Frequency Domain Multiplexed Readout of TES Detector Arrays With Baseband Feedback
SRON is developing an electronic read-out system for an array of Transition-Edge Sensors (TES) which combines the techniques of Frequency Domain Multiplexing (FDM) with Base-Band FeedBack (BBFB). Its potential astronomical applications are in the read-out of soft X-ray microcalorimeters of the XMS i...
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creator | den Hartog, Roland H Beyer, J Boersma, D Bruijn, M Gottardi, L Hoevers, H Rui Hou Kiviranta, M de Korte, P van der Kuur, J van Leeuwen, B Lindeman, M Nieuwenhuizen, A |
description | SRON is developing an electronic read-out system for an array of Transition-Edge Sensors (TES) which combines the techniques of Frequency Domain Multiplexing (FDM) with Base-Band FeedBack (BBFB). Its potential astronomical applications are in the read-out of soft X-ray microcalorimeters of the XMS instrument on the International X-ray Observatory (IXO) and the far-IR bolometers of the SAFARI instrument on the Japanese-European mission SPICA. In this paper we focus on the experimental verification of the system, demonstrating for 16 pixels that simultaneous read-out does not degrade the noise performance, and that crosstalk between pixels is close to the requirements for IXO. A detailed analysis of the BBFB system is presented, identifying its limitations and routes for improvement to the levels required for implementation on both missions. |
doi_str_mv | 10.1109/TASC.2010.2101998 |
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Its potential astronomical applications are in the read-out of soft X-ray microcalorimeters of the XMS instrument on the International X-ray Observatory (IXO) and the far-IR bolometers of the SAFARI instrument on the Japanese-European mission SPICA. In this paper we focus on the experimental verification of the system, demonstrating for 16 pixels that simultaneous read-out does not degrade the noise performance, and that crosstalk between pixels is close to the requirements for IXO. A detailed analysis of the BBFB system is presented, identifying its limitations and routes for improvement to the levels required for implementation on both missions.</description><identifier>ISSN: 1051-8223</identifier><identifier>EISSN: 1558-2515</identifier><identifier>DOI: 10.1109/TASC.2010.2101998</identifier><identifier>CODEN: ITASE9</identifier><language>eng</language><publisher>New York, NY: IEEE</publisher><subject>Applied sciences ; Arrays ; Bolometer; infrared, submillimeter wave, microwave and radiowave receivers and detectors ; Bolometers ; Detectors ; Electrical engineering. Electrical power engineering ; Electromagnets ; Electronics ; Exact sciences and technology ; FDM ; Feedback ; Frequency division multiplexing ; Frequency domains ; General equipment and techniques ; Infrared, submillimeter wave, microwave and radiowave instruments, equipment and techniques ; Instruments ; Instruments, apparatus, components and techniques common to several branches of physics and astronomy ; IXO ; microcalorimeters ; Missions ; Multiplexing ; Noise ; Physics ; Pixel ; Pixels ; Semiconductor electronics. Microelectronics. Optoelectronics. Solid state devices ; Sensors (chemical, optical, electrical, movement, gas, etc.); remote sensing ; SPICA ; SQUID read-out electronics ; SQUIDs ; Superconducting devices ; TES ; Various equipment and components</subject><ispartof>IEEE transactions on applied superconductivity, 2011-06, Vol.21 (3), p.289-293</ispartof><rights>2015 INIST-CNRS</rights><rights>Copyright The Institute of Electrical and Electronics Engineers, Inc. (IEEE) Jun 2011</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c402t-b8f459b9a439b34cd34f5e956163b74ecb908a7dcdde13bf898004a939d906ab3</citedby><cites>FETCH-LOGICAL-c402t-b8f459b9a439b34cd34f5e956163b74ecb908a7dcdde13bf898004a939d906ab3</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktohtml>$$Uhttps://ieeexplore.ieee.org/document/5704168$$EHTML$$P50$$Gieee$$H</linktohtml><link.rule.ids>309,310,314,776,780,785,786,792,23909,23910,25118,27901,27902,54733</link.rule.ids><linktorsrc>$$Uhttps://ieeexplore.ieee.org/document/5704168$$EView_record_in_IEEE$$FView_record_in_$$GIEEE</linktorsrc><backlink>$$Uhttp://pascal-francis.inist.fr/vibad/index.php?action=getRecordDetail&idt=24275972$$DView record in Pascal Francis$$Hfree_for_read</backlink></links><search><creatorcontrib>den Hartog, Roland H</creatorcontrib><creatorcontrib>Beyer, J</creatorcontrib><creatorcontrib>Boersma, D</creatorcontrib><creatorcontrib>Bruijn, M</creatorcontrib><creatorcontrib>Gottardi, L</creatorcontrib><creatorcontrib>Hoevers, H</creatorcontrib><creatorcontrib>Rui Hou</creatorcontrib><creatorcontrib>Kiviranta, M</creatorcontrib><creatorcontrib>de Korte, P</creatorcontrib><creatorcontrib>van der Kuur, J</creatorcontrib><creatorcontrib>van Leeuwen, B</creatorcontrib><creatorcontrib>Lindeman, M</creatorcontrib><creatorcontrib>Nieuwenhuizen, A</creatorcontrib><title>Frequency Domain Multiplexed Readout of TES Detector Arrays With Baseband Feedback</title><title>IEEE transactions on applied superconductivity</title><addtitle>TASC</addtitle><description>SRON is developing an electronic read-out system for an array of Transition-Edge Sensors (TES) which combines the techniques of Frequency Domain Multiplexing (FDM) with Base-Band FeedBack (BBFB). Its potential astronomical applications are in the read-out of soft X-ray microcalorimeters of the XMS instrument on the International X-ray Observatory (IXO) and the far-IR bolometers of the SAFARI instrument on the Japanese-European mission SPICA. In this paper we focus on the experimental verification of the system, demonstrating for 16 pixels that simultaneous read-out does not degrade the noise performance, and that crosstalk between pixels is close to the requirements for IXO. A detailed analysis of the BBFB system is presented, identifying its limitations and routes for improvement to the levels required for implementation on both missions.</description><subject>Applied sciences</subject><subject>Arrays</subject><subject>Bolometer; infrared, submillimeter wave, microwave and radiowave receivers and detectors</subject><subject>Bolometers</subject><subject>Detectors</subject><subject>Electrical engineering. Electrical power engineering</subject><subject>Electromagnets</subject><subject>Electronics</subject><subject>Exact sciences and technology</subject><subject>FDM</subject><subject>Feedback</subject><subject>Frequency division multiplexing</subject><subject>Frequency domains</subject><subject>General equipment and techniques</subject><subject>Infrared, submillimeter wave, microwave and radiowave instruments, equipment and techniques</subject><subject>Instruments</subject><subject>Instruments, apparatus, components and techniques common to several branches of physics and astronomy</subject><subject>IXO</subject><subject>microcalorimeters</subject><subject>Missions</subject><subject>Multiplexing</subject><subject>Noise</subject><subject>Physics</subject><subject>Pixel</subject><subject>Pixels</subject><subject>Semiconductor electronics. Microelectronics. Optoelectronics. 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Electrical power engineering</topic><topic>Electromagnets</topic><topic>Electronics</topic><topic>Exact sciences and technology</topic><topic>FDM</topic><topic>Feedback</topic><topic>Frequency division multiplexing</topic><topic>Frequency domains</topic><topic>General equipment and techniques</topic><topic>Infrared, submillimeter wave, microwave and radiowave instruments, equipment and techniques</topic><topic>Instruments</topic><topic>Instruments, apparatus, components and techniques common to several branches of physics and astronomy</topic><topic>IXO</topic><topic>microcalorimeters</topic><topic>Missions</topic><topic>Multiplexing</topic><topic>Noise</topic><topic>Physics</topic><topic>Pixel</topic><topic>Pixels</topic><topic>Semiconductor electronics. Microelectronics. Optoelectronics. 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Its potential astronomical applications are in the read-out of soft X-ray microcalorimeters of the XMS instrument on the International X-ray Observatory (IXO) and the far-IR bolometers of the SAFARI instrument on the Japanese-European mission SPICA. In this paper we focus on the experimental verification of the system, demonstrating for 16 pixels that simultaneous read-out does not degrade the noise performance, and that crosstalk between pixels is close to the requirements for IXO. A detailed analysis of the BBFB system is presented, identifying its limitations and routes for improvement to the levels required for implementation on both missions.</abstract><cop>New York, NY</cop><pub>IEEE</pub><doi>10.1109/TASC.2010.2101998</doi><tpages>5</tpages></addata></record> |
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subjects | Applied sciences Arrays Bolometer infrared, submillimeter wave, microwave and radiowave receivers and detectors Bolometers Detectors Electrical engineering. Electrical power engineering Electromagnets Electronics Exact sciences and technology FDM Feedback Frequency division multiplexing Frequency domains General equipment and techniques Infrared, submillimeter wave, microwave and radiowave instruments, equipment and techniques Instruments Instruments, apparatus, components and techniques common to several branches of physics and astronomy IXO microcalorimeters Missions Multiplexing Noise Physics Pixel Pixels Semiconductor electronics. Microelectronics. Optoelectronics. Solid state devices Sensors (chemical, optical, electrical, movement, gas, etc.) remote sensing SPICA SQUID read-out electronics SQUIDs Superconducting devices TES Various equipment and components |
title | Frequency Domain Multiplexed Readout of TES Detector Arrays With Baseband Feedback |
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