activity
19992023
most citedAn Ultraluminous X-ray Source Powered by An Accreting Neutron Star

767 citations · 6.5k across the 100 of their papers we have counts for

collaborators

101 papers

astro-ph.HE2023★ 5 cited

Tidal disruption events and quasi periodic eruptions

Natalie A. Webb, Didier Barret, Olivier Godet +4

Tidal disruption events (TDEs) occur when a star passes close to a massive black hole, so that the tidal forces of the black hole exceed the binding energy of a star and cause it t…

astro-ph.HE2023★ 24 cited

Statistical study of a large and cleaned sample of ultraluminous and hyperluminous X-ray sources

Hugo Tranin, Natalie Webb, Olivier Godet +1

Ultra-/hyper-luminous X-ray sources (ULX/HLX) could be interesting laboratories to improve our understanding of the supermassive black hole growth through super-Eddington accretion…

astro-ph.IM2023

XMM2ATHENA, the H2020 project to improve XMM-Newton analysis software and prepare for Athena

Natalie A. Webb, Francisco J. Carrera, Axel Schwope +31

XMM-Newton, a European Space Agency observatory, has been observing the X-ray, ultra-violet and optical sky for 23 years. During this time, astronomy has evolved from mainly studyi…

astro-ph.SR2023★ 3 cited

Accreting white dwarfs

Natalie A. Webb

White dwarfs are the most common endpoints of stellar evolution. They are often found in close binary systems in which the white dwarf is accreting matter from a companion star, ei…

astro-ph.HE2023★ 21 cited

Multimessenger study of merging massive black holes in the OBELISK simulation: gravitational waves, electromagnetic counterparts, and their link to galaxy and black hole populations

C. A. Dong-Páez, M. Volonteri, R. S. Beckmann +5

Massive black-hole (BH) mergers are predicted to be powerful sources of low-frequency gravitational waves (GWs). Coupling the detection of GWs with an electromagnetic (EM) detectio…

astro-ph.GA2023★ 14 cited

Black hole mergers as tracers of spinning massive black hole and galaxy populations in the OBELISK simulation

C. A. Dong-Páez, M. Volonteri, R. S. Beckmann +5

Massive black hole (BH) mergers will be key targets of future gravitational wave and electromagnetic observational facilities. In order to constrain BH evolution with the informati…