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Related papers: Current and Nascent SETI Instruments

200 papers

Over a period of several decades a concerted effort has been made to determine whether intelligent life exists outside of our solar system, known as the Search for Extraterrestrial Intelligence or SETI. This has been based primarily upon…

General Physics · Physics 2007-05-23 Fred H. Thaheld

The HERMES-TP/SP (High Energy Rapid Modular Ensemble of Satellites -- Technologic and Scientific Pathfinder) is an in-orbit demonstration of the so-called distributed astronomy concept. Conceived as a mini-constellation of six 3U…

The search for extraterrestrial intelligence (SETI) is to search for technosignatures associated with extraterrestrial life, such as engineered radio signals. In this paper, we apply the multibeam coincidence matching (MBCM) strategy, and…

The TEDI (TripleSpec - Exoplanet Discovery Instrument) will be the first instrument fielded specifically for finding low-mass stellar companions. The instrument is a near infra-red interferometric spectrometer used as a radial velocimeter.…

The China Seismo Electromagnetic Satellite (CSES) aims to contribute to the monitoring of earthquakes from space. This space mission, lead by a Chinese-Italian collaboration, will study phenomena of electromagnetic nature and their…

Instrumentation and Methods for Astrophysics · Physics 2019-08-14 V. Scotti , G. Osteria

For centuries, astronomers have discussed the possibility of inhabited worlds - from Herschel's 18th-century observations suggesting Mars may host life, to the systematic search for technosignatures that began in the 1960s using radio…

Instrumentation and Methods for Astrophysics · Physics 2025-10-22 Beatriz Villarroel , Wesley A. Watters , Alina Streblyanska , Enrique Solano , Stefan Geier , Lars Mattsson

With the installation of a new phased array system called Apertif, the instantaneous field of view of the Westerbork Synthesis Radio Telescope (WSRT) has increased to 8.7$\,$deg$^2$. This system has turned the WSRT in to an highly effective…

Instrumentation and Methods for Astrophysics · Physics 2019-11-13 Yogesh Maan , Joeri van Leeuwen

Observations of astrophysical transients have brought many novel discoveries and provided new insights into physical processes at work under extreme conditions in the Universe. Multi-wavelength and multi-messenger observations of variable…

Instrumentation and Methods for Astrophysics · Physics 2022-10-19 C. Hoischen , M. Füßling , S. Ohm , A. Balzer , H. Ashkar , K. Bernlöhr , P. Hofverberg , T. L. Holch , T. Murach , H. Prokoph , F. Schüssler , S. J. Zhu , D. Berge , K. Egberts , C. Stegmann

A new general purpose fixed target facility is proposed at the CERN SPS accelerator which is aimed at exploring the domain of hidden particles and make measurements with tau neutrinos. Hidden particles are predicted by a large number of…

Instrumentation and Detectors · Physics 2015-04-21 SHiP Collaboration , M. Anelli , S. Aoki , G. Arduini , J. J. Back , A. Bagulya , W. Baldini , A. Baranov , G. J. Barker , S. Barsuk , M. Battistin , J. Bauche , A. Bay , V. Bayliss , L. Bellagamba , G. Bencivenni , M. Bertani , O. Bezshyyko , D. Bick , N. Bingefors , A. Blondel , M. Bogomilov , A. Boyarsky , D. Bonacorsi , D. Bondarenko , W. Bonivento , J. Borburgh , T. Bradshaw , R. Brenner , D. Breton , N. Brook , M. Bruschi , A. Buonaura , S. Buontempo , S. Cadeddu , A. Calcaterra , M. Calviani , M. Campanelli , C. Capoccia , A. Cecchetti , A. Chatterjee , J. Chauveau , A. Chepurnov , M. Chernyavskiy , P. Ciambrone , C. Cicalo , G. Conti , K. Cornelis , M. Courthold , M. G. Dallavalle , N. D'Ambrosio , G. De Lellis , M. De Serio , L. Dedenko , A. Di Crescenzo , N. Di Marco , C. Dib , J. Dietrich , H. Dijkstra , D. Domenici , S. Donskov , D. Druzhkin , J. Ebert , U. Egede , A. Egorov , V. Egorychev , M. A. El Alaoui , T. Enik , A. Etenko , F. Fabbri , L. Fabbri , G. Fedorova , G. Felici , M. Ferro-Luzzi , R. A. Fini , M. Franke , M. Fraser , G. Galati , B. Giacobbe , B. Goddard , L. Golinka-Bezshyyko , D. Golubkov , A. Golutvin , D. Gorbunov , E. Graverini , J-L Grenard , A. M. Guler , C. Hagner , H. Hakobyan , J. C. Helo , E. van Herwijnen , D. Horvath , M. Iacovacci , G. Iaselli , R. Jacobsson , I. Kadenko , M. Kamiscioglu , C. Kamiscioglu , G. Khaustov , A. Khotjansev , B. Kilminster , V. Kim , N. Kitagawa , K. Kodama , A. Kolesnikov , D. Kolev , M. Komatsu , N. Konovalova , S. Koretskiy , I. Korolko , A. Korzenev , S. Kovalenko , Y. Kudenko , E. Kuznetsova , H. Lacker , A. Lai , G. Lanfranchi , A. Lauria , H. Lebbolo , J. -M. Levy , L. Lista , P. Loverre , A. Lukiashin , V. E. Lyubovitskij , A. Malinin , M. Manfredi , A. Perillo-Marcone , A. Marrone , R. Matev , E. N. Messomo , P. Mermod , S. Mikado , Yu. Mikhaylov , J. Miller , D. Milstead , O. Mineev , R. Mingazheva , G. Mitselmakher , M. Miyanishi , P. Monacelli , A. Montanari , M. C. Montesi , G. Morello , K. Morishima , S. Movtchan , V. Murzin , N. Naganawa , T. Naka , M. Nakamura , T. Nakano , N. Nurakhov , B. Obinyakov , K. Ocalan , S. Ogawa , V. Oreshkin , A. Orlov , J. Osborne , P. Pacholek , J. Panman , A. Paoloni , L. Paparella , A. Pastore , M. Patel , K. Petridis , M. Petrushin , M. Poli-Lener , N. Polukhina , V. Polyakov , M. Prokudin , G. Puddu , F. Pupilli , F. Rademakers , A. Rakai , T. Rawlings , F. Redi , S. Ricciardi , R. Rinaldesi , T. Roganova , A. Rogozhnikov , H. Rokujo , A. Romaniouk , G. Rosa , I. Rostovtseva , T. Rovelli , O. Ruchayskiy , T. Ruf , G. Saitta , V. Samoylenko , V. Samsonov , A. Sanz Ull , A. Saputi , O. Sato , W. Schmidt-Parzefall , N. Serra , S. Sgobba , M. Shaposhnikov , P. Shatalov , A. Shaykhiev , L. Shchutska , V. Shevchenko , H. Shibuya , Y. Shitov , S. Silverstein , S. Simone , M. Skorokhvatov , S. Smirnov , E. Solodko , V. Sosnovtsev , R. Spighi , M. Spinetti , N. Starkov , B. Storaci , C. Strabel , P. Strolin , S. Takahashi , P. Teterin , V. Tioukov , D. Tommasini , D. Treille , R. Tsenov , T. Tshchedrina , A. Ustyuzhanin , F. Vannucci , V. Venturi , M. Villa , Heinz Vincke , Helmut Vincke , M. Vladymyrov , S. Xella , M. Yalvac , N. Yershov , D. Yilmaz , A. U. Yilmazer , G. Vankova-Kirilova , Y. Zaitsev , A. Zoccoli

Orbital monitoring of exoplanetary and stellar systems is fundamental for analysing their architecture, dynamical stability and evolution, and mechanisms of formation. Current high-contrast extreme-adaptive optics imagers like SPHERE, GPI,…

The High Energy Modular Ensemble of Satellites (HERMES) project is aimed to realize a modular X/gamma-ray monitor for transient events, to be placed on-board of a CubeSat bus. This expandable platform will achieve a significant impact on…

We discuss the future possibilities for extragalactic star cluster research with the expected new ground-based and space-based telescopes and instrumentation. Significant gains are expected due to improved angular resolution, sensitivity,…

Astrophysics · Physics 2007-05-23 John S. Gallagher , Eva K. Grebel

The H.E.S.S. experiment (High Energy Stereoscopic System) is a new generation atmospheric Cherenkov detector measuring high-energy (>100 GeV) gamma radiation from the Universe. This paper briefly explains the imaging Cherenkov technique and…

Astrophysics · Physics 2019-08-14 U. Schwanke

The search for extraterrestrial intelligence (SETI) is a scientific endeavor which struggles with unique issues -- a strong indeterminacy in what data to look for and when to do so. This has led to attempts at finding both fundamental…

Information Theory · Computer Science 2021-07-22 Ian George , Xinan Chen , Lav R. Varshney

The advent of experimental science facilities-instruments and observatories, such as the Large Hadron Collider, the Laser Interferometer Gravitational Wave Observatory, and the upcoming Large Synoptic Survey Telescope-has brought about…

Distributed, Parallel, and Cluster Computing · Computer Science 2019-02-12 E. A. Huerta , Roland Haas , Shantenu Jha , Mark Neubauer , Daniel S. Katz

The HERMES-TP/SP mission, based on a nanosatellite constellation, has very stringent constraints of sensitivity and compactness, and requires an innovative wide energy range instrument. The instrument technology is based on the "siswich"…

The primary goal of the search for extraterrestrial intelligence (SETI) is to gain an understanding of the prevalence of technologically advanced beings (organic or inorganic) in the Galaxy. One way to approach this is to look for…

The existence of intelligent extraterrestrial life forms among the thousands of billions of galaxies that dance in the Universe is beyond doubt. Meeting with one of them is only a matter of time. SETI (Search for Extraterrestrial…

Popular Physics · Physics 2017-08-22 Olivier Auber

Exoplanet research has shown an incessant growth since the first claim of a hot giant planet around a solar-like star in the mid-1990s. Today, the new facilities are working to spot the first habitable rocky planets around low-mass stars as…

Instrumentation and Methods for Astrophysics · Physics 2018-08-08 Serena Benatti