activity
20042026
most citedA NICER View of the Nearest and Brightest Millisecond Pulsar: PSR J0437$\unicode{x2013}$4715

273 citations · 1.1k across the 34 of their papers we have counts for

collaborators
Showing 2024Show all

11 papers · 1 filter

astro-ph.HE2024★ 2 cited

Pulse Profiles of Accreting Neutron Stars from GRMHD Simulations

Pushpita Das, Tuomo Salmi, Jordy Davelaar +2

The pulsed X-ray emission from the neutron star surface acts as a window to study the state of matter in the neutron star interior. For accreting millisecond pulsars, the surface X…

astro-ph.IM2024★ 3 cited

STROBE-X Mission Overview

Paul S. Ray, Peter W. A. Roming, Andrea Argan +54

We give an overview of the science objectives and mission design of the Spectroscopic Time-Resolving Observatory for Broadband Energy X-rays (STROBE-X) observatory, which has been…

astro-ph.HE2024★ 15 cited

Probing fermionic asymmetric dark matter cores using global neutron star properties

Nathan Rutherford, Chanda Prescod-Weinstein, Anna Watts

It is possible for asymmetric dark matter (ADM) to accumulate in neutron star interiors and affect their global properties. Considering the effects of this accumulation, neutron st…

astro-ph.HE2024★ 86 cited

A NICER View of PSR J12311411: A Complex Case

Tuomo Salmi, Julia S. Deneva, Paul S. Ray +16

Recent constraints on neutron star mass and radius have advanced our understanding of the equation of state (EOS) of cold dense matter. Some of them have been obtained by modeling…

astro-ph.HE2024★ 2 cited

Parameter constraints for accreting millisecond pulsars with synthetic NICER data

Bas Dorsman, Tuomo Salmi, Anna L. Watts +10

Pulse profile modelling (PPM) is a technique for inferring mass, radius and hotspot properties of millisecond pulsars. PPM is now regularly used for analysis of rotation-powered mi…

nucl-th2024★ 35 cited

Neutron stars and the dense matter equation of state: from microscopic theory to macroscopic observations

Katerina Chatziioannou, H. Thankful Cromartie, Stefano Gandolfi +4

The past years have witnessed tremendous progress in understanding the properties of neutron stars and of the dense matter in their cores, made possible by electromagnetic observat…