collaborators

8 papers

astro-ph.HE2026

Understanding Pulsar Magnetospheres with the SKAO

L. S. Oswald, A. Basu, M. Chakraborty +21

The SKA telescopes will bring unparalleled sensitivity across a broad radio band, a wide field of view across the Southern sky, and the capacity for sub-arraying, all of which make…

astro-ph.HE2026

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.HE2025

Understanding pulsar magnetospheres with the SKAO

L. S. Oswald, A. Basu, M. Chakraborty +22

The SKA telescopes will bring unparalleled sensitivity across a broad radio band, a wide field of view across the Southern sky, and the capacity for sub-arraying, all of which make…

astro-ph.HE2025

Combining the second data release of the European Pulsar Timing Array with low-frequency pulsar data

F. Iraci, A. Chalumeau, C. Tiburzi +46

Low-frequency radio data improve the sensitivity of pulsar timing arrays (PTAs) to propagation effects such as dispersion measure (DM) variations, enabling better noise characteriz…

astro-ph.HE2025

A double dipole geometry for PSR~J0740+6620

J. Pétri, S. Guillot, L. Guillemot +5

Millisecond pulsars are known to show complex radio pulse profiles and polarisation position angle evolution with rotational phase. Small scale surface magnetic fields and multipol…

astro-ph.HE2025

A coherent radio burst from an X-ray neutron star in the Carina Nebula

K. M. Rajwade, J. Tian, G. Younes +10

The neutron star zoo comprises several sub-populations that range from energetic magnetars and thermally emitting X-ray neutron stars to radio-emitting pulsars. Despite studies ove…