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Black Hole

Lensing of space time around a black hole. At Oxford we study black holes observationally and theoretically on all size and time scales - it is some of our core work.

Credit: ALAIN RIAZUELO, IAP/UPMC/CNRS. CLICK HERE TO VIEW MORE IMAGES.

Dr Kaustubh Rajwade

Senior Researcher

Research theme

  • Astronomy and astrophysics

Sub department

  • Astrophysics

Research groups

  • The Square Kilometre Array (SKA)
kaustubh.rajwade@physics.ox.ac.uk
Denys Wilkinson Building, room 603
  • About
  • Publications

Spectrotemporal Analysis of a Sample of Bursts from FRB 121102

Research Notes of the AAS American Astronomical Society 4:9 (2020) 150

Authors:

Kaustubh Rajwade, Mitchell Mickaliger, Benjamin Stappers, Manisha Caleb, Rene P Breton, Aris Karastergiou, Evan Keane
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Possible periodic activity in the repeating FRB 121102

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 495:4 (2020) 3551-3558

Authors:

KM Rajwade, MB Mickaliger, BW Stappers, V Morello, D Agarwal, CG Bassa, RP Breton, M Caleb, A Karastergiou, EF Keane, DR Lorimer
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Details from ArXiV

Limits on absorption from a 332-MHz survey for fast radio bursts

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 493:3 (2020) 4418-4427

Authors:

KM Rajwade, MB Mickaliger, BW Stappers, CG Bassa, RP Breton, A Karastergiou, EF Keane
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MKT J170456.2-482100: the first transient discovered by MeerKAT

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 491:1 (2020) 560-575

Authors:

Ln Driessen, I McDonald, Dah Buckley, M Caleb, Ej Kotze, Sb Potter, Km Rajwade, A Rowlinson, Bw Stappers, E Tremou, Pa Woudt, Rp Fender, R Armstrong, P Groot, I Heywood, A Horesh, Aj van der Horst, E Koerding, Va McBride, Jca Miller-Jones, Kp Mooley, Ramj Wijers

Abstract:

© 2019 The Author(s) We report the discovery of the first transient with MeerKAT, MKT J170456.2−482100, discovered in ThunderKAT images of the low-mass X-ray binary GX339−4. MKT J170456.2−482100 is variable in the radio, reaching a maximum flux density of 0.71 ± 0.11 mJy on 2019 October 12, and is undetected in 15 out of 48 ThunderKAT epochs. MKT J170456.2−482100 is coincident with the chromospherically active K-type sub-giant TYC 8332-2529-1, and ∼ 18 yr of archival optical photometry of the star shows that it varies with a period of 21.25 ± 0.04 d. The shape and phase of the optical light curve changes over time, and we detect both X-ray and UV emission at the position of MKT J170456.2−482100, which may indicate that TYC 8332-2529-1 has large star spots. Spectroscopic analysis shows that TYC 8332-2529-1 is in a binary, and has a line-of-sight radial velocity amplitude of 43 km s−1. We also observe a spectral feature in antiphase with the K-type sub-giant, with a line-of-sight radial velocity amplitude of ∼ 12 ± 10 km s−1, whose origins cannot currently be explained. Further observations and investigation are required to determine the nature of the MKT J170456.2−482100 system.
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Details from ArXiV

A fast radio burst in the direction of the Virgo Cluster

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 490:1 (2019) 1-8

Authors:

Devansh Agarwal, Duncan R Lorimer, Anastasia Fialkov, Keith W Bannister, Ryan M Shannon, Wael Farah, Shivani Bhandari, Jean-Pierre Macquart, Chris Flynn, Giuliano Pignata, Nicolas Tejos, Benjamin Gregg, Stefan Osłowski, Kaustubh Rajwade, Mitchell B Mickaliger, Benjamin W Stappers, Di Li, Weiwei Zhu, Lei Qian, Youling Yue, Pei Wang, Abraham Loeb
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