A coherent polarimeter array for the Large Scale Polarization Explorer balloon experiment
We discuss the design and expected performance of STRIP (STRatospheric Italian Polarimeter), an array of coherent receivers designed to fly on board the LSPE (Large Scale Polarization Explorer) balloon experiment. The STRIP focal plane array comprises 49 elements in Q band and 7 elements in W-band u...
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| creator | Bersanelli, M Mennella, A Morgante, G Zannoni, M Addamo, G Baschirotto, A Battaglia, P Baù, A Cappellini, B Cavaliere, F Cuttaia, F F Del Torto Donzelli, S Farooqui, Z Frailis, M Franceschet, C Franceschi, E Gaier, T Galeotta, S Gervasi, M Gregorio, A Kangaslahti, P Krachmalnicoff, N Lawrence, C Maggio, G Mainini, R Maino, D Mandolesi, N Paroli, B Passerini, A Peverini, O A Poli, S Ricciardi, S Rossetti, M Sandri, M Seiffert, M Stringhetti, L Tartari, A Tascone, R Tavagnacco, D Terenzi, L Tomasi, M Tommasi, E Villa, F Virone, G Zacchei, A |
| description | We discuss the design and expected performance of STRIP (STRatospheric Italian Polarimeter), an array of coherent receivers designed to fly on board the LSPE (Large Scale Polarization Explorer) balloon experiment. The STRIP focal plane array comprises 49 elements in Q band and 7 elements in W-band using cryogenic HEMT low noise amplifiers and high performance waveguide components. In operation, the array will be cooled to 20 K and placed in the focal plane of a \(\sim 0.6\) meter telescope providing an angular resolution of \(\sim1.5\) degrees. The LSPE experiment aims at large scale, high sensitivity measurements of CMB polarization, with multi-frequency deep measurements to optimize component separation. The STRIP Q-band channel is crucial to accurately measure and remove the synchrotron polarized component, while the W-band channel, together with a bolometric channel at the same frequency, provides a crucial cross-check for systematic effects. |
| doi_str_mv | 10.48550/arxiv.1208.0164 |
| format | Article |
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The STRIP Q-band channel is crucial to accurately measure and remove the synchrotron polarized component, while the W-band channel, together with a bolometric channel at the same frequency, provides a crucial cross-check for systematic effects.</description><subject>Angular resolution</subject><subject>Bolometers</subject><subject>Experiments</subject><subject>Focal plane devices</subject><subject>Low noise</subject><subject>Physics - Cosmology and Nongalactic Astrophysics</subject><subject>Physics - Instrumentation and Methods for Astrophysics</subject><subject>Polarimeters</subject><subject>Polarization</subject><subject>Strip</subject><subject>Tungsten</subject><issn>2331-8422</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2012</creationdate><recordtype>article</recordtype><sourceid>ABUWG</sourceid><sourceid>AFKRA</sourceid><sourceid>AZQEC</sourceid><sourceid>BENPR</sourceid><sourceid>CCPQU</sourceid><sourceid>DWQXO</sourceid><sourceid>GOX</sourceid><recordid>eNotj0tLw0AUhQdBsNTuXcmA68TJPDKTZSn1AQUFu3EVrskdmxIzcTKV1F_vpHV14fBxzv0IuclYKo1S7B782PykGWcmZVkuL8iMC5ElRnJ-RRbDsGeM8VxzpcSMvC9p5XbosQu0dy345gsDegrew5Fa52nYId2A_0T6VkGL9PVE_UJoXEfXY986H_kPaFsXAxx7nDq6cE0uLbQDLv7vnGwf1tvVU7J5eXxeLTcJqEwmWIFFkErUos7zmoMVpo5ZjRUDiZVEyLRWRoKwYLXmYGQlLcstsKLgIObk9lx70i77OA7-WE765aQfgbsz0Hv3fcAhlHt38F18qYwMN5qZQoo_kPVfhg</recordid><startdate>20120801</startdate><enddate>20120801</enddate><creator>Bersanelli, M</creator><creator>Mennella, A</creator><creator>Morgante, G</creator><creator>Zannoni, M</creator><creator>Addamo, G</creator><creator>Baschirotto, A</creator><creator>Battaglia, P</creator><creator>Baù, A</creator><creator>Cappellini, B</creator><creator>Cavaliere, F</creator><creator>Cuttaia, F</creator><creator>F Del Torto</creator><creator>Donzelli, S</creator><creator>Farooqui, Z</creator><creator>Frailis, M</creator><creator>Franceschet, C</creator><creator>Franceschi, E</creator><creator>Gaier, T</creator><creator>Galeotta, S</creator><creator>Gervasi, M</creator><creator>Gregorio, A</creator><creator>Kangaslahti, P</creator><creator>Krachmalnicoff, N</creator><creator>Lawrence, C</creator><creator>Maggio, G</creator><creator>Mainini, R</creator><creator>Maino, D</creator><creator>Mandolesi, N</creator><creator>Paroli, B</creator><creator>Passerini, A</creator><creator>Peverini, O A</creator><creator>Poli, S</creator><creator>Ricciardi, S</creator><creator>Rossetti, M</creator><creator>Sandri, M</creator><creator>Seiffert, M</creator><creator>Stringhetti, L</creator><creator>Tartari, A</creator><creator>Tascone, R</creator><creator>Tavagnacco, D</creator><creator>Terenzi, L</creator><creator>Tomasi, M</creator><creator>Tommasi, E</creator><creator>Villa, F</creator><creator>Virone, G</creator><creator>Zacchei, 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><scope>GOX</scope></search><sort><creationdate>20120801</creationdate><title>A coherent polarimeter array for the Large Scale Polarization Explorer balloon experiment</title><author>Bersanelli, M ; Mennella, A ; Morgante, G ; Zannoni, M ; Addamo, G ; Baschirotto, A ; Battaglia, P ; Baù, A ; Cappellini, B ; Cavaliere, F ; Cuttaia, F ; F Del Torto ; Donzelli, S ; Farooqui, Z ; Frailis, M ; Franceschet, C ; Franceschi, E ; Gaier, T ; Galeotta, S ; Gervasi, M ; Gregorio, A ; Kangaslahti, P ; Krachmalnicoff, N ; Lawrence, C ; Maggio, G ; Mainini, R ; Maino, D ; Mandolesi, N ; Paroli, B ; Passerini, A ; Peverini, O A ; Poli, S ; Ricciardi, S ; Rossetti, M ; Sandri, M ; Seiffert, M ; Stringhetti, L ; Tartari, A ; Tascone, R ; Tavagnacco, D ; Terenzi, L ; Tomasi, M ; Tommasi, E ; Villa, F ; Virone, G ; Zacchei, A</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a514-ecafea453d3d66d2af38dcafdec0a4ec4ea177584a3faf772a84c4f06fa0992a3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2012</creationdate><topic>Angular resolution</topic><topic>Bolometers</topic><topic>Experiments</topic><topic>Focal plane devices</topic><topic>Low noise</topic><topic>Physics - 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The STRIP focal plane array comprises 49 elements in Q band and 7 elements in W-band using cryogenic HEMT low noise amplifiers and high performance waveguide components. In operation, the array will be cooled to 20 K and placed in the focal plane of a \(\sim 0.6\) meter telescope providing an angular resolution of \(\sim1.5\) degrees. The LSPE experiment aims at large scale, high sensitivity measurements of CMB polarization, with multi-frequency deep measurements to optimize component separation. The STRIP Q-band channel is crucial to accurately measure and remove the synchrotron polarized component, while the W-band channel, together with a bolometric channel at the same frequency, provides a crucial cross-check for systematic effects.</abstract><cop>Ithaca</cop><pub>Cornell University Library, arXiv.org</pub><doi>10.48550/arxiv.1208.0164</doi><oa>free_for_read</oa></addata></record> |
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| subjects | Angular resolution Bolometers Experiments Focal plane devices Low noise Physics - Cosmology and Nongalactic Astrophysics Physics - Instrumentation and Methods for Astrophysics Polarimeters Polarization Strip Tungsten |
| title | A coherent polarimeter array for the Large Scale Polarization Explorer balloon experiment |
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