English
Related papers

Related papers: A fast tunable driver of light source for the TRID…

200 papers

We explore the potential of current and next generation of coherent elastic neutrino-nucleus scattering (CE$\nu$NS) experiments in probing neutrino electromagnetic interactions. On the basis of a thorough statistical analysis, we determine…

High Energy Physics - Phenomenology · Physics 2019-07-19 O. G. Miranda , D. K. Papoulias , M. Tórtola , J. W. F. Valle

In the era of time-domain, multi-messenger astronomy, the detection of transient events on the high-energy electromagnetic sky has become more important than ever. Previous attempts to systematically search for onboard-untriggered events in…

Instrumentation and Methods for Astrophysics · Physics 2022-09-21 F. Kunzweiler , B. Biltzinger , J. Greiner , J. M. Burgess

HERMES (High Energy Rapid Modular Ensemble of Satellites) pathfinder is an in-orbit demonstration consisting of a constellation of six 3U nano-satellites hosting simple but innovative detectors for the monitoring of cosmic high-energy…

High Energy Astrophysical Phenomena · Physics 2023-09-06 Riccardo Crupi , Giuseppe Dilillo , Kester Ward , Elisabetta Bissaldi , Fabrizio Fiore , Andrea Vacchi

Transition Edge Sensor (TES) bolometers are a well-established technology with a strong track record in experimental cosmology, making them ideal for current and future radio astronomy instruments. The Tomographic Ionized-carbon Mapping…

Instrumentation and Methods for Astrophysics · Physics 2025-10-06 Victoria L. Butler , James J. Bock , Dongwoo T. Chung , Abigail T. Crites , King Lau , Ian Lowe , Dan P. Marrone , Evan C. Mayer , Benjamin J. Vaughan , Michael Zemcov

RISTRETTO is a visible high-resolution spectrograph fed by an extreme adaptive optics (AO) system, to be proposed as a visitor instrument on ESO VLT. The main science goal of RISTRETTO is to pioneer the detection and atmospheric…

The transmission electron microscope (TEM) has become an essential tool for innovation in nanoscience, material science, and biology. Despite these instruments being widely used across both industry and academia, academics may hesitate to…

Instrumentation and Detectors · Physics 2022-12-07 Patrick McBean , Zachary Milne , Arjun Kanthawar , Cameron O'Byrne , Khalid Hattar , Lewys Jones

Terahertz (THz) ultra-massive multiple-input multiple-output (UM-MIMO) promises ultra-high throughput, while its highly directional beams demand rapid and accurate beam tracking driven by precise user-state estimation. Moreover, large array…

Signal Processing · Electrical Eng. & Systems 2026-03-18 Zhi Zeng , Chong Han , Emil Björnson

The use of Time Projection Chambers (TPCs) in particle physics experiments has been growing since their invention, reaching sizes equivalent to buildings (ALICE or ATLAS at CERN). However, their application in another class of experiments,…

Instrumentation and Detectors · Physics 2024-12-24 Hector Mirallas

The Deep Underground Neutrino Experiment (DUNE) is a next-generation long-baseline neutrino oscillation experiment designed to make precision measurements in the world's most powerful neutrino beam. Neutrinos are measured at two detector…

High Energy Physics - Experiment · Physics 2025-01-28 Ciaran Hasnip

Atmospheric muons are important probes for studying primary cosmic rays and extensive air showers. Additionally, they constitute a significant background for many underground and deep-sea neutrino experiments, such as TRopIcal DEep-sea…

Optical SETI (Search for Extraterrestrial Intelligence) instruments that can explore the very fast time domain, especially with large sky coverage, offer an opportunity for new discoveries that can complement multimessenger and time domain…

LiteBIRD is a next-generation satellite mission to measure the polarization of the cosmic microwave background (CMB) radiation. On large angular scales the B-mode polarization of the CMB carries the imprint of primordial gravitational…

The Einstein Probe (EP) is a mission designed to monitor the sky in the soft X-ray band. It will perform systematic surveys and characterisation of high-energy transients and monitoring of variable objects at unprecedented sensitivity and…

High Energy Astrophysical Phenomena · Physics 2023-04-05 Weimin Yuan , Chen Zhang , Yong Chen , Zhixing Ling

A prototype detection unit of the KM3NeT deep-sea neutrino telescope has been installed at 3500m depth 80km offshore the Italian coast. KM3NeT in its final configuration will contain several hundreds of detection units. Each detection unit…

Instrumentation and Methods for Astrophysics · Physics 2016-04-06 KM3NeT Collaboration , S. Adrián-Martínez , M. Ageron , F. Aharonian , S. Aiello , A. Albert , F. Ameli , E. G. Anassontzis , G. C. Androulakis , M. Anghinolfi , G. Anton , S. Anvar , M. Ardid , T. Avgitas , K. Balasi , H. Band , G. Barbarino , E. Barbarito , F. Barbato , B. Baret , S. Baron , J. Barrios , A. Belias , E. Berbee , A. M. van den Berg , A. Berkien , V. Bertin , S. Beurthey , V. van Beveren , N. Beverini , S. Biagi , A. Biagioni , S. Bianucci , M. Billault , A. Birbas , H. Boer Rookhuizen , R. Bormuth , V. Bouché , B. Bouhadef , G. Bourlis , C. Boutonnet , M. Bouwhuis , C. Bozza , R. Bruijn , J. Brunner , G. Cacopardo , L. Caillat , M. Calamai , D. Calvo , A. Capone , L. Caramete , F. Caruso , S. Cecchini , A. Ceres , R. Cereseto , C. Champion , F. Château , T. Chiarusi , B. Christopoulou , M. Circella , L. Classen , R. Cocimano , A. Coleiro , S. Colonges , R. Coniglione , A. Cosquer , M. Costa , P. Coyle , A. Creusot , G. Cuttone , C. D'Amato , A. D'Amico , G. De Bonis , G. De Rosa , N. Deniskina , J. -J. Destelle , C. Distefano , F. Di Capua , C. Donzaud , D. Dornic , Q. Dorosti-Hasankiadeh , E. Drakopoulou , D. Drouhin , L. Drury , D. Durand , T. Eberl , D. Elsaesser , A. Enzenhöfer , P. Fermani , L. A. Fusco , D. Gajanana , T. Gal , S. Galatà , F. Garufi , M. Gebyehu , V. Giordano , N. Gizani , R. GraciaRuiz , K. Graf , R. Grasso , G. Grella , A. Grmek , R. Habel , H. van Haren , T. Heid , A. Heijboer , E. Heine , S. Henry , J. J. Hernández-Rey , B. Herold , M. A. Hevinga , M. van der Hoek , J. Hofestädt , J. Hogenbirk , C. Hugon , J. Hößl , M. Imbesi , C. W. James , P. Jansweijer , J. Jochum , M. de Jong , M. Jongen , M. Kadler , O. Kalekin , A. Kappes , E. Kappos , U. Katz , O. Kavatsyuk , P. Keller , G. Kieft , E. Koffeman , H. Kok , P. Kooijman , J. Koopstra , A. Korporaal , A. Kouchner , I. Kreykenbohm , V. Kulikovskiy , R. Lahmann , P. Lamare , G. Larosa , D. Lattuada , H. Le Provost , K. P. Leismüller , A. Leisos , D. Lenis , E. Leonora , M. LindseyClark , C. D. Llorens Alvarez , H. Löhner , A. Lonardo , S. Loucatos , F. Louis , E. Maccioni , K. Mannheim , K. Manolopoulos , A. Margiotta , O. Mariş , C. Markou , J. A. Martínez-Mora , A. Martini , R. Masullo , K. W. Melis , T. Michael , P. Migliozzi , E. Migneco , A. Miraglia , C. M. Mollo , M. Mongelli , M. Morganti , S. Mos , Y. Moudden , P. Musico , M. Musumeci , C. Nicolaou , C. A. Nicolau , A. Orlando , A. Orzelli , A. Papaikonomou , R. Papaleo , G. E. Păvălaş , H. Peek , C. Pellegrino , M. G. Pellegriti , C. Perrina , P. Piattelli , K. Pikounis , V. Popa , Th. Pradier , M. Priede , G. Pühlhofer , S. Pulvirenti , C. Racca , F. Raffaelli , N. Randazzo , P. A. Rapidis , P. Razis , D. Real , L. Resvanis , J. Reubelt , G. Riccobene , A. Rovelli , M. Saldaña , D. F. E. Samtleben , M. Sanguineti , A. Santangelo , P. Sapienza , J. Schmelling , J. Schnabel , V. Sciacca , M. Sedita , T. Seitz , I. Sgura , F. Simeone , V. Sipala , A. Spitaleri , M. Spurio , G. Stavropoulos , J. Steijger , T. Stolarczyk , D. Stransky , M. Taiuti , G. Terreni , D. Tézier , S. Théraube , L. F. Thompson , P. Timmer , L. Trasatti , A. Trovato , M. Tselengidou , A. Tsirigotis , S. Tzamarias , E. Tzamariudaki , B. Vallage , V. Van Elewyck , J. Vermeulen , P. Vernin , P. Vicini , S. Viola , D. Vivolo , P. Werneke , L. Wiggers , J. Wilms , E. de Wolf , R. H. L. van Wooning , E. Zonca , J. D. Zornoza , J. Zúñiga , A. Zwart

Turbulence is notoriously difficult to model due to its multi-scale nature and sensitivity to small perturbations. Classical solvers of turbulence simulation generally operate on finer grids and are computationally inefficient. In this…

Fluid Dynamics · Physics 2022-07-12 Yuchen Dang , Zheyuan Hu , Miles Cranmer , Michael Eickenberg , Shirley Ho

Investigating the spatial correlation between different emissions in an extended astrophysical source can provide crucial insights into their physical connection, hence it can be the key to understand the nature of the system. The…

Instrumentation and Methods for Astrophysics · Physics 2021-11-17 Alessandro Ignesti

Tidal Disruption Events (TDEs) are rare transients, which are considered as promising tools in probing supermassive black holes in quiescent galaxies. The majority of $\approx 60$ known TDEs has been discovered with time-domain surveys in…

High Energy Astrophysical Phenomena · Physics 2023-07-06 K. Bučar Bricman , S. van Velzen , M. Nicholl , A. Gomboc

The tumor microenvironment (TME) features distinct hallmarks, including acidosis, hypoxia, reactive oxygen species (ROS) generation, and altered ion fluxes, which are crucial targets for early cancer biomarker detection, tumor diagnosis,…

We present here a new robotic telescope called TRAPPIST (TRAnsiting Planets and PlanetesImals Small Telescope). Equipped with a high-quality CCD camera mounted on a 0.6 meter light weight optical tube, TRAPPIST has been installed in April…

Earth and Planetary Astrophysics · Physics 2015-05-27 M. Gillon , E. Jehin , P. Magain , V. Chantry , D. Hutsemekers , J. Manfroid , D. Queloz , S. Udry

NEXT (Neutrino Experiment with a Xenon TPC) is an experiment to search neutrinoless double beta decay processes (bb0nu) in Xe136. The NEXT technology is based in the use of time projection chambers operating at a typical pressure of 15 bar…

Instrumentation and Detectors · Physics 2014-11-11 Juan Jose Gomez-Cadenas