collaborators

5 papers

astro-ph.HE2026

The MeerKAT Thousand-Pulsar Polarisation Array II: Searches for Ultralight Axion-Like Dark Matter

Zi-Yan Yuwen, Michael Sarkis, Yin-Zhe Ma +4

We construct Pulsar Polarisation Arrays (PPA), using regular pulsars monitored in MeerKAT's Thousand Pulsar Array (TPA) Programme, to search for Axion-like Dark Matter (ALDM) withi…

astro-ph.HE2026

The MeerKAT Thousand-Pulsar Polarization Array I: Properties of the Polarization and Rotation Measure Time Series Data

Michael Sarkis, Zi-Yan Yuwen, Yin-Zhe Ma +4

The polarimetry of recent pulsar observations has provided a wealth of observational data with which to test physical theories of emission mechanisms, radiative transfer and even t…

astro-ph.CO2026

Exploring the High-Redshift 21-cm Signal via Self-Consistent Simulations using Artificial Neural Network Emulation

Colton R. Feathers, Eli Visbal, Steven Murray +2

We present a novel, self-consistent, semi-numeric Cosmic Dawn (CD) simulation in which small-scale star formation (SF) is calibrated to the \emph{AEOS} and \emph{Renaissance} hydro…

astro-ph.CO2026

Primordial black holes and the velocity acoustic oscillations features in 21 cm signals from the cosmic Dark Ages

Zhihe Zhang, Bin Yue, Yidong Xu +2

Astrophysical luminous objects such as the first stars have not yet formed in the Dark Ages. However, primordial black holes (PBHs) always exist throughout cosmic history since the…

astro-ph.CO2025

An independent estimate of H(z) at z = 0.5 from the stellar ages of brightest cluster galaxies

S. Ilani Loubser, Adebusola B. Alabi, Matt Hilton +6

Several cosmological observations (e.g., Cosmic Microwave Background (CMB), Supernovae Type Ia, and local distance ladder measurements such as Cepheids) have been used to measure t…