eXTP Large Area Detector: Qualification procedure of the mass production

A 7.24 × 12.03 cm 2 sensor, Silicon Drift Detector (SDD), has been developed for the enhanced X-ray Timing and Polarimetry (eXTP) mission of the Chinese Academy of...
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Autor*in:	Rachevski, A. [verfasserIn] Antonelli, M. [verfasserIn] Bellutti, P. [verfasserIn] Bonvicini, V. [verfasserIn] Borghi, G. [verfasserIn] Campana, R. [verfasserIn] Ceraudo, F. [verfasserIn] Cirrincione, D. [verfasserIn] Del Monte, E. [verfasserIn] Evangelista, Y. [verfasserIn] Feroci, M. [verfasserIn] Ficorella, F. [verfasserIn] Orzan, G. [verfasserIn] Pepponi, G. [verfasserIn] Picciotto, A. [verfasserIn] Rashevskaya, I. [verfasserIn] Zampa, G. [verfasserIn] Zampa, N. [verfasserIn] Zorzi, N. [verfasserIn] Vacchi, A. [verfasserIn]

Format:	E-Artikel
Sprache:	Englisch

Erschienen:	2022

Schlagwörter:	X-ray spectroscopy Silicon drift detectors

Übergeordnetes Werk:	Enthalten in: Nuclear instruments & methods in physics research / A - Amsterdam : North-Holland Publ. Co., 1984, 1046
Übergeordnetes Werk:	volume:1046

DOI / URN:	10.1016/j.nima.2022.167750

Katalog-ID:	ELV008875065

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520			\|a A 7.24 × 12.03 cm 2 sensor, Silicon Drift Detector (SDD), has been developed for the enhanced X-ray Timing and Polarimetry (eXTP) mission of the Chinese Academy of Science, with a large contribution by a European consortium inherited from the ESA-M3 LOFT mission study. In the frame of the project X-ray Observatories (XRO), active in the National Scientific Commission 2 of the INFN, we report the details of the qualification procedure to select from the mass production the 640 sensors that will equip the Large Area Detector (the eXTP instrument dedicated to the X-ray spectroscopy in the range 2-30 keV), with energy resolution below 240 eV FWHM at 6 keV during the entire mission duration of at least 5 years. This stringent requirement dictates the need to thoroughly verify the characteristics of each single sensor before integration in the final layout. We describe the dedicated testing facilities that have been developed. We report on the detector selection criteria and test results obtained in the pre-series production.
650		4	\|a X-ray spectroscopy
650		4	\|a Silicon drift detectors
700	1		\|a Antonelli, M. \|e verfasserin \|0 (orcid)0000-0003-3400-6710 \|4 aut
700	1		\|a Bellutti, P. \|e verfasserin \|4 aut
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700	1		\|a Borghi, G. \|e verfasserin \|0 (orcid)0000-0001-8488-4728 \|4 aut
700	1		\|a Campana, R. \|e verfasserin \|4 aut
700	1		\|a Ceraudo, F. \|e verfasserin \|0 (orcid)0000-0001-9110-3192 \|4 aut
700	1		\|a Cirrincione, D. \|e verfasserin \|0 (orcid)0000-0002-2861-0738 \|4 aut
700	1		\|a Del Monte, E. \|e verfasserin \|0 (orcid)0000-0002-3013-6334 \|4 aut
700	1		\|a Evangelista, Y. \|e verfasserin \|0 (orcid)0000-0001-6096-6710 \|4 aut
700	1		\|a Feroci, M. \|e verfasserin \|4 aut
700	1		\|a Ficorella, F. \|e verfasserin \|4 aut
700	1		\|a Orzan, G. \|e verfasserin \|4 aut
700	1		\|a Pepponi, G. \|e verfasserin \|0 (orcid)0000-0002-7397-1946 \|4 aut
700	1		\|a Picciotto, A. \|e verfasserin \|4 aut
700	1		\|a Rashevskaya, I. \|e verfasserin \|4 aut
700	1		\|a Zampa, G. \|e verfasserin \|0 (orcid)0000-0003-0238-4469 \|4 aut
700	1		\|a Zampa, N. \|e verfasserin \|0 (orcid)0000-0003-3842-993X \|4 aut
700	1		\|a Zorzi, N. \|e verfasserin \|0 (orcid)0000-0002-6650-3925 \|4 aut
700	1		\|a Vacchi, A. \|e verfasserin \|0 (orcid)0000-0003-3855-5856 \|4 aut
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allfields	10.1016/j.nima.2022.167750 doi (DE-627)ELV008875065 (ELSEVIER)S0168-9002(22)01042-7 DE-627 ger DE-627 rda eng 530 VZ 33.05 bkl 33.07 bkl 33.40 bkl Rachevski, A. verfasserin (orcid)0000-0002-2723-6297 aut eXTP Large Area Detector: Qualification procedure of the mass production 2022 nicht spezifiziert zzz rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier A 7.24 × 12.03 cm 2 sensor, Silicon Drift Detector (SDD), has been developed for the enhanced X-ray Timing and Polarimetry (eXTP) mission of the Chinese Academy of Science, with a large contribution by a European consortium inherited from the ESA-M3 LOFT mission study. In the frame of the project X-ray Observatories (XRO), active in the National Scientific Commission 2 of the INFN, we report the details of the qualification procedure to select from the mass production the 640 sensors that will equip the Large Area Detector (the eXTP instrument dedicated to the X-ray spectroscopy in the range 2-30 keV), with energy resolution below 240 eV FWHM at 6 keV during the entire mission duration of at least 5 years. This stringent requirement dictates the need to thoroughly verify the characteristics of each single sensor before integration in the final layout. We describe the dedicated testing facilities that have been developed. We report on the detector selection criteria and test results obtained in the pre-series production. X-ray spectroscopy Silicon drift detectors Antonelli, M. verfasserin (orcid)0000-0003-3400-6710 aut Bellutti, P. verfasserin aut Bonvicini, V. verfasserin (orcid)0000-0003-1826-5843 aut Borghi, G. verfasserin (orcid)0000-0001-8488-4728 aut Campana, R. verfasserin aut Ceraudo, F. verfasserin (orcid)0000-0001-9110-3192 aut Cirrincione, D. verfasserin (orcid)0000-0002-2861-0738 aut Del Monte, E. verfasserin (orcid)0000-0002-3013-6334 aut Evangelista, Y. verfasserin (orcid)0000-0001-6096-6710 aut Feroci, M. verfasserin aut Ficorella, F. verfasserin aut Orzan, G. verfasserin aut Pepponi, G. verfasserin (orcid)0000-0002-7397-1946 aut Picciotto, A. verfasserin aut Rashevskaya, I. verfasserin aut Zampa, G. verfasserin (orcid)0000-0003-0238-4469 aut Zampa, N. verfasserin (orcid)0000-0003-3842-993X aut Zorzi, N. verfasserin (orcid)0000-0002-6650-3925 aut Vacchi, A. verfasserin (orcid)0000-0003-3855-5856 aut Enthalten in Nuclear instruments & methods in physics research / A Amsterdam : North-Holland Publ. Co., 1984 1046 Online-Ressource (DE-627)266014666 (DE-600)1466532-3 (DE-576)074959743 0168-9002 nnns volume:1046 GBV_USEFLAG_U GBV_ELV SYSFLAG_U GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_151 GBV_ILN_224 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2027 GBV_ILN_2034 GBV_ILN_2038 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2056 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2118 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2190 GBV_ILN_2336 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4313 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4393 33.05 Experimentalphysik VZ 33.07 Spektroskopie VZ 33.40 Kernphysik VZ AR 1046
spelling	10.1016/j.nima.2022.167750 doi (DE-627)ELV008875065 (ELSEVIER)S0168-9002(22)01042-7 DE-627 ger DE-627 rda eng 530 VZ 33.05 bkl 33.07 bkl 33.40 bkl Rachevski, A. verfasserin (orcid)0000-0002-2723-6297 aut eXTP Large Area Detector: Qualification procedure of the mass production 2022 nicht spezifiziert zzz rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier A 7.24 × 12.03 cm 2 sensor, Silicon Drift Detector (SDD), has been developed for the enhanced X-ray Timing and Polarimetry (eXTP) mission of the Chinese Academy of Science, with a large contribution by a European consortium inherited from the ESA-M3 LOFT mission study. In the frame of the project X-ray Observatories (XRO), active in the National Scientific Commission 2 of the INFN, we report the details of the qualification procedure to select from the mass production the 640 sensors that will equip the Large Area Detector (the eXTP instrument dedicated to the X-ray spectroscopy in the range 2-30 keV), with energy resolution below 240 eV FWHM at 6 keV during the entire mission duration of at least 5 years. This stringent requirement dictates the need to thoroughly verify the characteristics of each single sensor before integration in the final layout. We describe the dedicated testing facilities that have been developed. We report on the detector selection criteria and test results obtained in the pre-series production. X-ray spectroscopy Silicon drift detectors Antonelli, M. verfasserin (orcid)0000-0003-3400-6710 aut Bellutti, P. verfasserin aut Bonvicini, V. verfasserin (orcid)0000-0003-1826-5843 aut Borghi, G. verfasserin (orcid)0000-0001-8488-4728 aut Campana, R. verfasserin aut Ceraudo, F. verfasserin (orcid)0000-0001-9110-3192 aut Cirrincione, D. verfasserin (orcid)0000-0002-2861-0738 aut Del Monte, E. verfasserin (orcid)0000-0002-3013-6334 aut Evangelista, Y. verfasserin (orcid)0000-0001-6096-6710 aut Feroci, M. verfasserin aut Ficorella, F. verfasserin aut Orzan, G. verfasserin aut Pepponi, G. verfasserin (orcid)0000-0002-7397-1946 aut Picciotto, A. verfasserin aut Rashevskaya, I. verfasserin aut Zampa, G. verfasserin (orcid)0000-0003-0238-4469 aut Zampa, N. verfasserin (orcid)0000-0003-3842-993X aut Zorzi, N. verfasserin (orcid)0000-0002-6650-3925 aut Vacchi, A. verfasserin (orcid)0000-0003-3855-5856 aut Enthalten in Nuclear instruments & methods in physics research / A Amsterdam : North-Holland Publ. Co., 1984 1046 Online-Ressource (DE-627)266014666 (DE-600)1466532-3 (DE-576)074959743 0168-9002 nnns volume:1046 GBV_USEFLAG_U GBV_ELV SYSFLAG_U GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_151 GBV_ILN_224 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2027 GBV_ILN_2034 GBV_ILN_2038 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2056 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2118 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2190 GBV_ILN_2336 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4313 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4393 33.05 Experimentalphysik VZ 33.07 Spektroskopie VZ 33.40 Kernphysik VZ AR 1046
allfields_unstemmed	10.1016/j.nima.2022.167750 doi (DE-627)ELV008875065 (ELSEVIER)S0168-9002(22)01042-7 DE-627 ger DE-627 rda eng 530 VZ 33.05 bkl 33.07 bkl 33.40 bkl Rachevski, A. verfasserin (orcid)0000-0002-2723-6297 aut eXTP Large Area Detector: Qualification procedure of the mass production 2022 nicht spezifiziert zzz rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier A 7.24 × 12.03 cm 2 sensor, Silicon Drift Detector (SDD), has been developed for the enhanced X-ray Timing and Polarimetry (eXTP) mission of the Chinese Academy of Science, with a large contribution by a European consortium inherited from the ESA-M3 LOFT mission study. In the frame of the project X-ray Observatories (XRO), active in the National Scientific Commission 2 of the INFN, we report the details of the qualification procedure to select from the mass production the 640 sensors that will equip the Large Area Detector (the eXTP instrument dedicated to the X-ray spectroscopy in the range 2-30 keV), with energy resolution below 240 eV FWHM at 6 keV during the entire mission duration of at least 5 years. This stringent requirement dictates the need to thoroughly verify the characteristics of each single sensor before integration in the final layout. We describe the dedicated testing facilities that have been developed. We report on the detector selection criteria and test results obtained in the pre-series production. X-ray spectroscopy Silicon drift detectors Antonelli, M. verfasserin (orcid)0000-0003-3400-6710 aut Bellutti, P. verfasserin aut Bonvicini, V. verfasserin (orcid)0000-0003-1826-5843 aut Borghi, G. verfasserin (orcid)0000-0001-8488-4728 aut Campana, R. verfasserin aut Ceraudo, F. verfasserin (orcid)0000-0001-9110-3192 aut Cirrincione, D. verfasserin (orcid)0000-0002-2861-0738 aut Del Monte, E. verfasserin (orcid)0000-0002-3013-6334 aut Evangelista, Y. verfasserin (orcid)0000-0001-6096-6710 aut Feroci, M. verfasserin aut Ficorella, F. verfasserin aut Orzan, G. verfasserin aut Pepponi, G. verfasserin (orcid)0000-0002-7397-1946 aut Picciotto, A. verfasserin aut Rashevskaya, I. verfasserin aut Zampa, G. verfasserin (orcid)0000-0003-0238-4469 aut Zampa, N. verfasserin (orcid)0000-0003-3842-993X aut Zorzi, N. verfasserin (orcid)0000-0002-6650-3925 aut Vacchi, A. verfasserin (orcid)0000-0003-3855-5856 aut Enthalten in Nuclear instruments & methods in physics research / A Amsterdam : North-Holland Publ. Co., 1984 1046 Online-Ressource (DE-627)266014666 (DE-600)1466532-3 (DE-576)074959743 0168-9002 nnns volume:1046 GBV_USEFLAG_U GBV_ELV SYSFLAG_U GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_151 GBV_ILN_224 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2027 GBV_ILN_2034 GBV_ILN_2038 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2056 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2118 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2190 GBV_ILN_2336 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4313 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4393 33.05 Experimentalphysik VZ 33.07 Spektroskopie VZ 33.40 Kernphysik VZ AR 1046
allfieldsGer	10.1016/j.nima.2022.167750 doi (DE-627)ELV008875065 (ELSEVIER)S0168-9002(22)01042-7 DE-627 ger DE-627 rda eng 530 VZ 33.05 bkl 33.07 bkl 33.40 bkl Rachevski, A. verfasserin (orcid)0000-0002-2723-6297 aut eXTP Large Area Detector: Qualification procedure of the mass production 2022 nicht spezifiziert zzz rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier A 7.24 × 12.03 cm 2 sensor, Silicon Drift Detector (SDD), has been developed for the enhanced X-ray Timing and Polarimetry (eXTP) mission of the Chinese Academy of Science, with a large contribution by a European consortium inherited from the ESA-M3 LOFT mission study. In the frame of the project X-ray Observatories (XRO), active in the National Scientific Commission 2 of the INFN, we report the details of the qualification procedure to select from the mass production the 640 sensors that will equip the Large Area Detector (the eXTP instrument dedicated to the X-ray spectroscopy in the range 2-30 keV), with energy resolution below 240 eV FWHM at 6 keV during the entire mission duration of at least 5 years. This stringent requirement dictates the need to thoroughly verify the characteristics of each single sensor before integration in the final layout. We describe the dedicated testing facilities that have been developed. We report on the detector selection criteria and test results obtained in the pre-series production. X-ray spectroscopy Silicon drift detectors Antonelli, M. verfasserin (orcid)0000-0003-3400-6710 aut Bellutti, P. verfasserin aut Bonvicini, V. verfasserin (orcid)0000-0003-1826-5843 aut Borghi, G. verfasserin (orcid)0000-0001-8488-4728 aut Campana, R. verfasserin aut Ceraudo, F. verfasserin (orcid)0000-0001-9110-3192 aut Cirrincione, D. verfasserin (orcid)0000-0002-2861-0738 aut Del Monte, E. verfasserin (orcid)0000-0002-3013-6334 aut Evangelista, Y. verfasserin (orcid)0000-0001-6096-6710 aut Feroci, M. verfasserin aut Ficorella, F. verfasserin aut Orzan, G. verfasserin aut Pepponi, G. verfasserin (orcid)0000-0002-7397-1946 aut Picciotto, A. verfasserin aut Rashevskaya, I. verfasserin aut Zampa, G. verfasserin (orcid)0000-0003-0238-4469 aut Zampa, N. verfasserin (orcid)0000-0003-3842-993X aut Zorzi, N. verfasserin (orcid)0000-0002-6650-3925 aut Vacchi, A. verfasserin (orcid)0000-0003-3855-5856 aut Enthalten in Nuclear instruments & methods in physics research / A Amsterdam : North-Holland Publ. Co., 1984 1046 Online-Ressource (DE-627)266014666 (DE-600)1466532-3 (DE-576)074959743 0168-9002 nnns volume:1046 GBV_USEFLAG_U GBV_ELV SYSFLAG_U GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_151 GBV_ILN_224 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2027 GBV_ILN_2034 GBV_ILN_2038 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2056 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2118 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2190 GBV_ILN_2336 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4313 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4393 33.05 Experimentalphysik VZ 33.07 Spektroskopie VZ 33.40 Kernphysik VZ AR 1046
allfieldsSound	10.1016/j.nima.2022.167750 doi (DE-627)ELV008875065 (ELSEVIER)S0168-9002(22)01042-7 DE-627 ger DE-627 rda eng 530 VZ 33.05 bkl 33.07 bkl 33.40 bkl Rachevski, A. verfasserin (orcid)0000-0002-2723-6297 aut eXTP Large Area Detector: Qualification procedure of the mass production 2022 nicht spezifiziert zzz rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier A 7.24 × 12.03 cm 2 sensor, Silicon Drift Detector (SDD), has been developed for the enhanced X-ray Timing and Polarimetry (eXTP) mission of the Chinese Academy of Science, with a large contribution by a European consortium inherited from the ESA-M3 LOFT mission study. In the frame of the project X-ray Observatories (XRO), active in the National Scientific Commission 2 of the INFN, we report the details of the qualification procedure to select from the mass production the 640 sensors that will equip the Large Area Detector (the eXTP instrument dedicated to the X-ray spectroscopy in the range 2-30 keV), with energy resolution below 240 eV FWHM at 6 keV during the entire mission duration of at least 5 years. This stringent requirement dictates the need to thoroughly verify the characteristics of each single sensor before integration in the final layout. We describe the dedicated testing facilities that have been developed. We report on the detector selection criteria and test results obtained in the pre-series production. X-ray spectroscopy Silicon drift detectors Antonelli, M. verfasserin (orcid)0000-0003-3400-6710 aut Bellutti, P. verfasserin aut Bonvicini, V. verfasserin (orcid)0000-0003-1826-5843 aut Borghi, G. verfasserin (orcid)0000-0001-8488-4728 aut Campana, R. verfasserin aut Ceraudo, F. verfasserin (orcid)0000-0001-9110-3192 aut Cirrincione, D. verfasserin (orcid)0000-0002-2861-0738 aut Del Monte, E. verfasserin (orcid)0000-0002-3013-6334 aut Evangelista, Y. verfasserin (orcid)0000-0001-6096-6710 aut Feroci, M. verfasserin aut Ficorella, F. verfasserin aut Orzan, G. verfasserin aut Pepponi, G. verfasserin (orcid)0000-0002-7397-1946 aut Picciotto, A. verfasserin aut Rashevskaya, I. verfasserin aut Zampa, G. verfasserin (orcid)0000-0003-0238-4469 aut Zampa, N. verfasserin (orcid)0000-0003-3842-993X aut Zorzi, N. verfasserin (orcid)0000-0002-6650-3925 aut Vacchi, A. verfasserin (orcid)0000-0003-3855-5856 aut Enthalten in Nuclear instruments & methods in physics research / A Amsterdam : North-Holland Publ. Co., 1984 1046 Online-Ressource (DE-627)266014666 (DE-600)1466532-3 (DE-576)074959743 0168-9002 nnns volume:1046 GBV_USEFLAG_U GBV_ELV SYSFLAG_U GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_150 GBV_ILN_151 GBV_ILN_224 GBV_ILN_370 GBV_ILN_602 GBV_ILN_702 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2027 GBV_ILN_2034 GBV_ILN_2038 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2056 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2118 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2190 GBV_ILN_2336 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4126 GBV_ILN_4242 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4313 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4338 GBV_ILN_4393 33.05 Experimentalphysik VZ 33.07 Spektroskopie VZ 33.40 Kernphysik VZ AR 1046
language	English
source	Enthalten in Nuclear instruments & methods in physics research / A 1046 volume:1046
sourceStr	Enthalten in Nuclear instruments & methods in physics research / A 1046 volume:1046
format_phy_str_mv	Article
bklname	Experimentalphysik Spektroskopie Kernphysik
institution	findex.gbv.de
topic_facet	X-ray spectroscopy Silicon drift detectors
dewey-raw	530
isfreeaccess_bool	false
container_title	Nuclear instruments & methods in physics research / A
authorswithroles_txt_mv	Rachevski, A. @@aut@@ Antonelli, M. @@aut@@ Bellutti, P. @@aut@@ Bonvicini, V. @@aut@@ Borghi, G. @@aut@@ Campana, R. @@aut@@ Ceraudo, F. @@aut@@ Cirrincione, D. @@aut@@ Del Monte, E. @@aut@@ Evangelista, Y. @@aut@@ Feroci, M. @@aut@@ Ficorella, F. @@aut@@ Orzan, G. @@aut@@ Pepponi, G. @@aut@@ Picciotto, A. @@aut@@ Rashevskaya, I. @@aut@@ Zampa, G. @@aut@@ Zampa, N. @@aut@@ Zorzi, N. @@aut@@ Vacchi, A. @@aut@@
publishDateDaySort_date	2022-01-01T00:00:00Z
hierarchy_top_id	266014666
dewey-sort	3530
id	ELV008875065
language_de	englisch
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title_sort	extp large area detector: qualification procedure of the mass production
title_auth	eXTP Large Area Detector: Qualification procedure of the mass production
abstract	A 7.24 × 12.03 cm 2 sensor, Silicon Drift Detector (SDD), has been developed for the enhanced X-ray Timing and Polarimetry (eXTP) mission of the Chinese Academy of Science, with a large contribution by a European consortium inherited from the ESA-M3 LOFT mission study. In the frame of the project X-ray Observatories (XRO), active in the National Scientific Commission 2 of the INFN, we report the details of the qualification procedure to select from the mass production the 640 sensors that will equip the Large Area Detector (the eXTP instrument dedicated to the X-ray spectroscopy in the range 2-30 keV), with energy resolution below 240 eV FWHM at 6 keV during the entire mission duration of at least 5 years. This stringent requirement dictates the need to thoroughly verify the characteristics of each single sensor before integration in the final layout. We describe the dedicated testing facilities that have been developed. We report on the detector selection criteria and test results obtained in the pre-series production.
abstractGer	A 7.24 × 12.03 cm 2 sensor, Silicon Drift Detector (SDD), has been developed for the enhanced X-ray Timing and Polarimetry (eXTP) mission of the Chinese Academy of Science, with a large contribution by a European consortium inherited from the ESA-M3 LOFT mission study. In the frame of the project X-ray Observatories (XRO), active in the National Scientific Commission 2 of the INFN, we report the details of the qualification procedure to select from the mass production the 640 sensors that will equip the Large Area Detector (the eXTP instrument dedicated to the X-ray spectroscopy in the range 2-30 keV), with energy resolution below 240 eV FWHM at 6 keV during the entire mission duration of at least 5 years. This stringent requirement dictates the need to thoroughly verify the characteristics of each single sensor before integration in the final layout. We describe the dedicated testing facilities that have been developed. We report on the detector selection criteria and test results obtained in the pre-series production.
abstract_unstemmed	A 7.24 × 12.03 cm 2 sensor, Silicon Drift Detector (SDD), has been developed for the enhanced X-ray Timing and Polarimetry (eXTP) mission of the Chinese Academy of Science, with a large contribution by a European consortium inherited from the ESA-M3 LOFT mission study. In the frame of the project X-ray Observatories (XRO), active in the National Scientific Commission 2 of the INFN, we report the details of the qualification procedure to select from the mass production the 640 sensors that will equip the Large Area Detector (the eXTP instrument dedicated to the X-ray spectroscopy in the range 2-30 keV), with energy resolution below 240 eV FWHM at 6 keV during the entire mission duration of at least 5 years. This stringent requirement dictates the need to thoroughly verify the characteristics of each single sensor before integration in the final layout. We describe the dedicated testing facilities that have been developed. We report on the detector selection criteria and test results obtained in the pre-series production.
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title_short	eXTP Large Area Detector: Qualification procedure of the mass production
remote_bool	true
author2	Antonelli, M. Bellutti, P. Bonvicini, V. Borghi, G. Campana, R. Ceraudo, F. Cirrincione, D. Del Monte, E. Evangelista, Y. Feroci, M. Ficorella, F. Orzan, G. Pepponi, G. Picciotto, A. Rashevskaya, I. Zampa, G. Zampa, N. Zorzi, N. Vacchi, A.
author2Str	Antonelli, M. Bellutti, P. Bonvicini, V. Borghi, G. Campana, R. Ceraudo, F. Cirrincione, D. Del Monte, E. Evangelista, Y. Feroci, M. Ficorella, F. Orzan, G. Pepponi, G. Picciotto, A. Rashevskaya, I. Zampa, G. Zampa, N. Zorzi, N. Vacchi, A.
ppnlink	266014666
mediatype_str_mv	c
isOA_txt	false
hochschulschrift_bool	false
doi_str	10.1016/j.nima.2022.167750
up_date	2024-07-06T21:12:21.601Z
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