Abstract LiteBIRD, the Lite (Light) satellite for the study of B-mode polarization and Inflation
from cosmic background Radiation Detection, is a space mission for primordial cosmology …

We present QUIJOTE intensity and polarization maps in four frequency bands centred
around 11, 13, 17, and 19 GHz, and covering approximately 29 000 deg2, including most of …

Galactic plane radio surveys play a key role in improving our understanding of a wide range
of astrophysical phenomena. Performing such a survey using the latest interferometric …

Most of the visible matter in the Universe is ionized, so that cosmic magnetic fields are quite
easy to generate and due to the lack of magnetic monopoles hard to destroy. Magnetic fields …

We summarize the second radio synchrotron background workshop, which took place on
2022 June 15–17 in Barolo, Italy. This meeting was convened because available …

We derive linearly polarized astrophysical component maps in the Northern Sky from the
QUIJOTE-MFI data at 11 and 13 GHz in combination with the Wilkinson Microwave …

cm intensity mapping has emerged as a promising technique to map the large-scale
structure of the Universe. However, the presence of foregrounds with amplitudes orders of …

We present F or SE (Foreground Scale Extender), a novel Python package that aims to
overcome the current limitations in the simulation of diffuse Galactic radiation, in the context …

We present the serendipitous detection of a new Galactic supernova remnant (SNR), G288.
8–6.3, using data from the Australian Square Kilometre Array Pathfinder (ASKAP) …

Galactic synchrotron emission exhibits large angular scale features known as radio spurs
and loops. Determining the physical size of these structures is important for understanding …