67 citations · 315 across the 17 of their papers we have counts for
17 papers
A Measurement of Gravitational Lensing of the Cosmic Microwave Background Using SPT-3G 2018 Data
Z. Pan, F. Bianchini, W. L. K. Wu +133
We present a measurement of gravitational lensing over 1500 deg of the Southern sky using SPT-3G temperature data at 95 and 150 GHz taken in 2018. The lensing amplitude relativ…
QUIJOTE scientific results -- XIII. Intensity and polarization study of supernova remnants in the QUIJOTE-MFI wide survey: CTB 80, Cygnus Loop, HB 21, CTA 1, Tycho and HB 9
Carlos Hugo López-Caraballo, Beatriz Ruiz-Granados, Ricardo Genova Santos +21
We use the new QUIJOTE-MFI wide survey (11, 13, 17 and 19 GHz) to produce spectral energy distributions (SEDs), on an angular scale of 1 deg, of the supernova remnants (SNRs) CTB 8…
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 -- VIII. Diffuse polarized foregrounds from component separation with QUIJOTE-MFI
E. de la Hoz, R. B. Barreiro, P. Vielva +23
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 WMAP K and Ka bands (23 and 33 GHz)…
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 -- VI. The Haze as seen by QUIJOTE
F. Guidi, R. T. Génova-Santos, J. A. Rubiño-Martín +22
The Haze is an excess of microwave intensity emission surrounding the Galactic centre. It is spatially correlated with the -ray Fermi bubbles, and with the S-PASS radio polariza…
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…
QUIJOTE scientific results -- IV. A northern sky survey in intensity and polarization at 10-20GHz with the Multi-Frequency Instrument
J. A. Rubino-Martin, F. Guidi, R. T. Genova-Santos +35
We present QUIJOTE intensity and polarization maps in four frequency bands centred around 11, 13, 17 and 19GHz, and covering approximately 29000 deg, including most of the Nort…
Searching for axion-like time-dependent cosmic birefringence with data from SPT-3G
K. R. Ferguson, A. J. Anderson, N. Whitehorn +78
Ultralight axionlike particles (ALPs) are compelling dark matter candidates because of their potential to resolve small-scale discrepancies between CDM predictions and cosmologi…
The PICASSO map-making code: application to a simulation of the QUIJOTE northern sky survey
F. Guidi, J. A. Rubiño-Martín, A. E. Pelaez-Santos +6
Map-making is an important step for the data analysis of Cosmic Microwave Background (CMB) experiments. It consists of converting the data, which are typically a long, complex and…
Study of the thermal and nonthermal emission components in M31: the Sardinia Radio Telescope view at 6.6 GHz
S. Fatigoni, F. Radiconi, E. S. Battistelli +21
The Andromeda galaxy is the best-known large galaxy besides our own Milky Way. Several images and studies exist at all wavelengths from radio to hard X-ray. Nevertheless, only a fe…
Detection of Spectral Variations of Anomalous Microwave Emission with QUIJOTE and C-BASS
R. Cepeda-Arroita, S. Harper, C. Dickinson +32
Anomalous Microwave Emission (AME) is a significant component of Galactic diffuse emission in the frequency range -GHz and a new window into the properties of sub-nanomet…
Strong evidence of Anomalous Microwave Emission from the flux density spectrum of M31
E. S. Battistelli, S. Fatigoni, M. Murgia +21
We have observed the Andromeda galaxy, Messier 31 (M31), at 6.7GHz with the Sardinia Radio Telescope. We mapped the radio emission in the C-band, re-analyzed WMAP and Planck maps,…
QUIJOTE Scientific results. III. Microwave spectrum of intensity and polarization in the Taurus molecular cloud Complex and L1527
F. Poidevin, J. A. Rubiño-Martín, C. Dickinson +17
We present new intensity and polarization observations of the Taurus molecular cloud (TMC) region in the frequency range 10-20 GHz with the Multi-Frequency Instrument (MFI) mounted…
The QUIJOTE Experiment: Prospects for CMB B-MODE polarization detection and foregrounds characterization
F. Poidevin, J. A. Rubino-Martin, R. Genova-Santos +47
QUIJOTE (Q-U-I JOint TEnerife) is an experiment designed to achieve CMB B-mode polarization detection and sensitive enough to detect a primordial gravitational-wave component if th…