Commensal Radio Transient Searches at MHz and GHz

MHz frequencies (~50 & ~150 MHz)

The MHz transient parameter space on timescales less than 1 day (Figure 13 from de Ruiter, Meyers, Rowlinson et al. 2023)

LOFAR

My team and I use LOFAR surveys to search for transient and variable sources on a range of timescales. Predominantly, we use the LOFAR Two-meter Sky Survey (LoTSS, Shimwell et al. 2017, 2019, 2022). LoTSS aims to survey the whole Northern Sky in 8 hour observations and we search within these data for transient and variable sources using a range of techniques. In the era of LOFAR2.0, we aim to automatically search all survey observations for transient and variable sources via the LORAX (proposal led by Rowlinson with an international team of experts).

Key results from my team include:

AARTFAAC

We have built a whole visible sky monitor using the central stations of LOFAR, known as AARTFAAC (Amsterdam ASTRON Radio Transients Facility And Analysis Centre, PI: Ralph Wijers). AARTFAAC piggybacks on standard LOFAR LBA observations and can make an image of the visible radio sky at ~50 MHz every second with a bandwidth of 3 MHz. With 6 LOFAR stations, we have achieved real-time calibration and imaging. Work is ongoing to extend the real-time calibration and imaging to use 12 LOFAR stations.

We have detected an unusual group of dispersed radio transients with AARTFAAC (Kuiack et al. 2021a, Ruhe et al. 2022). Analysis of these sources is ongoing.

We have detected an unusual group of dispersed radio transients with AARTFAAC (see figure). Analysis of these sources is ongoing.

We have an AARTFAAC YouTube account where you can watch past observations using the innermost 6 LOFAR stations.

Key results from our team include:

GHz frequencies (~1.4 GHz)

The GHz transient parameter space (Figure 5 from Fijma, Rowlinson et al. 2024)

MeerKAT

Working with the ThunderKAT team, I co-lead the commensal transient searches using MeerKAT survey data. Key results from my team include: