most citedPopulations of Neutron Star Ultraluminous X-ray Sources: Mind your b's and B's

10 citations · 19 across the 7 of their papers we have counts for

collaborators
Showing astro-ph.HEShow all

6 papers · 1 filter

astro-ph.HE2025★ 3 cited

The Advanced X-ray Imaging Satellite (AXIS) Community Science Book

Michael Koss, Nafisa Aftab, Steven W. Allen +395

The AXIS Community Science Book represents the collective effort of 592 scientists worldwide to define the transformative science enabled by the Advanced X-ray Imaging Satellite (A…

astro-ph.HE2025

A supermassive black hole under the radar: Repeating X-ray variability in a Seyfert galaxy

Matteo Imbrogno, Andrea Sacchi, Giovanni Miniutti +4

In the last few years, a few supermassive black holes (SMBHs) have shown short-term (of the order of hours) X-ray variability. Given the limited size of the sample, every new addit…

astro-ph.HE2025★ 3 cited

The hunt for new pulsating ultraluminous X-ray sources: a clustering approach

Nicolò Oreste Pinciroli Vago, Roberta Amato, Matteo Imbrogno +5

The discovery of fast and variable coherent signals in a handful of ultraluminous X-ray sources (ULXs) testifies to the presence of super-Eddington accreting neutron stars, and dra…

astro-ph.HE2025★ 2 cited

The population of hyperluminous X-ray sources as seen by XMM-Newton

Roberta Amato, Erwan Quintin, Hugo Tranin +7

Ultraluminous and hyperluminous X-ray sources (ULXs and HLXs) are among the brightest astrophysical objects in the X-ray sky. While ULXs most likely host stellar-mass compact objec…

astro-ph.HE2025★ 10 cited

Populations of Neutron Star Ultraluminous X-ray Sources: Mind your b's and B's

Konstantinos Kovlakas, Devina Misra, Roberta Amato +1

Ultraluminous X-ray sources (ULXs) with neutron star (NS) accretors challenge traditional accretion models, and have sparked a debate regarding the role of geometrical beaming and…

astro-ph.HE2024★ 1 cited

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…