The Cosmic Background Imager

Design and performance details are given for the Cosmic Background Imager (CBI), an interferometer array that is measuring the power spectrum of fluctuations in the cosmic microwave background radiation (CMBR) for multipoles in the range 400 < l < 3500. The CBI is located at an altitude of 500...

Ausführliche Beschreibung

Gespeichert in:
Bibliographische Detailangaben
Veröffentlicht in:arXiv.org 2001-10
Hauptverfasser: Padin, S, Shepherd, M C, Cartwright, J K, Keeney, R G, Mason, B S, Pearson, T J, Readhead, A C S, Schaal, W L, Sievers, J, Udomprasert, P S, Yamasaki, J K, Holzapfel, W L, Carlstrom, J E, Joy, M, Myers, S T, Otarola, A
Format: Artikel
Sprache:eng
Schlagworte:
Online-Zugang:Volltext
Tags: Tag hinzufügen
Keine Tags, Fügen Sie den ersten Tag hinzu!
container_end_page
container_issue
container_start_page
container_title arXiv.org
container_volume
creator Padin, S
Shepherd, M C
Cartwright, J K
Keeney, R G
Mason, B S
Pearson, T J
Readhead, A C S
Schaal, W L
Sievers, J
Udomprasert, P S
Yamasaki, J K
Holzapfel, W L
Carlstrom, J E
Joy, M
Myers, S T
Otarola, A
description Design and performance details are given for the Cosmic Background Imager (CBI), an interferometer array that is measuring the power spectrum of fluctuations in the cosmic microwave background radiation (CMBR) for multipoles in the range 400 < l < 3500. The CBI is located at an altitude of 5000 m in the Atacama Desert in northern Chile. It is a planar synthesis array with 13 0.9-m diameter antennas on a 6-m diameter tracking platform. Each antenna has a cooled, low-noise receiver operating in the 26-36 GHz band. Signals are cross-correlated in an analog filterbank correlator with ten 1 GHz bands. This allows spectral index measurements which can be used to distinguish CMBR signals from diffuse galactic foregrounds. A 1.2 kHz 180-deg phase switching scheme is used to reject cross-talk and low-frequency pick-up in the signal processing system. The CBI has a 3-axis mount which allows the tracking platform to be rotated about the optical axis, providing improved (u,v) coverage and a powerful discriminant against false signals generated in the receiving electronics. Rotating the tracking platform also permits polarization measurements when some of the antennas are configured for the orthogonal polarization.
doi_str_mv 10.48550/arxiv.0110124
format Article
fullrecord <record><control><sourceid>proquest</sourceid><recordid>TN_cdi_proquest_journals_2088841994</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>2088841994</sourcerecordid><originalsourceid>FETCH-proquest_journals_20888419943</originalsourceid><addsrcrecordid>eNpjYBAzNNAzsTA1NdBPLKrILNMzMDQ0MDQyYWLgNDI2NtS1MDEy4mDgLS7OMjAwMDIzNzI1NeZkkAnJSFVwzi_OzUxWcEpMzk4vyi_NS1HwzE1MTy3iYWBNS8wpTuWF0twMym6uIc4eugVF-YWlqcUl8Vn5pUV5QKl4IwMLCwsTQ0tLE2PiVAEAfwswyg</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>2088841994</pqid></control><display><type>article</type><title>The Cosmic Background Imager</title><source>Free E- Journals</source><creator>Padin, S ; Shepherd, M C ; Cartwright, J K ; Keeney, R G ; Mason, B S ; Pearson, T J ; Readhead, A C S ; Schaal, W L ; Sievers, J ; Udomprasert, P S ; Yamasaki, J K ; Holzapfel, W L ; Carlstrom, J E ; Joy, M ; Myers, S T ; Otarola, A</creator><creatorcontrib>Padin, S ; Shepherd, M C ; Cartwright, J K ; Keeney, R G ; Mason, B S ; Pearson, T J ; Readhead, A C S ; Schaal, W L ; Sievers, J ; Udomprasert, P S ; Yamasaki, J K ; Holzapfel, W L ; Carlstrom, J E ; Joy, M ; Myers, S T ; Otarola, A</creatorcontrib><description>Design and performance details are given for the Cosmic Background Imager (CBI), an interferometer array that is measuring the power spectrum of fluctuations in the cosmic microwave background radiation (CMBR) for multipoles in the range 400 &lt; l &lt; 3500. The CBI is located at an altitude of 5000 m in the Atacama Desert in northern Chile. It is a planar synthesis array with 13 0.9-m diameter antennas on a 6-m diameter tracking platform. Each antenna has a cooled, low-noise receiver operating in the 26-36 GHz band. Signals are cross-correlated in an analog filterbank correlator with ten 1 GHz bands. This allows spectral index measurements which can be used to distinguish CMBR signals from diffuse galactic foregrounds. A 1.2 kHz 180-deg phase switching scheme is used to reject cross-talk and low-frequency pick-up in the signal processing system. The CBI has a 3-axis mount which allows the tracking platform to be rotated about the optical axis, providing improved (u,v) coverage and a powerful discriminant against false signals generated in the receiving electronics. Rotating the tracking platform also permits polarization measurements when some of the antennas are configured for the orthogonal polarization.</description><identifier>EISSN: 2331-8422</identifier><identifier>DOI: 10.48550/arxiv.0110124</identifier><language>eng</language><publisher>Ithaca: Cornell University Library, arXiv.org</publisher><subject>Antenna arrays ; Antennas ; Background radiation ; Big Bang theory ; Cosmic microwave background ; Crosstalk ; Multipoles ; Polarization ; Signal processing ; Three axis ; Tracking ; Variations</subject><ispartof>arXiv.org, 2001-10</ispartof><rights>2001. This work is published under https://arxiv.org/licenses/assumed-1991-2003/license.html (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License.</rights><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>780,784,27925</link.rule.ids></links><search><creatorcontrib>Padin, S</creatorcontrib><creatorcontrib>Shepherd, M C</creatorcontrib><creatorcontrib>Cartwright, J K</creatorcontrib><creatorcontrib>Keeney, R G</creatorcontrib><creatorcontrib>Mason, B S</creatorcontrib><creatorcontrib>Pearson, T J</creatorcontrib><creatorcontrib>Readhead, A C S</creatorcontrib><creatorcontrib>Schaal, W L</creatorcontrib><creatorcontrib>Sievers, J</creatorcontrib><creatorcontrib>Udomprasert, P S</creatorcontrib><creatorcontrib>Yamasaki, J K</creatorcontrib><creatorcontrib>Holzapfel, W L</creatorcontrib><creatorcontrib>Carlstrom, J E</creatorcontrib><creatorcontrib>Joy, M</creatorcontrib><creatorcontrib>Myers, S T</creatorcontrib><creatorcontrib>Otarola, A</creatorcontrib><title>The Cosmic Background Imager</title><title>arXiv.org</title><description>Design and performance details are given for the Cosmic Background Imager (CBI), an interferometer array that is measuring the power spectrum of fluctuations in the cosmic microwave background radiation (CMBR) for multipoles in the range 400 &lt; l &lt; 3500. The CBI is located at an altitude of 5000 m in the Atacama Desert in northern Chile. It is a planar synthesis array with 13 0.9-m diameter antennas on a 6-m diameter tracking platform. Each antenna has a cooled, low-noise receiver operating in the 26-36 GHz band. Signals are cross-correlated in an analog filterbank correlator with ten 1 GHz bands. This allows spectral index measurements which can be used to distinguish CMBR signals from diffuse galactic foregrounds. A 1.2 kHz 180-deg phase switching scheme is used to reject cross-talk and low-frequency pick-up in the signal processing system. The CBI has a 3-axis mount which allows the tracking platform to be rotated about the optical axis, providing improved (u,v) coverage and a powerful discriminant against false signals generated in the receiving electronics. Rotating the tracking platform also permits polarization measurements when some of the antennas are configured for the orthogonal polarization.</description><subject>Antenna arrays</subject><subject>Antennas</subject><subject>Background radiation</subject><subject>Big Bang theory</subject><subject>Cosmic microwave background</subject><subject>Crosstalk</subject><subject>Multipoles</subject><subject>Polarization</subject><subject>Signal processing</subject><subject>Three axis</subject><subject>Tracking</subject><subject>Variations</subject><issn>2331-8422</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2001</creationdate><recordtype>article</recordtype><sourceid>ABUWG</sourceid><sourceid>AFKRA</sourceid><sourceid>AZQEC</sourceid><sourceid>BENPR</sourceid><sourceid>CCPQU</sourceid><sourceid>DWQXO</sourceid><recordid>eNpjYBAzNNAzsTA1NdBPLKrILNMzMDQ0MDQyYWLgNDI2NtS1MDEy4mDgLS7OMjAwMDIzNzI1NeZkkAnJSFVwzi_OzUxWcEpMzk4vyi_NS1HwzE1MTy3iYWBNS8wpTuWF0twMym6uIc4eugVF-YWlqcUl8Vn5pUV5QKl4IwMLCwsTQ0tLE2PiVAEAfwswyg</recordid><startdate>20011005</startdate><enddate>20011005</enddate><creator>Padin, S</creator><creator>Shepherd, M C</creator><creator>Cartwright, J K</creator><creator>Keeney, R G</creator><creator>Mason, B S</creator><creator>Pearson, T J</creator><creator>Readhead, A C S</creator><creator>Schaal, W L</creator><creator>Sievers, J</creator><creator>Udomprasert, P S</creator><creator>Yamasaki, J K</creator><creator>Holzapfel, W L</creator><creator>Carlstrom, J E</creator><creator>Joy, M</creator><creator>Myers, S T</creator><creator>Otarola, A</creator><general>Cornell University Library, arXiv.org</general><scope>8FE</scope><scope>8FG</scope><scope>ABJCF</scope><scope>ABUWG</scope><scope>AFKRA</scope><scope>AZQEC</scope><scope>BENPR</scope><scope>BGLVJ</scope><scope>CCPQU</scope><scope>DWQXO</scope><scope>HCIFZ</scope><scope>L6V</scope><scope>M7S</scope><scope>PIMPY</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>PRINS</scope><scope>PTHSS</scope></search><sort><creationdate>20011005</creationdate><title>The Cosmic Background Imager</title><author>Padin, S ; Shepherd, M C ; Cartwright, J K ; Keeney, R G ; Mason, B S ; Pearson, T J ; Readhead, A C S ; Schaal, W L ; Sievers, J ; Udomprasert, P S ; Yamasaki, J K ; Holzapfel, W L ; Carlstrom, J E ; Joy, M ; Myers, S T ; Otarola, A</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-proquest_journals_20888419943</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2001</creationdate><topic>Antenna arrays</topic><topic>Antennas</topic><topic>Background radiation</topic><topic>Big Bang theory</topic><topic>Cosmic microwave background</topic><topic>Crosstalk</topic><topic>Multipoles</topic><topic>Polarization</topic><topic>Signal processing</topic><topic>Three axis</topic><topic>Tracking</topic><topic>Variations</topic><toplevel>online_resources</toplevel><creatorcontrib>Padin, S</creatorcontrib><creatorcontrib>Shepherd, M C</creatorcontrib><creatorcontrib>Cartwright, J K</creatorcontrib><creatorcontrib>Keeney, R G</creatorcontrib><creatorcontrib>Mason, B S</creatorcontrib><creatorcontrib>Pearson, T J</creatorcontrib><creatorcontrib>Readhead, A C S</creatorcontrib><creatorcontrib>Schaal, W L</creatorcontrib><creatorcontrib>Sievers, J</creatorcontrib><creatorcontrib>Udomprasert, P S</creatorcontrib><creatorcontrib>Yamasaki, J K</creatorcontrib><creatorcontrib>Holzapfel, W L</creatorcontrib><creatorcontrib>Carlstrom, J E</creatorcontrib><creatorcontrib>Joy, M</creatorcontrib><creatorcontrib>Myers, S T</creatorcontrib><creatorcontrib>Otarola, A</creatorcontrib><collection>ProQuest SciTech Collection</collection><collection>ProQuest Technology Collection</collection><collection>Materials Science &amp; Engineering Collection</collection><collection>ProQuest Central (Alumni Edition)</collection><collection>ProQuest Central UK/Ireland</collection><collection>ProQuest Central Essentials</collection><collection>ProQuest Central</collection><collection>Technology Collection</collection><collection>ProQuest One Community College</collection><collection>ProQuest Central Korea</collection><collection>SciTech Premium Collection</collection><collection>ProQuest Engineering Collection</collection><collection>Engineering Database</collection><collection>Publicly Available Content Database</collection><collection>ProQuest One Academic Eastern Edition (DO NOT USE)</collection><collection>ProQuest One Academic</collection><collection>ProQuest One Academic UKI Edition</collection><collection>ProQuest Central China</collection><collection>Engineering Collection</collection></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Padin, S</au><au>Shepherd, M C</au><au>Cartwright, J K</au><au>Keeney, R G</au><au>Mason, B S</au><au>Pearson, T J</au><au>Readhead, A C S</au><au>Schaal, W L</au><au>Sievers, J</au><au>Udomprasert, P S</au><au>Yamasaki, J K</au><au>Holzapfel, W L</au><au>Carlstrom, J E</au><au>Joy, M</au><au>Myers, S T</au><au>Otarola, A</au><format>book</format><genre>document</genre><ristype>GEN</ristype><atitle>The Cosmic Background Imager</atitle><jtitle>arXiv.org</jtitle><date>2001-10-05</date><risdate>2001</risdate><eissn>2331-8422</eissn><abstract>Design and performance details are given for the Cosmic Background Imager (CBI), an interferometer array that is measuring the power spectrum of fluctuations in the cosmic microwave background radiation (CMBR) for multipoles in the range 400 &lt; l &lt; 3500. The CBI is located at an altitude of 5000 m in the Atacama Desert in northern Chile. It is a planar synthesis array with 13 0.9-m diameter antennas on a 6-m diameter tracking platform. Each antenna has a cooled, low-noise receiver operating in the 26-36 GHz band. Signals are cross-correlated in an analog filterbank correlator with ten 1 GHz bands. This allows spectral index measurements which can be used to distinguish CMBR signals from diffuse galactic foregrounds. A 1.2 kHz 180-deg phase switching scheme is used to reject cross-talk and low-frequency pick-up in the signal processing system. The CBI has a 3-axis mount which allows the tracking platform to be rotated about the optical axis, providing improved (u,v) coverage and a powerful discriminant against false signals generated in the receiving electronics. Rotating the tracking platform also permits polarization measurements when some of the antennas are configured for the orthogonal polarization.</abstract><cop>Ithaca</cop><pub>Cornell University Library, arXiv.org</pub><doi>10.48550/arxiv.0110124</doi><oa>free_for_read</oa></addata></record>
fulltext fulltext
identifier EISSN: 2331-8422
ispartof arXiv.org, 2001-10
issn 2331-8422
language eng
recordid cdi_proquest_journals_2088841994
source Free E- Journals
subjects Antenna arrays
Antennas
Background radiation
Big Bang theory
Cosmic microwave background
Crosstalk
Multipoles
Polarization
Signal processing
Three axis
Tracking
Variations
title The Cosmic Background Imager
url https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2024-12-21T11%3A20%3A37IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest&rft_val_fmt=info:ofi/fmt:kev:mtx:book&rft.genre=document&rft.atitle=The%20Cosmic%20Background%20Imager&rft.jtitle=arXiv.org&rft.au=Padin,%20S&rft.date=2001-10-05&rft.eissn=2331-8422&rft_id=info:doi/10.48550/arxiv.0110124&rft_dat=%3Cproquest%3E2088841994%3C/proquest%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_pqid=2088841994&rft_id=info:pmid/&rfr_iscdi=true