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The Panchromatic Afterglow of GW170817: The full uniform dataset, modeling, comparison with previous results and implications
Sphesihle Makhathini, Kunal P. Mooley, Murray Brightman +35
We present the full panchromatic afterglow light curve data of GW170817, including new radio data as well as archival optical and X-ray data, between 0.5 and 940 days post-merger.…
Radio Detections During Two State Transitions of the Intermediate Mass Black Hole HLX-1
Natalie Webb, David Cseh, Emil Lenc +7
Relativistic jets are streams of plasma moving at appreciable fractions of the speed of light. They have been observed from stellar mass black holes (320 solar masses, M$_…
The accretion disc, jets and environment of the intermediate mass black hole candidate ESO 243-49 HLX-1
N. A. Webb, D. Barret, V. Braito +13
The Ultra Luminous X-ray (ULX) source HLX-1 in the galaxy ESO 243-49 has an observed maximum unabsorbed X-ray luminosity of 1.3e42 erg/s (0.2-10.0 keV). From the conservative assum…
Exploring the Nature of the Brightest Hyper-luminous X-ray Source
Sean Farrell, Mathieu Servillat, Klaas Wiersema +7
The small subset of hyper-luminous X-ray sources with luminosities in excess of ~1E41 erg/s are hard to explain without the presence of an intermediate mass black hole, as signific…
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…