Preflight Detector Characterization of BLAST-TNG
The Next-Generation Balloon-borne Large-Aperture Submillimeter Telescope (BLAST-TNG) is a submillimeter imaging polarimeter which will map the polarized thermal emission from interstellar dust, revealing magnetic field structures in nearby giant molecular clouds, external galaxies and the diffuse in...
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| Veröffentlicht in: | Journal of low temperature physics 2020-09, Vol.200 (5-6), p.400-406 |
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| container_title | Journal of low temperature physics |
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| creator | Gordon, Sam Sinclair, Adrian Mauskopf, Philip Coppi, Gabriele Devlin, Mark Dober, Bradley Fissel, Laura Galitzki, Nicholas Gao, Jiansong Hubmayr, Johannes Lourie, Nathan Lowe, Ian McKenney, Christopher Nati, Federico Romualdez, Javier |
| description | The Next-Generation Balloon-borne Large-Aperture Submillimeter Telescope (BLAST-TNG) is a submillimeter imaging polarimeter which will map the polarized thermal emission from interstellar dust, revealing magnetic field structures in nearby giant molecular clouds, external galaxies and the diffuse interstellar medium in three bands centered at 250, 350 and 500-μm (spatial resolution of 30″, 41″ and 59″). Its camera contains over 2500 dual-polarization sensitive lumped element kinetic inductance detectors, which are read out using field-programmable gate array-based readout electronics. BLAST-TNG was scheduled for a 28-day Antarctic flight during the 2018/2019 summer season, but unfavorable weather conditions pushed the anticipated flight to 2019/2020. We present a summary of key results from the 2018/2019 preflight characterization of the detector and receiver. Included in this summary are detector yields, estimates of in-flight sensitivity, a measurement of the optical passbands and estimates of polarization efficiency. |
| doi_str_mv | 10.1007/s10909-020-02459-6 |
| format | Article |
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Its camera contains over 2500 dual-polarization sensitive lumped element kinetic inductance detectors, which are read out using field-programmable gate array-based readout electronics. BLAST-TNG was scheduled for a 28-day Antarctic flight during the 2018/2019 summer season, but unfavorable weather conditions pushed the anticipated flight to 2019/2020. We present a summary of key results from the 2018/2019 preflight characterization of the detector and receiver. 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Its camera contains over 2500 dual-polarization sensitive lumped element kinetic inductance detectors, which are read out using field-programmable gate array-based readout electronics. BLAST-TNG was scheduled for a 28-day Antarctic flight during the 2018/2019 summer season, but unfavorable weather conditions pushed the anticipated flight to 2019/2020. We present a summary of key results from the 2018/2019 preflight characterization of the detector and receiver. Included in this summary are detector yields, estimates of in-flight sensitivity, a measurement of the optical passbands and estimates of polarization efficiency.</description><subject>Apertures</subject><subject>Characterization and Evaluation of Materials</subject><subject>Condensed Matter Physics</subject><subject>Cosmic dust</subject><subject>Field programmable gate arrays</subject><subject>Galaxies</subject><subject>Imaging polarimeters</subject><subject>Inductance</subject><subject>Interstellar chemistry</subject><subject>Interstellar matter</subject><subject>Low temperature physics</subject><subject>Magnetic Materials</subject><subject>Magnetism</subject><subject>Molecular clouds</subject><subject>Physics</subject><subject>Physics and Astronomy</subject><subject>Polarization</subject><subject>Sensors</subject><subject>Spatial resolution</subject><subject>Thermal emission</subject><subject>Weather</subject><issn>0022-2291</issn><issn>1573-7357</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2020</creationdate><recordtype>article</recordtype><recordid>eNp9kDFPAzEMhSMEEqXwB5hOYg44Tnq5jKXQglQBEsccXUPcXlV6JUkH-PUEDomNwbKH9z3bj7FzAZcCQF9FAQYMB4RcamR4ecAGYqQl13KkD9kAAJEjGnHMTmJcA4CpSjlg8BQ8bdrlKhU3PnmXulBMVk1oXPKh_WxS222Ljorr-fi55vXD7JQdUbOJ_uy3D9nL9Lae3PH54-x-Mp5zJ4VJHKnCptRApiRHikATonaKjFbGexTKLbxfUB7JvII2WC1AEUmVz_dSySG76H13oXvf-5jsutuHbV5pUSmBGdBVVmGvcqGLMb9id6F9a8KHFWC_k7F9MjYnY3-SsWWGZA_FLN4uffiz_of6Ami_ZKE</recordid><startdate>20200901</startdate><enddate>20200901</enddate><creator>Gordon, Sam</creator><creator>Sinclair, Adrian</creator><creator>Mauskopf, Philip</creator><creator>Coppi, Gabriele</creator><creator>Devlin, Mark</creator><creator>Dober, Bradley</creator><creator>Fissel, Laura</creator><creator>Galitzki, Nicholas</creator><creator>Gao, Jiansong</creator><creator>Hubmayr, Johannes</creator><creator>Lourie, Nathan</creator><creator>Lowe, Ian</creator><creator>McKenney, Christopher</creator><creator>Nati, Federico</creator><creator>Romualdez, Javier</creator><general>Springer US</general><general>Springer Nature B.V</general><scope>AAYXX</scope><scope>CITATION</scope><orcidid>https://orcid.org/0000-0002-4668-444X</orcidid></search><sort><creationdate>20200901</creationdate><title>Preflight Detector Characterization of BLAST-TNG</title><author>Gordon, Sam ; Sinclair, Adrian ; Mauskopf, Philip ; Coppi, Gabriele ; Devlin, Mark ; Dober, Bradley ; Fissel, Laura ; Galitzki, Nicholas ; Gao, Jiansong ; Hubmayr, Johannes ; Lourie, Nathan ; Lowe, Ian ; McKenney, Christopher ; Nati, Federico ; Romualdez, Javier</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c319t-2f82a670f96fcf4f07f227c4f9749ee214cbeebfee2f9d07928b04ff34245e343</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2020</creationdate><topic>Apertures</topic><topic>Characterization and Evaluation of Materials</topic><topic>Condensed Matter Physics</topic><topic>Cosmic dust</topic><topic>Field programmable gate arrays</topic><topic>Galaxies</topic><topic>Imaging polarimeters</topic><topic>Inductance</topic><topic>Interstellar chemistry</topic><topic>Interstellar matter</topic><topic>Low temperature physics</topic><topic>Magnetic Materials</topic><topic>Magnetism</topic><topic>Molecular clouds</topic><topic>Physics</topic><topic>Physics and Astronomy</topic><topic>Polarization</topic><topic>Sensors</topic><topic>Spatial resolution</topic><topic>Thermal emission</topic><topic>Weather</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Gordon, Sam</creatorcontrib><creatorcontrib>Sinclair, Adrian</creatorcontrib><creatorcontrib>Mauskopf, Philip</creatorcontrib><creatorcontrib>Coppi, Gabriele</creatorcontrib><creatorcontrib>Devlin, Mark</creatorcontrib><creatorcontrib>Dober, Bradley</creatorcontrib><creatorcontrib>Fissel, Laura</creatorcontrib><creatorcontrib>Galitzki, Nicholas</creatorcontrib><creatorcontrib>Gao, Jiansong</creatorcontrib><creatorcontrib>Hubmayr, Johannes</creatorcontrib><creatorcontrib>Lourie, Nathan</creatorcontrib><creatorcontrib>Lowe, Ian</creatorcontrib><creatorcontrib>McKenney, Christopher</creatorcontrib><creatorcontrib>Nati, Federico</creatorcontrib><creatorcontrib>Romualdez, Javier</creatorcontrib><collection>CrossRef</collection><jtitle>Journal of low temperature physics</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Gordon, Sam</au><au>Sinclair, Adrian</au><au>Mauskopf, Philip</au><au>Coppi, Gabriele</au><au>Devlin, Mark</au><au>Dober, Bradley</au><au>Fissel, Laura</au><au>Galitzki, Nicholas</au><au>Gao, Jiansong</au><au>Hubmayr, Johannes</au><au>Lourie, Nathan</au><au>Lowe, Ian</au><au>McKenney, Christopher</au><au>Nati, Federico</au><au>Romualdez, Javier</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Preflight Detector Characterization of BLAST-TNG</atitle><jtitle>Journal of low temperature physics</jtitle><stitle>J Low Temp Phys</stitle><date>2020-09-01</date><risdate>2020</risdate><volume>200</volume><issue>5-6</issue><spage>400</spage><epage>406</epage><pages>400-406</pages><issn>0022-2291</issn><eissn>1573-7357</eissn><abstract>The Next-Generation Balloon-borne Large-Aperture Submillimeter Telescope (BLAST-TNG) is a submillimeter imaging polarimeter which will map the polarized thermal emission from interstellar dust, revealing magnetic field structures in nearby giant molecular clouds, external galaxies and the diffuse interstellar medium in three bands centered at 250, 350 and 500-μm (spatial resolution of 30″, 41″ and 59″). 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| subjects | Apertures Characterization and Evaluation of Materials Condensed Matter Physics Cosmic dust Field programmable gate arrays Galaxies Imaging polarimeters Inductance Interstellar chemistry Interstellar matter Low temperature physics Magnetic Materials Magnetism Molecular clouds Physics Physics and Astronomy Polarization Sensors Spatial resolution Thermal emission Weather |
| title | Preflight Detector Characterization of BLAST-TNG |
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