collaborators

6 papers

astro-ph.HE2026

A Broadband X-ray Analysis and Optical Counterpart Search of IC5052 ULX

Nabil Brice, Dominic J. Walton, Felix Fürst +10

We present broadband X-ray spectral and timing analysis of the Ultra-luminous X-ray source (ULX) in IC5052 using simultaneous XMM-Newton and NuSTAR observations from 2022, suppleme…

astro-ph.HE2026

Deep optical spectroscopic monitoring of the pulsating ULX NGC 1313 X-2 with longslit Gemini observations

Rajath Sathyaprakash, Timothy. P. Roberts

This study reports the nature of the companion star to the pulsating ULX NGC 1313 X-2, using long-slit spectroscopic data from Gemini-South observations, based on archival data fro…

astro-ph.HE2026

Significant or Not? The Impact of Randomisation During Data Reduction on Confirming a New Pulsating Ultraluminous X-ray Source Candidate in Centaurus A

Amy H. Knight, Timothy P. Roberts, Callum Potter +2

We report the discovery of a new candidate pulsating ultraluminous X-ray source (PULX) in NGC 5128 (Centaurus A). The candidate, 4XMM J132542.2-425943, is a transient source, ident…

astro-ph.HE2024

The long-term variability of a population of ULXs monitored by Chandra

Hannah P. Earnshaw, Gauri Patti, Murray Brightman +5

We present preliminary results of a Chandra Large Program to monitor the ultraluminous X-ray source (ULX) populations of three nearby, ULX-rich galaxies over the course of a year,…

astro-ph.HE2024

Exploring the case for hard-X-ray beaming in NGC 6946 X-1

Tobias Beuchert, Matthew J. Middleton, Roberto Soria +5

In order to understand the nature of super-Eddington accretion we must explore both the emission emerging directly from the inflow and its impact on the surroundings. In this paper…

astro-ph.HE2024

Skipping a beat: discovery of persistent quasi-periodic oscillations associated with pulsed fraction drop of the spin signal in M51 ULX-7

Matteo Imbrogno, Sara Elisa Motta, Roberta Amato +24

The discovery of pulsations in (at least) six ultraluminous X-ray sources (ULXs) has shown that neutron stars can accrete at (highly) super-Eddington rates, challenging the standar…