most citedImproving pulsar search efficiency in next-generation pulsar surveys with artificial intelligence

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astro-ph.IM2026

Pulsar Timing Array Sensitivity to Anisotropy: Empirical Sensitivity Curves, Scaling Relations, and the Multi-Resolution Pixel Basis

Taha T. Moursy, Nihan S. Pol, Gabriella Agazie +115

We quantify pulsar timing array (PTA) sensitivity to anisotropy in the gravitational wave background using the cross-correlation based Fisher information matrix in the pixel and sp…

astro-ph.IM2026

The Murchison Widefield Array Phase III upgrade: Sensitivity Doubled, Number of Baselines Quadrupled, Flexibility Enhanced, and EoR Observations Optimised

S. J. Tingay, M. Johnston-Hollitt, R. B. Wayth +32

We describe the latest iteration of upgrades (designated Phase III) to the Murchison Widefield Array (MWA), in the fourth paper in a series that covers the evolution of the telesco…

astro-ph.IM2026

MWA tied-array processing V: Super-resolved localisation via amplitude-only maximum likelihood direction finding

Bradley W. Meyers, Arash Bahramian

Interferometric localisation of transients and pulsars via tied-array beam processing is challenging and can be limited by the native spatial resolution achievable by the instrumen…

astro-ph.IM2026

CHIME/Slow overview and pilot survey: A new backend to search for second-duration radio transients with the CHIME telescope

Sujay Mate, Kevin Luke, Yash Bhusare +23

We present an overview of CHIME/Slow, a real-time transient search backend under development to search for second-duration radio transients using the CHIME telescope, and results o…

astro-ph.IM2025★ 1 cited

Improving pulsar search efficiency in next-generation pulsar surveys with artificial intelligence

Qiuyang Fu, Mengyao Xue, Weiwei Zhu +12

Pulsar searching with next-generation radio telescopes requires efficiently sifting through millions of candidates generated by search pipelines to identify the most promising ones…