Results 111 to 120 of about 12,076,896 (214)
Exploring the concept of a massive photon has been an important area in astronomy and physics. If photons have mass, their propagation in nonvacuum space would be affected by both the nonzero mass m _γ and the presence of a plasma medium. This would lead
Yu-Bin Wang +3 more
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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
We present a timing solution for the 5.31 ms spider millisecond pulsar (MSP) J1242−4712, discovered with the GMRT. PSR J1242−4712 orbits a companion of minimum mass 0.08 M _⊙ with an orbital period of 7.7 hr and occupies a relatively unexplored region in
Ankita Ghosh +9 more
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Challenges in Binary Pulsar Timing Detection of Dark Matter Subhalos
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
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We present a practical implementation of a phase-coherent mapping technique for pulsar timing arrays that resolves the full complex polarisation state of the gravitational-wave sky as a function of direction and frequency.
Małgorzata Curyło +3 more
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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
Pulsar timing anomaly detection using Bayesian estimation
The sensitivity of nanohertz gravitational wave detection relies heavily on the data quality of pulsar timing arrays. However, observational data inevitably contain non-Gaussian outliers, which severely degrade the accuracy of parameter estimation under ...
Liang Bo +5 more
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Improving Pulsar Timing Precision with Single Pulse Fluence Clustering
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
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Investigation of Accuracy of TOA and SNR of Radio Pulsar Signals for Vehicles Navigation. [PDF]
Kabakchiev H +4 more
europepmc +1 more source

