{"id":13743,"date":"2023-07-05T09:45:05","date_gmt":"2023-07-05T00:45:05","guid":{"rendered":"https:\/\/www.icrr.u-tokyo.ac.jp\/?post_type=event_researcher&#038;p=13743"},"modified":"2023-07-12T15:12:51","modified_gmt":"2023-07-12T06:12:51","slug":"new%e3%80%902023%e5%b9%b47%e6%9c%885%e6%97%a5%e3%80%91design-and-optimization-of-the-sipm-array-for-event-reconstruction-in-the-darwin-experiment-marta-ewelina-babicz-u-zurich-2","status":"publish","type":"event_researcher","link":"https:\/\/www.icrr.u-tokyo.ac.jp\/en\/event_researcher\/13743\/","title":{"rendered":"&#8220;Design and Optimization of the SiPM Array for Event Reconstruction in the DARWIN Experiment&#8221; \/ Marta Ewelina Babicz (U. Zurich)"},"content":{"rendered":"\n<figure class=\"wp-block-table\"><div class=\"js-scrollable\"><table><tbody><tr><td>Number<\/td><td>R5-4 \/ &nbsp;IPMU\/ILANCE\/ICRR joint seminar<\/td><\/tr><tr><td>Date&amp;Time<\/td><td>July 5, 2023  Wed. 13:30-(JST)<\/td><\/tr><tr><td>Place<\/td><td>IPMU, Seminar A (1F) and Zoom \u00a0<a href=\"https:\/\/ipmu.zoom.us\/j\/92044029378\">https:\/\/ipmu.zoom.us\/j\/92044029378<\/a><\/td><\/tr><tr><td>Speaker<\/td><td>Marta Ewelina Babicz (U. Zurich)<\/td><\/tr><tr><td>Title<\/td><td>&#8220;Design and Optimization of the SiPM Array for Event Reconstruction in the DARWIN&nbsp;Experiment&#8221;<\/td><\/tr><tr><td>Abstract<\/td><td>The DARWIN experiment is a facility that aims to detect dark matter via liquid xenon technology. To study challenges related to constructing and operating a&nbsp;multi-tonne scale detector, a vertical, full-scale demonstrator for the DARWIN experiment (Xenonscope) has been constructed at the University of Zurich. It is&nbsp;equipped with a double-walled stainless steel cryostat that can house up to 400kg of LXe. The facility includes a gas purification system, a cooling tower with a&nbsp;pulse tube refrigerator, and a slow control system for overseeing and sending alarms on relevant parameters. In the next phase of the project, a 2.6 m two-phase&nbsp;TPC will be added to demonstrate the drift of electrons in LXe over a long distance. One of the key features of Xenoscope is its SiPM array, which provides high&nbsp;sensitivity and resolution for detecting light signals from physical events. This seminar will focus on the design, optimization, and performance of the SiPM array&nbsp;in Xenoscope, including its readout electronics and deep learning algorithms for accurate event reconstruction.<\/td><\/tr><\/tbody><\/table><\/div><\/figure>\n","protected":false},"featured_media":0,"template":"","tag_year":[],"class_list":["post-13743","event_researcher","type-event_researcher","status-publish","hentry","en-US"],"aioseo_notices":[],"aioseo_head":"\n\t\t<!-- All in One SEO 5.0.2 - aioseo.com -->\n\t<meta name=\"robots\" content=\"max-image-preview:large\" \/>\n\t<link rel=\"canonical\" href=\"https:\/\/www.icrr.u-tokyo.ac.jp\/en\/event_researcher\/13743\/\" \/>\n\t<meta name=\"generator\" content=\"All in One SEO (AIOSEO) 5.0.2\" \/>\n\t\t<meta property=\"og:locale\" content=\"en_US\" \/>\n\t\t<meta property=\"og:site_name\" content=\"ICRR | Institute for Cosmic Ray Research University of Tokyo | \u30de\u30eb\u30c1\u30e1\u30c3\u30bb\u30f3\u30b8\u30e3\u30fc\u306e\u89b3\u6e2c\u3092\u901a\u3058\u3001\u5b87\u5b99\u306e\u8b0e\u306b\u8feb\u308a\u307e\u3059\" \/>\n\t\t<meta property=\"og:type\" content=\"article\" \/>\n\t\t<meta property=\"og:title\" content=\"\u201cDesign and Optimization of the SiPM Array for Event Reconstruction in the DARWIN Experiment\u201d \/ Marta Ewelina Babicz (U. 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