activity
20012026
most citedSpectroscopic identification of r-process nucleosynthesis in a double neutron star merger

1k citations · 7.2k across the 97 of their papers we have counts for

collaborators

100 papers

astro-ph.HE2026

The compact jets of the black hole X-ray binary Swift J1753.5-0127 during its 2023-2024 outburst

Noa Grollimund, Stéphane Corbel, Lauren Rhodes +14

X-ray binaries are excellent laboratories to study the coupling between accretion and ejection phenomena around compact objects through multiwavelength observations. Swift J1753.5-…

astro-ph.HE2026

Energy-dependent Optical/Near-infrared and X-ray Correlations in Swift J1727.8-1613

Ruican Ma, Federico Vincentelli, Diego Altamirano +5

We present a timing analysis of the black hole transient Swift J1727.8-1613 during its intermediate state. We use coordinated broadband X-ray observations from Insight-HXMT (2-150…

astro-ph.HE2026

Disc Winds From Accreting Systems in the 2040s

Noel Castro Segura, Virginia Cúneo, Francesco Tombesi +9

What does the temporal evolution of disc winds tell us about accreting systems and the accretion process? Studies of accretion-disc outflows across all mass scales, including accre…

astro-ph.IM2025

How Mass Flows Through Accretion Discs: A Spectral-Timing Vision for the 2040s

Simone Scaringi, Domitilla de Martino, Anna F. Pala +17

Understanding how mass and angular momentum flow through accretion discs remains a fundamental unsolved problem in astrophysics. Accreting white dwarfs offer an ideal laboratory fo…

astro-ph.IM2025

Observatory Science with eXTP

Ping Zhou, Jirong Mao, Liang Zhang +97

Scheduled for launch in 2030, the enhanced X-ray Timing and Polarization (eXTP) telescope is a Chinese space-based mission aimed at studying extreme conditions and phenomena in ast…

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…