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Relativistic Jet from Black Hole

An artist's impression of a relativistic jet propagating away from a black hole at close to the speed of light. Such jets are formed by the inner regions of the accretion flow: matter flowing inwards towards the black hole, via processes which are not yet fully understood. The accretion flow emits primarily in X-rays, the relativistic jet in the radio band: by combing observations in each band we can try and understand how such jets form and how much energy they carry away from the black hole.

Professor Rob Fender

Professor of Astrophysics

Research theme

  • Astronomy and astrophysics

Sub department

  • Astrophysics

Research groups

  • Hintze Centre for Astrophysical Surveys
  • MeerKAT
  • Pulsars, transients and relativistic astrophysics
  • Rubin-LSST
  • The Square Kilometre Array (SKA)
  • Gamma-ray astronomy
Rob.Fender@physics.ox.ac.uk
Telephone: 01865 (2)73435
Denys Wilkinson Building, room 712
  • About
  • Publications

Multiwavelength analysis of AT 2023sva: a luminous orphan afterglow with evidence for a structured jet

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 538:1 (2025) 351-372

Authors:

Gokul P Srinivasaragavan, Daniel A Perley, Anna YQ Ho, Brendan O’Connor, Antonio de Ugarte Postigo, Nikhil Sarin, S Bradley Cenko, Jesper Sollerman, Lauren Rhodes, David A Green, Dmitry S Svinkin, Varun Bhalerao, Gaurav Waratkar, AJ Nayana, Poonam Chandra, M Coleman Miller, Daniele B Malesani, Geoffrey Ryan, Suryansh Srijan, Eric C Bellm, Eric Burns, David J Titterington, Maria B Stone, Josiah Purdum, Tomás Ahumada, GC Anupama, Sudhanshu Barway, Michael W Coughlin, Andrew Drake, Rob Fender, José F Agüí Fernández, Dmitry D Frederiks, Stefan Geier, Matthew J Graham, Mansi M Kasliwal, SR Kulkarni, Harsh Kumar, Maggie L Li, Russ R Laher, Alexandra L Lysenko, Gopal Parwani, Richard A Perley, Anna V Ridnaia, Anirudh Salgundi, Roger Smith, Niharika Sravan, Vishwajeet Swain, Christina C Thöne, Anastasia E Tsvetkova, Mikhail V Ulanov, Jada Vail, Jacob L Wise, Avery Wold
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Finding radio transients with anomaly detection and active learning based on volunteer classifications

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 538:3 (2025) staf336

Authors:

Alex Andersson, Chris Lintott, Rob Fender, Michelle Lochner, Patrick Woudt, Jakob van den Eijnden, Alexander van der Horst, Assaf Horesh, Payaswini Saikia, Gregory R Sivakoff, Lilia Tremou, Mattia Vaccari

Abstract:

<jats:title>ABSTRACT</jats:title> <jats:p>In this work, we explore the applicability of unsupervised machine learning algorithms to finding radio transients. Facilities such as the Square Kilometre Array (SKA) will provide huge volumes of data in which to detect rare transients; the challenge for astronomers is how to find them. We demonstrate the effectiveness of anomaly detection algorithms using 1.3 GHz light curves from the SKA precursor MeerKAT. We make use of three sets of descriptive parameters (‘feature sets’) as applied to two anomaly detection techniques in the astronomaly package and analyse our performance by comparison with citizen science labels on the same data set. Using transients found by volunteers as our ground truth, we demonstrate that anomaly detection techniques can recall over half of the radio transients in the 10 per cent of the data with the highest anomaly scores. We find that the choice of anomaly detection algorithm makes a minor difference, but that feature set choice is crucial, especially when considering available resources for human inspection and/or follow-up. Active learning, where human labels are given for just 2 per cent of the data, improves recall by up to 20 percentage points, depending on the combination of features and model used. The best-performing results produce a factor of 5 times fewer sources requiring vetting by experts. This is the first effort to apply anomaly detection techniques to finding radio transients and shows great promise for application to other data sets, and as a real-time transient detection system for upcoming large surveys.</jats:p>
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Contemporaneous optical-radio observations of a fast radio burst in a close galaxy pair

(2025)

Authors:

KY Hanmer, I Pastor-Marazuela, J Brink, D Malesani, BW Stappers, PJ Groot, AJ Cooper, N Tejos, DAH Buckley, ED Barr, MC Bezuidenhout, S Bloemen, M Caleb, LN Driessen, R Fender, F Jankowski, M Kramer, DLA Pieterse, KM Rajwade, J Tian, PM Vreeswijk, R Wijnands, PA Woudt
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On the distance to the black hole X-ray binary Swift J1727.8$-$1613

(2025)

Authors:

Benjamin J Burridge, James CA Miller-Jones, Arash Bahramian, Steve R Prabu, Reagan Streeter, Noel Castro Segura, Jesús M Corral Santana, Christian Knigge, Evangelia Tremou, Francesco Carotenuto, Rob Fender, Payaswini Saikia
Details from ArXiV

The Observed Phase Space of Mass-loss History from Massive Stars Based on Radio Observations of a Large Supernova Sample

The Astrophysical Journal American Astronomical Society 979:2 (2025) 189

Authors:

Itai Sfaradi, Assaf Horesh, Rob Fender, Lauren Rhodes, Joe Bright, David Williams-Baldwin, Dave A Green
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