This work will present the corrugated-horns, polarizers and ortho-mode transducers developed for the 49-element coherent polarimeter array working in [39, 48] GHz to be embarked in the Large Scale Polarization Explorer. The latter is an ASI-funded balloon experiment designed to measure the CMB B-modes on large angular scales. The presentation will focus on the analysis, design, manufacturing and measurements of these components
The LSPE is a balloon-borne mission aimed at measuring the polarization of the Cosmic Microwave Back...
Coherent radiometers have been used for decades in the detection of polarization of astronomical sig...
The Q/U Imaging ExperimenT (QUIET) consists of a pair of radiometer arrays designed to measure the B...
This work will present the corrugated-horns, polarizers and ortho-mode transducers developed for the...
We discuss the design and expected performance of STRIP (STRatospheric Italian Polarimeter), an arra...
We discuss the design and expected performance of STRIP (STRatospheric Italian Polarimeter), an arra...
In this paper we discuss the design, manufacturing and characterization of the feed horn array of th...
In this paper we report on the design and validation process for the profiled corrugated horn antenn...
In this paper we report on the design and validation process for the profiled corrugated horn antenn...
In this paper we report on the design and validation process for the profiled corrugated horn antenn...
Characterization of the minute cosmic microwave background polarization signature requires multi-fre...
BaR-SPOrt (Balloon-borne Radiometers for Sky Polarisation Observations) is an experiment to measure ...
BaR-SPOrt (Balloon-borne Radiometers for Sky Polarisation Observations) is an experiment to measure ...
New technology has rapidly advanced the field of observational cosmology over the last 30 years. Th...
The Cosmic Microwave Background has proven to be an invaluable tool for cosmology, but much of the s...
The LSPE is a balloon-borne mission aimed at measuring the polarization of the Cosmic Microwave Back...
Coherent radiometers have been used for decades in the detection of polarization of astronomical sig...
The Q/U Imaging ExperimenT (QUIET) consists of a pair of radiometer arrays designed to measure the B...
This work will present the corrugated-horns, polarizers and ortho-mode transducers developed for the...
We discuss the design and expected performance of STRIP (STRatospheric Italian Polarimeter), an arra...
We discuss the design and expected performance of STRIP (STRatospheric Italian Polarimeter), an arra...
In this paper we discuss the design, manufacturing and characterization of the feed horn array of th...
In this paper we report on the design and validation process for the profiled corrugated horn antenn...
In this paper we report on the design and validation process for the profiled corrugated horn antenn...
In this paper we report on the design and validation process for the profiled corrugated horn antenn...
Characterization of the minute cosmic microwave background polarization signature requires multi-fre...
BaR-SPOrt (Balloon-borne Radiometers for Sky Polarisation Observations) is an experiment to measure ...
BaR-SPOrt (Balloon-borne Radiometers for Sky Polarisation Observations) is an experiment to measure ...
New technology has rapidly advanced the field of observational cosmology over the last 30 years. Th...
The Cosmic Microwave Background has proven to be an invaluable tool for cosmology, but much of the s...
The LSPE is a balloon-borne mission aimed at measuring the polarization of the Cosmic Microwave Back...
Coherent radiometers have been used for decades in the detection of polarization of astronomical sig...
The Q/U Imaging ExperimenT (QUIET) consists of a pair of radiometer arrays designed to measure the B...