<?xml version="1.0" encoding="utf-8" standalone="yes"?><rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>News |</title><link>https://jamillab.org/news/</link><atom:link href="https://jamillab.org/news/index.xml" rel="self" type="application/rss+xml"/><description>News</description><generator>HugoBlox Kit (https://hugoblox.com)</generator><language>en-us</language><image><url>https://jamillab.org/media/icon_hu_6fad4d7ed91b82b6.png</url><title>News</title><link>https://jamillab.org/news/</link></image><item><title>EXO-200 releases public dataset for AI/ML applications</title><link>https://jamillab.org/news/exo-200-public-data-release/</link><pubDate>Mon, 28 Sep 2026 00:00:00 +0000</pubDate><guid>https://jamillab.org/news/exo-200-public-data-release/</guid><description>&lt;p&gt;The EXO-200 collaboration has publicly released a subset of its calibration data, described in a new paper,
.&lt;/p&gt;
&lt;p&gt;The dataset contains approximately one million events recorded during ²²⁸Th calibration campaigns near the end of EXO-200 Phase-II operations in early 2018. For every event it provides the raw waveforms from the U-wire, V-wire, and avalanche photodiode readout channels, together with reconstructed quantities such as charge energy, light energy, and charge-cluster information.&lt;/p&gt;
&lt;p&gt;The data are distributed in HDF5 format and are intended to support data preservation, teaching, and the development of modern machine-learning techniques for rare-event physics.&lt;/p&gt;
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&lt;li&gt;Paper:
&lt;/li&gt;
&lt;li&gt;More on this line of research:
&lt;/li&gt;
&lt;/ul&gt;</description></item><item><title>Two new DarkSide-20k instrumentation papers</title><link>https://jamillab.org/news/darkside-20k-daq-and-veto-tiles/</link><pubDate>Fri, 03 Apr 2026 00:00:00 +0000</pubDate><guid>https://jamillab.org/news/darkside-20k-daq-and-veto-tiles/</guid><description>&lt;p&gt;The DarkSide-20k collaboration has released two papers documenting major pieces of the detector&amp;rsquo;s instrumentation. Both have since been published.&lt;/p&gt;
&lt;p&gt;&lt;strong&gt;The data acquisition system.&lt;/strong&gt;
(JINST 21, P09017) presents the DAQ that will read out the experiment&amp;rsquo;s 2720 SiPM-based channels. The system digitizes waveforms continuously, without a hardware trigger, and processes them online to reduce the data volume for long-term storage. A full &amp;ldquo;Quadrant&amp;rdquo; — one quarter of the final system — has been assembled and validated at TRIUMF.&lt;/p&gt;
&lt;p&gt;&lt;strong&gt;The veto photosensors.&lt;/strong&gt;
(Eur. Phys. J. C 86, 1089) describes the completed production and testing of the &amp;ldquo;vTiles&amp;rdquo;, arrays of 24 SiPMs that instrument the Inner Veto. Each tile was tested at room and cryogenic temperature; the final production yield exceeded 87%, above the 80% requirement, providing the 1920 tiles needed for 120 veto photodetector units plus spares.&lt;/p&gt;
&lt;p&gt;Read more about
.&lt;/p&gt;</description></item><item><title>New results on low-mass dark matter and double beta decay of ¹³⁴Xe</title><link>https://jamillab.org/news/low-mass-wimps-and-xe-134/</link><pubDate>Mon, 17 Nov 2025 00:00:00 +0000</pubDate><guid>https://jamillab.org/news/low-mass-wimps-and-xe-134/</guid><description>&lt;p&gt;Two new results were released on the same day, one from each side of our research program. Both have since been published.&lt;/p&gt;
&lt;p&gt;&lt;strong&gt;Low-mass dark matter in liquid argon.&lt;/strong&gt;
(Phys. Rev. D 113, 123045) combines new measurements from the ReD setup with calibration data from DarkSide-50 and results from the ARIS and SCENE experiments to better constrain how liquid argon responds to nuclear recoils at keV energies. Applying the updated model to DarkSide-50 data yields stronger exclusion limits on low-mass WIMP interactions, and the paper recasts the sensitivity projections for DarkSide-20k.&lt;/p&gt;
&lt;p&gt;&lt;strong&gt;Double beta decay of ¹³⁴Xe.&lt;/strong&gt;
(Phys. Rev. Lett. 136, 232502) reports no significant signal and sets a world-leading lower limit of 8.7 × 10²³ years (90% C.L.) on the half-life of the neutrinoless mode, along with a threefold improvement over the EXO-200 Phase I constraint on the two-neutrino mode.&lt;/p&gt;</description></item><item><title>DarkSide-20k SiPM tile production paper released</title><link>https://jamillab.org/news/darkside-20k-sipm-tile-production/</link><pubDate>Wed, 09 Jul 2025 00:00:00 +0000</pubDate><guid>https://jamillab.org/news/darkside-20k-sipm-tile-production/</guid><description>&lt;p&gt;A new DarkSide-20k paper,
, describes how the photosensors for the experiment&amp;rsquo;s 21 m² SiPM array are built and tested.&lt;/p&gt;
&lt;p&gt;The SiPMs are arranged into modular photosensors called Tiles, each integrating 24 SiPMs on a printed circuit board that provides signal amplification and power distribution; 16 Tiles form a Photo-Detector Unit. Production and quality control take place at Nuova Officina Assergi (NOA), an ISO-6 clean room at LNGS, and include wafer-level cryogenic characterization, die attaching, wire bonding, and electrical and optical validation of every Tile. The overall production yield exceeds 83.5%, meeting the requirements of the DarkSide-20k production plan.&lt;/p&gt;
&lt;p&gt;The paper was published in Eur. Phys. J. C 85, 1334 (2025). Read more about
and our
.&lt;/p&gt;</description></item></channel></rss>