The extended excess toward the Galactic Center (GC) in gamma rays inferred from Fermi-
LAT observations has been interpreted as being due to dark matter (DM) annihilation. Here …

We report the discovery of a highly polarized, highly variable, steep-spectrum radio source,
ASKAP J173608. 2− 321635, located∼ 4 from the Galactic Center in the Galactic plane. The …

Discovering radio pulsars, particularly millisecond pulsars (MSPs), is important for a range of
astrophysical applications, such as testing theories of gravity or probing the magneto-ionic …

The Snake is a remarkable Galactic Centre radio filament with a morphology characterized
by two kinks along its∼ 20 arcmin extent. The major and minor kinks are located where the …

The leading explanation of the Fermi Galactic Centre γ-ray excess is the extended emission
from an unresolved population of millisecond pulsars (MSPs) in the Galactic bulge. Such a …

We report on the results of an image-based search for pulsar candidates toward the Galactic
bulge. We used mosaic images from the MeerKAT radio telescope that were taken as part of …

We identified a highly polarized, steep-spectrum radio source in a deep image with the
Australian Square Kilometre Array Pathfinder (ASKAP) telescope at 888 MHz. After …

From an on-going survey of the Galactic bulge, we have discovered a number of compact,
steep spectrum radio sources. In this study, we have carried out more detailed observations …

Pulsars have been studied extensively over the last few decades and have proven
instrumental in exploring a wide variety of physics. Discovering more pulsars emitting at low …

We present the results of a high angular resolution (1.1 arcsec) and sensitivity (maximum
of∼ 0.1 mJy) radio survey at 1–2 GHz in the Galactic Bulge. This complements the X-ray …