QUBIC: a Fizeau interferometer targeting primordial B-modes

International audience QUBIC (Q and U Bolometric Interferometer for Cosmology) is a Fizeau interferometer sensi- tive to linear polarisation, to be deployed at the Antarctic Station of Dome C. This experiment in its nal conguration will be operated at 97, 150 and 220 GHz, and is intended to target C...

Full description

Bibliographic Details
Main Author: Tartari, A.
Other Authors: AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris Sciences et Lettres (PSL)-Université Paris Sciences et Lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), QUBIC
Format: Conference Object
Language:English
Published: HAL CCSD 2014
Subjects:
Online Access:https://hal.science/hal-01553934
id fthalin2p3:oai:HAL:hal-01553934v1
record_format openpolar
spelling fthalin2p3:oai:HAL:hal-01553934v1 2024-05-19T07:31:35+00:00 QUBIC: a Fizeau interferometer targeting primordial B-modes Tartari, A. AstroParticule et Cosmologie (APC (UMR_7164)) Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris Université Paris Sciences et Lettres (PSL)-Université Paris Sciences et Lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité) QUBIC La Thuile, Italy 2014-03-22 https://hal.science/hal-01553934 en eng HAL CCSD hal-01553934 https://hal.science/hal-01553934 INSPIRE: 1337857 49th Rencontres de Moriond on Cosmology https://hal.science/hal-01553934 49th Rencontres de Moriond on Cosmology, Mar 2014, La Thuile, Italy. pp.349-352 [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph] info:eu-repo/semantics/conferenceObject Conference papers 2014 fthalin2p3 2024-04-24T00:05:00Z International audience QUBIC (Q and U Bolometric Interferometer for Cosmology) is a Fizeau interferometer sensi- tive to linear polarisation, to be deployed at the Antarctic Station of Dome C. This experiment in its nal conguration will be operated at 97, 150 and 220 GHz, and is intended to target CMB primordial B-modes in a multipole window 20 ` 150, to achieve a nal sensitivity of r=0.01 (90%CL) after 1 year of operation. Here we review in particular its working princi- ples and we show how QUBIC interferometric conguration can be considered equivalent to a pupil-plane ltered imaging system. In this context, we show how our instrument can be self-calibrated. Finally, we conclude by showing an overall view on the 150 GHz unit, which will play the role of a demonstrator for the subsequent modules, and review the technological choices we did for each subsystem Conference Object Antarc* Antarctic HAL-IN2P3 (Institut national de physique nucléaire et de physique des particules)
institution Open Polar
collection HAL-IN2P3 (Institut national de physique nucléaire et de physique des particules)
op_collection_id fthalin2p3
language English
topic [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
spellingShingle [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
Tartari, A.
QUBIC: a Fizeau interferometer targeting primordial B-modes
topic_facet [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
description International audience QUBIC (Q and U Bolometric Interferometer for Cosmology) is a Fizeau interferometer sensi- tive to linear polarisation, to be deployed at the Antarctic Station of Dome C. This experiment in its nal conguration will be operated at 97, 150 and 220 GHz, and is intended to target CMB primordial B-modes in a multipole window 20 ` 150, to achieve a nal sensitivity of r=0.01 (90%CL) after 1 year of operation. Here we review in particular its working princi- ples and we show how QUBIC interferometric conguration can be considered equivalent to a pupil-plane ltered imaging system. In this context, we show how our instrument can be self-calibrated. Finally, we conclude by showing an overall view on the 150 GHz unit, which will play the role of a demonstrator for the subsequent modules, and review the technological choices we did for each subsystem
author2 AstroParticule et Cosmologie (APC (UMR_7164))
Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris
Université Paris Sciences et Lettres (PSL)-Université Paris Sciences et Lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité)
QUBIC
format Conference Object
author Tartari, A.
author_facet Tartari, A.
author_sort Tartari, A.
title QUBIC: a Fizeau interferometer targeting primordial B-modes
title_short QUBIC: a Fizeau interferometer targeting primordial B-modes
title_full QUBIC: a Fizeau interferometer targeting primordial B-modes
title_fullStr QUBIC: a Fizeau interferometer targeting primordial B-modes
title_full_unstemmed QUBIC: a Fizeau interferometer targeting primordial B-modes
title_sort qubic: a fizeau interferometer targeting primordial b-modes
publisher HAL CCSD
publishDate 2014
url https://hal.science/hal-01553934
op_coverage La Thuile, Italy
genre Antarc*
Antarctic
genre_facet Antarc*
Antarctic
op_source 49th Rencontres de Moriond on Cosmology
https://hal.science/hal-01553934
49th Rencontres de Moriond on Cosmology, Mar 2014, La Thuile, Italy. pp.349-352
op_relation hal-01553934
https://hal.science/hal-01553934
INSPIRE: 1337857
_version_ 1799469450287644672