BEGIN:VCALENDAR VERSION:2.0 PRODID:-//CERN//INDICO//EN BEGIN:VEVENT SUMMARY:Welcome to McGill DTSTART;VALUE=DATE-TIME:20251112T141500Z DTEND;VALUE=DATE-TIME:20251112T142500Z DTSTAMP;VALUE=DATE-TIME:20260907T032408Z UID:indico-contribution-538-3404@nyx.physics.mcgill.ca DESCRIPTION:Speakers: Kristina Öhrvall (McGill University)\nhttps://nyx.p hysics.mcgill.ca/event/538/contributions/3404/ LOCATION: URL:https://nyx.physics.mcgill.ca/event/538/contributions/3404/ END:VEVENT BEGIN:VEVENT SUMMARY:A journey to ITACA DTSTART;VALUE=DATE-TIME:20251112T224000Z DTEND;VALUE=DATE-TIME:20251112T224700Z DTSTAMP;VALUE=DATE-TIME:20260907T032408Z UID:indico-contribution-538-3420@nyx.physics.mcgill.ca DESCRIPTION:Speakers: Roberto Soleti ()\nHigh-pressure gaseous xenon time projection chambers with electroluminescence (HGXeTPC-EL)\, are among the leading technologies for the search of neutrinoless double beta decay. The ir combination of excellent energy resolution and detailed topological rec onstruction enables powerful discrimination between single-electron and do uble-electron tracks\, the latter representing the characteristic signatur e of a $0\\nu\\beta\\beta$ event near the decay energy. Background suppres sion in these detectors relies critically on this topological information\ , but its effectiveness is ultimately limited by the diffusion of drifting electrons and by the spatial blurring introduced during electroluminescen t amplification.\n\nTraditional approaches to mitigate diffusion\, such as the addition of molecular cooling agents (e.g.\, CO$_2$\, CH$_4$)\, are c onstrained by their strong quenching of xenon scintillation and electrolum inescence. To overcome these limitations\, we introduce ITACA (Ion Trackin g with Ammonium Cations Apparatus)\, a novel concept that exploits both th e prompt electron track and a delayed ion track to enhance event reconstru ction. In this scheme\, trace amounts of NH$_3$ (at ppb levels) convert xe non ions (Xe$^+$) into ammonium ions (NH$_4^+$) without affecting scintill ation or EL yields. Electrons drift to the anode within milliseconds\, for ming the conventional EL image\, while NH$_4^+$ ions drift slowly toward t he cathode on a timescale of seconds. Using the primary scintillation (S1) signal as a timing reference\, an electrostatic gate releases the ion clo ud onto a sensor array of molecular detectors\, which can be optically int errogated to reconstruct the ion track with sub-millimeter diffusion and w ithout EL smearing.\n\nBy combining the electron and ion images\, ITACA co uld significantly improve the topological background rejection of xenon TP Cs\, potentially by an order of magnitude. The applicability of this techn ique to liquid xenon detectors is also discussed\, though the higher densi ty and reduced track length in the liquid phase make ion tracking less pra ctical in that regime.\n\nhttps://nyx.physics.mcgill.ca/event/538/contribu tions/3420/ LOCATION: URL:https://nyx.physics.mcgill.ca/event/538/contributions/3420/ END:VEVENT BEGIN:VEVENT SUMMARY:X/Y multi-site reconstruction in dual-phase xenon detectors DTSTART;VALUE=DATE-TIME:20251112T222600Z DTEND;VALUE=DATE-TIME:20251112T224000Z DTSTAMP;VALUE=DATE-TIME:20260907T032408Z UID:indico-contribution-538-3391@nyx.physics.mcgill.ca DESCRIPTION:Speakers: Brian Lenardo (SLAC)\nIn liquid xenon detectors sear ching for neutrinoless double beta decay (0vbb)\, single-site/multi-site ( SS/MS) discrimination is critical for reducing backgrounds from 214Bi gamm a rays. Dual-phase detectors\, which utilize electroluminescence to measur e the ionization signals\, have demonstrated excellent multi-site identifi cation in the longitudinal (z) direction but have not demonstrated SS/MS d iscrimination in the transverse (x/y) plane. If multi-site interactions co uld be identified down to separations of a few mm\, 214Bi backgrounds coul d be reduced by a factor of two\, potentially increasing the sensitivity o f dual-phase detectors to 0vbb by up to ~50%. I will discuss the capabilit y and limitations of x/y SS/MS discrimination in dual-phase detectors with the traditional electroluminescence readout\, and introduce the possibili ty of adding additional wire grids to such detectors to improve spatial re construction via induction sensing.\n\nhttps://nyx.physics.mcgill.ca/event /538/contributions/3391/ LOCATION: URL:https://nyx.physics.mcgill.ca/event/538/contributions/3391/ END:VEVENT BEGIN:VEVENT SUMMARY:Are five tonnes of xenon enough? DTSTART;VALUE=DATE-TIME:20251112T215800Z DTEND;VALUE=DATE-TIME:20251112T221200Z DTSTAMP;VALUE=DATE-TIME:20260907T032408Z UID:indico-contribution-538-3389@nyx.physics.mcgill.ca DESCRIPTION:Speakers: Simon Viel (Carleton University)\nTarget mass is a k ey consideration in optimizing the design of a future neutrinoless double beta decay detector with xenon.  This short talk makes the case that in t he current context\, to achieve our scientific goals\, a target mass large r than 5 tonnes needs to be considered seriously.\n\nhttps://nyx.physics.m cgill.ca/event/538/contributions/3389/ LOCATION: URL:https://nyx.physics.mcgill.ca/event/538/contributions/3389/ END:VEVENT BEGIN:VEVENT SUMMARY:What is the limit of topological background rejection with a gas T PC? DTSTART;VALUE=DATE-TIME:20251112T214400Z DTEND;VALUE=DATE-TIME:20251112T215800Z DTSTAMP;VALUE=DATE-TIME:20260907T032408Z UID:indico-contribution-538-3390@nyx.physics.mcgill.ca DESCRIPTION:Speakers: Krishan Mistry (University of Texas at Arlington)\nG aseous xenon time projection chambers (GXeTPC) are an excellent detector t echnology for reducing radiogenic backgrounds in $0\\nu\\beta\\beta$ decay searches due to the extended beta tracks. The signal consists of two emit ted beta electrons with 2.45 MeV of energy\, and their track lengths scale inversely with the gas pressure\, reaching ~2 m in size for 1 bar of gas pressure or ~20 cm at 10 bar. The most significant backgrounds that can m imic this signature are gamma rays originating from radiogenic sources or beta decays from cosmogenically activated isotopes such as Xe-137. Such ba ckgrounds generally produce a single electron signature\, and GXeTPCs can reject a significant fraction of them using the amount of energy depositio n near the track ends and event multiplicities. In this talk\, I will be d iscussing how GXeTPCs can best use the topological information to reject t hese backgrounds\, including the use of new variables that exploit the ang ular information of the tracks\, and what factors can limit this.\n\nhttps ://nyx.physics.mcgill.ca/event/538/contributions/3390/ LOCATION: URL:https://nyx.physics.mcgill.ca/event/538/contributions/3390/ END:VEVENT BEGIN:VEVENT SUMMARY:Shielding and Outer Detectors DTSTART;VALUE=DATE-TIME:20251112T213000Z DTEND;VALUE=DATE-TIME:20251112T214400Z DTSTAMP;VALUE=DATE-TIME:20260907T032408Z UID:indico-contribution-538-3392@nyx.physics.mcgill.ca DESCRIPTION:Speakers: Teena Vallivilayil John (Postdoc)\nCosmogenic muons are a major background source in rare event search experiments. To mitigat e this background\, neutrinoless double beta decay ($0\\nu\\beta\\beta$) a nd direct detection dark matter experiments prefer to operate in deep unde rground laboratories\, where they can receive adequate shielding from cosm ic rays. However\, high energy muons can still reach underground and creat e backgrounds for these experiments. To reduce such cosmogenic muon backgr ounds\, the rare-event search experiments deploy an outer detector to tag the muons. The outer detector can act as a muon veto. An active muon veto detects light produced either via Cherenkov radiation (if the detector is filled with the water) or scintillation light (if the detector is filled w ith the scintillation medium). The outer detector is instrumented with pho ton detection modules\, such as photomultiplier tubes (PMTs) or silicon ph oto multipliers (SiPM). In addition\, the outer detector can also serve a s passive shielding\, moderating secondary neutrons produced by muon inter actions. In this talk\, I will discuss about requirements of the deep unde rground laboratories\, and the specifications of the outer detectors for t he current and future rare event search experiments.\n\nhttps://nyx.physic s.mcgill.ca/event/538/contributions/3392/ LOCATION: URL:https://nyx.physics.mcgill.ca/event/538/contributions/3392/ END:VEVENT BEGIN:VEVENT SUMMARY:Reaching the Normal Hierarchy for double beta decay DTSTART;VALUE=DATE-TIME:20251112T221200Z DTEND;VALUE=DATE-TIME:20251112T222600Z DTSTAMP;VALUE=DATE-TIME:20260907T032408Z UID:indico-contribution-538-3388@nyx.physics.mcgill.ca DESCRIPTION:Speakers: David Sinclair (Carleton University)\nTo reach the N ormal Hierarchy and thus definitively address the question of lepton numbe r conservation\, current background levels must be reduced by a factor of ~1000 and some of this must come from improved energy resolution. I sugges t this might be achieved in liquid xenon by a series of fundamental change s in design to include (a) the use of low IP additives such as TEA to allo w much higher detection efficiency together with charge and light measurem ents on each charge cluster\, (b) the use of fine pixelated detectors\, (c ) positive ion detection to reduce diffusion and preserve electron track i nformation and (d) improved high voltage design to allow operation at high er fields. Work on this should be done globally with the aim of a global d etector approach.\n\nhttps://nyx.physics.mcgill.ca/event/538/contributions /3388/ LOCATION: URL:https://nyx.physics.mcgill.ca/event/538/contributions/3388/ END:VEVENT BEGIN:VEVENT SUMMARY:Joint oversight committee talk DTSTART;VALUE=DATE-TIME:20251113T205000Z DTEND;VALUE=DATE-TIME:20251113T212000Z DTSTAMP;VALUE=DATE-TIME:20260907T032408Z UID:indico-contribution-538-3323@nyx.physics.mcgill.ca DESCRIPTION:Speakers: Nigel Smith ()\nhttps://nyx.physics.mcgill.ca/event/ 538/contributions/3323/ LOCATION: URL:https://nyx.physics.mcgill.ca/event/538/contributions/3323/ END:VEVENT BEGIN:VEVENT SUMMARY:Technical Coordination of large-scale 0nbb experiments DTSTART;VALUE=DATE-TIME:20251112T193000Z DTEND;VALUE=DATE-TIME:20251112T200000Z DTSTAMP;VALUE=DATE-TIME:20260907T032408Z UID:indico-contribution-538-3335@nyx.physics.mcgill.ca DESCRIPTION:Speakers: Francesc Moranbal ()\nhttps://nyx.physics.mcgill.ca/ event/538/contributions/3335/ LOCATION: URL:https://nyx.physics.mcgill.ca/event/538/contributions/3335/ END:VEVENT BEGIN:VEVENT SUMMARY:Review of the xenon technologies DTSTART;VALUE=DATE-TIME:20251112T153000Z DTEND;VALUE=DATE-TIME:20251112T160000Z DTSTAMP;VALUE=DATE-TIME:20260907T032408Z UID:indico-contribution-538-3322@nyx.physics.mcgill.ca DESCRIPTION:Speakers: Mike Heffner (LLNL)\nhttps://nyx.physics.mcgill.ca/e vent/538/contributions/3322/ LOCATION: URL:https://nyx.physics.mcgill.ca/event/538/contributions/3322/ END:VEVENT BEGIN:VEVENT SUMMARY:Impact of microphysics and simulations DTSTART;VALUE=DATE-TIME:20251113T170000Z DTEND;VALUE=DATE-TIME:20251113T173000Z DTSTAMP;VALUE=DATE-TIME:20260907T032408Z UID:indico-contribution-538-3369@nyx.physics.mcgill.ca DESCRIPTION:Speakers: Eric Dahl (Northwestern University)\nhttps://nyx.phy sics.mcgill.ca/event/538/contributions/3369/ LOCATION: URL:https://nyx.physics.mcgill.ca/event/538/contributions/3369/ END:VEVENT BEGIN:VEVENT SUMMARY:Electronics & DAQ DTSTART;VALUE=DATE-TIME:20251113T200000Z DTEND;VALUE=DATE-TIME:20251113T203000Z DTSTAMP;VALUE=DATE-TIME:20260907T032408Z UID:indico-contribution-538-3368@nyx.physics.mcgill.ca DESCRIPTION:Speakers: Curro Toledo ()\nhttps://nyx.physics.mcgill.ca/event /538/contributions/3368/ LOCATION: URL:https://nyx.physics.mcgill.ca/event/538/contributions/3368/ END:VEVENT BEGIN:VEVENT SUMMARY:Shielding/Water tank DTSTART;VALUE=DATE-TIME:20251113T193000Z DTEND;VALUE=DATE-TIME:20251113T200000Z DTSTAMP;VALUE=DATE-TIME:20260907T032408Z UID:indico-contribution-538-3366@nyx.physics.mcgill.ca DESCRIPTION:Speakers: Hugh Lippincott ()\nhttps://nyx.physics.mcgill.ca/ev ent/538/contributions/3366/ LOCATION: URL:https://nyx.physics.mcgill.ca/event/538/contributions/3366/ END:VEVENT BEGIN:VEVENT SUMMARY:Low radioactivity materials DTSTART;VALUE=DATE-TIME:20251112T210000Z DTEND;VALUE=DATE-TIME:20251112T213000Z DTSTAMP;VALUE=DATE-TIME:20260907T032408Z UID:indico-contribution-538-3364@nyx.physics.mcgill.ca DESCRIPTION:Speakers: Richard Saldanha ()\nhttps://nyx.physics.mcgill.ca/e vent/538/contributions/3364/ LOCATION: URL:https://nyx.physics.mcgill.ca/event/538/contributions/3364/ END:VEVENT BEGIN:VEVENT SUMMARY:Radioassay needs for future low-bkg experiments DTSTART;VALUE=DATE-TIME:20251112T203000Z DTEND;VALUE=DATE-TIME:20251112T210000Z DTSTAMP;VALUE=DATE-TIME:20260907T032408Z UID:indico-contribution-538-3363@nyx.physics.mcgill.ca DESCRIPTION:Speakers: Isaac Arnquist (Pacific Northwest National Laborator y)\nhttps://nyx.physics.mcgill.ca/event/538/contributions/3363/ LOCATION: URL:https://nyx.physics.mcgill.ca/event/538/contributions/3363/ END:VEVENT BEGIN:VEVENT SUMMARY:Ba tagging DTSTART;VALUE=DATE-TIME:20251113T163000Z DTEND;VALUE=DATE-TIME:20251113T170000Z DTSTAMP;VALUE=DATE-TIME:20260907T032408Z UID:indico-contribution-538-3352@nyx.physics.mcgill.ca DESCRIPTION:Speakers: Pablo Herrero Gomez (Hebrew University)\nhttps://nyx .physics.mcgill.ca/event/538/contributions/3352/ LOCATION: URL:https://nyx.physics.mcgill.ca/event/538/contributions/3352/ END:VEVENT BEGIN:VEVENT SUMMARY:Workshop summary and wrap-up DTSTART;VALUE=DATE-TIME:20251114T173000Z DTEND;VALUE=DATE-TIME:20251114T180000Z DTSTAMP;VALUE=DATE-TIME:20260907T032408Z UID:indico-contribution-538-3351@nyx.physics.mcgill.ca DESCRIPTION:Speakers: Thomas Brunner (McGill U)\nhttps://nyx.physics.mcgil l.ca/event/538/contributions/3351/ LOCATION: URL:https://nyx.physics.mcgill.ca/event/538/contributions/3351/ END:VEVENT BEGIN:VEVENT SUMMARY:Quo Vadis DTSTART;VALUE=DATE-TIME:20251114T163000Z DTEND;VALUE=DATE-TIME:20251114T173000Z DTSTAMP;VALUE=DATE-TIME:20260907T032408Z UID:indico-contribution-538-3350@nyx.physics.mcgill.ca DESCRIPTION:Speakers: Ben Jones (UTA)\nWhere do we want to go? Can we deve lop a consortium? How would we do this?\n\nhttps://nyx.physics.mcgill.ca/e vent/538/contributions/3350/ LOCATION: URL:https://nyx.physics.mcgill.ca/event/538/contributions/3350/ END:VEVENT BEGIN:VEVENT SUMMARY:Other technologies DTSTART;VALUE=DATE-TIME:20251114T160000Z DTEND;VALUE=DATE-TIME:20251114T163000Z DTSTAMP;VALUE=DATE-TIME:20260907T032408Z UID:indico-contribution-538-3349@nyx.physics.mcgill.ca DESCRIPTION:Speakers: Gabriel Orebi ()\nKamLAND2-ZEN\, THEIA\, LAR+Xe\, an d others\n\nhttps://nyx.physics.mcgill.ca/event/538/contributions/3349/ LOCATION: URL:https://nyx.physics.mcgill.ca/event/538/contributions/3349/ END:VEVENT BEGIN:VEVENT SUMMARY:Dual Phase TPC DTSTART;VALUE=DATE-TIME:20251114T150000Z DTEND;VALUE=DATE-TIME:20251114T153000Z DTSTAMP;VALUE=DATE-TIME:20260907T032408Z UID:indico-contribution-538-3348@nyx.physics.mcgill.ca DESCRIPTION:Speakers: Kaixuan Ni ()\nhttps://nyx.physics.mcgill.ca/event/5 38/contributions/3348/ LOCATION: URL:https://nyx.physics.mcgill.ca/event/538/contributions/3348/ END:VEVENT BEGIN:VEVENT SUMMARY:Liquid TPC DTSTART;VALUE=DATE-TIME:20251114T143000Z DTEND;VALUE=DATE-TIME:20251114T150000Z DTSTAMP;VALUE=DATE-TIME:20260907T032408Z UID:indico-contribution-538-3347@nyx.physics.mcgill.ca DESCRIPTION:Speakers: David Moore ()\nhttps://nyx.physics.mcgill.ca/event/ 538/contributions/3347/ LOCATION: URL:https://nyx.physics.mcgill.ca/event/538/contributions/3347/ END:VEVENT BEGIN:VEVENT SUMMARY:Gas TPC DTSTART;VALUE=DATE-TIME:20251114T140000Z DTEND;VALUE=DATE-TIME:20251114T143000Z DTSTAMP;VALUE=DATE-TIME:20260907T032408Z UID:indico-contribution-538-3346@nyx.physics.mcgill.ca DESCRIPTION:Speakers: Justo Martin Albo ()\nhttps://nyx.physics.mcgill.ca/ event/538/contributions/3346/ LOCATION: URL:https://nyx.physics.mcgill.ca/event/538/contributions/3346/ END:VEVENT BEGIN:VEVENT SUMMARY:Xenon storage and purification DTSTART;VALUE=DATE-TIME:20251113T160000Z DTEND;VALUE=DATE-TIME:20251113T163000Z DTSTAMP;VALUE=DATE-TIME:20260907T032408Z UID:indico-contribution-538-3344@nyx.physics.mcgill.ca DESCRIPTION:Speakers: Julien Masbou ()\nhttps://nyx.physics.mcgill.ca/even t/538/contributions/3344/ LOCATION: URL:https://nyx.physics.mcgill.ca/event/538/contributions/3344/ END:VEVENT BEGIN:VEVENT SUMMARY:Photon detection systems DTSTART;VALUE=DATE-TIME:20251113T153000Z DTEND;VALUE=DATE-TIME:20251113T160000Z DTSTAMP;VALUE=DATE-TIME:20260907T032408Z UID:indico-contribution-538-3343@nyx.physics.mcgill.ca DESCRIPTION:Speakers: Fabrice Retière ()\nhttps://nyx.physics.mcgill.ca/e vent/538/contributions/3343/ LOCATION: URL:https://nyx.physics.mcgill.ca/event/538/contributions/3343/ END:VEVENT BEGIN:VEVENT SUMMARY:Radon Control DTSTART;VALUE=DATE-TIME:20251113T190000Z DTEND;VALUE=DATE-TIME:20251113T193000Z DTSTAMP;VALUE=DATE-TIME:20260907T032408Z UID:indico-contribution-538-3342@nyx.physics.mcgill.ca DESCRIPTION:Speakers: Brian Mong (SLAC)\nhttps://nyx.physics.mcgill.ca/eve nt/538/contributions/3342/ LOCATION: URL:https://nyx.physics.mcgill.ca/event/538/contributions/3342/ END:VEVENT BEGIN:VEVENT SUMMARY:Panel on best strategy for Xe experiments DTSTART;VALUE=DATE-TIME:20251113T212000Z DTEND;VALUE=DATE-TIME:20251113T223500Z DTSTAMP;VALUE=DATE-TIME:20260907T032408Z UID:indico-contribution-538-3340@nyx.physics.mcgill.ca DESCRIPTION:Speakers: Art McDonald - Moderator ()\, Dan Akerib ()\, Jodi C ooley ()\, Juan José Gómez Cadenas ()\, Krishna Kumar ()\, Sean Pauling ()\nModerator: Dr. Art McDonald\nPanelists:\nDr. Jodi Cooley\nDr. Juan Jos é Gómez Cadenas\nDr. Dan Akerib\nDr. Krisha Kumar\nDr. Sean Pauling\n\nh ttps://nyx.physics.mcgill.ca/event/538/contributions/3340/ LOCATION: URL:https://nyx.physics.mcgill.ca/event/538/contributions/3340/ END:VEVENT BEGIN:VEVENT SUMMARY:Lessons learned from Dune and building in the current context DTSTART;VALUE=DATE-TIME:20251113T144000Z DTEND;VALUE=DATE-TIME:20251113T150000Z DTSTAMP;VALUE=DATE-TIME:20260907T032408Z UID:indico-contribution-538-3339@nyx.physics.mcgill.ca DESCRIPTION:Speakers: Mary Bishai ()\nhttps://nyx.physics.mcgill.ca/event/ 538/contributions/3339/ LOCATION: URL:https://nyx.physics.mcgill.ca/event/538/contributions/3339/ END:VEVENT BEGIN:VEVENT SUMMARY:Lessons learned from Global Argon Dark Matter DTSTART;VALUE=DATE-TIME:20251113T142000Z DTEND;VALUE=DATE-TIME:20251113T144000Z DTSTAMP;VALUE=DATE-TIME:20260907T032408Z UID:indico-contribution-538-3338@nyx.physics.mcgill.ca DESCRIPTION:Speakers: Jocelyn Monroe ()\nhttps://nyx.physics.mcgill.ca/eve nt/538/contributions/3338/ LOCATION: URL:https://nyx.physics.mcgill.ca/event/538/contributions/3338/ END:VEVENT BEGIN:VEVENT SUMMARY:Lessons learned from the formation of XLZD DTSTART;VALUE=DATE-TIME:20251113T140000Z DTEND;VALUE=DATE-TIME:20251113T142000Z DTSTAMP;VALUE=DATE-TIME:20260907T032408Z UID:indico-contribution-538-3337@nyx.physics.mcgill.ca DESCRIPTION:Speakers: Kim Palladino ()\nhttps://nyx.physics.mcgill.ca/even t/538/contributions/3337/ LOCATION: URL:https://nyx.physics.mcgill.ca/event/538/contributions/3337/ END:VEVENT BEGIN:VEVENT SUMMARY:Accessing underground labs DTSTART;VALUE=DATE-TIME:20251112T190000Z DTEND;VALUE=DATE-TIME:20251112T193000Z DTSTAMP;VALUE=DATE-TIME:20260907T032408Z UID:indico-contribution-538-3334@nyx.physics.mcgill.ca DESCRIPTION:Speakers: Erica Caden (SNOLAB)\nhttps://nyx.physics.mcgill.ca/ event/538/contributions/3334/ LOCATION: URL:https://nyx.physics.mcgill.ca/event/538/contributions/3334/ END:VEVENT BEGIN:VEVENT SUMMARY:Theory review of the nuclear matrix element calculation for 136Xe DTSTART;VALUE=DATE-TIME:20251112T183000Z DTEND;VALUE=DATE-TIME:20251112T190000Z DTSTAMP;VALUE=DATE-TIME:20260907T032408Z UID:indico-contribution-538-3333@nyx.physics.mcgill.ca DESCRIPTION:Speakers: Jason Holt (TRIUMF)\nhttps://nyx.physics.mcgill.ca/e vent/538/contributions/3333/ LOCATION: URL:https://nyx.physics.mcgill.ca/event/538/contributions/3333/ END:VEVENT BEGIN:VEVENT SUMMARY:The Chinese Xenon programme DTSTART;VALUE=DATE-TIME:20251112T163000Z DTEND;VALUE=DATE-TIME:20251112T170000Z DTSTAMP;VALUE=DATE-TIME:20260907T032408Z UID:indico-contribution-538-3327@nyx.physics.mcgill.ca DESCRIPTION:Speakers: Jianglai Liu ()\nhttps://nyx.physics.mcgill.ca/event /538/contributions/3327/ LOCATION: URL:https://nyx.physics.mcgill.ca/event/538/contributions/3327/ END:VEVENT BEGIN:VEVENT SUMMARY:Best current limits using 136Xe DTSTART;VALUE=DATE-TIME:20251112T160000Z DTEND;VALUE=DATE-TIME:20251112T163000Z DTSTAMP;VALUE=DATE-TIME:20260907T032408Z UID:indico-contribution-538-3326@nyx.physics.mcgill.ca DESCRIPTION:Speakers: Spencer Axani ()\nhttps://nyx.physics.mcgill.ca/even t/538/contributions/3326/ LOCATION: URL:https://nyx.physics.mcgill.ca/event/538/contributions/3326/ END:VEVENT BEGIN:VEVENT SUMMARY:Workshop Goals DTSTART;VALUE=DATE-TIME:20251112T142500Z DTEND;VALUE=DATE-TIME:20251112T150000Z DTSTAMP;VALUE=DATE-TIME:20260907T032408Z UID:indico-contribution-538-3321@nyx.physics.mcgill.ca DESCRIPTION:Speakers: Roxanne Guenette (University of Manchester)\nhttps:/ /nyx.physics.mcgill.ca/event/538/contributions/3321/ LOCATION: URL:https://nyx.physics.mcgill.ca/event/538/contributions/3321/ END:VEVENT BEGIN:VEVENT SUMMARY:Welcome/Logistics DTSTART;VALUE=DATE-TIME:20251112T140000Z DTEND;VALUE=DATE-TIME:20251112T141500Z DTSTAMP;VALUE=DATE-TIME:20260907T032408Z UID:indico-contribution-538-3320@nyx.physics.mcgill.ca DESCRIPTION:Speakers: Thomas Brunner (McGill U)\nhttps://nyx.physics.mcgil l.ca/event/538/contributions/3320/ LOCATION: URL:https://nyx.physics.mcgill.ca/event/538/contributions/3320/ END:VEVENT END:VCALENDAR