Achievable noise performance of spectroscopic prototype DEPFET detectors
A new generation of spectroscopic X-ray DEPFET detectors has been produced in the course of the detector development for the Wide Field Imager (WFI) of Athena. These devices served to perform a detailed analysis of the noise composition, which was enabled by the development of appropriate test algor...
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Veröffentlicht in: | Journal of instrumentation 2018-12, Vol.13 (12), p.P12001-P12001 |
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creator | Treberspurg, W. Meidinger, N. Müller-Seidlitz, J. Herrmann, S. |
description | A new generation of spectroscopic X-ray DEPFET detectors has been produced in the course of the detector development for the Wide Field Imager (WFI) of Athena. These devices served to perform a detailed analysis of the noise composition, which was enabled by the development of appropriate test algorithms. A result of the analysis is the distinction of different components, which sum up to the total noise. In particular the contribution of shot noise, white noise and 1/f noise to the readout noise is determined as well as the signal noise caused by the generation of charge carriers. The resulting parametrization enables the adaptation and optimization of operation modes to given purposes. The studied prototype detectors included 64×64 pixels with a linear gate design and provided an excellent noise, below 1.6 e−ENC at a readout time faster than 10 μs/pixel and a temperature of -80 ˆC in rolling-shutter operation. This performance is enabled by an extended signal integration time. A further noise reduction is prevented by the signal noise, caused by charge carrier generation. In order to demonstrate the low noise properties of the DEPFET transistor, the measurement conditions were adapted and a noise of 0.95 e−ENC was measured at the expense of the sensor size—by operating only parts of the sensor in window mode—and dynamic range—by using the Al Kα line at about 1.49 keV for calibration. |
doi_str_mv | 10.1088/1748-0221/13/12/P12001 |
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These devices served to perform a detailed analysis of the noise composition, which was enabled by the development of appropriate test algorithms. A result of the analysis is the distinction of different components, which sum up to the total noise. In particular the contribution of shot noise, white noise and 1/f noise to the readout noise is determined as well as the signal noise caused by the generation of charge carriers. The resulting parametrization enables the adaptation and optimization of operation modes to given purposes. The studied prototype detectors included 64×64 pixels with a linear gate design and provided an excellent noise, below 1.6 e−ENC at a readout time faster than 10 μs/pixel and a temperature of -80 ˆC in rolling-shutter operation. This performance is enabled by an extended signal integration time. A further noise reduction is prevented by the signal noise, caused by charge carrier generation. In order to demonstrate the low noise properties of the DEPFET transistor, the measurement conditions were adapted and a noise of 0.95 e−ENC was measured at the expense of the sensor size—by operating only parts of the sensor in window mode—and dynamic range—by using the Al Kα line at about 1.49 keV for calibration.</description><identifier>ISSN: 1748-0221</identifier><identifier>EISSN: 1748-0221</identifier><identifier>DOI: 10.1088/1748-0221/13/12/P12001</identifier><language>eng</language><publisher>Bristol: IOP Publishing</publisher><subject>Algorithms ; CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS ; Current carriers ; Detectors ; imaging spectroscopy ; instrumental noise ; K alpha line ; Low noise ; Noise ; Noise generation ; Noise reduction ; Optimization ; OTHER INSTRUMENTATION ; Parameterization ; Pixels ; Prototypes ; Sensors ; Shot noise ; solid state detectors ; Spectroscopy ; Transistors ; White noise ; X-ray detectors and telescopes</subject><ispartof>Journal of instrumentation, 2018-12, Vol.13 (12), p.P12001-P12001</ispartof><rights>Copyright IOP Publishing Dec 2018</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><cites>FETCH-LOGICAL-c305t-db72e405cec03b93a85ac0f7a50688a4186cbb21b7e3e032718aec318b62f5f03</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>230,314,776,780,881,27901,27902</link.rule.ids><backlink>$$Uhttps://www.osti.gov/servlets/purl/1490418$$D View this record in Osti.gov$$Hfree_for_read</backlink></links><search><creatorcontrib>Treberspurg, W.</creatorcontrib><creatorcontrib>Meidinger, N.</creatorcontrib><creatorcontrib>Müller-Seidlitz, J.</creatorcontrib><creatorcontrib>Herrmann, S.</creatorcontrib><creatorcontrib>SLAC National Accelerator Lab., Menlo Park, CA (United States)</creatorcontrib><creatorcontrib>Max Planck Inst. for Extraterrestrial Physics, Garching (Germany)</creatorcontrib><title>Achievable noise performance of spectroscopic prototype DEPFET detectors</title><title>Journal of instrumentation</title><description>A new generation of spectroscopic X-ray DEPFET detectors has been produced in the course of the detector development for the Wide Field Imager (WFI) of Athena. These devices served to perform a detailed analysis of the noise composition, which was enabled by the development of appropriate test algorithms. A result of the analysis is the distinction of different components, which sum up to the total noise. In particular the contribution of shot noise, white noise and 1/f noise to the readout noise is determined as well as the signal noise caused by the generation of charge carriers. The resulting parametrization enables the adaptation and optimization of operation modes to given purposes. The studied prototype detectors included 64×64 pixels with a linear gate design and provided an excellent noise, below 1.6 e−ENC at a readout time faster than 10 μs/pixel and a temperature of -80 ˆC in rolling-shutter operation. This performance is enabled by an extended signal integration time. A further noise reduction is prevented by the signal noise, caused by charge carrier generation. In order to demonstrate the low noise properties of the DEPFET transistor, the measurement conditions were adapted and a noise of 0.95 e−ENC was measured at the expense of the sensor size—by operating only parts of the sensor in window mode—and dynamic range—by using the Al Kα line at about 1.49 keV for calibration.</description><subject>Algorithms</subject><subject>CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS</subject><subject>Current carriers</subject><subject>Detectors</subject><subject>imaging spectroscopy</subject><subject>instrumental noise</subject><subject>K alpha line</subject><subject>Low noise</subject><subject>Noise</subject><subject>Noise generation</subject><subject>Noise reduction</subject><subject>Optimization</subject><subject>OTHER INSTRUMENTATION</subject><subject>Parameterization</subject><subject>Pixels</subject><subject>Prototypes</subject><subject>Sensors</subject><subject>Shot noise</subject><subject>solid state detectors</subject><subject>Spectroscopy</subject><subject>Transistors</subject><subject>White noise</subject><subject>X-ray detectors and telescopes</subject><issn>1748-0221</issn><issn>1748-0221</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2018</creationdate><recordtype>article</recordtype><recordid>eNpNkEFLw0AQhRdRsFb_ggQ9x8zsZpPNsdRqhYI96HnZbCc0pc3G3VTov3dLRDzNwHu8efMxdo_whKBUhmWuUuAcMxQZ8myNHAAv2ORPuPy3X7ObEHYAspI5TNhyZrctfZt6T0nn2kBJT75x_mA6S4lrktCTHbwL1vWtTXrvBjecekqeF-uXxUeyoSHqzodbdtWYfaC73zlln1GfL9PV--vbfLZKrQA5pJu65JSDtGRB1JUwShoLTWkkFEqZHFVh65pjXZIgELxEZcgKVHXBG9mAmLKHMdeFodXBtvH-1rquizU05hXEiGh6HE2x79eRwqB37ui72EtzUciiQlQYXcXosvG_4KnRvW8Pxp80gj6j1Wdq-kxNo9DI9YhW_ADTjGt0</recordid><startdate>20181203</startdate><enddate>20181203</enddate><creator>Treberspurg, W.</creator><creator>Meidinger, N.</creator><creator>Müller-Seidlitz, J.</creator><creator>Herrmann, S.</creator><general>IOP Publishing</general><general>Institute of Physics (IOP)</general><scope>AAYXX</scope><scope>CITATION</scope><scope>7U5</scope><scope>8FD</scope><scope>L7M</scope><scope>OIOZB</scope><scope>OTOTI</scope></search><sort><creationdate>20181203</creationdate><title>Achievable noise performance of spectroscopic prototype DEPFET detectors</title><author>Treberspurg, W. ; Meidinger, N. ; Müller-Seidlitz, J. ; Herrmann, S.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c305t-db72e405cec03b93a85ac0f7a50688a4186cbb21b7e3e032718aec318b62f5f03</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2018</creationdate><topic>Algorithms</topic><topic>CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS</topic><topic>Current carriers</topic><topic>Detectors</topic><topic>imaging spectroscopy</topic><topic>instrumental noise</topic><topic>K alpha line</topic><topic>Low noise</topic><topic>Noise</topic><topic>Noise generation</topic><topic>Noise reduction</topic><topic>Optimization</topic><topic>OTHER INSTRUMENTATION</topic><topic>Parameterization</topic><topic>Pixels</topic><topic>Prototypes</topic><topic>Sensors</topic><topic>Shot noise</topic><topic>solid state detectors</topic><topic>Spectroscopy</topic><topic>Transistors</topic><topic>White noise</topic><topic>X-ray detectors and telescopes</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Treberspurg, W.</creatorcontrib><creatorcontrib>Meidinger, N.</creatorcontrib><creatorcontrib>Müller-Seidlitz, J.</creatorcontrib><creatorcontrib>Herrmann, S.</creatorcontrib><creatorcontrib>SLAC National Accelerator Lab., Menlo Park, CA (United States)</creatorcontrib><creatorcontrib>Max Planck Inst. for Extraterrestrial Physics, Garching (Germany)</creatorcontrib><collection>CrossRef</collection><collection>Solid State and Superconductivity Abstracts</collection><collection>Technology Research Database</collection><collection>Advanced Technologies Database with Aerospace</collection><collection>OSTI.GOV - Hybrid</collection><collection>OSTI.GOV</collection><jtitle>Journal of instrumentation</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Treberspurg, W.</au><au>Meidinger, N.</au><au>Müller-Seidlitz, J.</au><au>Herrmann, S.</au><aucorp>SLAC National Accelerator Lab., Menlo Park, CA (United States)</aucorp><aucorp>Max Planck Inst. for Extraterrestrial Physics, Garching (Germany)</aucorp><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Achievable noise performance of spectroscopic prototype DEPFET detectors</atitle><jtitle>Journal of instrumentation</jtitle><date>2018-12-03</date><risdate>2018</risdate><volume>13</volume><issue>12</issue><spage>P12001</spage><epage>P12001</epage><pages>P12001-P12001</pages><issn>1748-0221</issn><eissn>1748-0221</eissn><abstract>A new generation of spectroscopic X-ray DEPFET detectors has been produced in the course of the detector development for the Wide Field Imager (WFI) of Athena. These devices served to perform a detailed analysis of the noise composition, which was enabled by the development of appropriate test algorithms. A result of the analysis is the distinction of different components, which sum up to the total noise. In particular the contribution of shot noise, white noise and 1/f noise to the readout noise is determined as well as the signal noise caused by the generation of charge carriers. The resulting parametrization enables the adaptation and optimization of operation modes to given purposes. The studied prototype detectors included 64×64 pixels with a linear gate design and provided an excellent noise, below 1.6 e−ENC at a readout time faster than 10 μs/pixel and a temperature of -80 ˆC in rolling-shutter operation. This performance is enabled by an extended signal integration time. A further noise reduction is prevented by the signal noise, caused by charge carrier generation. In order to demonstrate the low noise properties of the DEPFET transistor, the measurement conditions were adapted and a noise of 0.95 e−ENC was measured at the expense of the sensor size—by operating only parts of the sensor in window mode—and dynamic range—by using the Al Kα line at about 1.49 keV for calibration.</abstract><cop>Bristol</cop><pub>IOP Publishing</pub><doi>10.1088/1748-0221/13/12/P12001</doi><oa>free_for_read</oa></addata></record> |
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subjects | Algorithms CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS Current carriers Detectors imaging spectroscopy instrumental noise K alpha line Low noise Noise Noise generation Noise reduction Optimization OTHER INSTRUMENTATION Parameterization Pixels Prototypes Sensors Shot noise solid state detectors Spectroscopy Transistors White noise X-ray detectors and telescopes |
title | Achievable noise performance of spectroscopic prototype DEPFET detectors |
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