activity
19922026
most citedPSR J0030+0451 Mass and Radius from NICER Data and Implications for the Properties of Neutron Star Matter

1.8k citations · 9k across the 56 of their papers we have counts for

collaborators

57 papers

astro-ph.HE2026

The Radius of the Neutron Star PSR J0614-3329 from NICER Data

M. C. Miller, A. J. Dittmann, I. M. Holt +14

Neutron star radius measurements, particularly using X-ray data collected with the Neutron star Interior Composition Explorer (NICER), have provided invaluable information for mode…

astro-ph.HE2026

The Impact of Errors in the Shape Function of Rotating Neutron Stars in the Oblate Schwarzschild Approximation

John Ming Ngo, Charlee Amason, Sharon M. Morsink

Measurements of thermal X-ray flux emitted by neutron stars can constrain their radii and the equation of state of cold dense matter. Accurate flux modeling of rapidly rotating neu…

astro-ph.HE2025★ 8 cited

The Radius of PSR J0437-4715 from NICER Data

M. C. Miller, A. J. Dittmann, I. M. Holt +12

Neutron star Interior Composition Explorer (NICER) data have been used to estimate the masses and radii of the rotation-powered millisecond pulsars PSR J00300451, PSR J074066…

astro-ph.HE2025★ 2 cited

Rotating Neutron Stars with Dark Matter Halos

Shafayat Shawqi, Andreas Konstantinou, Sharon M. Morsink

If dark matter (DM) exists in halos around rotating neutron stars (NSs), it will be essential to understand the effects of rotation on the distribution of DM and baryonic matter (B…

astro-ph.HE2025★ 2 cited

Gravitational Redshift for Rapidly Rotating Neutron Stars

Zsombor Jakab, Sharon Morsink

The Oblate Schwarzschild (OS) approximation is a method often used to compute the flux of X-rays emitted from a rapidly rotating neutron star. In this approximation, the oblate sha…

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…