activity
20242026
collaborators

12 papers

astro-ph.HE2026

Accurate distances of the Galactic spiral arms from dust-scattered X-ray emission of gamma-ray bursts

B. Vaia, I. Fornasiero, A. Tiengo +5

The details of the spiral structure of the Milky Way are still debated due to large uncertainties in the distance estimates obtained through the most common tracers. X-ray dust sca…

astro-ph.HE2026

Chasing Gamma-Ray Signals from Binary Neutron Star Coalescences with the Cherenkov Telescope Array: Prospects and Observing Strategies

S. Abe, J. Abhir, A. Abhishek +457

The detection of gravitational waves (GWs) from a binary neutron star (BNS) merger by Advanced LIGO and Advanced Virgo (GW170817), together with its electromagnetic counterpart, th…

astro-ph.HE2026

A high-resolution X-ray view of the ultra-fast outflow in MAXI J1810-222

C. Pinto, M. Del Santo, A. D'Aì +10

In previous work, it was reported that the Galactic black hole candidate MAXI J1810-222 exhibited a notable absorption spectral feature at around 1 keV in low-resolution X-ray spec…

astro-ph.HE2026

The elusive cyclotron line in 4U 1901+03: hidden, yet present

Elena Ambrosi, Antonino D' Aì, Giancarlo Cusumano +8

Context. Cyclotron resonant scattering features (CRSFs) in accreting X-ray pulsars are often difficult to detect, especially when shallow or variable. Recent studies have shown tha…

astro-ph.HE2026

Unveiling the biconical geometry of the outflow in the ultraluminous X-ray source NGC 5204 X-1

S. Caserta, C. Pinto, T. Di Salvo +9

Ultraluminous X-ray sources (ULXs) are non-nuclear X-ray binary systems that exceed the Eddington luminosity for a 10 Msun black hole. The majority of these sources are thought to…

astro-ph.GA2025

Discovery of a Luminosity-dependent Continuum Lag in NGC 4151 from Photometric and Spectroscopic Continuum Reverberation Mapping

Hai-Cheng Feng, Sha-Sha Li, Mouyuan Sun +17

Accretion onto supermassive black holes (SMBHs) powers active galactic nuclei (AGNs) and drives feedback that shapes galaxy evolution. Constraining AGN accretion disk structure is…