Results 31 to 40 of about 13,694 (217)

Scattering Delay Mitigation in High-accuracy Pulsar Timing: Cyclic Spectroscopy Techniques

open access: yesThe Astrophysical Journal, 2023
We simulate scattering delays from the interstellar medium to examine the effectiveness of three estimators in recovering these delays in pulsar timing data. Two of these estimators use the more traditional process of fitting autocorrelation functions to
Jacob E. Turner   +5 more
doaj   +1 more source

Detection and localization of continuous gravitational waves with pulsar timing arrays: the role of pulsar terms [PDF]

open access: yes, 2016
A pulsar timing array is a Galactic-scale detector of nanohertz gravitational waves (GWs). Its target signals contain two components: the `Earth term' and the `pulsar term' corresponding to GWs incident on the Earth and pulsar respectively.
Hobbs, George   +7 more
core   +3 more sources

Pulsar time delay estimation method based on two-level compressed sensing

open access: yesActa Physica Sinica, 2018
In the traditional compressed sensing algorithms, the precision of the time delay estimation is closely related to the number of atoms in the dictionary. The bigger the atom number, the smaller the atomic interval becomes, thus the higher the accuracy of the time delay estimation will be.
null Kang Zhi-Wei   +4 more
openaire   +1 more source

Probing the properties of the pulsar wind via studying the dispersive effects in the pulses from the pulsar companion in a double neutron-star binary system [PDF]

open access: yes, 2017
The velocity and density distribution of $e^\pm$ in the pulsar wind are crucial distinction among magnetosphere models, and contains key parameters determining the high energy emission of pulsar binaries.
Cheng, K. S., Yi, Shu-Xu
core   +2 more sources

An evidence based time-frequency search method for gravitational waves from pulsar glitches

open access: yesJournal of Physics: Conference Series, 2008
We review and expand on a Bayesian model selection technique for the detection of gravitational waves from neutron star ring-downs associated with pulsar glitches. The algorithm works with power spectral densities constructed from overlapping time segments of gravitational wave data.
Clark, J.   +3 more
openaire   +2 more sources

Frequency-Dependent Template Profiles for High Precision Pulsar Timing [PDF]

open access: yes, 2018
Pulsar timing experiments require high fidelity template profiles in order to minimize the biases in pulse time-of-arrival (TOA) measurements and their uncertainties.
Pennucci, Timothy T.
core   +2 more sources

Observing gravitational wave bursts in pulsar timing measurements

open access: yes, 2010
We propose a novel method for observing the gravitational wave signature of super-massive black hole (SMBH) mergers. This method is based on detection of a specific type of gravitational waves, namely gravitational wave burst with memory (BWM), using ...
Baskaran   +42 more
core   +1 more source

Generative pulsar timing analysis

open access: yes, 2015
A new Bayesian method for the analysis of folded pulsar timing data is presented that allows for the simultaneous evaluation of evolution in the pulse profile in either frequency or time, along with the timing model and additional stochastic processes ...
Alexander, P., Hobson, M. P., Lentati, L
core   +1 more source

The optimal filters for the construction of the ensemble pulsar time [PDF]

open access: yes, 2008
The algorithm of the ensemble pulsar time based on the optimal Wiener filtration method has been constructed. This algorithm allows the separation of the contributions to the post-fit pulsar timing residuals of the atomic clock and pulsar itself. Filters
Rodin, Alexander E.
core   +1 more source

Pulsar Timing with the Fermi LAT

open access: yes, 2010
We present an overview of precise pulsar timing using data from the Large Area Telescope (LAT) on Fermi. We describe the analysis techniques including a maximum likelihood method for determining pulse times of arrival from unbinned photon data.
Kerr, Matthew   +3 more
core   +1 more source

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