W
W. Hampel
Researcher at Max Planck Society
Publications - 7
Citations - 1010
W. Hampel is an academic researcher from Max Planck Society. The author has contributed to research in topics: GALLEX & Solar neutrino. The author has an hindex of 6, co-authored 7 publications receiving 942 citations. Previous affiliations of W. Hampel include Alfried Krupp von Bohlen und Halbach Foundation.
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Journal ArticleDOI
GNO solar neutrino observations: results for GNO I
M. Altmann,M. Balata,P. Belli,E. Bellotti,R. Bernabei,E. Burkert,C. Cattadori,Giorgio Cerichelli,Marco Chiarini,M. Cribier,S. d'Angelo,G. Del Re,K.H. Ebert,Franz von Feilitzsch,N. Ferrari,W. Hampel,J. Handt,E. Henrich,G. Heusser,J. Kiko,T. Kirsten,T. Lachenmaier,J.-C. Lanfranchi,Matthias Laubenstein,D. Motta,W. Rau,H. Richter,S. Wänninger,Marcin Wójcik,L. Zanotti +29 more
TL;DR: The first GNO solar neutrino results for the measuring period GNO I, solar exposure time May 20, 1998 till January 12, 2000 were reported in this article, where counting results for solar runs SR1-SR19 were used till April 4, 2000.
Journal ArticleDOI
Final results of the 51Cr neutrino source experiments in GALLEX
W. Hampel,G. Heusser,J. Kiko,T. Kirsten,Matthias Laubenstein,Ernst Pernicka,W. Rau,U. Rönn,C. Schlosser,M. Wojcik,R.v. Ammon,K.H. Ebert,T. Fritsch,D. Heidt,E. Henrich,L. Stieglitz,F. Weirich,M. Balata,F.X. Hartmann,M. Sann,E. Bellotti,C. Cattadori,Oliviero Cremonesi,N. Ferrari,Ettore Fiorini,L. Zanotti,M. Altmann,F.v. Feilitzsch,R. Mößbauer,G. Berthomieu,E. Schatzman,I. Carmi,I. Dostrovsky,C. Bacci,P. Belli,R. Bernabei,S. d'Angelo,L. Paoluzi,A. Bevilacqua,M. Cribier,L. Gosset,J. Rich,Michel Spiro,Charling Tao,D. Vignaud,J. Boger,R.L. Hahn,J.K. Rowley,R.W. Stoenner,J. Weneser +49 more
TL;DR: The radiochemical GALLEX experiment has been measuring the solar neutrino flux since May 1991 and has performed an investigation with two intense 51Crneutrino sources (> 60 PBq) that were produced in the Siloe nuclear reactor and used at the Gran Sasso National Laboratory, one between June and October 1994, and the second between October 95 and February 96.
Journal ArticleDOI
GALLEX solar neutrino observations. The results from GALLEX I and early results from GALLEX II
P. Anselmann,W. Hampel,G. Heusser,J. Kiko,T. Kirsten,Matthias Laubenstein,Ernst Pernicka,S. Pezzoni,R. Plaga,U. Rönn,M. Sann,C. Schlosser,R. Wink,M. Wojcik,R.v. Ammon,K.H. Ebert,T. Fritsch,K. Hellriegel,E. Henrich,L. Stieglitz,F. Weyrich,M. Balata,N. Ferrari,H. Lalla,E. Bellotti,C. Cattadori,Oliviero Cremonesi,Ettore Fiorini,L. Zanotti,M. Altmann,F.v. Feilitzsch,R. Möβbauer,U. Schanda,G. Berthomieu,E. Schatzman,I. Carmi,I. Dostrovsky,C. Bacci,P. Belli,R. Bernabei,S. d'Angelo,L. Paoluzi,S. Charbit,M. Cribier,G. Dupont,L. Gosset,J. Rich,Michel Spiro,T. Stolarczyk,Charling Tao,D. Vignaud,R.L. Hahn,F.X. Hartmann,J.K. Rowley,R.W. Stoenner,J. Weneser +55 more
TL;DR: The first period of data taking in the GALLEX solar neutrino experiment has been completed and the final result from the 15 runs of this periodpis (81±17 [ stat.]±9 [ syst.]) SNU (1 σ ) as discussed by the authors.
Journal ArticleDOI
Pulse shape discrimination for Gerda Phase I data
Matteo Agostini,M. Allardt,E. Andreotti,A. M. Bakalyarov,M. Balata,I. R. Barabanov,M. Barnabe Heider,M. Barnabe Heider,N. Barros,Laura Baudis,Christian Bauer,N. Becerici-Schmidt,E. Bellotti,S. Belogurov,S. T. Belyaev,Giovanni Benato,Alessandro Bettini,L. B. Bezrukov,T. Bode,V. Brudanin,R. Brugnera,D. Budjáš,Allen Caldwell,C. Cattadori,A. Chernogorov,F. Cossavella,E. V. Demidova,A. Domula,V. Egorov,R. Falkenstein,A. D. Ferella,K. Freund,N. Frodyma,A. M. Gangapshev,A. M. Gangapshev,A. Garfagnini,Claudio Gotti,P. Grabmayr,V. I. Gurentsov,K. N. Gusev,K. N. Gusev,K. N. Gusev,K. K. Guthikonda,W. Hampel,A. Hegai,M. Heisel,S. Hemmer,G. Heusser,Werner Hofmann,Mikael Hult,L. V. Inzhechik,L. Ioannucci,J. Janicskó Csáthy,J. Jochum,M. Junker,Thomas Kihm,I. V. Kirpichnikov,A. Kirsch,A. A. Klimenko,A. A. Klimenko,K. T. Knöpfle,O.I. Kochetov,V. N. Kornoukhov,V. V. Kuzminov,Matthias Laubenstein,A. Lazzaro,V. I. Lebedev,B. Lehnert,H. Y. Liao,Manfred Lindner,Ivano Lippi,Xianpeng Liu,A. Lubashevskiy,Bayarto Lubsandorzhiev,Guillaume Lutter,C. Macolino,A. A. Machado,Bela Majorovits,W. Maneschg,M. Misiaszek,Igor Nemchenok,S. Nisi,C.M. O'Shaughnessy,Luciano Pandola,K. Pelczar,G. Pessina,Alberto Pullia,Stefano Riboldi,N. Rumyantseva,Cinzia Sada,M. Salathe,C. Schmitt,J. Schreiner,Oliver Schulz,B. Schwingenheuer,Stefan Schönert,E. Shevchik,M. Shirchenko,M. Shirchenko,H. Simgen,A.A. Smolnikov,Luca Stanco,H. Strecker,M. Tarka,C. A. Ur,A. A. Vasenko,O. Volynets,K. von Sturm,K. von Sturm,V. Wagner,Marc Walter,A. Wegmann,T. Wester,Marcin Wójcik,E. A. Yanovich,P. Zavarise,I. Zhitnikov,S. V. Zhukov,D. R. Zinatulina,Kai Zuber,G. Zuzel +120 more
TL;DR: In this paper, the double escape peak (DEP) and Compton edge events of 2.615MeV γ rays from 208Tl decays as well as two-neutrino double beta (2νββ) decays of 76Ge are used as proxies for 0νβ β decay.
Journal ArticleDOI
Conceptual design and simulation of a water Cherenkov muon veto for the XENON1T experiment
Elena Aprile,F. Agostini,M. Alfonsi,K. Arisaka,F. Arneodo,M. Auger,C. Balan,P. Barrow,Laura Baudis,Boris Bauermeister,A. Behrens,P. Beltrame,K. Bokeloh,Amos Breskin,April S. Brown,Ethan Brown,S. Bruenner,Giacomo Bruno,Ran Budnik,João Cardoso,Auke-Pieter Colijn,H. Contreras,Jean-Pierre Cussonneau,M. P. Decowski,E. Duchovni,S. Fattori,A. D. Ferella,W. Fulgione,M. Garbini,C. Geis,Luke Goetzke,C. Grignon,Eilam Gross,W. Hampel,R. Itay,Florian Kaether,G. Kessler,A. Kish,H. Landsman,R. F. Lang,M. Le Calloch,D. Lellouch,L. Levinson,C. Levy,Sebastian Lindemann,Manfred Lindner,J. A. M. Lopes,K. Lung,A. Lyashenko,S. MacMullin,T. Marrodán Undagoitia,Julien Masbou,F. V. Massoli,D. Mayani Paras,A. J. Melgarejo Fernandez,Y. Meng,M. Messina,B. Miguez,A. Molinario,G. Morana,M. Murra,J. Naganoma,Uwe Oberlack,S. E. A. Orrigo,E. Pantic,R. Persiani,F. Piastra,J. Pienaar,G. Plante,N. Priel,S. Reichard,C. Reuter,A. Rizzo,S. Rosendahl,J.M.F. dos Santos,Gabriella Sartorelli,S. Schindler,J. Schreiner,Marc Schumann,L. Scotto Lavina,M. Selvi,P. Shagin,H. Simgen,A. Teymourian,D. Thers,A. Tiseni,Gian Carlo Trinchero,O. Vitells,Hongwei Wang,M. Weber,Ch. Weinheimer +90 more
TL;DR: In this paper, a water Cherenkov detector of 10 m height and diameter has been developed, equipped with 8 inch photomultipliers and cladded by a reflective foil.