activity
20182023
most citedProlonged sub-luminous state of the new transitional pulsar candidate CXOU J110926.4-650224

38 citations · 266 across the 18 of their papers we have counts for

collaborators

18 papers

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.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.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.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.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.HE2019★ 3 cited

Discovery and Identification of MAXI J1621-501 as a Type I X-ray Burster with a Super-Orbital Period

Nicholas M. Gorgone, Chryssa Kouveliotou, Hitoshi Negoro +26

MAXI J1621-501 is the first Swift/XRT Deep Galactic Plane Survey transient that was followed up with a multitude of space missions (NuSTAR, Swift, Chandra, NICER, INTEGRAL, and MAX…

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.HE2019★ 38 cited

Prolonged sub-luminous state of the new transitional pulsar candidate CXOU J110926.4-650224

Francesco Coti Zelati, Alessandro Papitto, Domitilla de Martino +12

We report on a multi-wavelength study of the unclassified X-ray source CXOU J110926.4-650224 (J1109). We identified the optical counterpart as a blue star with a magnitude of $\sim…

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★ 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★ 27 cited

XMM-Newton detection of the 2.1 ms coherent pulsations from IGR J17379-3747

A. Sanna, E. Bozzo, A. Papitto +7

We report on the detection of X-ray pulsations at 2.1 ms from the known X-ray burster IGR J17379-3747 using XMM-Newton. The coherent signal shows a clear Doppler modulation from wh…

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…