collaborators

9 papers

astro-ph.GA2026

Probing Anomalous Microwave Emission with the Square Kilometre Array

Matías Vidal, Simón Casassus, Roke Cepeda-Arroita +15

Anomalous microwave emission (AME) represents an excess of radiation in the 10-60 GHz range, distinct from synchrotron, free-free, or thermal dust emission. Although most commonly…

astro-ph.GA2026

All-sky modeling of Galactic emission at radio and microwave frequencies

Gabriel A. Hoerning, Clive Dickinson, Stuart E. Harper +13

We present a new all-sky model of low-frequency diffuse Galactic emission in the regime where synchrotron, free-free, and spinning dust dominate. The model extends the Planck 2015…

astro-ph.GA2026

A comparison between Galactic magnetic field models and polarized synchrotron emission with C-BASS at 4.76 GHz and S-PASS at 2.3 GHz

Vasundhara Shaw, S. E. Harper, C. Dickinson +9

We compare a set of contemporary Galactic magnetic field (GMF) models with polarized synchrotron observations from the S-PASS and C-BASS radio surveys and combine them to create a…

astro-ph.GA2026

Spectral Properties of Anomalous Microwave Emission in 144 Galactic Clouds

Roke Cepeda-Arroita, J. A. Rubiño-Martín, R. T. Génova-Santos +23

Anomalous Microwave Emission (AME) is a diffuse microwave component thought to arise from spinning dust grains, yet remains poorly understood. We analyze AME in 144 Galactic clouds…

astro-ph.CO2026

The BINGO project X. Cosmological parameter constraints from HI Intensity Mapping lognormal simulations

Pablo Motta, Filipe B. Abdalla, Camila P. Novaes +12

Context. Building on the transformative success of optical redshift surveys, the emerging technique of neutral hydrogen (HI) intensity mapping (IM) offers a novel probe of large-sc…

astro-ph.CO2025

COMAP Pathfinder -- Season 2 results IV. A stack on eBOSS/DESI quasars

D. A. Dunne, K. A. Cleary, J. G. S. Lunde +16

We present a stack of data from the second season of the CO Mapping Array Project (COMAP) Pathfinder on the positions of quasars from eBOSS and DESI. COMAP is a Line Intensity Mapp…