Transient study using LoTSS – framework development and preliminary results

Author:

de Ruiter Iris1ORCID,Meyers Zachary S23,Rowlinson Antonia14ORCID,Shimwell Timothy W45,Ruhe David16,Wijers Ralph A M J1ORCID

Affiliation:

1. Anton Pannekoek Institute for Astronomy, University of Amsterdam , Science Park 904, NL-1098 XH Amsterdam , the Netherlands

2. Deutsches Elektronen-Synchrotron DESY , Platanenallee 6, D-15738 Zeuthen , Germany

3. Erlangen Center for Astroparticle Physics (ECAP), Friedrich-Alexander-Universität Erlangen-Nuremberg , D-91058 Erlangen , Germany

4. ASTRON, the Netherlands Institute for Radio Astronomy , Postbus 2, NL-7990 AA Dwingeloo , the Netherlands

5. Leiden Observatory, Leiden University , PO Box 9513, NL-2300 RA Leiden , the Netherlands

6. AI4Science (AMLab), Informatics Institute, University of Amsterdam , Science Park 904, NL-1098 XH Amsterdam , the Netherlands

Abstract

ABSTRACT We present a search for transient radio sources on time-scales of seconds to hours at 144 MHz using the LOFAR Two-metre Sky Survey (LoTSS). This search is conducted by examining short time-scale images derived from the LoTSS data. To allow imaging of LoTSS on short time-scales, a modern imaging procedure and fast filtering strategy are introduced. This includes sky model source subtraction, no cleaning or primary beam correction, a simple source finder, fast filtering schemes, and source catalogue matching. This new strategy is first tested by injecting simulated transients, with a range of flux densities and durations, into the data. We find the limiting sensitivity to be 113 and 6 mJy for 8 s and 1 h transients, respectively. The new imaging and filtering strategies are applied to 58 fields of the LoTSS survey, corresponding to LoTSS-DR1 (2 per cent of the survey). One transient source is identified in the 8 s and 2 min snapshot images. The source shows 1 min duration flare in the 8 h observation. Our method puts the most sensitive constraints on/estimates of the transient surface density at low frequencies at time-scales of seconds to hours; <4.0 × 10−4 deg−2 at 1 h at a sensitivity of 6.3 mJy; 5.7 × 10−7 deg−2 at 2 min at a sensitivity of 30 mJy; and 3.6 × 10−8 deg−2 at 8 s at a sensitivity of 113 mJy. In the future, we plan to apply the strategies presented in this paper to all LoTSS data.

Funder

CNRS

Science Foundation Ireland

Science and Technology Facilities Council

Ministry of Science and Higher Education

Istituto Nazionale di Astrofisica

INAF

NWO

Publisher

Oxford University Press (OUP)

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