activity
20132025
most citedRapid Modification of Neutron Star Surface Magnetic Field: A proposed mechanism for explaining Radio Emission State Changes in Pulsars

31 citations · 38 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.HE2025★ 4 cited

Born to be recycled: a comprehensive population synthesis of the Galactic millisecond pulsars

Mattéo Sautron, Jérôme Pétri, Dipanjan Mitra +2

Millisecond pulsars (MSPs) are the oldest but fastest pulsars known to date. In the 1980s, to explain how these pulsars could be formed, a new hypothesis was formulated: the recycl…

astro-ph.HE2024★ 2 cited

Localisation of the non-thermal X-ray emission of PSR~J2229+6114 from its multi-wavelength pulse profiles

J. Pétri, S. Guillot, L. Guillemot +5

Pulsars are detected over the whole electromagnetic spectrum, from radio wavelengths up to very high energies, in the GeV-TeV range. Whereas the radio emission site for young pulsa…

astro-ph.HE2024

The Galactic population of canonical pulsars II

Mattéo Sautron, Jérôme Pétri, Dipanjan Mitra +1

Pulsars are highly magnetized rotating neutron stars, emitting in a broad electromagnetic energy range. Reproducing the observed pulsars population refines our understanding of the…

astro-ph.HE2021★ 31 cited

Rapid Modification of Neutron Star Surface Magnetic Field: A proposed mechanism for explaining Radio Emission State Changes in Pulsars

U. Geppert, R. Basu, D. Mitra +2

The radio emission in many pulsars show sudden changes, usually within a period, that cannot be related to the steady state processes within the inner acceleration region (IAR) abo…

astro-ph.HE2013★ 1 cited

A combined GMRT/CLFST image of IC443 at 150 MHz

D. Mitra, D. A. Green, A. Pramesh Rao

IC443 is a relatively large Galactic (~45 arcmin) SNR with a high radio surface brightness. It has fine scale structure down to arcsec scales, and so is difficult to image on all a…