activity
20142023
most citedSearching for continuous Gravitational Waves in the second data release of the International Pulsar Timing Array

76 citations · 99 across the 5 of their papers we have counts for

collaborators

6 papers

astro-ph.HE2024

A Gaussian-processes approach to fitting for time-variable spherical solar wind in pulsar timing data

Iuliana C. Niţu, Michael J. Keith, Caterina Tiburzi +26

Propagation effects are one of the main sources of noise in high-precision pulsar timing. For pulsars below an ecliptic latitude of , the ionised plasma in the solar wind…

gr-qc202376 cited

Searching for continuous Gravitational Waves in the second data release of the International Pulsar Timing Array

M. Falxa, S. Babak, P. T. Baker +123

The International Pulsar Timing Array 2nd data release is the combination of datasets from worldwide collaborations. In this study, we search for continuous waves: gravitational wa…

astro-ph.HE20238 cited

Pulsar Scintillation Studies with LOFAR: II. Dual-frequency scattering study of PSR J0826+2637 with LOFAR and NenuFAR

Ziwei Wu, William A. Coles, Joris P. W. Verbiest +28

Interstellar scattering (ISS) of radio pulsar emission can be used as a probe of the ionised interstellar medium (IISM) and causes corruptions in pulsar timing experiments. Two typ…

astro-ph.SR2021

No Pulsar Companion Around the Nearest Low Mass White Dwarf

Tilemachos M. Athanasiadis, Nataliya K. Porayko, John Antoniadis +5

2MASS J050051.85093054.9 is the closest known low-mass helium-core white dwarf in a binary system. We used three high-band international LOFAR stations to perform a targeted sea…

astro-ph.HE201615 cited

Rapidly rotating neutron star progenitors

K. A. Postnov, A. G. Kuranov, D. A. Kolesnikov +2

Rotating proto-neutron stars can be important sources of gravitational waves to be searched for by present-day and future interferometric detectors. It was demonstrated by Imshenni…

astro-ph.IM2014

Pulsar timing constraints on narrow-band stochastic signals

Konstantin A. Postnov, Nataliya K. Porayko

We consider the sensitivity of the pulsar timing array (PTA) technique to specific kind of narrow-band stochastic signals in nano-Hz frequency range. Specifically, we examine the n…