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20242026
most citedHERMES: Gamma Ray Burst and Gravitational Wave counterpart hunter

7 citations · 18 across the 12 of their papers we have counts for

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10 papers · 1 filter

astro-ph.HE2026

Detection of kilosecond hard lags in the new pulsating ULX candidate NGC 7456 ULX-1

W. Leone, F. Pintore, C. Pinto +19

Context. Ultraluminous X-ray sources (ULXs) are thought to be powered, in many cases, by super-Eddington accretion onto compact objects. While soft X-ray lags have been detected in…

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

The first IXPE view of the eclipsing ADC source 4U 1822-37

A. Anitra, A. Gnarini, T. Di Salvo +17

Accretion-disc corona sources are high-inclination low-mass X-ray binaries in which the innermost regions are hidden and the observed X-ray emission is dominated by radiation scatt…

astro-ph.HE2026

CubeSats Reach the Millisecond X-Ray Domain: Crab Pulsar Timing with SpIRIT/HERMES

Wladimiro Leone, R. Mearns, T. Di Salvo +70

The High Energy Rapid Modular Ensemble of Satellites (HERMES) instrument is a compact X/-ray spectrometer operating on board the 6U (11 kg) SpIRIT CubeSat. The payload is partic…

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.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

X-ray view of emission lines in optical spectra: Spectral analysis of the two low-mass X-ray binary systems Swift J1357.2-0933 and MAXI J1305-704

A. Anitra, C. Miceli, T. Di Salvo +6

We propose a novel approach for determining the orbital inclination of low-mass X-ray binary systems by modelling the H and H line profiles emitted by the accretion disc, wit…

astro-ph.HE2024★ 7 cited

HERMES: Gamma Ray Burst and Gravitational Wave counterpart hunter

G. Ghirlanda, L. Nava, O. Salafia +67

Gamma Ray Bursts (GRBs) bridge relativistic astrophysics and multi-messenger astronomy. Space-based gamma/X-ray wide field detectors have proven essential to detect and localize th…

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…

astro-ph.HE2024

Confirmation of the presence of a CRSF in the NICER spectrum of X 1822-371

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

X 1822-371 is an eclipsing binary system with a period close to 5.57 hr and an orbital period derivative of 1.42(3) s s. The extremely h…