activity
20162025
most citedDense matter with eXTP

135 citations · 268 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.HE2025★ 2 cited

Identification and characterisation of the gamma-ray counterpart of the transitional pulsar candidate CXOU J110926.4-650224

A. Manca, F. Coti Zelati, J. Li +9

Transitional millisecond pulsars (tMSPs) represent a crucial link between the rotation-powered and accretion-powered states of binary pulsars. During their active X-ray state, tMSP…

astro-ph.HE2021

GrailQuest & HERMES: Hunting for Gravitational Wave Electromagnetic Counterparts and Probing Space-Time Quantum Foam

L. Burderi, T. Di Salvo, A. Sanna +5

GrailQuest (Gamma-ray Astronomy International Laboratory for Quantum Exploration of Space-Time) is an ambitious astrophysical mission concept that uses a fleet of small satellites…

astro-ph.HE2018★ 72 cited

Observatory science with eXTP

Jean J. M. in 't Zand, Enrico Bozzo, Jinlu Qu +181

In this White Paper we present the potential of the enhanced X-ray Timing and Polarimetry (eXTP) mission for studies related to Observatory Science targets. These include flaring s…

astro-ph.HE2018★ 135 cited

Dense matter with eXTP

Anna L. Watts, Wenfei Yu, Juri Poutanen +73

In this White Paper we present the potential of the Enhanced X-ray Timing and Polarimetry (eXTP) mission for determining the nature of dense matter; neutron star cores host an extr…

astro-ph.HE2016★ 45 cited

Timing of the accreting millisecond pulsar SAX J1748.9-2021 during its 2015 outburst

A. Sanna, L. Burderi, A. Riggio +6

We report on the timing analysis of the 2015 outburst of the intermittent accreting millisecond X-ray pulsar SAX J1748.9-2021 observed on March 4 by the X-ray satellite XMM-Newton.…

astro-ph.HE2016★ 14 cited

New orbital ephemerides for the dipping source 4U 1323-619: constraining the distance to the source

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

4U 1323-619 is a low mass X-ray binary system that shows type I X-ray bursts and dips. The most accurate estimation of the orbital period is 2.941923(36) hrs and a distance from th…