activity
20022025
most citedA Population of Fast Radio Bursts at Cosmological Distances

1k citations · 6.1k across the 64 of their papers we have counts for

collaborators

64 papers

astro-ph.HE2025

Radio emission from beyond the light cylinder in millisecond pulsars

Michael Kramer, Simon Johnston

A striking aspect of the radio profiles of many millisecond pulsars (MSPs) is that they consist of components separated from each other by regions lacking in emission. We devise a…

astro-ph.HE2024

Unveiling frequency-dependent eclipsing in spider millisecond pulsars using broadband polarization observations with the Parkes

Sangita Kumari, Bhaswati Bhattacharyya, Rahul Sharan +6

This study presents an orbital phase-dependent analysis of three black widow spider millisecond pulsars (BW MSPs), aiming to investigate the magnetic field within the eclipse envir…

astro-ph.HE2024

Multiwavelength pulsations and surface temperature distribution in the middle-aged pulsar B1055-52

Armin Vahdat, Bettina Posselt, George G. Pavlov +3

We present a detailed study of the X-ray emission from PSR B1055-52 using XMM-Newton observations from 2019 and 2000. The phase-integrated X-ray emission from this pulsar is poorly…

astro-ph.HE2023★ 23 cited

Linear to circular conversion in the polarized radio emission of a magnetar

Marcus E. Lower, Simon Johnston, Maxim Lyutikov +13

Radio emission from magnetars provides a unique probe of the relativistic, magnetized plasma within the near-field environment of these ultra-magnetic neutron stars. The transmitte…

astro-ph.HE2023

The Polarized Cosmic Hand: IXPE Observations of PSR B1509-58/MSH 15-52

Roger W. Romani, Josephine Wong, Niccolo Di Lalla +99

We describe IXPE polarization observations of the Pulsar Wind Nebula (PWN) MSH15-52, the `Cosmic Hand'. We find X-ray polarization across the PWN, with B field vectors generally al…

astro-ph.HE2022★ 58 cited

The Thousand-Pulsar-Array programme on MeerKAT XI: Application of the rotating vector model

Simon Johnston, Michael Kramer, Aris Karastergiou +4

In spite of the rich phenomenology of the polarization properties of radio pulsars, the rotating vector model (RVM) created 50 years ago remains the best method to determine the be…