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The Murriyang radio telescope.

The Murriyang radio telescope.

Dr Joe Bright

Researcher in Radio Astronomy

Research theme

  • Astronomy and astrophysics

Sub department

  • Astrophysics

Research groups

  • MeerKAT
  • Pulsars, transients and relativistic astrophysics
  • Breakthrough Listen
joe.bright@physics.ox.ac.uk
Telephone: 01865 (2)83125
Denys Wilkinson Building, room 558
  • About
  • Allen Telescope Array Acknowledgements
  • Publications

AT 2021loi: A Bowen Fluorescence Flare with a Rebrightening Episode Occurring in a Previously Known AGN

The Astrophysical Journal American Astronomical Society 953:1 (2023) 32

Authors:

Lydia Makrygianni, Benny Trakhtenbrot, Iair Arcavi, Claudio Ricci, Marco C Lam, Assaf Horesh, Itai Sfaradi, K Azalee Bostroem, Griffin Hosseinzadeh, D Andrew Howell, Craig Pellegrino, Rob Fender, David A Green, David RA Williams, Joe Bright
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Bursts from Space: MeerKAT – the first citizen science project dedicated to commensal radio transients

Monthly Notices of the Royal Astronomical Society Oxford University Press 523:2 (2023) 2219-2235

Authors:

Alex Andersson, chris Lintott, rob Fender, joe Bright, francesco Carotenuto, ian Heywood, Lauren Rhodes, Sara Motta, David Williams

Abstract:

The newest generation of radio telescopes is able to survey large areas with high sensitivity and cadence, producing data volumes that require new methods to better understand the transient sky. Here, we describe the results from the first citizen science project dedicated to commensal radio transients, using data from the MeerKAT telescope with weekly cadence. Bursts from Space: MeerKAT was launched late in 2021 and received ∼89 000 classifications from over 1000 volunteers in 3 months. Our volunteers discovered 142 new variable sources which, along with the known transients in our fields, allowed us to estimate that at least 2.1 per cent of radio sources are varying at 1.28 GHz at the sampled cadence and sensitivity, in line with previous work. We provide the full catalogue of these sources, the largest of candidate radio variables to date. Transient sources found with archival counterparts include a pulsar (B1845-01) and an OH maser star (OH 30.1–0.7), in addition to the recovery of known stellar flares and X-ray binary jets in our observations. Data from the MeerLICHT optical telescope, along with estimates of long time-scale variability induced by scintillation, imply that the majority of the new variables are active galactic nuclei. This tells us that citizen scientists can discover phenomena varying on time-scales from weeks to several years. The success both in terms of volunteer engagement and scientific merit warrants the continued development of the project, while we use the classifications from volunteers to develop machine learning techniques for finding transients.
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The Black Hole Candidate Swift J1728.9–3613 and the Supernova Remnant G351.9–0.9

The Astrophysical Journal American Astronomical Society 947:1 (2023) 38

Authors:

Mayura Balakrishnan, Paul A Draghis, Jon M Miller, Joe Bright, Robert Fender, Mason Ng, Edward Cackett, Andrew Fabian, Kip Kuntz, James CA Miller-Jones, Daniel Proga, Paul S Ray, John Raymond, Mark Reynolds, Abderahmen Zoghbi
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Precise Measurements of Self-absorbed Rising Reverse Shock Emission from Gamma-ray Burst 221009A

(2023)

Authors:

Joe S Bright, Lauren Rhodes, Wael Farah, Rob Fender, Alexander J van der Horst, James K Leung, David RA Williams, Gemma E Anderson, Pikky Atri, David R DeBoer, Stefano Giarratana, David A Green, Ian Heywood, Emil Lenc, Tara Murphy, Alexander W Pollak, Pranav H Premnath, Paul F Scott, Sofia Z Sheikh, Andrew Siemion, David J Titterington
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Details from ArXiV

Search and identification of transient and variable radio sources using MeerKAT observations: a case study on the MAXI J1820+070 field

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 517:2 (2022) 2894-2911

Authors:

A Rowlinson, J Meijn, J Bright, AJ van der Horst, S Chastain, S Fijma, R Fender, I Heywood, RAMJ Wijers, PA Woudt, A Andersson, GR Sivakoff, E Tremou, LN Driessen
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