Review of Radio Frequency Interference and Potential Impacts on the CMB-S4 Cosmic Microwave Background Survey
International audience CMB-S4 will map the cosmic microwave background to unprecedented precision, while simultaneously surveying the millimeter-wave time-domain sky, in order to advance our understanding of cosmology and the universe. CMB-S4 will observe from two sites, the South Pole and the Ataca...
Published in: | Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy XI |
---|---|
Main Authors: | , , , , , , , , , |
Other Authors: | , , |
Format: | Conference Object |
Language: | English |
Published: |
HAL CCSD
2022
|
Subjects: | |
Online Access: | https://hal.science/hal-03762906 https://doi.org/10.1117/12.2629651 |
id |
ftccsdartic:oai:HAL:hal-03762906v1 |
---|---|
record_format |
openpolar |
spelling |
ftccsdartic:oai:HAL:hal-03762906v1 2023-07-23T04:21:49+02:00 Review of Radio Frequency Interference and Potential Impacts on the CMB-S4 Cosmic Microwave Background Survey Barron, Darcy R. Bender, Amy N. Birdwell, Ian E. Carlstrom, John E. Delabrouille, Jacques Guns, Sam Kovac, John Lawrence, Charles R. Paine, Scott Whitehorn, Nathan Centre Pierre Binétruy (CPB) Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-University of California Berkeley (UC Berkeley) University of California (UC)-University of California (UC) Montréal, Canada 2022-07-17 https://hal.science/hal-03762906 https://doi.org/10.1117/12.2629651 en eng HAL CCSD info:eu-repo/semantics/altIdentifier/arxiv/2207.13204 info:eu-repo/semantics/altIdentifier/doi/10.1117/12.2629651 hal-03762906 https://hal.science/hal-03762906 ARXIV: 2207.13204 doi:10.1117/12.2629651 INSPIRE: 2126919 Proc.SPIE Int.Soc.Opt.Eng. SPIE Astronomical Telescopes + Instrumentation 2022 https://hal.science/hal-03762906 SPIE Astronomical Telescopes + Instrumentation 2022, Jul 2022, Montréal, Canada. pp.1219002, ⟨10.1117/12.2629651⟩ cosmic microwave background millimeter-wave astronomy time-domain astronomy radio frequency interference CMB-S4 transition-edge sensors [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det] [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph] info:eu-repo/semantics/conferenceObject Conference papers 2022 ftccsdartic https://doi.org/10.1117/12.2629651 2023-07-01T23:53:01Z International audience CMB-S4 will map the cosmic microwave background to unprecedented precision, while simultaneously surveying the millimeter-wave time-domain sky, in order to advance our understanding of cosmology and the universe. CMB-S4 will observe from two sites, the South Pole and the Atacama Desert of Chile. A combination of small- and large-aperture telescopes with hundreds of thousands of polarization-sensitive detectors will observe in several frequency bands from 20-300 GHz, surveying more than 50 percent of the sky to arcminute resolution with unprecedented sensitivity. CMB-S4 seeks to make a dramatic leap in sensitivity while observing across a broad range of largely unprotected spectrum which is increasingly being utilized for terrestrial and satellite transmissions. Fundamental aspects of CMB instrument technology leave them vulnerable to radio frequency interference (RFI) across a wide range of frequencies, including frequencies outside of their observing bands. Ground-based CMB instruments achieve their extraordinary sensitivities by deploying large focal planes of superconducting bolometers to extremely dry, high-altitude sites, with large fractional bandwidths, wide fields of view, and years of integration time. Suitable observing sites have historically offered significant protection from RFI, both naturally through their extremely remote locations as well as through restrictions on local emissions. Since the coupling mechanisms are complex, safe levels or frequencies of emission that would not interfere with CMB measurements cannot always be determined through straightforward calculations. We discuss models of interference for various types of RFI relevant to CMB-S4, mitigation strategies, and the potential impacts on survey sensitivity. Conference Object South pole Archive ouverte HAL (Hyper Article en Ligne, CCSD - Centre pour la Communication Scientifique Directe) Canada South Pole Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy XI 1 |
institution |
Open Polar |
collection |
Archive ouverte HAL (Hyper Article en Ligne, CCSD - Centre pour la Communication Scientifique Directe) |
op_collection_id |
ftccsdartic |
language |
English |
topic |
cosmic microwave background millimeter-wave astronomy time-domain astronomy radio frequency interference CMB-S4 transition-edge sensors [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det] [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph] |
spellingShingle |
cosmic microwave background millimeter-wave astronomy time-domain astronomy radio frequency interference CMB-S4 transition-edge sensors [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det] [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph] Barron, Darcy R. Bender, Amy N. Birdwell, Ian E. Carlstrom, John E. Delabrouille, Jacques Guns, Sam Kovac, John Lawrence, Charles R. Paine, Scott Whitehorn, Nathan Review of Radio Frequency Interference and Potential Impacts on the CMB-S4 Cosmic Microwave Background Survey |
topic_facet |
cosmic microwave background millimeter-wave astronomy time-domain astronomy radio frequency interference CMB-S4 transition-edge sensors [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det] [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph] |
description |
International audience CMB-S4 will map the cosmic microwave background to unprecedented precision, while simultaneously surveying the millimeter-wave time-domain sky, in order to advance our understanding of cosmology and the universe. CMB-S4 will observe from two sites, the South Pole and the Atacama Desert of Chile. A combination of small- and large-aperture telescopes with hundreds of thousands of polarization-sensitive detectors will observe in several frequency bands from 20-300 GHz, surveying more than 50 percent of the sky to arcminute resolution with unprecedented sensitivity. CMB-S4 seeks to make a dramatic leap in sensitivity while observing across a broad range of largely unprotected spectrum which is increasingly being utilized for terrestrial and satellite transmissions. Fundamental aspects of CMB instrument technology leave them vulnerable to radio frequency interference (RFI) across a wide range of frequencies, including frequencies outside of their observing bands. Ground-based CMB instruments achieve their extraordinary sensitivities by deploying large focal planes of superconducting bolometers to extremely dry, high-altitude sites, with large fractional bandwidths, wide fields of view, and years of integration time. Suitable observing sites have historically offered significant protection from RFI, both naturally through their extremely remote locations as well as through restrictions on local emissions. Since the coupling mechanisms are complex, safe levels or frequencies of emission that would not interfere with CMB measurements cannot always be determined through straightforward calculations. We discuss models of interference for various types of RFI relevant to CMB-S4, mitigation strategies, and the potential impacts on survey sensitivity. |
author2 |
Centre Pierre Binétruy (CPB) Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-University of California Berkeley (UC Berkeley) University of California (UC)-University of California (UC) |
format |
Conference Object |
author |
Barron, Darcy R. Bender, Amy N. Birdwell, Ian E. Carlstrom, John E. Delabrouille, Jacques Guns, Sam Kovac, John Lawrence, Charles R. Paine, Scott Whitehorn, Nathan |
author_facet |
Barron, Darcy R. Bender, Amy N. Birdwell, Ian E. Carlstrom, John E. Delabrouille, Jacques Guns, Sam Kovac, John Lawrence, Charles R. Paine, Scott Whitehorn, Nathan |
author_sort |
Barron, Darcy R. |
title |
Review of Radio Frequency Interference and Potential Impacts on the CMB-S4 Cosmic Microwave Background Survey |
title_short |
Review of Radio Frequency Interference and Potential Impacts on the CMB-S4 Cosmic Microwave Background Survey |
title_full |
Review of Radio Frequency Interference and Potential Impacts on the CMB-S4 Cosmic Microwave Background Survey |
title_fullStr |
Review of Radio Frequency Interference and Potential Impacts on the CMB-S4 Cosmic Microwave Background Survey |
title_full_unstemmed |
Review of Radio Frequency Interference and Potential Impacts on the CMB-S4 Cosmic Microwave Background Survey |
title_sort |
review of radio frequency interference and potential impacts on the cmb-s4 cosmic microwave background survey |
publisher |
HAL CCSD |
publishDate |
2022 |
url |
https://hal.science/hal-03762906 https://doi.org/10.1117/12.2629651 |
op_coverage |
Montréal, Canada |
geographic |
Canada South Pole |
geographic_facet |
Canada South Pole |
genre |
South pole |
genre_facet |
South pole |
op_source |
Proc.SPIE Int.Soc.Opt.Eng. SPIE Astronomical Telescopes + Instrumentation 2022 https://hal.science/hal-03762906 SPIE Astronomical Telescopes + Instrumentation 2022, Jul 2022, Montréal, Canada. pp.1219002, ⟨10.1117/12.2629651⟩ |
op_relation |
info:eu-repo/semantics/altIdentifier/arxiv/2207.13204 info:eu-repo/semantics/altIdentifier/doi/10.1117/12.2629651 hal-03762906 https://hal.science/hal-03762906 ARXIV: 2207.13204 doi:10.1117/12.2629651 INSPIRE: 2126919 |
op_doi |
https://doi.org/10.1117/12.2629651 |
container_title |
Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy XI |
container_start_page |
1 |
_version_ |
1772188051105120256 |