activity
19962026
most citedBounds on the Compactness of Neutron Stars from Brightness Oscillations

138 citations · 706 across the 16 of their papers we have counts for

collaborators

18 papers

astro-ph.HE2026

What We Have Learned from NICER About Neutron Star Radii

M. C. Miller

The cores of neutron stars have a combination of density, temperature, and neutron-proton asymmetry that cannot be replicated in laboratories or understood using first-principles q…

astro-ph.HE2026

Systematic Effects of Hydrogen and Helium Atmosphere Mismatch on Radius Inference in PSR~J0740+6620-like Synthetic NICER Data

Isiah M. Holt, M. Coleman Miller, Alexander J. Dittmann +1

Constraints on neutron star radii provide insight into the properties of the cold, dense matter in their interiors. Previous studies using synthetic Neutron star Interior Compositi…

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.HE2025

An Investigation of Systematic Effects from Background Priors on PSR J07406620 Radius Estimates using Synthetic NICER and XMM-Newton Data

Isiah M. Holt, M. Coleman Miller, Alexander J. Dittmann +1

Accurate and precise measurements of neutron star radii provide invaluable information about the cold, dense matter in neutron star cores. Analyses of synthetic X-ray pulse wavefor…

astro-ph.HE2024

A More Precise Measurement of the Radius of PSR J0740+6620 Using Updated NICER Data

Alexander J. Dittmann, M. Coleman Miller, Frederick K. Lamb +9

PSR J0740+6620 is the neutron star with the highest precisely determined mass, inferred from radio observations to be . Measurements of its radius therefo…

astro-ph.HE2023★ 5 cited

Nontrivial features in the speed of sound inside neutron stars

Debora Mroczek, M. Coleman Miller, Jacquelyn Noronha-Hostler +1

Measurements of neutron star masses, radii, and tidal deformability have direct connections to nuclear physics via the equation of state (EoS), which for the cold, catalyzed matter…