activity
20172019
most citedPSR J0030+0451 Mass and Radius from NICER Data and Implications for the Properties of Neutron Star Matter

1.8k citations · 4.6k across the 11 of their papers we have counts for

collaborators

8 papers

astro-ph.HE2019174 cited

Constraining the Neutron Star Mass-Radius Relation and Dense Matter Equation of State with NICER. I. The Millisecond Pulsar X-ray Data Set

Slavko Bogdanov, Sebastien Guillot, Paul S. Ray +27

We present the set of deep Neutron Star Interior Composition Explorer (NICER) X-ray timing observations of the nearby rotation-powered millisecond pulsars PSRs J0437-4715, J0030+04…

astro-ph.HE20191.8k cited

PSR J0030+0451 Mass and Radius from NICER Data and Implications for the Properties of Neutron Star Matter

M. C. Miller, F. K. Lamb, A. J. Dittmann +18

Neutron stars are not only of astrophysical interest, but are also of great interest to nuclear physicists, because their attributes can be used to determine the properties of the…

astro-ph.HE2019272 cited

A NICER view of PSR J0030+0451: Implications for the dense matter equation of state

G. Raaijmakers, T. E. Riley, A. L. Watts +14

Both the mass and radius of the millisecond pulsar PSR J0030+0451 have been inferred via pulse-profile modeling of X-ray data obtained by NASA's NICER mission. In this Letter we st…

astro-ph.HE201925 cited

Modelling decretion discs in Be/X-ray binaries

R. O. Brown, M. J. Coe, W. C. G. Ho +1

As the largest population of high mass X-ray binaries, Be/X-ray binaries provide an excellent laboratory to investigate the extreme physics of neutron stars. It is generally accept…

astro-ph.HE20198 cited

Modelling the observable behaviour of SXP 5.05

R. O. Brown, M. J. Coe, W. C. G. Ho +1

SXP 5.05 is a Be/X-ray binary with a neutron star companion located in the Small Magellanic Cloud. It was first detected in 2013, and later that year, SXP 5.05 underwent a massive…

astro-ph.HE201955 cited

Diffusive nuclear burning in cooling simulations and application to new temperature data of the Cassiopeia A neutron star

M. J. P. Wijngaarden, Wynn C. G. Ho, Philip Chang +4

A critical relation in the study of neutron star cooling is the one between surface temperature and interior temperature. This relation is determined by the composition of the neut…