activity
20082026
most citedA bimodal burst energy distribution of a repeating fast radio burst source

287 citations · 1.3k across the 22 of their papers we have counts for

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Showing astro-ph.HEShow all

12 papers · 1 filter

astro-ph.HE2026★ 4 cited

Searching for Anisotropy in the Gravitational Wave Background Using the Parkes Pulsar Timing Array

Yiqin Chen, Shi-Yi Zhao, Zhi-Zhang Peng +17

In recent years, several pulsar timing array collaborations have reported evidence for a nanohertz gravitational wave background (GWB). Such a background signal could be produced b…

astro-ph.HE2025★ 1 cited

Frequency- and phase-resolved polarimetry of millisecond pulsars and its application to timing

Małgorzata Curyło, Andrew Zic, Shuangqiang Wang +16

Pulsar timing is used for a variety of applications including tests of fundamental physics, probing the structure of neutron stars, and detecting nanohertz gravitational waves. Dev…

astro-ph.HE2025★ 5 cited

Ultra-Wideband Polarimetry of the April 2021 Profile Change Event in PSR J1713+0747

Rami F. Mandow, Andrew Zic, J. R. Dawson +15

The millisecond pulsar PSR J1713+0747 is a high-priority target for pulsar timing array experiments due to its long-term timing stability, and bright, narrow pulse profile. In Apri…

astro-ph.HE2021★ 287 cited

A bimodal burst energy distribution of a repeating fast radio burst source

D. Li, P. Wang, W. W. Zhu +29

The event rate, energy distribution, and time-domain behaviour of repeating fast radio bursts (FRBs) contains essential information regarding their physical nature and central engi…

astro-ph.HE2020★ 105 cited

Identifying and mitigating noise sources in precision pulsar timing data sets

Boris Goncharov, D. J. Reardon, R. M. Shannon +14

Pulsar timing array projects measure the pulse arrival times of millisecond pulsars for the primary purpose of detecting nanohertz-frequency gravitational waves. The measurements i…

astro-ph.HE2019★ 39 cited

Mode switching and oscillations in PSR B1828-11

I. H. Stairs, A. G. Lyne, M. Kramer +7

The young pulsar PSR B1828-11 has long been known to show correlated shape and spin-down changes with timescales of roughly 500 and 250 days, perhaps associated with large-scale ma…

astro-ph.HE2012★ 30 cited

Timing the main-sequence-star binary pulsar J1740-3052

E. C. Madsen, I. H. Stairs, M. Kramer +7

PSR J1740-3052 is a young pulsar in orbit around a companion that is most likely a B-type main-sequence star. Since its discovery more than a decade ago, data have been taken at se…

astro-ph.HE2011★ 30 cited

Observations of Energetic High Magnetic Field Pulsars with the Fermi Large Area Telescope

D. Parent, M. Kerr, P. R. Den Hartog +27

We report the detection of gamma-ray pulsations from the high-magnetic-field rotation-powered pulsar PSR J1119-6127 using data from the Fermi Large Area Telescope. The gamma-ray li…

astro-ph.HE2010★ 95 cited

Detection of the energetic pulsar PSR B1509-58 and its pulsar wind nebula in MSH 15-52 using the Fermi-Large Area Telescope

LAT Collaboration, Pulsar Timing Consortium

We report the detection of high energy gamma-ray emission from the young and energetic pulsar PSR B150958 and its pulsar wind nebula (PWN) in the composite supernova remnant SNR…

astro-ph.HE2010★ 118 cited

The Vela Pulsar: Results from the First Year of Fermi LAT Observations

A. A. Abdo

We report on analysis of timing and spectroscopy of the Vela pulsar using eleven months of observations with the Large Area Telescope on the Fermi Gamma-Ray Space Telescope. The in…

astro-ph.HE2010★ 58 cited

Discovery of Pulsed -rays from PSR J0034-0534 with the Fermi LAT: A Case for Co-located Radio and -ray Emission Regions

The Fermi LAT Collaboration, Pulsar Timing Consortium

Millisecond pulsars (MSPs) have been firmly established as a class of gamma-ray emitters via the detection of pulsations above 0.1 GeV from eight MSPs by the Fermi Large Area Teles…

astro-ph.HE2009★ 36 cited

Discovery of Pulsed Gamma Rays from the Young Radio Pulsar PSR J1028-5819 with the Fermi Large Area Telescope

LAT Collaboration

Radio pulsar PSR J1028-5819 was recently discovered in a high-frequency search (at 3.1 GHz)in the error circle of the EGRET source 3EG J1027-5817. The spin-down power of this young…