activity
20152025
most citedHERMES: An ultra-wide band X and gamma-ray transient monitor on board a nano-satellite constellation

63 citations · 662 across the 34 of their papers we have counts for

collaborators

34 papers

astro-ph.IM2025

Observatory Science with eXTP

Ping Zhou, Jirong Mao, Liang Zhang +97

Scheduled for launch in 2030, the enhanced X-ray Timing and Polarization (eXTP) telescope is a Chinese space-based mission aimed at studying extreme conditions and phenomena in ast…

astro-ph.HE2022★ 7 cited

Spectral analysis of the AMXP IGR J17591-2342 during its 2018 outburst

A. Manca, A. F. Gambino, A. Sanna +9

The Accreting Millisecond X-ray Pulsar IGR J17591-2342 is a LMXB system that went in outburst on August 2018 and it was monitored by the NICER observatory and partially by other fa…

astro-ph.HE2021★ 15 cited

Spectral analysis of the low-mass X-ray pulsar 4U 1822-371: Reflection component in a high-inclination system

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

The X-ray source 4U 1822-371 is an eclipsing low-mass X-ray binary and X-ray pulsar, hosting a NS that shows periodic pulsations in the X-ray band. The inclination angle of the sys…

astro-ph.HE2021★ 8 cited

Fe K and Fe K line detection in the NuSTAR spectrum of the ultra-bright Z-source Scorpius X-1

S. M. Mazzola, R. Iaria, T. Di Salvo +8

Low-mass X-ray binaries hosting a low-magnetised neutron star, which accretes matter via Roche-lobe overflow, are generally grouped in two classes, named Atoll and Z sources after…

astro-ph.IM2021★ 1 cited

A note on some discrepancies in convolution models in X-ray spectral analysis

Riccardo La Placa, Angelo Gambino

Convolution models are powerful tools in many fields of spectral and image analysis owing to their wide applicability, and X-ray astrophysical spectral analysis is no exception. We…

astro-ph.HE2021★ 5 cited

Timing techniques applied to distributed modular high-energy astronomy: the HERMES project

A. Sanna, A. F. Gambino, L. Burderi +15

The HERMES-TP/SP (High Energy Rapid Modular Ensemble of Satellites -- Technologic and Scientific Pathfinder) is an in-orbit demonstration of the so-called distributed astronomy con…

astro-ph.HE2021★ 24 cited

The HERMES-Technologic and Scientific Pathfinder

F. Fiore, L. Burderi, M. Lavagna +12

HERMES-TP/SP (High Energy Rapid Modular Ensemble of Satellites Technologic and Scientific Pathfinder) is a constellation of six 3U nano-satellites hosting simple but innovative X-r…

astro-ph.IM2021★ 28 cited

The scientific payload on-board the HERMES-TP and HERMES-SP CubeSat missions

Y. Evangelista, F. Fiore, F. Fuschino +22

HERMES (High Energy Rapid Modular Ensemble of Satellites) Technological and Scientific pathfinder is a space borne mission based on a LEO constellation of nano-satellites. The 3U C…

astro-ph.HE2020★ 12 cited

Evidence of a non-conservative mass transfer in the ultra-compact X-ray source XB 1916-053

R. Iaria, A. Sanna, T. Di Salvo +5

The dipping source XB 1916-053 is a compact binary system with an orbital period of 50 min harboring a neutron star. Using ten new {\it Chandra} observations and one {\it Swift/XRT…

astro-ph.HE2020★ 17 cited

Reflection component in the Bright Atoll Source GX 9+9

R. Iaria, S. M. Mazzola, T. Di Salvo +5

GX 9+9 (4U 1728-16) is a low mass X-ray binary (LMXB) source harboring a neutron star. Although it belongs to the subclass of the bright Atoll sources together with GX 9+1, GX 3+1,…

astro-ph.HE2020★ 13 cited

Timing of the accreting millisecond pulsar IGR J17591-2342: evidence of spin-down during accretion

A. Sanna, L. Burderi, K. C. Gendreau +8

We report on the phase-coherent timing analysis of the accreting millisecond X-ray pulsar IGR J17591-2342, using Neutron Star Interior Composition Explorer (NICER) data taken durin…

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.HE2019

Broadband spectral analysis of MXB 1659-298 in its soft and hard state

S. M. Mazzola, R. Iaria, A. F. Gambino +6

The X-ray transient eclipsing source MXB 1659-298 went in outburst in 1999 and 2015, respectively, during which it was observed by XMM-Newton, NuSTAR and Swift. Using these observa…

astro-ph.HE2019★ 30 cited

Indications of non-conservative mass-transfer in AMXPs

A. Marino, T. Di Salvo, L. Burderi +7

Context. Since the discovery of the first Accreting Millisecond X-ray Pulsar SAX J1808.4-3658 in 1998, the family of these sources kept growing on. Currently, it counts 22 members.…

astro-ph.HE2019★ 11 cited

Updated orbital ephemeris of the ADC source X 1822-371: a stable orbital expansion over 40 years

S. M. Mazzola, R. Iaria, T. Di Salvo +6

The source X 1822-371 is an eclipsing compact binary system with a period close to 5.57 hr and an orbital period derivative of 1.51(7) s s$^{-1…

astro-ph.HE2019★ 15 cited

Spectral analysis of the dipping LMXB system XB 1916-053

A. F. Gambino, R. Iaria, T. Di Salvo +6

Context: XB 1916-053 is a low mass X-ray binary system (LMXB) hosting a neutron star (NS) and showing periodic dips. The spectrum of the persistent emission was modeled with a blac…

astro-ph.IM2018★ 63 cited

HERMES: An ultra-wide band X and gamma-ray transient monitor on board a nano-satellite constellation

F. Fuschino, R. Campana, C. Labanti +49

The High Energy Modular Ensemble of Satellites (HERMES) project is aimed to realize a modular X/gamma-ray monitor for transient events, to be placed on-board of a CubeSat bus. This…

astro-ph.HE2018★ 14 cited

The broadband spectral analysis of 4U 1702-429 using XMM-Newton and BeppoSAX data

S. M. Mazzola, R. Iaria, T. Di Salvo +8

Most of the X-ray binary systems containing neutron stars classified as Atoll sources show two different spectral states, called soft and hard. Moreover, a large number of these sy…

astro-ph.HE2018★ 45 cited

NuSTAR and XMM-Newton broad-band spectrum of SAX J1808.4-3658 during its latest outburst in 2015

T. Di Salvo, A. Sanna, L. Burderi +4

The first discovered accreting millisecond pulsar, SAX J1808.4-3658, went into X-ray outburst in April 2015. We triggered a 100 ks XMM-Newton ToO, taken at the peak of the outburst…

astro-ph.HE2018★ 35 cited

NuSTAR and NICER reveal IGR J17591-2342 as a new accreting millisecond X-ray pulsar

A. Sanna, C. Ferrigno, P. S. Ray +21

We report on the discovery by the Nuclear Spectroscopic Telescope Array (NuSTAR) and the Neutron Star Interior Composition Explorer (NICER) of the accreting millisecond X-ray pulsa…

astro-ph.HE2018★ 24 cited

SWIFT J1756.9-2508: spectral and timing properties of its 2018 outburst

A. Sanna, F. Pintore, A. Riggio +8

We discuss the spectral and timing properties of the accreting millisecond X-ray pulsar SWIFT J1756.9-2508 observed by XMM-Newton, NICER and NuSTAR during the X-ray outburst occurr…

astro-ph.HE2018★ 15 cited

Broadband spectral analysis of MXB 1659-298 in its soft and hard state

R. Iaria, S. M. Mazzola, T. Bassi +7

The X-ray transient eclipsing source MXB 1659-298 went into outburst in 1999 and 2015. During these two outbursts the source was observed by XMM-Newton, nuSTAR, and Swift/XRT. Usin…

astro-ph.HE2017★ 13 cited

Evidence of a non-conservative mass transfer for XTE J0929-314

A. Marino, T. Di Salvo, A. F. Gambino +5

Context. In 1998 the first accreting millisecond pulsar, SAX J1808.4-3658, was discovered and to date 18 systems showing coherent, high frequency (> 100 Hz) pulsations in low mass…

astro-ph.HE2017★ 5 cited

Updating the orbital ephemeris of the dipping source XB 1254-690 and the distance to the source

A. F. Gambino, R. Iaria, T. Di Salvo +5

XB 1254-690 is a dipping low mass X-ray binary system hosting a neutron star and showing type I X-ray bursts. We aim at obtaining more accurate orbital ephemeris and at constrainin…