collaborators

6 papers

astro-ph.HE2025

Super-Eddington Accretion through a Multiwavelength Lens: Searching for Counterparts of Ultraluminous X-ray Sources

R. Amato, M. Bachetti, R. Soria +8

Ultraluminous X-ray sources (ULXs) represent the closest and most accessible laboratories to study sustained super-Eddington accretion onto compact objects. Over the past decade, t…

astro-ph.IM2025

Accretion and Ejection Physics at High Time Resolution

F. M. Vincentelli, P. Casella, A. Veledina +18

Accretion onto compact objects is one of the most fundamental phenomena in the astrophysics, powering some of the most luminous objects in the sky. Along with this, accretion has a…

astro-ph.IM2025

The multiple facets of millisecond pulsar binaries

A. Miraval Zanon, G. Illiano, F. Ambrosino +17

Millisecond pulsar (MSP) binaries are unique laboratories for studying matter and radiation under extreme conditions that are unattainable on Earth. Recent detections of optical mi…

astro-ph.HE2025

On the nature of the X-ray binary transient MAXI J1834-021: clues from its first observed outburst

A. Manca, A. Marino, A. Borghese +14

MAXI J1834-021 is a new X-ray transient that was discovered in February 2023. We analysed the spectral and timing properties of MAXI J1834-021 using NICER, NuStar and Swift data co…

astro-ph.HE2025

Unveiling the reflection spectrum in the ultracompact LMXB 4U 1820-30

A. Anitra, A. Gnarini, T. Di Salvo +12

4U 1820-30 is a ultracompact X-ray binary located in the globular cluster NGC 6624, consisting of a neutron star accreting material from a helium white dwarf companion characterize…

astro-ph.IM2025

X-ray spectral fitting with Monte Carlo Dropout Neural Networks

A. Tutone, A. Anitra, E. Ambrosi +11

We present a novel approach using neural networks to recover X-ray spectral model parameters and quantify uncertainties, balancing accuracy and computational efficiency against tra…