Millimeter-Wave Polarimeters Using Kinetic Inductance Detectors for TolTEC and Beyond
Microwave kinetic inductance detectors (MKIDs) provide a compelling path forward to the large-format polarimeter, imaging, and spectrometer arrays needed for next-generation experiments in millimeter-wave cosmology and astronomy. We describe the development of feedhorn-coupled MKID detectors for the...
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Veröffentlicht in: | Journal of low temperature physics 2018, Vol.193 (3-4), p.120-127 |
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container_title | Journal of low temperature physics |
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creator | Austermann, J. E. Beall, J. A. Bryan, S. A. Dober, B. Gao, J. Hilton, G. Hubmayr, J. Mauskopf, P. McKenney, C. M. Simon, S. M. Ullom, J. N. Vissers, M. R. Wilson, G. W. |
description | Microwave kinetic inductance detectors (MKIDs) provide a compelling path forward to the large-format polarimeter, imaging, and spectrometer arrays needed for next-generation experiments in millimeter-wave cosmology and astronomy. We describe the development of feedhorn-coupled MKID detectors for the TolTEC millimeter-wave imaging polarimeter being constructed for the 50-m Large Millimeter Telescope (LMT). Observations with TolTEC are planned to begin in early 2019. TolTEC will comprise
∼
7000
polarization-sensitive MKIDs and will represent the first MKID arrays fabricated and deployed on monolithic 150 mm diameter silicon wafers—a critical step toward future large-scale experiments with over
10
5
detectors. TolTEC will operate in observational bands at 1.1, 1.4, and 2.0 mm and will use dichroic filters to define a physically independent focal plane for each passband, thus allowing the polarimeters to use simple, direct-absorption inductive structures that are impedance matched to incident radiation. This work is part of a larger program at NIST-Boulder to develop MKID-based detector technologies for use over a wide range of photon energies spanning millimeter-waves to X-rays. We present the detailed pixel layout and describe the methods, tools, and flexible design parameters that allow this solution to be optimized for use anywhere in the millimeter and sub-millimeter bands. We also present measurements of prototype devices operating in the 1.1 mm band and compare the observed optical performance to that predicted from models and simulations. |
doi_str_mv | 10.1007/s10909-018-1949-5 |
format | Article |
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∼
7000
polarization-sensitive MKIDs and will represent the first MKID arrays fabricated and deployed on monolithic 150 mm diameter silicon wafers—a critical step toward future large-scale experiments with over
10
5
detectors. TolTEC will operate in observational bands at 1.1, 1.4, and 2.0 mm and will use dichroic filters to define a physically independent focal plane for each passband, thus allowing the polarimeters to use simple, direct-absorption inductive structures that are impedance matched to incident radiation. This work is part of a larger program at NIST-Boulder to develop MKID-based detector technologies for use over a wide range of photon energies spanning millimeter-waves to X-rays. We present the detailed pixel layout and describe the methods, tools, and flexible design parameters that allow this solution to be optimized for use anywhere in the millimeter and sub-millimeter bands. We also present measurements of prototype devices operating in the 1.1 mm band and compare the observed optical performance to that predicted from models and simulations.</description><identifier>ISSN: 0022-2291</identifier><identifier>EISSN: 1573-7357</identifier><identifier>DOI: 10.1007/s10909-018-1949-5</identifier><identifier>PMID: 34815585</identifier><language>eng</language><publisher>New York: Springer US</publisher><subject>Astronomy ; Characterization and Evaluation of Materials ; Computer simulation ; Condensed Matter Physics ; Cosmology ; Design parameters ; Detectors ; Focal plane ; Imaging polarimeters ; Impedance matching ; Incident radiation ; Inductance ; Low temperature physics ; Magnetic Materials ; Magnetism ; Millimeter waves ; Physics ; Physics and Astronomy ; Sensors ; Silicon wafers</subject><ispartof>Journal of low temperature physics, 2018, Vol.193 (3-4), p.120-127</ispartof><rights>This is a U.S. government work and its text is not subject to copyright protection in the United States; however, its text may be subject to foreign copyright protection 2018</rights><rights>Copyright Springer Science & Business Media 2018</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><orcidid>0000-0002-6338-0069</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://link.springer.com/content/pdf/10.1007/s10909-018-1949-5$$EPDF$$P50$$Gspringer$$H</linktopdf><linktohtml>$$Uhttps://link.springer.com/10.1007/s10909-018-1949-5$$EHTML$$P50$$Gspringer$$H</linktohtml><link.rule.ids>230,315,782,786,887,27931,27932,41495,42564,51326</link.rule.ids></links><search><creatorcontrib>Austermann, J. E.</creatorcontrib><creatorcontrib>Beall, J. A.</creatorcontrib><creatorcontrib>Bryan, S. A.</creatorcontrib><creatorcontrib>Dober, B.</creatorcontrib><creatorcontrib>Gao, J.</creatorcontrib><creatorcontrib>Hilton, G.</creatorcontrib><creatorcontrib>Hubmayr, J.</creatorcontrib><creatorcontrib>Mauskopf, P.</creatorcontrib><creatorcontrib>McKenney, C. M.</creatorcontrib><creatorcontrib>Simon, S. M.</creatorcontrib><creatorcontrib>Ullom, J. N.</creatorcontrib><creatorcontrib>Vissers, M. R.</creatorcontrib><creatorcontrib>Wilson, G. W.</creatorcontrib><title>Millimeter-Wave Polarimeters Using Kinetic Inductance Detectors for TolTEC and Beyond</title><title>Journal of low temperature physics</title><addtitle>J Low Temp Phys</addtitle><description>Microwave kinetic inductance detectors (MKIDs) provide a compelling path forward to the large-format polarimeter, imaging, and spectrometer arrays needed for next-generation experiments in millimeter-wave cosmology and astronomy. We describe the development of feedhorn-coupled MKID detectors for the TolTEC millimeter-wave imaging polarimeter being constructed for the 50-m Large Millimeter Telescope (LMT). Observations with TolTEC are planned to begin in early 2019. TolTEC will comprise
∼
7000
polarization-sensitive MKIDs and will represent the first MKID arrays fabricated and deployed on monolithic 150 mm diameter silicon wafers—a critical step toward future large-scale experiments with over
10
5
detectors. TolTEC will operate in observational bands at 1.1, 1.4, and 2.0 mm and will use dichroic filters to define a physically independent focal plane for each passband, thus allowing the polarimeters to use simple, direct-absorption inductive structures that are impedance matched to incident radiation. This work is part of a larger program at NIST-Boulder to develop MKID-based detector technologies for use over a wide range of photon energies spanning millimeter-waves to X-rays. We present the detailed pixel layout and describe the methods, tools, and flexible design parameters that allow this solution to be optimized for use anywhere in the millimeter and sub-millimeter bands. We also present measurements of prototype devices operating in the 1.1 mm band and compare the observed optical performance to that predicted from models and simulations.</description><subject>Astronomy</subject><subject>Characterization and Evaluation of Materials</subject><subject>Computer simulation</subject><subject>Condensed Matter Physics</subject><subject>Cosmology</subject><subject>Design parameters</subject><subject>Detectors</subject><subject>Focal plane</subject><subject>Imaging polarimeters</subject><subject>Impedance matching</subject><subject>Incident radiation</subject><subject>Inductance</subject><subject>Low temperature physics</subject><subject>Magnetic Materials</subject><subject>Magnetism</subject><subject>Millimeter waves</subject><subject>Physics</subject><subject>Physics and Astronomy</subject><subject>Sensors</subject><subject>Silicon wafers</subject><issn>0022-2291</issn><issn>1573-7357</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2018</creationdate><recordtype>article</recordtype><recordid>eNpVkV1LwzAUhoMobk5_gHcFr6MnX21zI-icOpzoxYaXIU3T2dEls2kH-_dmbCBeHTjn4eU9PAhdE7glANldICBBYiA5JpJLLE7QkIiM4YyJ7BQNASjFlEoyQBchrABA5ik7RwPGcyJELoZo8V43Tb22nW3xl97a5NM3uj0sQrIItVsmb7WzXW2SqSt702lnbPIU76bzEal8m8x9M5-ME-3K5NHuvCsv0Vmlm2CvjnOEFs-T-fgVzz5epuOHGd5QQjosTGppym2RFVYTzpgsmRGUspQzLozl1ACVwIUEYyRU0hJJCw0ZSUtRZhUboftD7qYv1rY01nWtbtQmPqDbnfK6Vv8vrv5WS79VeQoZTyEG3BwDWv_T29Cple9bFzur2DBngshURIoeqBCT3dK2fxQBtVehDipUVKH2KpRgvzyseu4</recordid><startdate>2018</startdate><enddate>2018</enddate><creator>Austermann, J. E.</creator><creator>Beall, J. A.</creator><creator>Bryan, S. A.</creator><creator>Dober, B.</creator><creator>Gao, J.</creator><creator>Hilton, G.</creator><creator>Hubmayr, J.</creator><creator>Mauskopf, P.</creator><creator>McKenney, C. M.</creator><creator>Simon, S. M.</creator><creator>Ullom, J. N.</creator><creator>Vissers, M. R.</creator><creator>Wilson, G. W.</creator><general>Springer US</general><general>Springer Nature B.V</general><scope>5PM</scope><orcidid>https://orcid.org/0000-0002-6338-0069</orcidid></search><sort><creationdate>2018</creationdate><title>Millimeter-Wave Polarimeters Using Kinetic Inductance Detectors for TolTEC and Beyond</title><author>Austermann, J. E. ; Beall, J. A. ; Bryan, S. A. ; Dober, B. ; Gao, J. ; Hilton, G. ; Hubmayr, J. ; Mauskopf, P. ; McKenney, C. M. ; Simon, S. M. ; Ullom, J. N. ; Vissers, M. R. ; Wilson, G. W.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-p211t-5c6e264eb7bea14339d3c522364345ce42c02904590cc90f9e192ba0716d5d7f3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2018</creationdate><topic>Astronomy</topic><topic>Characterization and Evaluation of Materials</topic><topic>Computer simulation</topic><topic>Condensed Matter Physics</topic><topic>Cosmology</topic><topic>Design parameters</topic><topic>Detectors</topic><topic>Focal plane</topic><topic>Imaging polarimeters</topic><topic>Impedance matching</topic><topic>Incident radiation</topic><topic>Inductance</topic><topic>Low temperature physics</topic><topic>Magnetic Materials</topic><topic>Magnetism</topic><topic>Millimeter waves</topic><topic>Physics</topic><topic>Physics and Astronomy</topic><topic>Sensors</topic><topic>Silicon wafers</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Austermann, J. E.</creatorcontrib><creatorcontrib>Beall, J. A.</creatorcontrib><creatorcontrib>Bryan, S. A.</creatorcontrib><creatorcontrib>Dober, B.</creatorcontrib><creatorcontrib>Gao, J.</creatorcontrib><creatorcontrib>Hilton, G.</creatorcontrib><creatorcontrib>Hubmayr, J.</creatorcontrib><creatorcontrib>Mauskopf, P.</creatorcontrib><creatorcontrib>McKenney, C. M.</creatorcontrib><creatorcontrib>Simon, S. M.</creatorcontrib><creatorcontrib>Ullom, J. N.</creatorcontrib><creatorcontrib>Vissers, M. R.</creatorcontrib><creatorcontrib>Wilson, G. W.</creatorcontrib><collection>PubMed Central (Full Participant titles)</collection><jtitle>Journal of low temperature physics</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Austermann, J. E.</au><au>Beall, J. A.</au><au>Bryan, S. A.</au><au>Dober, B.</au><au>Gao, J.</au><au>Hilton, G.</au><au>Hubmayr, J.</au><au>Mauskopf, P.</au><au>McKenney, C. M.</au><au>Simon, S. M.</au><au>Ullom, J. N.</au><au>Vissers, M. R.</au><au>Wilson, G. W.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Millimeter-Wave Polarimeters Using Kinetic Inductance Detectors for TolTEC and Beyond</atitle><jtitle>Journal of low temperature physics</jtitle><stitle>J Low Temp Phys</stitle><date>2018</date><risdate>2018</risdate><volume>193</volume><issue>3-4</issue><spage>120</spage><epage>127</epage><pages>120-127</pages><issn>0022-2291</issn><eissn>1573-7357</eissn><abstract>Microwave kinetic inductance detectors (MKIDs) provide a compelling path forward to the large-format polarimeter, imaging, and spectrometer arrays needed for next-generation experiments in millimeter-wave cosmology and astronomy. We describe the development of feedhorn-coupled MKID detectors for the TolTEC millimeter-wave imaging polarimeter being constructed for the 50-m Large Millimeter Telescope (LMT). Observations with TolTEC are planned to begin in early 2019. TolTEC will comprise
∼
7000
polarization-sensitive MKIDs and will represent the first MKID arrays fabricated and deployed on monolithic 150 mm diameter silicon wafers—a critical step toward future large-scale experiments with over
10
5
detectors. TolTEC will operate in observational bands at 1.1, 1.4, and 2.0 mm and will use dichroic filters to define a physically independent focal plane for each passband, thus allowing the polarimeters to use simple, direct-absorption inductive structures that are impedance matched to incident radiation. This work is part of a larger program at NIST-Boulder to develop MKID-based detector technologies for use over a wide range of photon energies spanning millimeter-waves to X-rays. We present the detailed pixel layout and describe the methods, tools, and flexible design parameters that allow this solution to be optimized for use anywhere in the millimeter and sub-millimeter bands. We also present measurements of prototype devices operating in the 1.1 mm band and compare the observed optical performance to that predicted from models and simulations.</abstract><cop>New York</cop><pub>Springer US</pub><pmid>34815585</pmid><doi>10.1007/s10909-018-1949-5</doi><tpages>8</tpages><orcidid>https://orcid.org/0000-0002-6338-0069</orcidid></addata></record> |
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subjects | Astronomy Characterization and Evaluation of Materials Computer simulation Condensed Matter Physics Cosmology Design parameters Detectors Focal plane Imaging polarimeters Impedance matching Incident radiation Inductance Low temperature physics Magnetic Materials Magnetism Millimeter waves Physics Physics and Astronomy Sensors Silicon wafers |
title | Millimeter-Wave Polarimeters Using Kinetic Inductance Detectors for TolTEC and Beyond |
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