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Related papers: The COSINE-100 Data Acquisition System

200 papers

We assess the tension between DAMA/LIBRA and the latest dark matter annual modulation results from the ANAIS-112 and COSINE-100 NaI experiments, under a range of hypotheses ranging from physical to general parameterisations. We find that,…

We present the most recent results from XENON100, the current phase of the XENON dark matter search program. XENON100 is a dual phase time-projection chamber operated at the Laboratori Nazionali del Gran Sasso (LNGS) whose ultra-low…

Cosmology and Nongalactic Astrophysics · Physics 2013-05-14 Paolo Beltrame

In the case of underground experiments for neutrino physics or rare event searches, the background caused by cosmic muons contributes significantly and therefore must be identified and rejected. We proposed and optimized a new detector…

Instrumentation and Detectors · Physics 2017-04-05 Y. P. Zhang , J. L. Xu , H. Q. Lu , P. Zhang , C. C. Zhang , C. G. Yang

This paper describes the design, fabrication, commissioning and use of a CALibration source Insertion System (CALIS) in the DarkSide-50 direct dark matter search experiment. CALIS deploys radioactive sources into the liquid scintillator…

Instrumentation and Detectors · Physics 2018-01-17 P. Agnes , I. F. M. Albuquerque , T. Alexander , A. K. Alton , D. M. Asner , H. O. Back , B. Baldin , K. Biery , V. Bocci , G. Bonfini , W. Bonivento , M. Bossa , B. Bottino , A. Brigatti , J. Brodsky , F. Budano , S. Bussino , M. Cadeddu , L. Cadonati , M. Cadoni , F. Calaprice , N. Canci , A. Candela , M. Caravati , M. Cariello , M. Carlini , S. Catalanotti , P. Cavalcante , A. Chepurnov , C. Cicalo , A. G. Cocco , G. Covone , D. D'Angelo , M. D'Incecco , S. Davini , S. De Cecco , M. De Deo , M. De Vincenzi , A. Derbin , A. Devoto , F. Di Eusanio , G. Di Pietro , C. Dionisi , E. Edkins , A. Empl , A. Fan , G. Fiorillo , K. Fomenko , G. Forster , D. Franco , F. Gabriele , C. Galbiati , S. Giagu , C. Giganti , G. K. Giovanetti , A. M. Goretti , F. Granato , L. Grandi , M. Gromov , M. Guan , Y. Guardincerri , B. R. Hackett , K. Herner , D. Hughes , P. Humble , E. V. Hungerford , Al. Ianni , An. Ianni , I. James , T. N. Johnson , C. Jollet , K. Keeter , C. L. Kendziora , G. Koh , D. Korablev , G. Korga , A. Kubankin , X. Li , M. Lissia , B. Loer , P. Lombardi , G. Longo , Y. Ma , I. N. Machulin , A. Mandarano , S. M. Mari , J. Maricic , L. Marini , C. J. Martoff , A. Meregaglia , P. D. Meyers , R. Milincic , J. D. Miller , D. Montanari , A. Monte , B. J. Mount , V. N. Muratova , P. Musico , J. Napolitano , A. Navrer Agasson , S. Odrowski , M. Orsini , F. Ortica , L. Pagani , M. Pallavicini , E. Pantic , S. Parmeggiano , K. Pelczar , N. Pelliccia , A. Pocar , S. Pordes , D. A. Pugachev , H. Qian , K. Randle , G. Ranucci , M. Razeti , A. Razeto , B. Reinhold , A. L. Renshaw , M. Rescigno , Q. Riffard , A. Romani , B. Rossi , N. Rossi , D. Rountree , D. Sablone , P. Saggese , R. Saldanha , W. Sands , C. Savarese , B. Schlitzer , E. Segreto , D. A. Semenova , E. Shields , P. N. Singh , M. D. Skorokhvatov , O. Smirnov , A. Sotnikov , C. Stanford , Y. Suvorov , R. Tartaglia , J. Tatarowicz , G. Testera , A. Tonazzo , P. Trinchese , E. V. Unzhakov , M. Verducci , A. Vishneva , B. Vogelaar , M. Wada , S. Walker , H. Wang , Y. Wang , A. W. Watson , S. Westerdale , J. Wilhelmi , M. M. Wojcik , Xi. Xiang , X. Xiao , J. Xu , C. Yang , A. Zec , W. Zhong , C. Zhu , G. Zuzel

For many years annually modulating $\sim$ keV scintillations have been observed in the DAMA/NaI and DAMA/Libra experiments. A dark matter - electron scattering interpretation is now favoured given the stringent constraints on nuclear recoil…

High Energy Physics - Phenomenology · Physics 2016-07-01 R. Foot

ANAIS (Annual modulation with NaI Scintillators) is a dark matter direct detection experiment located at the Canfranc Underground Laboratory (LSC), in Spain. The goal is to confirm or refute in a model independent way the DAMA/LIBRA…

Instrumentation and Methods for Astrophysics · Physics 2020-05-20 J. Amaré , S. Cebrián , D. Cintas , I. Coarasa , E. García , M. Martínez , M. A. Oliván , Y. Ortigoza , A. Ortiz de Solórzano , J. Puimedón , A. Salinas , M. L. Sarsa , P. Villar

Molybdenum based crystals such as Li$_2$MoO$_4$ and CaMoO$_4$ are emerging as leading candidates for next generation experiments searching for neutrino-less double beta decay with cryogenic calorimeters (CUPID, AMoRE). The exquisite energy…

Instrumentation and Detectors · Physics 2019-08-30 N. Casali , L. Cardani , I. Colantoni , A. Cruciani , S. Di Domizio , M. Martinez , G. Pettinari , M. Vignati

A scintillating bolometer based on a large cubic Li$_{2}$$^{100}$MoO$_4$ crystal (45 mm side) and a Ge wafer (scintillation detector) has been operated in the CROSS cryogenic facility at the Canfranc underground laboratory in Spain. The…

Instrumentation and Detectors · Physics 2021-03-24 The CUPID Interest Group , A. Armatol , E. Armengaud , W. Armstrong , C. Augier , F. T. Avignone , O. Azzolini , I. C. Bandac , A. S. Barabash , G. Bari , A. Barresi , D. Baudin , F. Bellini , G. Benato , M. Beretta , L. Bergé , Ch. Bourgeois , M. Biassoni , J. Billard , V. Boldrini , A. Branca , C. Brofferio , C. Bucci , J. M. Calvo-Mozota , J. Camilleri , A. Candela , S. Capelli , L. Cappelli , L. Cardani , P. Carniti , N. Casali , A. Cazes , E. Celi , C. Chang , M. Chapellier , A. Charrier , D. Chiesa , M. Clemenza , I. Colantoni , F. Collamati , S. Copello , F. Cova , O. Cremonesi , R. J. Creswick , A. Cruciani , A. D'Addabbo , G. D'Imperio , I. Dafinei , F. A. Danevich , M. de Combarieu , M. De Deo , M. De Jesus , P. de Marcillac , S. Dell'Oro , S. Di Domizio , V. Dompe , A. Drobizhev , L. Dumoulin , G. Fantini , M. Fasoli , M. Faverzani , E. Ferri , F. Ferri , F. Ferroni , E. Figueroa-Feliciano , J. Formaggio , A. Franceschi , C. Fu , S. Fu , B. K. Fujikawa , J. Gascon , A. Giachero , L. Gironi , A. Giuliani , P. Gorla , C. Gotti , P. Gras , M. Gros , E. Guerard , T. D. Gutierrez , K. Han , E. V. Hansen , K. M. Heeger , D. L. Helis , H. Z. Huang , R. G. Huang , A. Ianni , L. Imbert , J. Johnston , A. Juillard , G. Karapetrov , G. Keppel , H. Khalife , V. V. Kobychev , Yu. G. Kolomensky , S. I. Konovalov , Y. Liu , P. Loaiza , L. Ma , M. Madhukuttan , F. Mancarella , R. Mariam , L. Marini , S. Marnieros , M. Martinez , R. H. Maruyama , B. Mauri , D. Mayer , Y. Mei , S. Milana , D. Misiak , T. Napolitano , M. Nastasi , X. -F. Navick , J. Nikkel , R. Nipoti , S. Nisi , C. Nones , E. B. Norman , V. Novosad , I. Nutini , T. O'Donnell , G. Olivier , E. Olivieri , C. Oriol , J. L. Ouellet , S. Pagan , C. Pagliarone , L. Pagnanini , P. Pari , L. Pattavina , B. Paul , M. Pavan , H. Peng , G. Pessina , V. Pettinacci , C. Pira , S. Pirro , D. V. Poda , T. Polakovic , O. G. Polischuk , S. Pozzi , E. Previtali , A. Puiu , A. Ressa , D. Reynet , R. Rizzoli , C. Rosenfeld , V. Sanglard , J. A. Scarpaci , B. Schmidt , V. Sharma , V. N. Shlegel , V. Singh , M. Sisti , D. Speller , P. T. Surukuchi , L. Taffarello , O. Tellier , C. Tomei , V. I. Tretyak , A. Tsymbaliuk , A. Vedda , M. Velazquez , K. J. Vetter , S. L. Wagaarachchi , G. Wang , L. Wang , B. Welliver , J. Wilson , K. Wilson , L. A. Winslow , M. Xue , L. Yan , J. Yang , V. Yefremenko , V. I. Yumatov , M. M. Zarytskyy , J. Zhang , A. S. Zolotarova , S. Zucchelli

The DAMIC experiment uses fully depleted, high resistivity CCDs to search for dark matter particles. With an energy threshold $\sim$50 eV$_{ee}$, and excellent energy and spatial resolutions, the DAMIC CCDs are well-suited to identify and…

The XENON experiment aims at the direct detection of dark matter in the form of WIMPs (Weakly Interacting Massive Particles) via their elastic scattering off Xenon nuclei. With a fiducial mass of 1000 kg of liquid xenon, a sufficiently low…

Astrophysics · Physics 2007-05-23 XENON Collaboration , Elena Aprile

We present first significant limits on WIMP dark matter by the phonon-light technique, where combined phonon and light signals from a scintillating cryogenic detector are used. Data from early 2004 with two 300 g CRESST-II prototype…

The most discussed topic in direct search for dark matter is arguably the verification of the DAMA claim. In fact, the observed annual modulation of the signal rate in an array of NaI(Tl) detectors can be interpreted as the awaited…

The multichannel data acquisition system is intended to be used in the EMMA experiment studying cosmic rays. The array will be in the Pihasalmi mine (central Finland) at a depth of about 85 m. The scintillator counters (SC-1) of the array…

The MiniCLEAN dark matter experiment will exploit a single-phase liquid-argon detector instrumented with photomultiplier tubes submerged in the cryogen with nearly 4pi coverage of a 500 kg (150 kg) target (fiducial) mass. The high light…

Instrumentation and Detectors · Physics 2011-10-06 Andrew Hime

LUX is a two-phase (liquid/gas) xenon time projection chamber designed to detect nuclear recoils from interactions with dark matter particles. Signals from the LUX detector are processed by custom-built analog electronics which provide…

We have searched for periodic variations of the electronic recoil event rate in the (2-6) keV energy range recorded between February 2011 and March 2012 with the XENON100 detector, adding up to 224.6 live days in total. Following a detailed…

A direction sensitive dark matter detector using organic crystals is being developed. It exploits the anisotropic scintillation efficiency of organic crystals with respect to the direction of nuclear recoils relative to crystallographic…

Astrophysics · Physics 2016-12-07 H. Sekiya , M. Minowa , Y. Shimizu , W. Suganuma , Y. Inoue

The NUCLEUS experiment aims to measure coherent elastic neutrino nucleus scattering of reactor anti-neutrinos using cryogenic calorimeters. Operating at an overburden of 3 m.w.e., muon-induced backgrounds are expected to be one of the…

DarkSide-50 is a detector for dark matter candidates in the form of weakly interacting massive particles (WIMPs). It utilizes a liquid argon time projection chamber (LAr TPC) for the inner main detector. The TPC is surrounded by a liquid…

Instrumentation and Detectors · Physics 2017-02-06 P. Agnes , L. Agostino , I. F. M. Albuquerque , T. Alexander , A. K. Alton , K. Arisaka , H. O. Back , B. Baldin , K. Biery , G. Bonfini , M. Bossa , B. Bottino , A. Brigatti , J. Brodsky , F. Budano , S. Bussino , M. Cadeddu , M. Cadoni , F. Calaprice , N. Canci , A. Candela , H. Cao , M. Cariello , M. Carlini , S. Catalanotti , P. Cavalcante , A. Chepurnov , A. G. Cocco , G. Covone , L. Crippa , D. D'Angelo , M. D'Incecco , S. Davini , S. De Cecco , M. De Deo , M. De Vincenzi , A. Derbin , A. Devoto , F. Di Eusanio , G. Di Pietro , E. Edkins , A. Empl , A. Fan , G. Fiorillo , K. Fomenko , G. Foster , D. Franco , F. Gabriele , C. Galbiati , C. Giganti , A. M. Goretti , F. Granato , L. Grandi , M. Gromov , M. Guan , Y. Guardincerri , B. R. Hackett , K. R. Herner , E. V. Hungerford , Aldo Ianni , Andrea Ianni , I. James , C. Jollet , K. Keeter , C. L. Kendziora , V. Kobychev , G. Koh , D. Korablev , G. Korga , A. Kubankin , X. Li , M. Lissia , P. Lombardi , S. Luitz , Y. Ma , I. N. Machulin , A. Mandarano , S. M. Mari , J. Maricic , L. Marini , C. J. Martoff , A. Meregaglia , P. D. Meyers , T. Miletic , R. Milincic , D. Montanari , A. Monte , M. Montuschi , M. E. Monzani , P. Mosteiro , B. J. Mount , V. N. Muratova , P. Musico , J. Napolitano , A. Nelson , S. Odrowski , M. Orsini , F. Ortica , L. Pagani , M. Pallavicini , E. Pantic , S. Parmeggiano , K. Pelczar , N. Pelliccia , A. Pocar , S. Pordes , D. A. Pugachev , H. Qian , K. Randle , G. Ranucci , A. Razeto , B. Reinhold , A. L. Renshaw , Q. Riffard , A. Romani , B. Rossi , N. Rossi , S. D. Rountree , D. Sablone , P. Saggese , R. Saldanha , W. Sands , S. Sangiorgio , C. Savarese , E. Segreto , D. A. Semenov , E. Shields , P. N. Singh , M. D. Skorokhvatov , O. Smirnov , A. Sotnikov , C. Stanford , Y. Suvorov , R. Tartaglia , J. Tatarowicz , G. Testera , A. Tonazzo , P. Trinchese , E. V. Unzhakov , A. Vishneva , R. B. Vogelaar , M. Wada , S. Walker , H. Wang , Y. Wang , A. W. Watson , S. Westerdale , J. Wilhelmi , M. M. Wojcik , X. Xiang , J. Xu , C. Yang , J. Yoo , S. Zavatarelli , A. Zec , W. Zhong , C. Zhu , G. Zuzel

XMASS-I uses single phase liquid xenon technology for aiming at the direct detection of dark matter. The detector observes only scintillation light by 2 inch 642 PMTs which are placed in sphere shape around an active volume. With its large…

Cosmology and Nongalactic Astrophysics · Physics 2018-05-28 Masaki Yamashita
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