Eleonora Barbavara
YOU?
Author Swipe
View article: The Atacama Cosmology Telescope: DR6 power spectra, likelihoods and ΛCDM parameters
The Atacama Cosmology Telescope: DR6 power spectra, likelihoods and ΛCDM parameters Open
We present power spectra of the cosmic microwave background (CMB) anisotropy in temperature and polarization, measured from the Data Release 6 maps made from Atacama Cosmology Telescope (ACT) data. These cover 19,000 deg 2 of sky in bands …
View article: The thermal and kinematic Sunyaev-Zeldovich effect in galaxy clusters and filaments using multifrequency temperature maps of the cosmic microwave background: Abell 399--Abell 401 cluster pair case study
The thermal and kinematic Sunyaev-Zeldovich effect in galaxy clusters and filaments using multifrequency temperature maps of the cosmic microwave background: Abell 399--Abell 401 cluster pair case study Open
We present a multifrequency and multi-instrument methodology to study the physical properties of galaxy clusters and cosmic filaments using cosmic microwave background observations. Our approach enables simultaneous measurement of both the…
View article: The Atacama Cosmology Telescope: DR6 Maps
The Atacama Cosmology Telescope: DR6 Maps Open
We present Atacama Cosmology Telescope (ACT) Data Release 6 (DR6) maps of the Cosmic Microwave Background temperature and polarization anisotropy at arcminute resolution over three frequency bands centered on 98, 150 and 220 GHz. The maps …
View article: The Atacama Cosmology Telescope: DR6 Constraints on Extended Cosmological Models
The Atacama Cosmology Telescope: DR6 Constraints on Extended Cosmological Models Open
We use new cosmic microwave background (CMB) primary temperature and polarization anisotropy measurements from the Atacama Cosmology Telescope (ACT) Data Release 6 (DR6) to test foundational assumptions of the standard cosmological model a…
View article: The Atacama Cosmology Telescope: DR6 Power Spectra, Likelihoods and $Λ$CDM Parameters
The Atacama Cosmology Telescope: DR6 Power Spectra, Likelihoods and $Λ$CDM Parameters Open
We present power spectra of the cosmic microwave background (CMB) anisotropy in temperature and polarization, measured from the Data Release 6 maps made from Atacama Cosmology Telescope (ACT) data. These cover 19,000 deg$^2$ of sky in band…
View article: The Atacama Cosmology Telescope: A census of bridges between galaxy clusters
The Atacama Cosmology Telescope: A census of bridges between galaxy clusters Open
According to CMB measurements, baryonic matter constitutes about $5\%$ of the mass-energy density of the universe. A significant population of these baryons, for a long time referred to as `missing', resides in a low density, warm-hot inte…
View article: The MISTRAL Instrument and the Characterization of Its Detector Array
The MISTRAL Instrument and the Characterization of Its Detector Array Open
The MIllimeter Sardinia radio Telescope Receiver based on Array of Lumped elements KIDs, MISTRAL, is a cryogenic LEKID camera, operating in the W band ( $${77}{-}{103\,\textrm{GHz}}$$ ) from the Gregorian focus of the 64-m aperture …
View article: Dark performance of the MISTRAL LEKIDs
Dark performance of the MISTRAL LEKIDs Open
MISTRAL, Millimetric Sardinia radio Telescope Receiver based on Array of Lumped elements KIDs, is a W-Band cryogenic LEKID camera installed on the Sardinia Radio Telescope (SRT), in Italy. The MISTRAL detector array has been designed to wo…
View article: High angular resolution Sunyaev Zel’dovich observations: The case of MISTRAL
High angular resolution Sunyaev Zel’dovich observations: The case of MISTRAL Open
The MIllimeter Sardinia radio Telescope Receiver based on Array of Lumped
\nelements kids, MISTRAL, is a millimetric ($\\simeq 90GHz$) multipixel camera
\nbeing built for the Sardinia Radio Telescope. It is going to be a facility
\ninstrum…
View article: MISTRAL and its KIDs
MISTRAL and its KIDs Open
View article: Erratum to: Millimetric Sardinia radio Telescope Receiver based on Array of Lumped elements kids
Erratum to: Millimetric Sardinia radio Telescope Receiver based on Array of Lumped elements kids Open
View article: A high-resolution view of the filament of gas between Abell 399 and Abell 401 from the Atacama Cosmology Telescope and MUSTANG-2
A high-resolution view of the filament of gas between Abell 399 and Abell 401 from the Atacama Cosmology Telescope and MUSTANG-2 Open
We report a significant detection of the hot intergalactic medium in the filamentary bridge connecting the galaxy clusters Abell 399 and Abell 401. This result is enabled by a low-noise, high-resolution map of the thermal Sunyaev–Zeldovich…
View article: A high-resolution view of the filament of gas between Abell 399 and\n Abell 401 from the Atacama Cosmology Telescope and MUSTANG-2
A high-resolution view of the filament of gas between Abell 399 and\n Abell 401 from the Atacama Cosmology Telescope and MUSTANG-2 Open
We report a significant detection of the hot intergalactic medium in the\nfilamentary bridge connecting the galaxy clusters Abell 399 and Abell 401. This\nresult is enabled by a low-noise, high-resolution map of the thermal\nSunyaev-Zeldov…