Gilles Roudil, François Pajot, Florent Castellani, Sophie Beaumont, Michel Dupieux, David Murat, Yann Parot, Laurent Ravera, Joseph Adams, Simon Bandler, James Chervenak, Edoardo Cucchetti, Christophe Daniel, William Doriese, Malcolm Durking, Hervé Geoffray, Gene Hilton, Baptiste Mot, Philippe Peille, Damien Prêle, Carl Reintsema, Kazuhiro Sakai, Joel Ullom, Nicholas Wakeham, Alexei Molin
{"title":"Status of the end-to-end demonstration readout chain for Athena/X-IFU","authors":"Gilles Roudil, François Pajot, Florent Castellani, Sophie Beaumont, Michel Dupieux, David Murat, Yann Parot, Laurent Ravera, Joseph Adams, Simon Bandler, James Chervenak, Edoardo Cucchetti, Christophe Daniel, William Doriese, Malcolm Durking, Hervé Geoffray, Gene Hilton, Baptiste Mot, Philippe Peille, Damien Prêle, Carl Reintsema, Kazuhiro Sakai, Joel Ullom, Nicholas Wakeham, Alexei Molin","doi":"10.21203/rs.3.rs-3544860/v1","DOIUrl":null,"url":null,"abstract":"Abstract The X-ray Integral Field Unit (X-IFU) of the Athena observatory, scheduled for launch in the mid 2030's, will provide X-ray imaging spectroscopy data with unprecedented spectral and spatial resolution. The detection chain, based on a ~ 1.5 kilo-pixel array of transition edge sensors (TESs) cooled down to 55 mK, is under development by a large international collaboration. In order to perform an end-to-end demonstration of the X-IFU readout chain, a 50 mK test bench (Elsa), is being developed at IRAP in collaboration with CNES. Based on a commercial ADR cryostat, it includes a 1024-pixel TES array provided by NASA/GSFC with its associated cold readout chain provided by NIST. The validation of the performance of the system was performed using a NIST and NASA/GSFC laboratory warm readout chain. These laboratory electronics will be replaced step by step by the demonstration models of the space qualified electronics designed for the X-IFU: the digital readout electronics by IRAP and the warm front-end electronics by APC. We present here the status of the 50 mK test bench, its performance budget, and the demonstration of a prototype of a first element of the flight electronics.","PeriodicalId":500086,"journal":{"name":"Research Square (Research Square)","volume":null,"pages":null},"PeriodicalIF":0.0000,"publicationDate":"2023-11-14","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Research Square (Research Square)","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.21203/rs.3.rs-3544860/v1","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 0
Abstract
Abstract The X-ray Integral Field Unit (X-IFU) of the Athena observatory, scheduled for launch in the mid 2030's, will provide X-ray imaging spectroscopy data with unprecedented spectral and spatial resolution. The detection chain, based on a ~ 1.5 kilo-pixel array of transition edge sensors (TESs) cooled down to 55 mK, is under development by a large international collaboration. In order to perform an end-to-end demonstration of the X-IFU readout chain, a 50 mK test bench (Elsa), is being developed at IRAP in collaboration with CNES. Based on a commercial ADR cryostat, it includes a 1024-pixel TES array provided by NASA/GSFC with its associated cold readout chain provided by NIST. The validation of the performance of the system was performed using a NIST and NASA/GSFC laboratory warm readout chain. These laboratory electronics will be replaced step by step by the demonstration models of the space qualified electronics designed for the X-IFU: the digital readout electronics by IRAP and the warm front-end electronics by APC. We present here the status of the 50 mK test bench, its performance budget, and the demonstration of a prototype of a first element of the flight electronics.