activity
20122026
most citedLOFT: the Large Observatory For X-ray Timing

43 citations · 86 across the 16 of their papers we have counts for

collaborators

17 papers

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…

gr-qc2026

Impact of coalescence signals on the search for continuous gravitational waves with Einstein Telescope

Elena Codazzo, Lorenzo Mirasola, Matteo Di Giovanni +7

The current network of gravitational wave detectors has already revealed hundreds of compact binary coalescences (CBCs), including binary neutron stars, binary black holes, and bla…

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

Flashing fast: characterising the 2025 outburst of MAXI J1957+032

A. Sanna, G. Illiano, M. C. Baglio +13

MAXI J1957+032 is an accreting millisecond X-ray pulsar that shows brief, recurrent outbursts in an ultra-compact ~1 h orbit. We characterise the 2025 outburst using X-ray timing a…

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

The 2025 outburst of IGR J17511-3057: timing and spectral insights from NICER and NuSTAR

A. Sanna, G. K. Jaisawal, T. E. Strohmayer +13

IGR J17511-3057 was observed in a new outburst phase starting in February 2025 and lasting at least nine days. We investigated the spectral and temporal properties of IGR J17511-30…

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

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…

astro-ph.IM2025

HERMES Pathfinder & SpIRIT: a progress report

F. Fiore, M. Trenti, Y. Evangelista +87

HERMES Pathfinder is an in-orbit demonstration consisting of a constellation of six 3U cubesats hosting simple but innovative X-ray/gamma-ray detectors for the monitoring of cosmic…

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.IM2019★ 6 cited

ESA Voyage 2050 white paper -- GrailQuest: hunting for Atoms of Space and Time hidden in the wrinkle of Space-Time

L. Burderi, A. Sanna, T. Di Salvo +30

GrailQuest (Gamma Ray Astronomy International Laboratory for QUantum Exploration of Space-Time) is a mission concept based on a constellation (hundreds/thousands) of nano/micro/sma…

astro-ph.HE2016★ 27 cited

Study of the reflection spectrum of the LMXB 4U 1702-429

R. Iaria, T. Di Salvo, M. Del Santo +7

The source 4U 1702-429 (Ara X-1) is a low-mass X-ray binary system hosting a neutron star. Albeit the source is quite bright ( erg s) its broadband spectrum ha…

astro-ph.IM2012★ 43 cited

LOFT: the Large Observatory For X-ray Timing

M. Feroci, J. W. den Herder, E. Bozzo +245

The LOFT mission concept is one of four candidates selected by ESA for the M3 launch opportunity as Medium Size missions of the Cosmic Vision programme. The launch window is curren…