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20182026
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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.GA2020

Resolved spectral variations of the centimetre-wavelength continuum from the rho Oph W photo-dissociation-region

Simon Casassus, Matias Vidal, Carla Arce-Tord +5

Cm-wavelength radio continuum emission in excess of free-free, synchrotron and Rayleigh-Jeans dust emission (excess microwave emission, EME), and often called `anomalous microwave…

astro-ph.GA2019

Resolved observations at 31 GHz of spinning dust emissivity variations in Oph

Carla Arce-Tord, Matias Vidal, Simon Casassus +9

The Oph molecular cloud is one of the best examples of spinning dust emission, first detected by the Cosmic Background Imager (CBI). Here we present 4.5 arcmin observations wit…

astro-ph.GA2019

Modelling the spinning dust emission from LDN 1780

Matias Vidal, Clive Dickinson, S. E. Harper +2

We study the anomalous microwave emission (AME) in the Lynds Dark Nebula (LDN) 1780 on two angular scales. Using available ancillary data at an angular resolution of 1 degree, we c…

astro-ph.GA2018

The State-of-Play of Anomalous Microwave Emission (AME) Research

Clive Dickinson, Y. Ali-Haïmoud, A. Barr +30

Anomalous Microwave Emission (AME) is a component of diffuse Galactic radiation observed at frequencies in the range -60 GHz. AME was first detected in 1996 and recogni…