Davide Vaccaro, Jan van der Kuur, Paul van der Hulst, Tobias Vos, Martin de Wit, Luciano Gottardi, Kevin Ravensberg, Emanuele Taralli, Joseph Adams, Simon Bandler, Douglas Bennet, James Chervenak, Bertrand Doriese, Malcolm Durkin, Jonathan Gard, Carl Reintsema, Kazuhiro Sakai, Steven Smith, Joel Ullom, Nicholas Wakeham, Jan-Willem den Herder, Brian jackson, Pourya Khosropanah, Jian-Rong Gao, Peter Roelfsema, Aurora Simionescu
{"title":"用于 NewAthena X-IFU 的时分复用读出的低温试验台的系统性能","authors":"Davide Vaccaro, Jan van der Kuur, Paul van der Hulst, Tobias Vos, Martin de Wit, Luciano Gottardi, Kevin Ravensberg, Emanuele Taralli, Joseph Adams, Simon Bandler, Douglas Bennet, James Chervenak, Bertrand Doriese, Malcolm Durkin, Jonathan Gard, Carl Reintsema, Kazuhiro Sakai, Steven Smith, Joel Ullom, Nicholas Wakeham, Jan-Willem den Herder, Brian jackson, Pourya Khosropanah, Jian-Rong Gao, Peter Roelfsema, Aurora Simionescu","doi":"arxiv-2409.05643","DOIUrl":null,"url":null,"abstract":"The X-ray Integral Field Unit (X-IFU) is an instrument of ESA's future\nNewAthena space observatory, with the goal to provide high-energy resolution\n($<$ 4 eV at X-ray energies up to 7 keV) and high-spatial resolution (9\")\nspectroscopic imaging over the X-ray energy range from 200 eV to 12 keV, by\nmeans of an array of about 1500 transition-edge sensors (TES) read out via\nSQUID time-division multiplexing (TDM). In 2022, to aid in the transfer of TDM\nreadout technology from the laboratory toward flight hardware, our team\ncommissioned a new TDM-based laboratory test-bed at SRON. This setup hosts an\narray of $75\\times 75\\ \\mu$m$^2$ TESs that are read out via 2-column $\\times$\n32-row TDM. A system component that is critical to high-performance operation\nis the wiring harness that connects the room-temperature electronics to the\ncryogenic readout componentry. In November 2023, we implemented a re-designed\nflex harness, which in the SRON test-bed has a length close to what is\nenvisioned for the X-IFU flight harness. We report here on our characterization\nof the TDM system with the new flex harness, which allowed the system to\nachieve a co-added energy resolution at a level of 2.7~eV FWHM at 6~keV via\n32-row readout. In addition, we provide an outlook on the upcoming integration\nof TDM readout into the X-IFU Focal-Plane Assembly Development Model.","PeriodicalId":501163,"journal":{"name":"arXiv - PHYS - Instrumentation and Methods for Astrophysics","volume":"22 1","pages":""},"PeriodicalIF":0.0000,"publicationDate":"2024-09-09","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"System performance of a cryogenic test-bed for the time-division multiplexing readout for NewAthena X-IFU\",\"authors\":\"Davide Vaccaro, Jan van der Kuur, Paul van der Hulst, Tobias Vos, Martin de Wit, Luciano Gottardi, Kevin Ravensberg, Emanuele Taralli, Joseph Adams, Simon Bandler, Douglas Bennet, James Chervenak, Bertrand Doriese, Malcolm Durkin, Jonathan Gard, Carl Reintsema, Kazuhiro Sakai, Steven Smith, Joel Ullom, Nicholas Wakeham, Jan-Willem den Herder, Brian jackson, Pourya Khosropanah, Jian-Rong Gao, Peter Roelfsema, Aurora Simionescu\",\"doi\":\"arxiv-2409.05643\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"The X-ray Integral Field Unit (X-IFU) is an instrument of ESA's future\\nNewAthena space observatory, with the goal to provide high-energy resolution\\n($<$ 4 eV at X-ray energies up to 7 keV) and high-spatial resolution (9\\\")\\nspectroscopic imaging over the X-ray energy range from 200 eV to 12 keV, by\\nmeans of an array of about 1500 transition-edge sensors (TES) read out via\\nSQUID time-division multiplexing (TDM). In 2022, to aid in the transfer of TDM\\nreadout technology from the laboratory toward flight hardware, our team\\ncommissioned a new TDM-based laboratory test-bed at SRON. This setup hosts an\\narray of $75\\\\times 75\\\\ \\\\mu$m$^2$ TESs that are read out via 2-column $\\\\times$\\n32-row TDM. A system component that is critical to high-performance operation\\nis the wiring harness that connects the room-temperature electronics to the\\ncryogenic readout componentry. In November 2023, we implemented a re-designed\\nflex harness, which in the SRON test-bed has a length close to what is\\nenvisioned for the X-IFU flight harness. We report here on our characterization\\nof the TDM system with the new flex harness, which allowed the system to\\nachieve a co-added energy resolution at a level of 2.7~eV FWHM at 6~keV via\\n32-row readout. In addition, we provide an outlook on the upcoming integration\\nof TDM readout into the X-IFU Focal-Plane Assembly Development Model.\",\"PeriodicalId\":501163,\"journal\":{\"name\":\"arXiv - PHYS - Instrumentation and Methods for Astrophysics\",\"volume\":\"22 1\",\"pages\":\"\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"2024-09-09\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"arXiv - PHYS - Instrumentation and Methods for Astrophysics\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/arxiv-2409.05643\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"arXiv - PHYS - Instrumentation and Methods for Astrophysics","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/arxiv-2409.05643","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
System performance of a cryogenic test-bed for the time-division multiplexing readout for NewAthena X-IFU
The X-ray Integral Field Unit (X-IFU) is an instrument of ESA's future
NewAthena space observatory, with the goal to provide high-energy resolution
($<$ 4 eV at X-ray energies up to 7 keV) and high-spatial resolution (9")
spectroscopic imaging over the X-ray energy range from 200 eV to 12 keV, by
means of an array of about 1500 transition-edge sensors (TES) read out via
SQUID time-division multiplexing (TDM). In 2022, to aid in the transfer of TDM
readout technology from the laboratory toward flight hardware, our team
commissioned a new TDM-based laboratory test-bed at SRON. This setup hosts an
array of $75\times 75\ \mu$m$^2$ TESs that are read out via 2-column $\times$
32-row TDM. A system component that is critical to high-performance operation
is the wiring harness that connects the room-temperature electronics to the
cryogenic readout componentry. In November 2023, we implemented a re-designed
flex harness, which in the SRON test-bed has a length close to what is
envisioned for the X-IFU flight harness. We report here on our characterization
of the TDM system with the new flex harness, which allowed the system to
achieve a co-added energy resolution at a level of 2.7~eV FWHM at 6~keV via
32-row readout. In addition, we provide an outlook on the upcoming integration
of TDM readout into the X-IFU Focal-Plane Assembly Development Model.