output
20072026
most citedSearch for an isotropic gravitational-wave background with the Parkes Pulsar Timing Array

1.2k citations

48 papers

astro-ph.SR2026★ 1 cited

The effect of interstellar scattering on coherent radio emission from stars: the case of CU Vir

J. S. Morgan, B. Das, H. E. Bignall

A subset of magnetic stars exhibit periodic radio pulses produced by the coherent electron cyclotron maser mechanism. These pulses are known to exhibit both temporal and spectral v…

astro-ph.HE2026★ 2 cited

ASKAP J005512.2-255834: A Luminous, Long-Lived Radio Transient at z = 0.1 -- an Orphan Afterglow or an off-nuclear TDE from an IMBH?

Ashna Gulati, Tara Murphy, David L. Kaplan +24

We report the discovery of a slowly evolving, extragalactic radio transient, ASKAP J005512.2--255834 (hereafter ASKAP J0055-2558), identified using the Australian SKA Pathfinder in…

astro-ph.IM2025

Enhancing evidence estimation through informed probability density approximation

El Mehdi Zahraoui, Patricio Maturana-Russel, Avi Vajpeyi +3

We introduce the Morph approximation, a class of product approximations of probability densities that selects low-order disjoint parameter blocks by maximizing the sum of their tot…

astro-ph.HE2025★ 1 cited

Tackling artefacts in the timing of relativistic pulsar binaries: towards the SKA

Huanchen Hu, Nataliya K. Porayko, Willem van Straten +3

Common signal-processing approximations produce artefacts when timing pulsars in relativistic binary systems, especially edge-on systems with tight orbits, such as the Double Pulsa…

astro-ph.HE2025

Search for H2 cloudlets in our backyard

A. V. Popkova, M. S. Pshirkov, A. V. Tuntsov

Several observational lines of evidence imply that a fraction of the dark matter in the Galaxy may be comprised of small cold clouds of molecular hydrogen. Such objects are difficu…

astro-ph.HE2024★ 2 cited

Magnetic amplification in premerger neutron stars through resonance-induced magnetorotational instabilities

Arthur G. Suvorov, Hao-Jui Kuan, Alexis Reboul-Salze +1

Tidal resonances in the final seconds of a binary neutron-star inspiral can excite oscillation modes in one or both of the constituents to large amplitudes. Under favorable circums…