WDs and neutron stars are far-reaching and multi-faceted laboratories in the hunt for dark
matter. We review detection prospects of wave-like, particulate, macroscopic and black hole …

ABSTRACT The HTRU-S Low Latitude survey data within 1° of the Galactic Centre (GC)
were searched for pulsars using the Fast Folding Algorithm (FFA). Unlike traditional Fast …

The discovery of radio pulsars (PSRs) around the supermassive black hole (SMBH) in our
Galactic Center (GC), Sagittarius A*(Sgr A*), will have significant implications for tests of …

We present the discovery of 37 pulsars from∼ 20 yr old archival data of the Parkes
Multibeam Pulsar Survey using a new FFT-based search pipeline optimized for discovering …

Radio wave scattering can cause severe reductions in detection sensitivity for surveys of
Galactic and extragalactic fast (∼ ms duration) transients. While Galactic sources like …

The MMGPS-L is the most sensitive pulsar survey in the Southern Hemisphere. We present
a follow-up study of one of these new discoveries, PSR J1208-5936, a 28.71-ms recycled …

The first test of strong-field gravity came from measurements of the relativistic orbital decay
in a binary pulsar system (Taylor & Weisberg 1982, 1989), with subsequent tests of …

Radio searches for extraterrestrial intelligence have mainly targeted the discovery of
narrowband continuous-wave beacons and artificially dispersed broadband bursts. Periodic …

The MPIfR-MeerKAT Galactic Plane survey at L-band (MMGPS-L) is the most sensitive
pulsar survey in the Southern Hemisphere, providing 78 discoveries in an area of 900 sq …

Neutron Stars (NSs), among the densest objects in the Universe, are exceptional
laboratories for investigating Dark Matter (DM) properties. Recent theoretical and …