135 citations · 540 across the 12 of their papers we have counts for
12 papers
Future Detections of the Warm-Hot Intergalactic Medium using Bright Power Law Sources with NewAthena
Joseph Fisher, Antonio Martin-Carrillo, Thomas Dauser +3
Context. Hydrodynamical cosmological simulations based on the -Cold Dark Matter (CDM) model predict that 40% of the baryons in the local Universe are missing. These mis…
XMM-Newton Campaign On Ultraluminous X-ray Source NGC 1313 X-1: Wind vs. State Variability
C. Pinto, D. J. Walton, E. Kara +12
Most ultraluminous X-ray sources (ULXs) are thought to be powered by neutron stars and black holes accreting beyond the Eddington limit. If the compact object is a black hole or a…
Understanding the environment around the intermediate mass black hole candidate ESO 243-49 HLX-1
N. A. Webb, A. Guérou, B. Ciambur +12
Aims. ESO 243-49 HLX-1, otherwise known as HLX-1, is an intermediate mass black hole (IMBH) candidate located 8" (3.7 Kpc) from the centre of the edge-on S0 galaxy ESO 243-49. How…
Spectral Changes in the Hyperluminous Pulsar in NGC 5907 as a Function of Super-Orbital Phase
F. Fuerst, D. J. Walton, D. Stern +5
We present broad-band, multi-epoch X-ray spectroscopy of the pulsating ultra-luminous X-ray source (ULX) in NGC 5907. Simultaneous XMM-Newton and NuSTAR data from 2014 are best des…
Investigating slim disk solutions for HLX-1 in ESO 243-49
O. Godet, B. Plazolles, T. Kawaguchi +7
The hyper luminous X-ray source HLX-1 in the galaxy ESO 243-49, currently the best intermediate mass black hole candidate, displays spectral transitions similar to those observed i…
Further Observations of the Intermediate Mass Black Hole Candidate ESO 243-49 HLX-1
S. A. Farrell, M. Servillat, S. R. Oates +4
The brightest Ultra-Luminous X-ray source HLX-1 in the galaxy ESO 243-49 currently provides strong evidence for the existence of intermediate mass black holes. Here we present the…