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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…
QUIJOTE Scientific Results -- XVII. Studying the Anomalous Microwave Emission in the Andromeda Galaxy with QUIJOTE-MFI
M. Fernández-Torreiro, R. T. Génova-Santos, J. A. Rubiño-Martín +21
The Andromeda Galaxy (M31) is the Local Group galaxy that is most similar to the Milky Way (MW). The similarities between the two galaxies make M31 useful for studying integrated p…
QUIJOTE scientific results -- X. Spatial variations of Anomalous Microwave Emission along the Galactic plane
M. Fernández-Torreiro, J. A. Rubiño-Martín, C. H. López-Caraballo +21
Anomalous Microwave Emission (AME) is an important emission component between 10 and 60 GHz that is not yet fully understood. It seems to be ubiquituous in our Galaxy and is observ…
QUIJOTE scientific results -- IX. Radio sources in the QUIJOTE-MFI wide survey maps
D. Herranz, M. López-Caniego, C. H. López-Caraballo +22
We present the catalogue of Q-U-I JOint TEnerife (QUIJOTE) Wide Survey radio sources extracted from the maps of the Multi-Frequency Instrument compiled between 2012 and 2018. The c…
QUIJOTE Scientific Results -- VII. Galactic AME sources in the QUIJOTE-MFI Northern Hemisphere Wide-Survey
F. Poidevin, R. T. Génova-Santos, J. A. Rubiño-Martín +20
The QUIJOTE-MFI Northern Hemisphere Wide-Survey has provided maps of the sky above declinations at 11, 13, 17 and 19GHz. These data are combined with ancillary data…
QUIJOTE scientific results -- V. The microwave intensity and polarisation spectra of the Galactic regions W49, W51 and IC443
D. Tramonte, R. T. Génova-Santos, J. A. Rubiño-Martín +20
We present new intensity and polarisation maps obtained with the QUIJOTE experiment towards the Galactic regions W49, W51 and IC443, covering the frequency range from 10 to 20 GHz…