activity
19952022
most citedIsolated neutron stars: Magnetic fields, distances, and spectra

112 citations · 1k across the 32 of their papers we have counts for

collaborators

31 papers

astro-ph.HE2022★ 31 cited

Measuring the mass of the black widow PSR J1555-2908

M. R. Kennedy, R. P. Breton, C. J. Clark +8

Accurate measurements of the masses of neutron stars are necessary to test binary evolution models, and to constrain the neutron star equation of state. In pulsar binaries with no…

astro-ph.HE2021★ 15 cited

Profile changes associated with DM events in PSR J1713+0747

Fang Xi Lin, Hsiu-Hsien Lin, Jing Luo +5

Propagation effects in the interstellar medium and intrinsic profile changes can cause variability in the timing of pulsars, which limits the accuracy of fundamental science done v…

astro-ph.HE2021★ 8 cited

A search for radio pulsars in five nearby supernova remnants

S. Sett, R. P. Breton, C. J. Clark +2

Most neutron stars are expected to be born in supernovae, but only about half of supernova remnants (SNRs) are associated with a compact object. In many cases, a supernova progenit…

astro-ph.HE2020★ 47 cited

PSR J1012+5307: a millisecond pulsar with an extremely low-mass white dwarf companion

D. Mata Sánchez, A. G. Istrate, M. H. van Kerkwijk +2

Binaries harbouring millisecond pulsars enable a unique path to determine neutron star masses: radio pulsations reveal the motion of the neutron star, while that of the companion c…

astro-ph.HE2018★ 26 cited

A Dense Companion to the Short-Period Millisecond Pulsar Binary PSR J0636+5128

D. L. Kaplan, K. Stovall, M. H. van Kerkwijk +2

PSR J0636+5128 is a millisecond pulsar in one of the most compact pulsar binaries known, with a 96\,min orbital period. The pulsar mass function suggests a very low-mass companion,…

astro-ph.HE2018★ 29 cited

Nebular spectroscopy of SN 2014J: Detection of stable nickel in near infrared spectra

S. Dhawan, A. Flörs, B. Leibundgut +5

We present near infrared (NIR) spectroscopy of the nearby supernova 2014J obtained 450 d after explosion. We detect the [Ni II] 1.939 m line in the spectra indicating the…