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1.
Measurement of the neutrino velocity with the OPERA detector in the CNGS beam / OPERA Collaboration
The OPERA neutrino experiment at the underground Gran Sasso Laboratory has measured the velocity of neutrinos from the CERN CNGS beam over a baseline of about 730 km with much higher accuracy than previous studies conducted with accelerator neutrinos. The measurement is based on high-statistics data taken by OPERA in the years 2009, 2010 and 2011. [...]
arXiv:1109.4897.- 2012 - 24 p. - Published in : JHEP 10 (2012) 093 Fulltext: PDF; Springer Open Access article: PDF; External links: Interactions.org article; Press Release; Nautilus article
2.
Measurement of the neutrino velocity with the OPERA detector in the CNGS beam using the 2012 dedicated data / OPERA Collaboration
In spring 2012 CERN provided two weeks of a short bunch proton beam dedicated to the neutrino velocity measurement over a distance of 730 km. The OPERA neutrino experiment at the underground Gran Sasso Laboratory used an upgraded setup compared to the 2011 measurements, improving the measurement time accuracy. [...]
arXiv:1212.1276.- 2013 - 14 p. - Published in : JHEP 01 (2013) 153 Fulltext: PDF; Springer Open Access article: PDF; External link: Preprint
3.
Study of neutrino interactions with the electronic detectors of the OPERA experiment / OPERA Collaboration
The OPERA experiment is based on a hybrid technology combining electronic detectors and nuclear emulsions. OPERA collected muon-neutrino interactions during the 2008 and 2009 physics runs of the CNGS neutrino beam, produced at CERN with an energy range of about 5-35 GeV. [...]
arXiv:1102.1882.- 2011 - 22 p. - Published in : New J. Phys. 13 (2011) 053051 Fulltext: arXiv:1102.1882 - PDF; njp11_5_053051 - PDF; External link: Preprint
4.
The detection of neutrino interactions in the emulsion/lead target of the OPERA experiment / Agafonova, N. (Moscow, INR) ; Anokhina, A. (SINP, Moscow) ; Aoki, S. (Kobe U.) ; Ariga, A. (Bern U., LHEP) ; Ariga, T. (Bern U., LHEP) ; Arrabito, L. (Lyon, IPN) ; Autiero, D. (Lyon, IPN) ; Badertscher, A. (Zurich, ETH) ; Bagulya, A. (Lebedev Inst.) ; Bersani Greggio, F. (Frascati) et al.
The OPERA neutrino detector in the underground Gran Sasso Laboratory (LNGS) was designed to perform the first detection of neutrino oscillations in appearance mode through the study of $\nu_\mu\to\nu_\tau$ oscillations. The apparatus consists of an emulsion/lead target complemented by electronic detectors and it is placed in the high energy long-baseline CERN to LNGS beam (CNGS) 730 km away from the neutrino source. [...]
arXiv:0903.2973.- 2009 - 17 p. - Published in : JINST 4 (2009) P06020 Fulltext: PDF; SISSA/IOP Open Access article : PDF; External link: Preprint
5.
Search for $\nu_\mu \rightarrow \nu_e$ oscillations with the OPERA experiment in the CNGS beam / OPERA collaboration
A first result of the search for \numu $\rightarrow$ \nue oscillations in the OPERA experiment, located at the Gran Sasso Underground Laboratory, is presented. The experiment looked for the appearance of \nue in the CNGS neutrino beam using the data collected in 2008 and 2009. [...]
arXiv:1303.3953.- 2013 - 3 p. Fulltext: PDF; External link: Preprint
6.
New results on $\nu_\mu \to \nu_\tau$ appearance with the OPERA experiment in the CNGS beam / OPERA Collaboration
The OPERA neutrino experiment is designed to perform the first observation of neutrino oscillations in direct appearance mode in the $\nu_\mu \to \nu_\tau$ channel, via the detection of the $\tau$-leptons created in charged current $\nu_\tau$ interactions. The detector, located in the underground Gran Sasso Laboratory, consists of an emulsion/lead target with an average mass of about 1.2 kt, complemented by electronic detectors. [...]
arXiv:1308.2553.- 2013 - 32 p.
Article from SCOAP3: PDF; Fulltext: PDF; External link: Preprint
7.
Observation of a first $\nu_\tau$ candidate event in the OPERA experiment in the CNGS beam / OPERA Collaboration
The OPERA neutrino detector in the underground Gran Sasso Laboratory (LNGS) has been designed to perform the first detection of neutrino oscillations in direct appearance mode through the study of the $\nu_\mu\rightarrow\nu_\tau$ channel. The hybrid apparatus consists of an emulsion/lead target complemented by electronic detectors and it is placed in the high energy long-baseline CERN to LNGS beam (CNGS) 730 km away from the neutrino source. [...]
arXiv:1006.1623.- 2010 - 19 p. - Published in : Phys. Lett. B 691 (2010) 138-145 Fulltext: arXiv:1006.1623 - PDF; S0370269310007537 - XML; External link: Interactions.org article
8.
Emulsion sheet doublets as interface trackers for the OPERA experiment / OPERA Collaboration
New methods for efficient and unambiguous interconnection between electronic counters and target units based on nuclear photographic emulsion films have been developed. The application to the OPERA experiment, that aims at detecting oscillations between mu neutrino and tau neutrino in the CNGS neutrino beam, is reported in this paper. [...]
arXiv:0804.1985.- 2008 - 20 p. - Published in : JINST 3 (2008) P07005 Fulltext: PDF; SISSA/IOP Open Access article: PDF; External link: Fulltext
9.
Measurement of the atmospheric muon charge ratio with the OPERA detector / OPERA Collaboration
The OPERA detector at the Gran Sasso underground laboratory (LNGS) was used to measure the atmospheric muon charge ratio in the TeV energy region. We analyzed 403069 atmospheric muons corresponding to 113.4 days of livetime during the 2008 CNGS run. [...]
arXiv:1003.1907.- 2010 - 14 p. - Published in : Eur. Phys. J. C 67 (2010) 25-37 Fulltext: arXiv:1003.1907 - PDF; 10052_2010_1284_OnlinePDF - PDF; External link: Preprint
10.
Momentum measurement by the Multiple Coulomb Scattering method in the OPERA lead emulsion target / OPERA Collaboration
A new method of momentum measurement of charged particles through Multiple Coulomb Scattering (MCS) in the OPERA lead emulsion target is presented. It is based on precise measurements of track angular deviations performed thanks to the very high resolution of nuclear emulsions. [...]
arXiv:1106.6211.- 2012 - 15 p. - Published in : New J. Phys. 14 (2012) 013026 Fulltext: arXiv:1106.6211 - PDF; njp12_1_013026 - PDF; IOP Open Access article: PDF; External link: Preprint

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