H. Geoffray, S. Bandler, W. Doriese, M. Kirivanta, D. PRELE, L. Ravera, A. Argan, M. Barbera, J. Kuur, B. Leeuwen, H. Weers, R. Hoogeveen, J. Herder, S. Smith, J. Adams, J. Chervenak, M. Durkin, C. Reintsema, J. Ullom, Y. Parot, D. Barret, C. Macculi, L. Piro, F. Brachet, A. Ledot, B. Jackson
{"title":"Conceptual design of the detection chain for the X-IFU on Athena","authors":"H. Geoffray, S. Bandler, W. Doriese, M. Kirivanta, D. PRELE, L. Ravera, A. Argan, M. Barbera, J. Kuur, B. Leeuwen, H. Weers, R. Hoogeveen, J. Herder, S. Smith, J. Adams, J. Chervenak, M. Durkin, C. Reintsema, J. Ullom, Y. Parot, D. Barret, C. Macculi, L. Piro, F. Brachet, A. Ledot, B. Jackson","doi":"10.1117/12.2563628","DOIUrl":null,"url":null,"abstract":"CNES (French Space Agency) is in charge of the development of the X-IFU instrument for Athena. The main sensor array detection chain sub-system of the X-IFU instrument is one of the major sub-subsystem of the instrument, as the main contributor to the performance. This sub-system involves major partners of the X-IFU instrument, e.g GFSC, SRON, VTT, APC, and IRAP. The purpose of this paper is to present the baseline of the definition of the X-IFU detection chain in the frame at end of phase A/beginning of phase B. The readout is based on Time Domain Multiplexing (TDM). There are strong design issues which couple the different sub-components of the detection chain (the main sensor array, the cold electronics stages, and the warm electronics). The detection chain environment (thermal, mechanical and EMI/EMC environment) also requires a transverse analysis. This paper focuses on those aspects while providing design description of the sub-components of the detection chain.","PeriodicalId":170593,"journal":{"name":"Space Telescopes and Instrumentation 2020: Ultraviolet to Gamma Ray","volume":"118 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"2020-12-13","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"3","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Space Telescopes and Instrumentation 2020: Ultraviolet to Gamma Ray","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.1117/12.2563628","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 3
Abstract
CNES (French Space Agency) is in charge of the development of the X-IFU instrument for Athena. The main sensor array detection chain sub-system of the X-IFU instrument is one of the major sub-subsystem of the instrument, as the main contributor to the performance. This sub-system involves major partners of the X-IFU instrument, e.g GFSC, SRON, VTT, APC, and IRAP. The purpose of this paper is to present the baseline of the definition of the X-IFU detection chain in the frame at end of phase A/beginning of phase B. The readout is based on Time Domain Multiplexing (TDM). There are strong design issues which couple the different sub-components of the detection chain (the main sensor array, the cold electronics stages, and the warm electronics). The detection chain environment (thermal, mechanical and EMI/EMC environment) also requires a transverse analysis. This paper focuses on those aspects while providing design description of the sub-components of the detection chain.