activity
20172026
most citedExoClock Project III: 450 new exoplanet ephemerides from ground and space observations

77 citations · 539 across the 43 of their papers we have counts for

collaborators

43 papers

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.IM2025

Accretion and Ejection Physics at High Time Resolution

F. M. Vincentelli, P. Casella, A. Veledina +18

Accretion onto compact objects is one of the most fundamental phenomena in the astrophysics, powering some of the most luminous objects in the sky. Along with this, accretion has a…

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

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.HE2024★ 1 cited

X-ray and optical polarization aligned with the radio jet ejecta in GX 339-4

G. Mastroserio, B. De Marco, M. C. Baglio +27

We present the first X-ray polarization measurements of GX 339-4. IXPE observed this source twice during its 2023-2024 outburst, once in the soft-intermediate state and again durin…

astro-ph.HE2024★ 7 cited

Swift X-Ray and UV Observations of six Gaia Binaries supposedly containing a Neutron Star

B. Sbarufatti, F. Coti Zelati, A. Marino +3

Recent observations have led to the discovery of numerous optically selected binaries containing an undetected component with mass consistent with a compact object (neutron star or…

astro-ph.HE2024

An X-ray and radio view of the 2022 reactivation of the magnetar SGRJ1935+2154

A. Y. Ibrahim, A. Borghese, F. Coti Zelati +19

Recently, the Galactic magnetar SGR J1935+2154 has garnered attention due to its emission of an extremely luminous radio burst, reminiscent of Fast Radio Bursts (FRBs). SGR J1935+2…

astro-ph.HE2023★ 2 cited

Low Magnetic-Field Neutron Stars in X-ray Binaries

Tiziana Di Salvo, Alessandro Papitto, Alessio Marino +2

In this chapter we give an overview of the properties of X-ray binary systems containing a weakly magnetized neutron star. These are old (Giga-years life-time) semi-detached binary…

astro-ph.HE2023

Spectral Analysis of the LMXB XTE J1810-189 with NICER Data

A. Manca, A. Sanna, A. Marino +6

XTE J1810-189 is a Low-Mass X-ray Binary transient system hosting a neutron star, which underwent a three-month-long outburst in 2020. In order to study its spectral evolution duri…

astro-ph.HE2023★ 16 cited

The accretion/ejection link in the neutron star X-ray binary 4U 1820-30 I: A boundary layer-jet coupling?

A. Marino, T. D. Russell, M. Del Santo +16

The accretion flow / jet correlation in neutron star (NS) low-mass X-ray binaries (LMXBs) is far less understood when compared to black hole (BH) LMXBs. In this paper we will prese…

astro-ph.HE2023★ 1 cited

Thermonuclear Type-I X-ray Bursts and Burst Oscillations from the Eclipsing AMXP Swift J1749.4-2807

A. C. Albayati, P. Bult, D. Altamirano +10

Swift J1749.4-2807 is the only known eclipsing accreting millisecond X-ray pulsar. In this paper, we report on 7 thermonuclear (Type-I) X-ray bursts observed by NICER during its 20…

astro-ph.HE2023★ 36 cited

First detection of X-ray polarization from the accreting neutron star 4U 1820-303

Alessandro Di Marco, Fabio La Monaca, Juri Poutanen +116

This paper reports the first detection of polarization in the X-rays for atoll-source 4U 1820-303, obtained with the Imaging X-ray Polarimetry Explorer (IXPE) at 99.999% confidence…

astro-ph.HE2023★ 10 cited

An ultrafast outflow in the black hole candidate MAXI J1810-222?

M. Del Santo, C. Pinto, A. Marino +9

The transient X-ray source MAXI J1810-222 was discovered in 2018 and has been active ever since. A long combined radio and X-ray monitoring campaign was performed with ATCA and Swi…

astro-ph.HE2023★ 14 cited

Localisation of gamma-ray bursts from the combined SpIRIT+HERMES-TP/SP nano-satellite constellation

Matt Thomas, Michele Trenti, Riccardo Campana +24

Multi-messenger observations of the transient sky to detect cosmic explosions and counterparts of gravitational wave mergers critically rely on orbiting wide-FoV telescopes to cove…

astro-ph.HE2022★ 19 cited

Timing analysis of the 2022 outburst of the accreting millisecond X-ray pulsar SAX J1808.43658: hints of an orbital shrinking

Giulia Illiano, Alessandro Papitto, Andrea Sanna +19

We present a pulse timing analysis of NICER observations of the accreting millisecond X-ray pulsar SAX J1808.43658 during the outburst that started on 2022 August 19. Similar to…

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.EP2022★ 77 cited

ExoClock Project III: 450 new exoplanet ephemerides from ground and space observations

A. Kokori, A. Tsiaras, B. Edwards +214

The ExoClock project has been created with the aim of increasing the efficiency of the Ariel mission. It will achieve this by continuously monitoring and updating the ephemerides o…

astro-ph.HE2022★ 11 cited

Unveiling the disc structure in ultraluminous X-ray source NGC 55 ULX-1

F. Barra, C. Pinto, D. J. Walton +11

Despite two decades of studies, it is still not clear whether ULX spectral transitions are due to stochastic variability in the wind or variations in the accretion rate or in the s…

astro-ph.HE2022★ 6 cited

A transient ultraluminous X-ray source in NGC 55

A. Robba, C. Pinto, F. Pintore +14

Ultraluminous X-ray sources (ULXs) are a class of accreting compact objects with X-ray luminosities above 10 erg s. The average number of ULXs per galaxy is still not…

astro-ph.HE2022★ 20 cited

Outflows and spectral evolution in the eclipsing AMXP SWIFT J1749.4-2807 with NICER, XMM-Newton and NuSTAR

A. Marino, A. Anitra, S. M. Mazzola +18

The neutron star low-mass X-ray binary SWIFT J1749.4-2807 is the only known eclipsing accreting millisecond X-ray pulsar. In this manuscript we perform a spectral characterization…

astro-ph.HE2022★ 10 cited

On the peculiar long-term orbital evolution of the eclipsing accreting millisecond X-ray pulsar SWIFT J1749.4-2807

A. Sanna, L. Burderi, T. Di Salvo +15

We present the pulsar timing analysis of the accreting millisecond X-ray pulsar SWIFT J1749.4-2807 monitored by NICER and XMM-Newton during its latest outburst after almost eleven…

astro-ph.HE2022★ 8 cited

Investigating the nature and properties of MAXI J1810-222 with radio and X-ray observations

T. D. Russell, M. Del Santo, A. Marino +10

We present results from radio and X-ray observations of the X-ray transient MAXI J1810-222. The nature of the accretor in this source has not been identified. In this paper, we sho…

astro-ph.HE2022★ 10 cited

Investigating the nature of the ultraluminous X-ray sources in the galaxy NGC 925

Chiara Salvaggio, Anna Wolter, Fabio Pintore +7

Variability is a powerful tool to investigate properties of X-ray binaries (XRB), in particular for Ultraluminous X-ray sources (ULXs) that are mainly detected in the X-ray band. F…