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Particle identification in gaseous detectors traditionally relies on energy loss measurements (dE/dx); however, uncertainties in total energy deposition limit its resolution. The cluster counting technique (dN/dx) offers an alternative…

Neutron Resonance Transmission Analysis (NRTA) is a spectroscopic technique which uses the resonant absorption of neutrons in the epithermal range to infer the isotopic composition of an object. This spectroscopic technique has relevance in…

Instrumentation and Detectors · Physics 2021-05-19 Ethan A. Klein , Farheen Naqvi , Jacob E. Bickus , Hin Y. Lee , Robert J. Goldston , Areg Danagoulian

Theoretical predictions for neutrino fluxes indicate that km$^{3}$ scale detectors are needed to detect certain astrophysical sources. The three Mediterranean experiments, ANTARES, NEMO and NESTOR are working together on a design study,…

Astrophysics · Physics 2019-08-14 J. Carr , D. Dornic , F. Jouvenot , G. Maurin

The Spectrograph of the RISTRETTO instrument is now currently being manufactured. RISTETTO is an instrument designed to detect and characterize the reflected light of nearby exoplanets. It combines high contrast imaging and high resolution…

A new pixel detector for the CMS experiment was built in order to cope with the instantaneous luminosities anticipated for the Phase~I Upgrade of the LHC. The new CMS pixel detector provides four-hit tracking with a reduced material budget…

Instrumentation and Detectors · Physics 2017-06-02 M. Dragicevic , M. Friedl , J. Hrubec , H. Steininger , A. Gädda , J. Härkönen , T. Lampén , P. Luukka , T. Peltola , E. Tuominen , E. Tuovinen , A. Winkler , P. Eerola , T. Tuuva , G. Baulieu , G. Boudoul , L. Caponetto , C. Combaret , D. Contardo , T. Dupasquier , G. Gallbit , N. Lumb , L. Mirabito , S. Perries , M. Vander Donckt , S. Viret , C. Bonnin , L. Charles , L. Gross , J. Hosselet , D. Tromson , L. Feld , W. Karpinski , K. Klein , M. Lipinski , G. Pierschel , M. Preuten , M. Rauch , M. Wlochal , M. Aldaya , C. Asawatangtrakuldee , K. Beernaert , D. Bertsche , C. Contreras-Campana , G. Eckerlin , D. Eckstein , T. Eichhorn , E. Gallo , J. Garay Garcia , K. Hansen , M. Haranko , A. Harb , J. Hauk , J. Keaveney , A. Kalogeropoulos , C. Kleinwort , W. Lohmann , R. Mankel , H. Maser , G. Mittag , C. Muhl , A. Mussgiller , D. Pitzl , O. Reichelt , M. Savitskyi , P. Schütze , V. Sola , S. Spannagel , R. Walsh , A. Zuber , H. Biskop , P. Buhmann , M. Centis-Vignali , E. Garutti , J. Haller , M. Hoffmann , R. Klanner , T. Lapsien , M. Matysek , A. Perieanu , Ch. Scharf , P. Schleper , A. Schmidt , J. Schwandt , J. Sonneveld , G. Steinbrück , B. Vormwald , J. Wellhausen , M. Abbas , C. Amstutz , T. Barvich , Ch. Barth , F. Boegelspacher , W. De Boer , E. Butz , M. Casele , F. Colombo , A. Dierlamm , B. Freund , F. Hartmann , S. Heindl , U. Husemann , A. Kornmeyer , S. Kudella , Th. Muller , H. J. Simonis , P. Steck , M. Weber , Th. Weiler , T. Kiss , F. Siklér , T. Tölyhi , V. Veszprémi , P. Cariola , D. Creanza , M. De Palma , G. De Robertis , L. Fiore , M. Franco , F. Loddo , G. Sala , L. Silvestris , G. Maggi , S. My , G. Selvaggi , S. Albergo , G. Cappello , S. Costa , A. Di Mattia , F. Giordano , R. Potenza , M. A. Saizu , A. Tricomi , C. Tuve , E. Focardi , M. E. Dinardo , S. Fiorendi , S. Gennai , S. Malvezzi , R. A. Manzoni , D. Menasce , L. Moroni , D. Pedrini , P. Azzi , N. Bacchetta , D. Bisello , M. Dall'Osso , N. Pozzobon , M. Tosi , L. Alunni Solestizi , M. Biasini , G. M. Bilei , C. Cecchi , B. Checcucci , D. Ciangottini , L. Fanò , C. Gentsos , M. Ionica , R. Leonardi , E. Manoni , G. Mantovani , S. Marconi , V. Mariani , M. Menichelli , A. Modak , A. Morozzi , F. Moscatelli , D. Passeri , P. Placidi , V. Postolache , A. Rossi , A. Saha , A. Santocchia , L. Storchi , D. Spiga , K. Androsov , P. Azzurri , G. Bagliesi , A. Basti , T. Boccali , L. Borrello , F. Bosi , R. Castaldi , M. Ceccanti , M. A. Ciocci , R. Dell'Orso , S. Donato , G. Fedi , A. Giassi , M. T. Grippo , F. Ligabue , G. Magazzu , P. Mammini , F. Mariani , E. Mazzoni , A. Messineo , A. Moggi , F. Morsani , F. Palla , F. Palmonari , A. Profeti , F. Raffaelli , A. Ragonesi , A. Rizzi , A. Soldani , P. Spagnolo , R. Tenchini , G. Tonelli , A. Venturi , P. G. Verdini , D. Abbaneo , I. Ahmed , E. Albert , G. Auzinger , G. Berruti , J. Bonnaud , J. Daguin , A. D'Auria , S. Detraz , O. Dondelewski , B. Engegaard , F. Faccio , N. Frank , K. Gill , A. Honma , A. Kornmayer , A. Labaza , F. Manolescu , I. McGill , S. Mersi , S. Michelis , A. Onnela , M. Ostrega , S. Pavis , A. Peisert , J. -F. Pernot , P. Petagna , H. Postema , K. Rapacz , C. Sigaud , P. Tropea , J. Troska , A. Tsirou , F. Vasey , B. Verlaat , P. Vichoudis , L. Zwalinski , F. Bachmair , R. Becker , D. di Calafiori , B. Casal , P. Berger , L. Djambazov , M. Donega , C. Grab , D. Hits , J. Hoss , G. Kasieczka , W. Lustermann , B. Mangano , M. Marionneau , P. Martinez Ruiz del Arbol , M. Masciovecchio , M. Meinhard , L. Perozzi , U. Roeser , A. Starodumov , V. Tavolaro , R. Wallny , D. Zhu , K. Bösiger , L. Caminada , F. Canelli , V. Chiochia , A. de Cosa , C. Galloni , T. Hreus , B. Kilminster , C. Lange , R. Maier , J. Ngadiuba , D. Pinna , P. Robmann , S. Taroni , Y. Yang , W. Bertl , K. Deiters , W. Erdmann , R. Horisberger , H. -C. Kaestli , D. Kotlinski , U. Langenegger , B. Meier , T. Rohe , S. Streuli , P. -H. Chen , C. Dietz , F. Fiori , U. Grundler , W. -S. Hou , R. -S. Lu , M. Moya , J. -F. Tsai , Y. M. Tzeng , D. Cussans , J. Goldstein , M. Grimes , D. Newbold , P. Hobson , I. D. Reid , G. Auzinger , R. Bainbridge , P. Dauncey , G. Hall , T. James , A. -M. Magnan , M. Pesaresi , D. M. Raymond , K. Uchida , T. Durkin , K. Harder , C. Shepherd-Themistocleous , M. Chertok , J. Conway , R. Conway , C. Flores , R. Lander , D. Pellett , F. Ricci-Tam , M. Squires , J. Thomson , R. Yohay , K. Burt , J. Ellison , G. Hanson , M. Olmedo , W. Si , B. R. Yates , A. Dominguez , R. Bartek , B. Bentele , J. P. Cumalat , W. T. Ford , F. Jensen , A. Johnson , M. Krohn , S. Leontsinis , T. Mulholland , K. Stenson , S. R. Wagner , A. Apresyan , G. Bolla , K. Burkett , J. N. Butler , A. Canepa , H. W. K. Cheung , D. Christian , W. E. Cooper , G. Deptuch , G. Derylo , C. Gingu , S. Grünendahl , S. Hasegawa , J. Hoff , J. Howell , M. Hrycyk , S. Jindariani , M. Johnson , F. Kahlid , S. Kwan , C. M. Lei , R. Lipton , R. Lopes De Sá , T. Liu , S. Los , M. Matulik , P. Merkel , S. Nahn , A. Prosser , R. Rivera , B. Schneider , G. Sellberg , A. Shenai , K. Siehl , L. Spiegel , N. Tran , L. Uplegger , E. Voirin , D. R. Berry , X. Chen , L. Ennesser , A. Evdokimov , C. E. Gerber , S. Makauda , C. Mills , I. D. Sandoval Gonzalez , J. Alimena , L. J. Antonelli , B. Francis , A. Hart , C. S. Hill , N. Parashar , J. Stupak , D. Bortoletto , M. Bubna , N. Hinton , M. Jones , D. H. Miller , X. Shi , P. Baringer , A. Bean , S. Khalil , A. Kropivnitskaya , D. Majumder , E. Schmitz , G. Wilson , A. Ivanov , R. Mendis , T. Mitchell , N. Skhirtladze , R. Taylor , I. Anderson , D. Fehling , A. Gritsan , P. Maksimovic , C. Martin , K. Nash , M. Osherson , M. Swartz , M. Xiao , J. G. Acosta , L. M. Cremaldi , S. Oliveros , L. Perera , D. Summers , K. Bloom , D. R. Claes , C. Fangmeier , R. Gonzalez Suarez , J. Monroy , J. Siado , E. Bartz , Y. Gershtein , E. Halkiadakis , S. Kyriacou , A. Lath , K. Nash , M. Osherson , S. Schnetzer , R. Stone , M. Walker , S. Malik , S. Norberg , J. E. Ramirez Vargas , M. Alyari , J. Dolen , A. Godshalk , C. Harrington , I. Iashvili , A. Kharchilava , D. Nguyen , A. Parker , S. Rappoccio , B. Roozbahani , J. Alexander , J. Chaves , J. Chu , S. Dittmer , K. McDermott , N. Mirman , A. Rinkevicius , A. Ryd , E. Salvati , L. Skinnari , L. Soffi , Z. Tao , J. Thom , J. Tucker , M. Zientek , B. Akgün , K. M. Ecklund , M. Kilpatrick , T. Nussbaum , J. Zabel , P. D'Angelo , W. Johns , K. Rose

High precision differential astrometry assesses the positions, distances, and motions of celestial objects in relation to the stars. The focal plane of such space telescope must be calibrated with a precision down to the level of 1e-5 pixel…

Instrumentation and Methods for Astrophysics · Physics 2024-10-30 Fabrice Pancher , Sebastien Soler , Fabien Malbet , Manon Lizzana , Pierre Kern , Thierry Lepine , Alain Leger

The development prospects have been considered of a scintillator-photodiode type detector with improved energy resolution attaining several per cent ($R=1-2%$). The main contributions to the scintielectron detector energy resolution have…

High Energy Physics - Experiment · Physics 2007-05-23 S. V. Naydenov , V. D. Ryzhikov

Spectroscopic measurements are presented using the PID350 pixelated gamma radiation detectors. A high-speed data acquisition system has been developed in order to reduce the data loss during the data reading in case of a high flux of…

Instrumentation and Detectors · Physics 2010-11-16 K. Karafasoulis , K. Zachariadou , S. Seferlis , I. Papadakis , D. Loukas , C. Lambropoulos , C. Potiriadis

The distinction between point and line resolution in transmission electron microscopy (TEM) arises because an ability to image sub-0.2 nm fringes is a necessary, but not a sufficient, condition for imaging individual atoms. In scanned tip…

Instrumentation and Detectors · Physics 2007-05-23 P. Fraundorf , J. Tentschert

Many naturally-occuring models in the sciences are well-approximated by simplified models, using multiscale techniques. In such settings it is natural to ask about the relationship between inverse problems defined by the original problem…

Numerical Analysis · Mathematics 2019-02-28 Kit Newton , Qin Li , Andrew Stuart

Beamstrahlung will constitute an important source of background in a pixel vertex detector at the future International Linear Collider. Electron and positron tracks of this origin impact the pixel planes at angles generally larger than…

Instrumentation and Detectors · Physics 2015-05-13 L. Maczewski , M. Adamus , J. Ciborowski , G. Grzelak , P. Luzniak P. Niezurawski A. Zarnecki

We present the design of a Faraday cup-like charged particle detector in a four quadrant configuration aimed at facilitating the alignment of low-intensity beams of exotic particles. The device is capable of assessing the current on the…

Instrumentation and Detectors · Physics 2024-02-13 Kilian Brenner , Michael Zimmermann , Maik Butterling , Andreas Wagner , Christoph Hugenschmidt , Francesco Guatieri

Aims. The derivation of spectroscopic parameters for M dwarf stars is very important in the fields of stellar and exoplanet characterization. The goal of this work is the creation of an automatic computational tool, able to derive quickly…

Solar and Stellar Astrophysics · Physics 2020-04-08 A. Antoniadis-Karnavas , S. G. Sousa , E. Delgado-Mena , N. C. Santos , G. D. C. Teixeira , V. Neves

The concept of super-resolution refers to various methods for improving the angular resolution of an optical imaging system beyond the classical diffraction limit. Although several techniques to narrow the central lobe of the illumination…

Instrumentation and Methods for Astrophysics · Physics 2017-04-11 Luca Olmi , Pietro Bolli , Luca Cresci , Francesco D'Agostino , Massimo Migliozzi , Daniela Mugnai , Enzo Natale , Renzo Nesti , Dario Panella , Lorenzo Stefani

The time-resolved electron beam envelope parameters including sectional distribution and position are important and necessary for the study of beam transmission characteristics in the magnetic field and verifying the magnetic field setup…

Accelerator Physics · Physics 2015-02-10 Jiang Xiaoguo , Wang Yuan , Yang Zhiyong , Zhang Huang , Wang Yi , Wei Tao

Here we present a computational tool for optical tweezers which calculates the particle tracking signal measured with a quadrant detector and the shot-noise limit to position resolution. The tool is a piece of Matlab code which functions…

Instrumentation and Detectors · Physics 2021-05-27 Michael A. Taylor , Warwick P. Bowen

This paper presents an attractive method towards sensing and quantifying the concentration of dielectric particles suspended in a highly conductive medium. Fast electrical impedance spectroscopy (EIS) measurements were performed, based on…

Signal Processing · Electrical Eng. & Systems 2019-03-26 Roberto G. Ramírez-Chavarría , Celia Sánchez-Pérez

For its physics program with a high-intensity hadron beam of up to 2e7 particles/s, the COMPASS experiment at CERN requires tracking of charged particles scattered by very small angles with respect to the incident beam direction. While good…

We consider a method for obtaining information on polarization of astronomical objects radiation at diffraction limited resolution - differential speckle polarimetry. As an observable we propose to use averaged cross spectrum of two…

Instrumentation and Methods for Astrophysics · Physics 2015-06-12 Boris Safonov

In this paper, we present the design and characterization of a photosensor system developed for the RELICS experiment. An extended dynamic range base was designed to mitigate photomultiplier tube (PMT) saturation caused by intense cosmic…

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