We report results from continued timing observations of PSR J0740+ 6620, a high-mass, 2.8
ms radio pulsar in orbit with a likely ultracool white dwarf companion. Our data set consists …

Young and rotation-powered neutron stars (NSs) are commonly observed as rapidly-
spinning pulsars. They dissipate their rotational energy by emitting pulsar wind with …

Despite its importance to our understanding of physics at supranuclear densities, the
equation of state (EoS) of matter deep within neutron stars remains poorly understood …

Fewer than a dozen gamma-ray pulsars were known when the Fermi Gamma-ray Space
Telescope was launched on 2008 June 11, and the extent and diversity of the population …

The first gravitational wave detections of mergers between black holes and neutron stars
represent a remarkable new regime of high-energy transient astrophysics. The signals …

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 …

The conventional wisdom, dating back to 2012, is that the mass distribution of Galactic
double neutron stars (DNSs) is well-fit by a Gaussian distribution with a mean of 1.33 M⊙ …

The maximal gravitational mass of nonrotating neutron stars (M TOV) is one of the key
parameters of compact objects and only loose bounds can be set based on the first …

We present the design, implementation, and performance of the digital pulsar observing
system constructed for the Canadian Hydrogen Intensity Mapping Experiment (CHIME) …

We present an overview of the LOFAR Tied-Array All-Sky Survey (LOTAAS) for radio pulsars
and fast transients. The survey uses the high-band antennas of the LOFAR Superterp, the …