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Multiwire and microstrip porous detectors have been developed and investigated for DC operation. The multiwire porous detector consists of anode wires, an Al cathode and a gap between them filled with porous CsI. The microstrip porous…

Instrumentation and Detectors · Physics 2007-05-23 M. P. Lorikyan

Dark matter detectors that utilize liquid xenon have now achieved tonne-scale targets, giving them sensitivity to all flavours of supernova neutrinos via coherent elastic neutrino-nucleus scattering. Considering for the first time a…

High Energy Astrophysical Phenomena · Physics 2016-12-21 Rafael F. Lang , Christopher McCabe , Shayne Reichard , Marco Selvi , Irene Tamborra

In recent years cooling technology for Liquid Xenon (LXe) detectors has advanced driven by the development of Dark Matter (DM) detectors with target mass in the 100 - 1,000 kg range. The next generation of DM detectors based on LXe will be…

Instrumentation and Detectors · Physics 2019-09-24 K. L. Giboni , P. Juyal , E. Aprile , Y. Zhang , J. Naganoma

The CDEX (China Dark matter Experiment) aims at detection of WIMPs (Weakly Interacting Massive Particles) and 0vbb (Neutrinoless double beta decay) of 76Ge. It now uses ~10 kg HPGe (High Purity Germanium) detectors in CJPL (China Jinping…

Instrumentation and Detectors · Physics 2020-10-26 Jinfu Zhu , Tianhao Wang , Tao Xue , Liangjun Wei , Jingjun Wen , Lin Jiang , Jianmin Li

A prototype detector is being developed which combines the functions of a Time Projection Chamber for charged particle tracking and a Cherenkov detector for particle identification. The TPC consists of a 10x10x10 cm3 drift volume where the…

Instrumentation and Detectors · Physics 2015-12-18 Craig Woody , Babak Azmoun , Richard Majka , Michael Phipps , Martin Purschke , Nikolai Smirnov

The scientific potential of X-ray polarimetry has long been recognized, but the challenges in measuring polarization have left it largely unexplored, particularly in the hard X-ray regime. While tremendous advancement has been made in soft…

Instrumentation and Methods for Astrophysics · Physics 2026-03-27 Abhay Kumar , Santosh V. Vadawale , N. P. S. Mithun , Tanmoy Chattopadhyay , S. K. Goyal , A. R. Patel , M. Shanmugam

Microcalorimeter instruments aboard future X-ray observatories will require an anti-coincidence (anti-co) detector to veto charged particle events and reduce the non-X-ray background. We have developed a large-format, TES-based prototype…

Dual-phase xenon time projection chambers achieve optimal sensitivity for dark matter in the 10 to 1000 GeV/c$^2$ mass range, but sub-GeV dark matter particles lack sufficient energy to produce nuclear recoils above detection thresholds in…

High Energy Astrophysical Phenomena · Physics 2026-01-05 Erin Barillier , Laura Manenti , Knut Mora , Paolo Padovani , Isaac Sarnoff , Yongheng Xu , Bjorn Penning , Francesco Arneodo

BlueMUSE (Blue Multi Unit Spectroscopic Explorer) is a blue-optimised, medium spectral resolution, panoramic integral field spectrograph proposed for the Very Large Telescope (VLT) and based on the MUSE concept. BlueMUSE will open up a new…

Instrumentation and Methods for Astrophysics · Physics 2021-01-20 Alexandre Jeanneau , Johan Kosmalski , Eduard Muslimov , Emmanuel Hugot , Roland Bacon , Johan Richard

The Ricochet experiment aims to measure the coherent elastic neutrino-nucleus scattering process from antineutrinos emitted by a research nuclear reactor operated by the Institut Laue-Langevin (Grenoble, France). This article presents a…

High Energy Physics - Experiment · Physics 2026-01-08 Antoine Armatol , Corinne Augier , Louis Bailly-Salins , Guillaume Baulieu , Laurent Bergé , Julien Billard , Juliette Blé , Guillaume Bres , Jean-Louis Bret , Alexandre Broniatowski , Martino Calvo , Antonella Cavanna , Antoine Cazes , Emanuela Celi , David Chaize , Mohammed Chala , Maurice Chappellier , Luke Chaplinsky , Guillaume Chemin , Ran Chen , Jules Colas , Laurent Couraud , Elspeth Cudmore , Maryvonne De Jesus , Nicole Dombrowski , Louis Dumoulin , Alan Durnez , Olivier Exshaw , Sylvain Ferriol , Enectali Figueroa-Feliciano , Joseph A. Formaggio , Stephane Fuard , Jules Gascon , Andrea Giuliani , Corinne Goy , Cyrille Guerin , Elsa Guy , Leïla Haegel , Scott A. Hertel , Christophe Hoarau , Ziqing Hong , Jean-Christophe Ianigro , Yong Jin , Alexandre Juillard , Temirlan Khussainov , Andrew Kubik , Jacob Lamblin , Hugues Lattaud , Tatiana Le-Bellec , Laetitia Leroy , Mingyu Li , Alexey Lubashevskiy , Stefanos Marnieros , Nicolas Martini , Julien Minet , Alessandro Monfardini , Franck Mounier , Valentina Novati , Emiliano Olivieri , Pratyush K. Patel , Eric Perbet , Harold Douglas Pinckney , Denys V. Poda , Dmitrii Ponomarev , Wouter Van De Pontseele , Jean-Sébastien Real , Faith C. Reyes , Alejandro Rodriguez , Murielle Rousseau , Sergey Rozov , Irina Rozova , Brianna Ryan , Deeksha Sabhari , Silvia Scorza , Renaud Serra , Yegor Shevchik , Torsten Soldner , Anne Stutz , Christian Ulysse , Lionel Vagneron , Sergey Vasilyev , Francis Vezzu , Paul Vittaz , Evgeny Yakushev , Jiatong Yang , Daniya Zinatulina

We have developed a fine-pitch hard X-ray (HXR) detector using a cadmium telluride (CdTe) semiconductor for imaging and spectroscopy for the second launch of the Focusing Optics Solar X-ray Imager (FOXSI). FOXSI is a rocket experiment to…

Instrumentation and Methods for Astrophysics · Physics 2016-10-26 S. Ishikawa , M. Katsuragawa , S. Watanabe , Y. Uchida , S. Takeda , T. Takahashi , S. Saito , L. Glesener , J. C. Buitrago-Casas , S. Krucker , S. Christe

The worldwide race towards direct dark matter detection in the form of Weakly Interacting Massive Particles (WIMPs) has been dramatically accelerated by the remarkable progress and evolution of liquid xenon time projection chambers…

Instrumentation and Methods for Astrophysics · Physics 2012-06-28 Elena Aprile , XENON1T collaboration

High-purity germanium crystals approximately 12 cm in diameter were grown in a hydrogen atmosphere using the Czochralski method. The dislocation density of the crystals was determined to be in the range of 2000 - 4200 cm-2, which meets a…

Instrumentation and Detectors · Physics 2015-05-08 Guojian Wang , Mark Amman , Hao Mei , Dongming Mei , Klaus Irmscher , Yutong Guan , Gang Yang

The tRopIcal DEep-sea Neutrino Telescope (TRIDENT) is a future large-scale next-generation neutrino telescope. In September 2021, the TRIDENT pathfinder experiment (TRIDENT EXplorer, T-REX for short) completed in-situ measurements of…

Instrumentation and Detectors · Physics 2023-03-07 M. X. Wang , G. H. Gong , P. Miao , Z. Y. Sun , J. N. Tang , W. H. Wu , D. L. Xu

A one-coordinate gaseous detector of soft X-ray photons for wide-angle X-ray scattering (WAXS) studies is being developed. The detector operates in counting mode and is based on multi-stage Gas Electron Multiplier(GEM). Full size detector…

Instrumentation and Detectors · Physics 2008-11-26 V. M. Aulchenko , P. A. Papushev , M. R. Sharafutdinov , L. I. Shekhtman , V. M. Titov , B. P. Tolochko , V. V. Zhulanov

The proposed new Electron-Ion Collider poses a technical and intellectual challenge for the detector design to accommodate the long-term diverse physics goals envisaged by the program. This requires a 4{\pi} detector system capable of…

A combination of microchannel plate optics and a 32x32 pixel microcalorimeter would allow the successor to the Rossi XTE to explore new domains of spectroscopic timing in a MIDEX class mission. With ~10 times the area and ~100 times the…

Astrophysics · Physics 2009-11-10 Martin Elvis

This paper describes the electronics of NEXT-White (NEW) detector PMT plane, a high pressure xenon TPC with electroluminescent amplification (HPXe-EL) currently operating at the Laboratorio Subterra\'aneo de Canfranc (LSC) in Huesca, Spain.…

Instrumentation and Detectors · Physics 2018-12-26 V. Álvarez , V. Herrero , R. Esteve , A. Laing , J. Rodríguez , M. Querol , F. Monrabal , J. F. Toledo , J. J. Gómez-Cadenas

The NeXT mission has been proposed to study high-energy non-thermal phenomena in the universe. The high-energy response of the super mirror will enable us to perform the first sensitive imaging observations up to 80 keV. The focal plane…