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20242026
most citedThe puzzling orbital residuals of XTE J1710-281: is a Jovian planet orbiting around the binary system?

2 citations · 4 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.HE2026

4U 1624-490 as a possible intermediate-mass X-ray binary: constraints from XRISM and NuSTAR spectroscopy

R. Iaria, A. Anitra, T. Di Salvo +7

High-inclination dipping neutron-star X-ray binaries provide a direct view of accretion-flow structure because the line of sight intercepts ionised plasma above the disc. We analys…

astro-ph.HE2026

Time lags as proxy of spectral evolution in gamma-ray bursts

C. Maraventano, F. Daigne, R. Mochkovitch +3

Positive lags in gamma-ray bursts (GRBs), where hard photons anticipate softer ones, provide a unique window into the temporal evolution of their prompt emission. Negative lags, wh…

astro-ph.HE2025

A mysterious feature in the NICER spectrum of 4U 1820-30: A gravitationally redshifted absorption line?

R. Iaria, T. Di Salvo, A. Anitra +6

A mysterious absorption feature at approximately 3.8 keV has been identified in the NICER spectrum of the low-mass X-ray binary system 4U 1820-30. We interpret this feature as a gr…

astro-ph.IM2025★ 1 cited

Time domain astrophysics with transient sources. Delay estimate via Cross Correlation Function techniques

W. Leone, L. Burderi, T. di Salvo +10

The timing analysis of transient events allows for investigating numerous still open areas of modern astrophysics. The article explores all the mathematical and physical tools requ…

astro-ph.HE2025★ 1 cited

High energy time lags of Gamma Ray Bursts

C. Maraventano, G. Ghirlanda, L. Nava +5

Positive lags between the arrival time of different photon energies are commonly observed in Gamma-Ray Bursts (GRBs), where soft photons lag behind harder ones. However, some GRBs…

astro-ph.HE2024★ 2 cited

The puzzling orbital residuals of XTE J1710-281: is a Jovian planet orbiting around the binary system?

R. Iaria, T. Di Salvo, A. Anitra +8

XTE J1710-281 is a transient eclipsing binary system with a period close to 3.28 hours, hosting a neutron star. The average eclipse duration is 420 seconds, and eclipse arrival tim…