Results 81 to 90 of about 613 (180)

Challenges in Binary Pulsar Timing Detection of Dark Matter Subhalos

open access: yesThe Astrophysical Journal Letters
Recently, binary pulsar timing has been proposed as a viable probe of dark matter subhalos with masses of ∼10 ^7 M _⊙ in the solar neighborhood.
Zheng-Long Wang   +3 more
doaj   +1 more source

Augmentation Method for X-Ray Pulsar Navigation Using Time Difference of Arrival and Range Measurement, Based on Polarization Encoded Pulse Position Modulation

open access: yesAerospace
This paper addresses the use of the position difference between the reference satellite and the target spacecraft to improve X-ray pulsar navigation (XPNAV) for Earth orbit spacecraft. This is achieved by first installing an X-ray detector on the reference satellite whose position is accurately known.
Rong Jiao, Hua Zhang
openaire   +2 more sources

Graph-based Summary Statistics for Revealing the Stochastic Gravitational-wave Background in Pulsar Timing Arrays

open access: yesThe Astrophysical Journal
In this work, we propose a graph-based method implemented on the pulsar timing residuals for stochastic gravitational-wave background (SGWB) detection within the nanohertz frequency regime and examining uncertainties of its parameters.
M. Alakhras, S. M. S. Movahed
doaj   +1 more source

Investigation of Accuracy of TOA and SNR of Radio Pulsar Signals for Vehicles Navigation. [PDF]

open access: yesSensors (Basel), 2023
Kabakchiev H   +4 more
europepmc   +1 more source

Improving Pulsar Timing Precision with Single Pulse Fluence Clustering

open access: yesThe Astrophysical Journal
Traditional pulsar timing techniques involve averaging large numbers of single pulses to obtain a high signal-to-noise ratio (S/N) profile, which is cross-correlated with a template to measure a time of arrival (TOA).
Sofia V. Sosa Fiscella   +2 more
doaj   +1 more source

Algorithmic Pulsar Timer for Binaries

open access: yesThe Astrophysical Journal
Pulsar timing is a powerful tool that, by accounting for every rotation of a pulsar, precisely measures the spin frequency, spin frequency derivatives, astrometric position, binary parameters when applicable, properties of the interstellar medium, and ...
Jackson Taylor   +2 more
doaj   +1 more source

The NANOGrav 12.5 yr Dataset: Chromatic Noise Characterization and Mitigation with Time-domain Kernels

open access: yesThe Astrophysical Journal
Pulsar timing arrays (PTAs) have recently entered the detection era, quickly moving beyond the goal of simply improving sensitivity at the lowest frequencies for the sake of observing the stochastic gravitational wave background (GWB), and focusing on ...
Jeffrey S. Hazboun   +66 more
doaj   +1 more source

Optimising gravitational-wave sky maps for pulsar timing arrays

open access: yesAstronomy & Astrophysics
Context. Pulsar timing arrays (PTAs) have recently reported compelling evidence for the presence of a gravitational-wave background signal. Mapping the gravitational-wave background is key to understanding how it is formed, since anisotropy is a tracer ...
Grunthal Kathrin   +5 more
doaj   +1 more source

Future Space-based γ-Ray Pulsar Timing Arrays

open access: yesThe Astrophysical Journal Letters
Radio pulsar timing arrays (PTAs) of millisecond pulsars (MSPs) are beginning to detect nHz gravitational waves (GWs). MSPs are bright γ -ray emitters, and all-sky monitoring of ∼100 MSPs with the Fermi Large Area Telescope enables the γ -ray PTA (GPTA).
M. Kerr   +5 more
doaj   +1 more source

Home - About - Disclaimer - Privacy