activity
20162026
most citedeXTP -- enhanced X-ray Timing and Polarimetry Mission

176 citations · 1.6k across the 84 of their papers we have counts for

collaborators
Showing 2018Show all

7 papers · 1 filter

astro-ph.HE2018★ 34 cited

Physics and astrophysics of strong magnetic field systems with eXTP

Andrea Santangelo, Silvia Zane, Hua Feng +38

In this paper we present the science potential of the enhanced X-ray Timing and Polarimetry (eXTP) mission for studies of strongly magnetized objects. We will focus on the physics…

astro-ph.SR2018★ 57 cited

Distances to the globular clusters 47 Tucanae and NGC 362 using Gaia DR2 parallaxes

Seery Chen, Harvey Richer, Ilaria Caiazzo +1

Using parallaxes from Gaia DR2, we estimate the distance to the globular clusters 47 Tuc and NGC 362, taking advantage of the background stars in the Small Magellanic Cloud and qua…

astro-ph.GA2018★ 171 cited

A Multi-Mass Velocity Dispersion Model of 47 Tucanae Indicates No Evidence for an Intermediate Mass Black Hole

Christopher Mann, Harvey Richer, Jeremy Heyl +6

In this paper, we analyze stellar proper motions in the core of the globular cluster 47 Tucanae to explore the possibility of an intermediate-mass black hole (IMBH) influence on th…

astro-ph.HE2018★ 3 cited

Probing Black Hole Magnetic Fields with QED

Ilaria Caiazzo, Jeremy Heyl

The effect of vacuum birefringence is one of the first predictions of quantum electrodynamics (QED): the presence of a charged Dirac field makes the vacuum birefringent when thread…

astro-ph.HE2018★ 18 cited

Vacuum birefringence and the X-ray polarization from black-hole accretion disks

Ilaria Caiazzo, Jeremy Heyl

In the next decade, x-ray polarimetry will open a new window on the high-energy Universe, as several missions that include an x-ray polarimeter are currently under development. Obs…

astro-ph.HE2018★ 33 cited

PSR J17552550: A young radio pulsar with a massive, compact companion

C. Ng, M. U. Kruckow, T. M. Tauris +9

Radio pulsars found in binary systems with short orbital periods are usually fast spinning as a consequence of recycling via mass transfer from their companion stars; this process…