Commensal transient searches in eight short gamma-ray burst fields

Author:

Chastain S I1ORCID,van der Horst A J1,Rowlinson A23ORCID,Rhodes L4ORCID,Andersson A5ORCID,Diretse R6,Fender R P5,Woudt P A7ORCID

Affiliation:

1. Department of Physics, George Washington University , 725 21st St NW, Washington, DC 20052 , USA

2. Anton Pannekoek Institute, University of Amsterdam , Postbus 94249, NL-1090 GE Amsterdam , The Netherlands

3. ASTRON, the Netherlands Institute for Radio Astronomy , Oude Hoogeveensedijk 4, NL-7991 PD Dwingeloo , The Netherlands

4. Astrophysics, Department of Physics, University of Oxford , Keble Road, Oxford OX1 3RH , UK

5. Astrophysics, Department of Physics, University of Oxford , Denys Wilkinson Building, Keble Road, Oxford OX1 3RH , UK

6. Inter-University Institute for Data-Intensive Astronomy, Department of Astronomy, University of Cape Town , Private Bag X3, Rondebosch 7701 , South Africa

7. Department of Astronomy, University of Cape Town , Private Bag X3, Rondebosch 7701 , South Africa

Abstract

ABSTRACT A new generation of radio telescopes with excellent sensitivity, instantaneous uv coverage, and large fields of view, are providing unprecedented opportunities for performing commensal transient searches. Here, we present such a commensal search in deep observations of short gamma-ray burst fields carried out with the MeerKAT radio telescope in South Africa at 1.3 GHz. These four hour observations of eight different fields span survey lengths of weeks to months. We also carry out transient searches in time slices of the full observations, at time-scales of 15 min and 8 s. We find 122 variable sources on the long time-scales, of which 52 are likely active galactic nuclei, but there are likely also some radio flaring stars. While the variability is intrinsic in at least two cases, most of it is consistent with interstellar scintillation. In this study, we also place constraints on transient rates based on state-of-the-art transient simulations codes. We place an upper limit of 2 × 10−4 transients per day per square degree for transients with peak flux of 5 mJy, and an upper limit of 2.5 × 10−2 transients per day per square degree for transients with a fluence of 10 Jy ms, the minimum detectable fluence of our survey.

Funder

Science and Technology Facilities Council

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

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