activity
20202026
most citedIdentification of 3XMM J000511.8+634018 as a new polar at P(orb)=133.5 min -- is it inside or outside the period gap?

13 citations · 17 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.HE2026

Mass and radius measurements of the neutron star 47~Tuc X7 -- A new bias-free method

C. Kazantsev, S. Guillot, L. Mauviard +2

Neutron star (NS) radius measurements provide precious information to constrain the dense matter equation of state (EOS). Quiescent low-mass X-ray binaries (qLMXBs) have been used…

astro-ph.HE2026★ 2 cited

Multi-wavelength emission modelling of PSR~J04374715

J. Pétri, P. Stammler, L. Guillemot +4

The diversity of pulsar light-curves and radio polarisation properties originates in the structure of the magnetic field close to the stellar surface. For millisecond pulsars, this…

astro-ph.GA2025★ 2 cited

The multimessenger view of Pulsar Timing Array black holes with the Horizon-AGN simulation

Hippolyte Quelquejay Leclere, Kunyang Li, Marta Volonteri +5

We use the Horizon-AGN cosmological simulation to study the properties of supermassive black hole binaries (MBHBs) contributing most to the gravitational wave background (GWB) sign…

astro-ph.HE2024

On the nature of the 2.4 hr-period eclipsing cataclysmic variable W2 in 47 Tuc

R. Amato, N. La Palombara, M. Imbrogno +5

W2 (CXOGlb J002415.8-720436) is a cataclysmic variable (CV) in the Galactic globular cluster 47 Tucanae. Its modulation was discovered within the CATS@BAR project. The source shows…

astro-ph.SR2020★ 13 cited

Identification of 3XMM J000511.8+634018 as a new polar at P(orb)=133.5 min -- is it inside or outside the period gap?

A. D. Schwope, H. Worpel, N. A. Webb +2

We aimed to identify the variable X-ray source 3XMM J000511.8+634018, which was serendipitously discovered through routine inspections while the 3XMM catalogue was compiled. We ana…