activity
20202026
most citedA NICER View of the Nearest and Brightest Millisecond Pulsar: PSR J0437$\unicode{x2013}$4715

273 citations · 1k across the 23 of their papers we have counts for

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astro-ph.HE2026

Equation of state and neutron star properties with new mass-radius constraints from PSR~J1614--2230, PSR~J2124--3358, and 47~Tuc~X7

Melissa Mendes, Isak Svensson, Hannah Gottling +9

We study the impact of new mass-radius information from PSR J1614-2230, PSR J2124-3358, and 47 Tuc X7 in a combined equation of state inference based on chiral effective field theo…

astro-ph.HE2026

A NICER view of PSR J16142230: a massive and compact millisecond pulsar

Lucien Mauviard, Sebastien Guillot, Lami Suleiman +17

Using pulse profile modeling, we obtain the mass-radius measurement of a millisecond pulsar (MSP) with data from the Neutron Star Interior Composition ExploreR, XMM-Newton and the…

astro-ph.HE2026

A NICER view of the millisecond pulsar PSR J21243358: evidence for a helium atmosphere

Denis González-Caniulef, Sebastien Guillot, Pierre Stammler +12

Pulse profile modeling has proven to be a powerful technique for determining the mass and radius of neutron stars. To date, this method has been applied to a handful of millisecond…

astro-ph.HE2026

Pulse profile modelling of the 2024 outburst of the accreting millisecond pulsar SRGA J144459.2-604207

Bas Dorsman, Tuomo Salmi, Anna L. Watts +14

Pulse profile modelling via relativistic ray-tracing can constrain the system parameters of neutron stars, notably their mass and radius. Among these objects, accreting millisecond…

astro-ph.HE2026

A NICER View of PSR J0030+0451: Updated Constraints from Six Years of NICER Observations

Yves Kini, Lucien Mauviard, Tuomo Salmi +13

Pulse-profile modeling of rotation-powered millisecond pulsars targeted by NICER has enabled mass--radius constraints of several neutron star sources, with implications for the den…