contribution

First comprehensive variability and transient search at 1.4 GHz in E-CDFS, establishing upper limits on transient rates and evaluating source-finding algorithms.

Findings

Only 1% of sources are variable at 4-sigma level.

No transients detected above 0.21 mJy flux density.

Radio sky at 1.4 GHz is relatively quiet.

Abstract

We report on an analysis of the Extended Chandra Deep Field South (E-CDFS) region using archival data from the Very Large Array, with the goal of studying radio variability and transients at the sub-mJy level. The 49 epochs of E-CDFS observations at 1.4 GHz sample timescales from one day to 3 months. We find that only a fraction (1%) of unresolved radio sources above 40 uJy are variable at the 4-sigma level. There is no evidence that the fractional variability changes along with the known transition of radio source populations below one milliJansky. Optical identifications of the sources show that the variable radio emission is associated with the central regions of an active galactic nucleus or a star-forming galaxy. After a detailed comparison of the efficacy of various source-finding algorithms, we use the best to carry out a transient search. No transients were found. This implies that the areal density of transients with peak flux density greater than 0.21 mJy is less than 0.37 deg^-2 (at a confidence level of 95%). This result is approximately an order of magnitude below the transient rate measured at 5 GHz by Bower et al. (2007) but it is consistent with more recent upper limits from Frail et al. (2012). Our findings suggest that the radio sky at 1.4 GHz is relatively quiet. For multi-wavelength transient searches, such as the electromagnetic counterparts to gravitational waves, this frequency may be optimal for reducing the high background of false positives.