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A seismic time reversal experiment based on Time Reversal Mirror (TRM) technique was conducted in the mesoscopically scaled medium at the LSBB Laboratory, France. Two sets of 50 Hz geophones were distributed at one meter intervals in two…

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

The European Solar Telescope (EST) is a project of a new-generation solar telescope. It has a large aperture of 4~m, which is necessary for achieving high spatial and temporal resolution. The high polarimetric sensitivity of the EST will…

Instrumentation and Methods for Astrophysics · Physics 2018-11-05 Jan Jurcak , Manuel Collados , Jorrit Leenaarts , Michiel van Noort , Rolf Schlichenmaier

The third-generation of gravitational wave observatories, such as the Einstein Telescope (ET) and Cosmic Explorer (CE), aim for an improvement in sensitivity of at least a factor of ten over a wide frequency range compared to the current…

Instrumentation and Methods for Astrophysics · Physics 2022-10-05 A. Utina , A. Amato , J. Arends , C. Arina , M. de Baar , M. Baars , P. Baer , N. van Bakel , W. Beaumont , A. Bertolini , M. van Beuzekom , S. Biersteker , A. Binetti , H. J. M. ter Brake , G. Bruno , J. Bryant , H. J. Bulten , L. Busch , P. Cebeci , C. Collette , S. Cooper , R. Cornelissen , P. Cuijpers , M. van Dael , S. Danilishin , D. Dixit , S. van Doesburg , M. Doets , R. Elsinga , V. Erends , J. van Erps , A. Freise , H. Frenaij , R. Garcia , M. Giesberts , S. Grohmann , H. Van Haevermaet , S. Heijnen , J. V. van Heijningen , E. Hennes , J. -S. Hennig , M. Hennig , T. Hertog , S. Hild , H. -D. Hoffmann , G. Hoft , M. Hopman , D. Hoyland , G. A. Iandolo , C. Ietswaard , R. Jamshidi , P. Jansweijer , A. Jones , P. Jones , N. Knust , G. Koekoek , X. Koroveshi , T. Kortekaas , A. N. Koushik , M. Kraan , M. van de Kraats , S. L. Kranzhoff , P. Kuijer , K. A. Kukkadapu , K. Lam , N. Letendre , P. Li , R. Limburg , F. Linde , J. -P. Locquet , P. Loosen , H. Lueck , M. Martınez , A. Masserot , F. Meylahn , M. Molenaar , C. Mow-Lowry , J. Mundet , B. Munneke , L. van Nieuwland , E. Pacaud , D. Pascucci , S. Petit , Z. Van Ranst , G. Raskin , P. M. Recaman , N. van Remortel , L. Rolland , L. de Roo , E. Roose , J. C. Rosier , D. Ryckbosch , K. Schouteden , A. Sevrin , A. Sider , A. Singha , V. Spagnuolo , A. Stahl , J. Steinlechner , S. Steinlechner , B. Swinkels , N. Szilasi , M. Tacca , H. Thienpont , A. Vecchio , H. Verkooijen , C. H. Vermeer , M. Vervaeke , G. Visser , R. Walet , P. Werneke , C. Westhofen , B. Willke , A. Xhahi , T. Zhang

Since 2005 ESO has been working with its community and industry to develop an extremely large optical/infrared telescope. ESO's Extremely Large Telescope, or ELT for short, is a revolutionary ground-based telescope that will have a 39-metre…

Instrumentation and Methods for Astrophysics · Physics 2023-03-01 Paolo Padovani , Michele Cirasuolo , Remco van der Burg , Faustine Cantalloube , Elizabeth George , Markus Kasper , Kieran Leschinski , Carlos Martins , Julien Milli , Sabine Möhler , Mark Neeser , Benoit Neichel , Angel Otarola , Rubén Sánchez-Janssen , Benoit Serra , Alain Smette , Elena Valenti , Christophe Verinaud , Joël Vernet , Olivier Absil , Guido Agapito , Morten Andersen , Carmelo Arcidiacono , Matej Arko , Pierre Baudoz , Olivier Beltramo-Martin , Enrico Biancalani , Thomas Bierwirth , Leonard Burtscher , Giulia Carlà , Julio A. Castro-Almazán , Anne-Laure Cheffot , Lodovico Coccato , Carlos Correia , Romain Fetick , Giuliana Fiorentino , Thierry Fusco , Begoña García-Lorenzo , Nicola Gentile Fusillo , Oscar Gonzalez , Andrea Grazian , Marco Gullieuszik , Olivier Hainaut , Valentin Ivanov , Melanie Kaasinen , Darshan Kaddad , Tomasz Kamiński , Wolfgang Kausch , Florian Kerber , Stefan Kimeswenger , Rosita Kokotanekova , Arseniy Kuznetsov , Alexis Lau , Miska Le Louarn , Frédéric Lemmel , Jochen Liske , Gaspare Lo Curto , David Lucsanyi , Lars Lundin , Stefan Noll , Sylvain Oberti , James Osborn , Elena Masciadri , Dinko Milaković , Michael T. Murphy , Fernando Pedichini , Miguel Pereira Santaella , Roberto Piazzesi , Javier Piqueras López , Cédric Plantet , Thibaut Prod'homme , Norbert Przybilla , Mathieu Puech , Derryck T. Reid , Ansgar Reiners , Rutger Rijnenberg , Myriam Rodrigues , Fabio Rossi , Laurence Routledge , Hans Smit , Mathias Tecza , Niranjan Thatte , Roy van Boekel , Aprajita Verma , Arthur Vigan

The Einstein Telescope (ET) is a third generation gravitational wave detector that includes a room-temperature high-frequency (ET-HF) and a cryogenic low-frequency laser interferometer (ET-LF). The cryogenic ET-LF is crucial for exploiting…

Instrumentation and Methods for Astrophysics · Physics 2023-12-11 Xhesika Koroveshi , Lennard Busch , Ettore Majorana , Paola Puppo , Piero Rapagnani , Fulvio Ricci , Paolo Ruggi , Steffen Grohmann

In 2006 ESO Council authorized a Phase B study of a European AO-telescope with a 42 m segmented primary with a 5-mirror design, the E-ELT. Several reports and working groups have already presented science cases for an E-ELT, specifically…

Astrophysics of Galaxies · Physics 2015-05-18 Nils Ryde

The Einstein Telescope (ET), a proposed European ground-based gravitational-wave detector of third-generation, is an evolution of second-generation detectors such as Advanced LIGO, Advanced Virgo, and KAGRA which could be operating in the…

Einstein Telescope (ET) is expected to achieve sensitivity improvements exceeding an order of magnitude compared to current gravitational-wave detectors. The rigorous characterization in optical birefringence of materials and coatings has…

The beam test for the SiW-ECAL technological prototype was conducted using electron beam in June-July 2019 at DESY test beam facility in Hamburg, Germany. In the beam test, there were two main programs: MIP program (without tungsten) and…

Instrumentation and Detectors · Physics 2020-02-28 Yu Kato , Kiichi Goto , Taikan Suehara , CALICE SiW-ECAL group

We have developed a calibration system based on a micro-electromechanical systems (MEMS) mirror that is capable of delivering an optical beam over a wavelength range of 180 -- 2000 nm (0.62 -- 6.89 eV) in a sub-Kelvin environment. This…

The MEV project aims at developing a muon telescope expressly designed for the muography of Etna Volcano. In particular, one of the active craters in the summit area of the volcano would be a suitable target for this experiment. A muon…

The Wide-field Infrared Transient Explorer (WINTER) is a 1x1 degree infrared survey telescope under development at MIT and Caltech, and slated for commissioning at Palomar Observatory in 2021. WINTER is a seeing-limited infrared time-domain…

Dielectric tensor tomography is an imaging technique for mapping three-dimensional distributions of dielectric properties in transparent materials. This work introduces an enhanced illumination strategy employing a micro-electromechanical…

The Einstein Telescope is the next-generation gravitational wave interferometer which, compared to current detectors, will enable the observation of gravitational signals at lower frequencies with a sensitivity improved by approximately two…

Instrumentation and Detectors · Physics 2025-08-12 Federico Armato , Barbara Garaventa , Andrea Chincarini

Two types of orbital detectors of extreme energy cosmic rays are being developed nowadays: (i) TUS and KLYPVE with reflecting optical systems (mirrors) and (ii) JEM-EUSO with high-transmittance Fresnel lenses. They will cover much larger…