PALFA discovery of a highly relativistic double neutron star binary

K Stovall, PCC Freire, S Chatterjee… - The Astrophysical …, 2018 - iopscience.iop.org
We report the discovery and initial follow-up of a double neutron star (DNS) system, PSR
J1946+ 2052, with the Arecibo L-Band Feed Array pulsar (PALFA) survey. PSR J1946+ …

Optical spectroscopy and demographics of redback millisecond pulsar binaries

J Strader, S Swihart, L Chomiuk… - The Astrophysical …, 2019 - iopscience.iop.org
Optical Spectroscopy and Demographics of Redback Millisecond Pulsar Binaries - IOPscience
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High energy radiation from spider pulsars

CY Hui, KL Li - Galaxies, 2019 - mdpi.com
The population of millisecond pulsars (MSPs) has been expanded considerably in the last
decade. Not only is their number increasing, but also various classes of them have been …

An observationally derived kick distribution for neutron stars in binary systems

TN O'Doherty, A Bahramian… - Monthly Notices of …, 2023 - academic.oup.com
Understanding the natal kicks received by neutron stars (NSs) during formation is a critical
component of modelling the evolution of massive binaries. Natal kicks are an integral input …

Binary pulsar distances and velocities from gaia data release 2

RJ Jennings, DL Kaplan, S Chatterjee… - The Astrophysical …, 2018 - iopscience.iop.org
The second data release from the Gaia mission (Gaia DR2) includes, among its billion
entries, astrometric parameters for binary companions to a number of known pulsars …

Study of 72 pulsars discovered in the PALFA survey: Timing analysis, glitch activity, emission variability, and a pulsar in an eccentric binary

E Parent, H Sewalls, PCC Freire… - The Astrophysical …, 2022 - iopscience.iop.org
We present new discoveries and results from long-term timing of 72 pulsars discovered in
the Pulsar Arecibo L-band Feed Array (PALFA) survey, including precise determination of …

Comparison of dynamical and kinematic reference frames via pulsar positions from timing, Gaia, and interferometric astrometry

N Liu, Z Zhu, J Antoniadis, JC Liu, H Zhang… - Astronomy & …, 2023 - aanda.org
Context. Pulsars are special objects whose positions can be determined independently from
timing, radio interferometric, and Gaia astrometry at sub-milliarcsecond (mas) precision; …

4FGL J1120. 0–2204: A Unique Gamma-Ray-bright Neutron Star Binary with an Extremely Low-mass Proto-white Dwarf

SJ Swihart, J Strader, E Aydi, L Chomiuk… - The Astrophysical …, 2022 - iopscience.iop.org
We have discovered a new X-ray-emitting compact binary that is the likely counterpart to the
unassociated Fermi-LAT GeV γ-ray source 4FGL J1120. 0–2204, the second brightest Fermi …

Superradiance in rotating stars and pulsar-timing constraints on dark photons

V Cardoso, P Pani, TT Yu - Physical Review D, 2017 - APS
In the presence of massive bosonic degrees of freedom, rotational superradiance can trigger
an instability that spins down black holes. This leads to peculiar gravitational-wave …

Mass measurements for two binary pulsars discovered in the PALFA survey

WW Zhu, PCC Freire, B Knispel, B Allen… - The Astrophysical …, 2019 - iopscience.iop.org
In this paper, we present the results of timing observations of PSRs J1949+ 3106 and
J1950+ 2414, two binary millisecond pulsars (MSPs) discovered in data from the Arecibo …