Axion clouds around neutron stars
Recent work has shown that axions can be efficiently produced via nonstationary pair
plasma discharges in the polar cap region of pulsars. Here, we point out that for axion …
plasma discharges in the polar cap region of pulsars. Here, we point out that for axion …
A commensal Fast Radio Burst search pipeline for the Murchison Widefield Array
We present a demonstration version of a commensal pipeline for Fast Radio Burst (FRB)
searches using a real-time incoherent beam from the Murchison Widefield Array (MWA). The …
searches using a real-time incoherent beam from the Murchison Widefield Array (MWA). The …
System equivalent flux density of Stokes I, Q, U, and V of a polarimetric interferometer
AT Sutinjo, DCX Ung, M Sokolowski - Astronomy & Astrophysics, 2022 - aanda.org
Aims. We present the system equivalent flux density (SEFD) expressions for all four Stokes
parameters: I, Q, U, and V. Methods. The expressions were derived based on our derivation …
parameters: I, Q, U, and V. Methods. The expressions were derived based on our derivation …
An Active Ribbon Dipole as an Array Element Prototype for the Lunar Very Low Frequency Radio Telescope
This work is concerned with a detailed study of an active antenna, which can serve as a
prototype of a phased array antenna element for a future lunar very-low-frequency (VLF) …
prototype of a phased array antenna element for a future lunar very-low-frequency (VLF) …
Beamforming approaches towards detecting the 21-cm global signal from Cosmic Dawn with radio array telescopes
DC Price - Publications of the Astronomical Society of Australia, 2022 - cambridge.org
The formation of the first stars and galaxies during 'Cosmic Dawn'is thought to have imparted
a faint signal onto the 21-cm spin temperature from atomic Hydrogen gas in the early …
a faint signal onto the 21-cm spin temperature from atomic Hydrogen gas in the early …