F. Columbro
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View article: Characterization of a half wave plate and a polarizer for accurate starlight polarimetry
Characterization of a half wave plate and a polarizer for accurate starlight polarimetry Open
In the process of developing a space-based imaging Stokes polarimeter for starlight polarization measurements, we established a procedure to characterize its two main optical components: the wave plate and the polarizer. We demonstrate tha…
View article: Requirements on bandpass resolution and measurement precision for LiteBIRD
Requirements on bandpass resolution and measurement precision for LiteBIRD Open
Systematic effects can hinder the sought-after detection of primordial gravitational waves, impacting the reconstruction of the B -mode polarization signal which they generate in the cosmic microwave background (CMB). In this work, we stud…
View article: LiteBIRD science goals and forecasts: constraining isotropic cosmic birefringence
LiteBIRD science goals and forecasts: constraining isotropic cosmic birefringence Open
Cosmic birefringence (CB) is the rotation of the photons' linear polarisation plane during propagation. Such an effect is a tracer of parity-violating extensions of standard electromagnetism and would probe the existence of a new cosmologi…
View article: MISTRAL: Science Perspectives and Performance Forecasts
MISTRAL: Science Perspectives and Performance Forecasts Open
The MIllimeter Sardinia radio Telescope Receiver based on Array of Lumped elements (MISTRAL) KIDs is a millimeter camera operating at 90GHz that was recently installed on the Sardinia Radio Telescope (SRT) as part of the SRT-HighFreq progr…
View article: The kinetic inductance detectors for the MISTRAL instrument: Installation and characterization at the Sardinia Radio Telescope
The kinetic inductance detectors for the MISTRAL instrument: Installation and characterization at the Sardinia Radio Telescope Open
View article: The Cryogenic System of the MISTRAL Instrument: Design and In-lab Performance
The Cryogenic System of the MISTRAL Instrument: Design and In-lab Performance Open
We describe the design and performance of the cryostat and the multi-stage sub-K single-shot sorption cooler for the MIllimeter Sardinia Radio Telescope Receiver based on Array of Lumped elements kids (MISTRAL) experiment. MISTRAL is a W-b…
View article: Requirements on the gain calibration for LiteBIRD polarisation data with blind component separation
Requirements on the gain calibration for LiteBIRD polarisation data with blind component separation Open
The detection of primordial B modes of the cosmic microwave background (CMB) could provide information about the early stages of the Universe's evolution. The faintness of this signal requires exquisite calibration accuracy and control of …
View article: Multi-dimensional optimisation of the scanning strategy for the LiteBIRD space mission
Multi-dimensional optimisation of the scanning strategy for the LiteBIRD space mission Open
Large angular scale surveys in the absence of atmosphere are essential for measuring the primordial B-mode power spectrum of the Cosmic Microwave Background (CMB). Since this proposed measurement is about three to four orders of magnitude …
View article: Spectral Imaging with QUBIC: building astrophysical components from Time-Ordered-Data using Bolometric Interferometry
Spectral Imaging with QUBIC: building astrophysical components from Time-Ordered-Data using Bolometric Interferometry Open
The detection of B-modes in the CMB polarization pattern is a major issue in modern cosmology and must therefore be handled with analytical methods that produce reliable results. We describe a method that uses the frequency dependency of t…
View article: Spectral Imaging with QUBIC: building frequency maps from Time-Ordered-Data using Bolometric Interferometry
Spectral Imaging with QUBIC: building frequency maps from Time-Ordered-Data using Bolometric Interferometry Open
The search for relics from the inflation era in the form of B-mode polarization of the CMB is a major challenge in cosmology. The main obstacle appears to come from the complexity of Galactic foregrounds that need to be removed. Multi-freq…
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: A 350 GHz array of LEKIDs for balloon-borne CMB observations
A 350 GHz array of LEKIDs for balloon-borne CMB observations Open
We present the design, optimization and laboratory characterization of an array of Lumped Element Kinetic
\nInductance Detectors sensitive in a frequency band centered at 350 GHz. The array consists of 313 feed-horn
\ncoupled pixels with r…
View article: A Cryogenic Testbed for Polarization Modulators and Cryogenic Mechanisms
A Cryogenic Testbed for Polarization Modulators and Cryogenic Mechanisms Open
We developed a cryogenic facility to assess the performance of different types of cryogenic mechanisms. The facility can host very large (up to $$\sim {1}\,\hbox {m}^{3}$$ ) and heavy (up to $$\sim {30}\,\hbox {kg}$$ ) instrume…
View article: LiteBIRD Science Goals and Forecasts. Mapping the Hot Gas in the Universe
LiteBIRD Science Goals and Forecasts. Mapping the Hot Gas in the Universe Open
We assess the capabilities of the LiteBIRD mission to map the hot gas distribution in the Universe through the thermal Sunyaev-Zeldovich (SZ) effect. Our analysis relies on comprehensive simulations incorporating various sources of Galacti…
View article: Systematic effects induced by half-wave plate differential optical load and TES nonlinearity for LiteBIRD
Systematic effects induced by half-wave plate differential optical load and TES nonlinearity for LiteBIRD Open
LiteBIRD, a forthcoming satellite mission, aims to measure the polarization of the Cosmic Microwave Background (CMB) across the entire sky. The experiment will employ three telescopes, Transition-Edge Sensor (TES) bolometers and rotating H…
View article: Measuring the CMB spectral distortions with COSMO: the multi-mode antenna system
Measuring the CMB spectral distortions with COSMO: the multi-mode antenna system Open
In this work, we present the design and manufacturing of the two multi-mode antenna arrays of the COSMO experiment and the preliminary beam pattern measurements of their fundamental mode compared with simulations. COSMO is a cryogenic Mart…
View article: Impact of beam far side-lobe knowledge in the presence of foregrounds for LiteBIRD
Impact of beam far side-lobe knowledge in the presence of foregrounds for LiteBIRD Open
We present a study of the impact of a beam far side-lobe lack of knowledge on the measurement of the Cosmic Microwave Background B -mode signal at large scale. Beam far side-lobes induce a mismatch in the transfer function of Galactic fore…
View article: LiteBIRD science goals and forecasts: a full-sky measurement of gravitational lensing of the CMB
LiteBIRD science goals and forecasts: a full-sky measurement of gravitational lensing of the CMB Open
We explore the capability of measuring lensing signals in LiteBIRD full-sky polarization maps. With a 30 arcmin beam width and an impressively low polarization noise of 2.16 μ K-arcmin, LiteBIRD will be able to measure the full-sky polariz…
View article: LiteBIRD science goals and forecasts: improving sensitivity to inflationary gravitational waves with multitracer delensing
LiteBIRD science goals and forecasts: improving sensitivity to inflationary gravitational waves with multitracer delensing Open
We estimate the efficiency of mitigating the lensing B -mode polarization, the so-called delensing, for the LiteBIRD experiment with multiple external data sets of lensing-mass tracers. The current best bound on the tensor-to-scalar ratio,…
View article: LiteBIRD Science Goals and Forecasts: Primordial Magnetic Fields
LiteBIRD Science Goals and Forecasts: Primordial Magnetic Fields Open
We present detailed forecasts for the constraints on primordial magnetic fields (PMFs) that will be obtained with the LiteBIRD satellite. The constraints are driven by the effects of PMFs on the CMB anisotropies: the gravitational effects …
View article: OLIMPO: A balloon-borne SZE imager to probe ICM dynamics and the WHIM
OLIMPO: A balloon-borne SZE imager to probe ICM dynamics and the WHIM Open
OLIMPO is a proposed Antarctic balloon-borne Sunyaev-Zel’dovich effect (SZE) imager to study gas dynamics associated with structure formation along with the properties of the warm-hot intergalactic medium (WHIM) residing in the connective …
View article: Observing galaxy clusters and the cosmic web through the Sunyaev Zel’dovich effect with MISTRAL
Observing galaxy clusters and the cosmic web through the Sunyaev Zel’dovich effect with MISTRAL Open
Galaxy clusters and surrounding medium, can be studied using X-ray bremsstrahlung emission and Sunyaev Zel’dovich (SZ) effect. Both astrophysical probes, sample the same environment with different parameters dependance. The SZ effect is re…
View article: Impact of beam far side-lobe knowledge in the presence of foregrounds for LiteBIRD
Impact of beam far side-lobe knowledge in the presence of foregrounds for LiteBIRD Open
We present a study of the impact of an uncertainty in the beam far side-lobe knowledge on the measurement of the Cosmic Microwave Background $B$-mode signal at large scale. It is expected to be one of the main source of systematic effects …
View article: LiteBIRD Science Goals and Forecasts: A full-sky measurement of gravitational lensing of the CMB
LiteBIRD Science Goals and Forecasts: A full-sky measurement of gravitational lensing of the CMB Open
We explore the capability of measuring lensing signals in $LiteBIRD$ full-sky polarization maps. With a $30$ arcmin beam width and an impressively low polarization noise of $2.16\,μ$K-arcmin, $LiteBIRD$ will be able to measure the full-sky…
View article: LiteBIRD Science Goals and Forecasts. A Case Study of the Origin of Primordial Gravitational Waves using Large-Scale CMB Polarization
LiteBIRD Science Goals and Forecasts. A Case Study of the Origin of Primordial Gravitational Waves using Large-Scale CMB Polarization Open
We study the possibility of using the $LiteBIRD$ satellite $B$-mode survey to constrain models of inflation producing specific features in CMB angular power spectra. We explore a particular model example, i.e. spectator axion-SU(2) gauge f…
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: Observing galaxy clusters and the cosmic web through the Sunyaev Zel'dovich effect with MISTRAL
Observing galaxy clusters and the cosmic web through the Sunyaev Zel'dovich effect with MISTRAL Open
Galaxy clusters and surrounding medium, can be studied using X-ray bremsstrahlung emission and Sunyaev Zel'dovich (SZ) effect. Both astrophysical probes, sample the same environment with different parameters dependance. The SZ effect is re…
View article: Probing cosmic inflation with the LiteBIRD cosmic microwave background polarization survey
Probing cosmic inflation with the LiteBIRD cosmic microwave background polarization survey Open
LiteBIRD, the Lite (Light) satellite for the study of B-mode polarization and Inflation from cosmic background Radiation Detection, is a space mission for primordial cosmology and fundamental physics. The Japan Aerospace Exploration Agency…
View article: The COSmic Monopole Observer (COSMO)
The COSmic Monopole Observer (COSMO) Open
The COSmic Monopole Observer (COSMO) is an experiment to measure low-level spectral distortions in the isotropic component of the Cosmic Microwave Background (CMB). Deviations from a pure blackbody spectrum are expected at low level (< …
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…