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The Jiangmen Underground Neutrino Observatory (JUNO) is a 20-kton liquid scintillator-based, low-radioactivity, multi-purpose neutrino detector located 693 meters (1800 m.w.e.) underground in the Guangdong province, China. To detect…

Instrumentation and Detectors · Physics 2026-04-29 Cedric Cerna , Miao He , Xiaoshan Jiang , Juan Pedro Ochoa-Ricoux , Frederic Perrot , Angel Abusleme , Thomas Adam , Fengpeng An , Costas Andreopoulos , Giuseppe Andronico , Joao Pedro Athayde Marcondes de Andre , Nikolay Anfimov , Vito Antonelli , Tatiana Antoshkina , Didier Auguste , Nikita Balashov , Andrea Barresi , Davide Basilico , Eric Baussan , Marco Beretta , Antonio Bergnoli , Svetlana Biktemerova , Thilo Birkenfeld , Simon Blyth , Manuel Boehles , Anastasia Bolshakova , Mathieu Bongrand , Clement Bordereau , Matteo Borghesi , Dominique Breton , Augusto Brigatti , Riccardo Brugnera , Riccardo Bruno , Antonio Budano , Jose Busto , Marcel Buchner , Anatael Cabrera , Barbara Caccianiga , Hao Cai , Xiao Cai , Yi-zhou Cai , Stephane Callier , Antonio Cammi , Augustin Campeny , Guofu Cao , Jun Cao , Yaoqi Cao , Rossella Caruso , Nunzio Giudice , Maxim Gonchar , Guanda Gong , Guanghua Gong , Yuri Gornushkin , Marco Grassi , Maxim Gromov , Vasily Gromov , Minhao Gu , Xiaofei Gu , Yu Gu , Mengyun Guan , Yuduo Guan , Nunzio Guardone , Rosa Maria Guizzetti , Cong Guo , Wanlei Guo , Caren Hagner , Hechong Han , Yang Han , Chuanhui Hao , Vidhya Thara Hariharan , Wei He , Xinhai He , Tobias Heinz , Patrick Hellmuth , Yuekun Heng , Rafael Herrera , YuenKeung Hor , Shaojing Hou , Fatima Houria , Gerard Claverie , Catia Clementi , Barbara Clerbaux , Claudio Coletta , Davide Chiesa , Pietro Chimenti , Ziliang Chu , Artem Chukanov , Marta Colomer Molla , Fabio Mantovani , Stefano M. Mari , Agnese Martini , Johann Martyn , Matthias Mayer , Davit Mayilyan , Yue Meng , Anselmo Meregaglia , Lino Miramonti , Michele Montuschi , Iwan Morton-Blake , Xiangyi Mu , Lakshmi Murgod , Massimiliano Nastasi , Dmitry V. Naumov , Elena Naumova , Igor Nemchenok , Elisabeth Neuerburg , Alexey Nikolaev , Feipeng Ning , Zhe Ning , Yujie Niu , Hiroshi Nunokawa , Lothar Oberauer , Sebastian Olivares , Alexander Olshevskiy , Domizia Orestano , Fausto Ortica , Rainer Othegraven , Yifei Pan , Alessandro Paoloni , George Parker , Yatian Pei , Luca Pelicci , Anguo Peng , Yu Peng , Zhaoyuan Peng , Elisa Percalli , Willy Perrin , Fabrizio Petrucci , Oliver Pilarczyk , Artyom Popov , Pascal Poussot , Ezio Previtali , Fazhi Qi , Ming Qi , Sen Qian , Xiaohui Qian , Zhaoxiang Wu , Zhi Wu , Michael Wurm , Jacques Wurtz , Dongmei Xia , Shishen Xian , Ziqian Xiang , Fei Xiao , Pengfei Xiao , Tianying Xiao , Xiang Xiao , Wei-Jun Xie , Xiaochuan Xie , Yuguang Xie , Zhizhong Xing , Benda Xu , Cheng Xu , Chuang Xu , Donglian Xu , Fanrong Xu , Jiayang Xu , Jilei Xu , Jinghuan Xu , Meihang Xu , Shiwen Xu , Xunjie Xu , Dongyang Xue , Jingqin Xue , Baojun Yan , Qiyu Yan , Taylor Yan , Xiongbo Yan , Changgen Yang , Chengfeng Yang , Fengfan Yang , Jie Yang , Kaiwei Yang , Lei Yang , Pengfei Yang , Xiaoyu Yang , Xuhui Yang , Zekun Yang , Haifeng Yao , Jiaxuan Ye , Mei Ye , Ziping Ye , Frederic Yermia , Jilong Yin , Weiqing Yin , Xiaohao Yin , Zhengyun You , Boxiang Yu , Chiye Yu , Chunxu Yu , Hongzhao Yu , Peidong Yu , Simi Yu , Zeyuan Yu , Cenxi Yuan , Noman Zafar , Jilberto Zamora , Vitalii Zavadskyi , Fanrui Zeng , Shan Zeng , Tingxuan Zeng , Liang Zhan , Bin Zhang , Feiyang Zhang , Han Zhang , Hangchang Zhang , Haosen Zhang , Honghao Zhang , Jiawen Zhang , Jie Zhang , Jingbo Zhang , Junwei Zhang , Lei Zhang , Ping Zhang , Qingmin Zhang , Rongping Zhang , Shiqi Zhang , Shuihan Zhang , Tao Zhang , Xiaomei Zhang , Xu Zhang , Xuantong Zhang , Yibing Zhang , Yinhong Zhang , Yiyu Zhang , Yongpeng Zhang , Yuanyuan Zhang , Yumei Zhang , Zhicheng Zhang , Zhijian Zhang , Jie Zhao , Runze Zhao , Shujun Zhao , Yangheng Zheng , Li Zhou , Shun Zhou , Xiang Zhou , Xing Zhou , Jingsen Zhu , Kangfu Zhu , Kejun Zhu , Bo Zhuang , Honglin Zhuang , Jiaheng Zou

The final stages of stellar evolution can be constrained by studying pre-SN variability. The incredible amount of data coming from the upcoming Rubin Legacy Survey of Space and Time (LSST) will be fundamental to this type of work. However,…

Instrumentation and Methods for Astrophysics · Physics 2026-03-24 Tobias Géron , Maria R. Drout , W. V. Jacobson-Galán , C. D. Kilpatrick

Completed in May 2008, the ANTARES neutrino telescope is located in the Mediterranean Sea, 40 km off the coast of Toulon, at a depth of about 2500 m. Consisting of 12 detector lines housing nearly 900 optical modules, the ANTARES telescope…

High Energy Astrophysical Phenomena · Physics 2019-08-13 Anthony M Brown

PandaX-4T is a dark matter direct detection experiment located in China jinping underground laboratory. The central apparatus is a dual-phase xenon detector containing 4 ton liquid xenon in the sensitive volume, with about 500…

The ANTARES Collaboration is building an underwater neutrino telescope in the Mediterranean sea. The telescope is designed to search for high energy (E $>1$ TeV) galactic and extra-galactic neutrino sources, but could also be sensitive to…

Astrophysics · Physics 2009-11-11 Y. Becherini

On May 2008 the ANTARES collaboration completed the installation of a neutrino telescope in the Mediterranean Sea. This detector consists of a tridimensional array of almost 900 photomultipliers (PMTs) distributed in 12 lines. These PMTs…

Instrumentation and Methods for Astrophysics · Physics 2009-11-17 Juan Pablo Gomez-Gonzalez

For sensitive optical interferometry, it is crucial to control the evolution of the optical path difference (OPD) of the wavefront between the individual telescopes of the array. The OPD between a pair of telescopes is induced by…

Instrumentation and Methods for Astrophysics · Physics 2021-12-28 Saavidra Perera , Jörg-Uwe Pott , Julien Woillez , Martin Kulas , Wolfgang Brandner , Sylvestre Lacour , Felix Widmann

Photomultiplier tubes (PMTs) with large-area cathodes are increasingly being used in cosmic-ray experiments to enhance detection efficiency. The optical modules (OMs) of the High-Energy Underwater Neutrino Telescope (HUNT) have employed a…

High Energy Physics - Experiment · Physics 2024-08-06 Yijiang Peng , Zike Wang , Bo Gao , Yiyue Tang , Mingjun Chen , Kai Li , Ling Ren , Xiaohao You , Maoyuan Liu

We introduce the DM Radio, a dual search for axion and hidden photon dark matter using a tunable superconducting lumped-element resonator. We discuss the prototype DM Radio Pathfinder experiment, which will probe hidden photons in the 500…

The recent launch of Einstein Probe (EP) in early 2024 opened up a new window onto the transient X-ray sky, allowing for real-time discovery and follow-up of fast X-ray transients (FXRTs). Multi-wavelength observations of FXRTs and their…

High Energy Astrophysical Phenomena · Physics 2024-07-29 R. Ricci , E. Troja , Y. Yang , M. Yadav , Y. Liu , H. Sun , X. Wu , H. Gao , B. Zhang , W. Yuan

The Jinping Neutrino Experiment(JNE), conducted within the China Jinping Underground Laboratory, aims to detect and analyze of solar neutrinos, geo-neutrinos, and supernova neutrinos. A one-ton prototype will soon be in commision with an…

Instrumentation and Detectors · Physics 2024-04-17 H. Yang , T. Xue , L. Jiang , C. Xu , Q. Pan , B. Liang , G. Gong , B. Xu , Z. Wang , S. Chen , Y. Liu , J. Li

The CYGNO collaboration is developing a novel strategy for directional Dark Matter searches based on a gaseous Time Projection Chamber (TPC). The detector is optimized for the exploration of light (0.5-50 GeV) WIMPs-like particles and…

Transient sources such as supernovae (SNe) and tidal disruption events are candidates of high energy neutrino sources. However, SNe commonly occur in the universe and a chance coincidence of their detection with a neutrino signal cannot be…

High Energy Astrophysical Phenomena · Physics 2022-10-05 Shigeru Yoshida , Kohta Murase , Masaomi Tanaka , Nobuhiro Shimizu , Aya Ishihara

A six-night optical turbulence monitoring campaign has been carried at Cerro Paranal observatory in February and March, 2023 to facilitate the development and characterisation of two novel atmospheric site monitoring instruments - the…

Instrumentation and Methods for Astrophysics · Physics 2024-02-15 Ryan Griffiths , Lisa Bardou , Timothy Butterley , James Osborn , Richard Wilson , Edison Bustos , Andrei Tokovinin , Miska Le Louarn , Angel Otarola

NEXT-DEMO is a high-pressure xenon gas TPC which acts as a technological test-bed and demonstrator for the NEXT-100 neutrinoless double beta decay experiment. In its current configuration the apparatus fully implements the NEXT-100 design…

The DUNE experiment is a future long-baseline neutrino oscillation experiment aiming at measuring the neutrino CP-violating phase and establishing the neutrino mass hierarchy, as well as at a rich physics programme from supernovae over…

High Energy Physics - Experiment · Physics 2022-11-24 Oliver Lantwin

NEXT (Neutrino Experiment with a Xenon TPC) aims to observe the neutrinoless double beta decay of \ensuremath{{}^{136}\rm Xe} in a high-pressure gas xenon Time Projection Chamber using electroluminescence to amplify the signal from…

Instrumentation and Detectors · Physics 2019-08-14 Paola Ferrario

The South Pole Telescope Summertime Line Intensity Mapper (SPT-SLIM) is a pathfinder experiment that will demonstrate the use of on-chip filter-bank spectrometers for mm-wave line intensity mapping (LIM). The SPT-SLIM focal plane consists…

The gaseous Xenon(Xe) time projection chamber (TPC) is an attractive detector technique for neutrinoless double beta decay and WIMP dark matter searches. While it is less dense compared to Liquid Xe detectors, it has intrinsic advantages in…

Instrumentation and Detectors · Physics 2016-04-13 Y. Nakajima , A. Goldshmidt , H. S. Matis , T. Miller , D. R. Nygren , C. A. B. Oliveira , J. Renner