Updated constraints on sterile neutrino mixing in the OPERA experiment using a new $\nu_e$ identification method,
N. Agafonova et al.,
PTEP 2023 (2023) 033C01,arXiv:2211.04636.
[OPERA:2022svg]
Final results on neutrino oscillation parameters from the OPERA experiment in the CNGS beam,
N. Agafonova et al.(OPERA),
Phys.Rev. D100 (2019) 051301,arXiv:1904.05686.
[OPERA:2019kzo]
Final results of the OPERA experiment on $\nu_\tau$ appearance in the CNGS beam,
N. Agafonova et al.(OPERA),
Phys.Rev.Lett. 120 (2018) 211801,arXiv:1804.04912.
[OPERA:2018nar]
Final results of the search for $\nu_\mu \to \nu_{e}$ oscillations with the OPERA detector in the CNGS beam,
N. Agafonova et al.(OPERA),
JHEP 06 (2018) 151,arXiv:1803.11400.
[OPERA:2018ksq]
Discovery of tau neutrino appearance in the CNGS neutrino beam with the OPERA experiment,
N. Agafonova et al.(OPERA),
Phys. Rev. Lett. 115 (2015) 121802,arXiv:1507.01417.
[OPERA:2015wbl]
Limits on muon-neutrino to tau-neutrino oscillations induced by a sterile neutrino state obtained by OPERA at the CNGS beam,
N. Agafonova et al.(OPERA),
JHEP 1506 (2015) 069,arXiv:1503.01876.
[OPERA:2015zci]
Observation of tau neutrino appearance in the CNGS beam with the OPERA experiment,
N. Agafonova et al.(OPERA),
PTEP 2014 (2014) 101C01,arXiv:1407.3513.
[OPERA:2014nnd]
Evidence for $\nu_\mu\to\nu_\tau$ appearance in the CNGS neutrino beam with the OPERA experiment,
N. Agafonova et al.(OPERA),
Phys. Rev. D89 (2014) 051102,arXiv:1401.2079.
[OPERA:2014fax]
New results on $\nu_\mu \to \nu_\tau$ appearance with the OPERA experiment in the CNGS beam,
N. Agafonova et al.(OPERA),
JHEP 1311 (2013) 036,arXiv:1308.2553.
[OPERA:2013tlg]
Search for $\nu_\mu\to\nu_e$ oscillations with the OPERA experiment in the CNGS beam,
N. Agafonova et al.(OPERA),
JHEP 1307 (2013) 004,arXiv:1303.3953.
[OPERA:2013wvp]
Search for $\nu_{\mu}\to\nu_{\tau}$ oscillation with the OPERA experiment in the CNGS beam,
N. Agafonova et al.(OPERA),
arXiv:1107.2594, 2011. [OPERA:2011oja]
Observation of a first $\nu_\tau$ candidate in the OPERA experiment in the CNGS beam,
N. Agafonova et al.(OPERA),
Phys. Lett. B691 (2012) 138-145,arXiv:1006.1623.
[Efthymiopoulos:2012wfa]
Measurement of the cosmic ray muon flux seasonal variation with the OPERA detector,
N. Agafonova et al.(OPERA),
JCAP 1910 (2019) 003,arXiv:1810.10783.
[OPERA:2018jif]
Measurement of TeV atmospheric muon charge ratio with the full OPERA data,
N. Agafonova et al.(OPERA),
Eur. Phys. J. C74 (2014) 2933,arXiv:1403.0244.
[OPERA:2014blf]
Measurement of the atmospheric muon charge ratio with the OPERA detector,
N. Agafonova et al.(OPERA),
Eur. Phys. J. C67 (2010) 25-37,arXiv:1003.1907.
[OPERA:2010cos]
First observation of a tau neutrino charged current interaction with charm production in the Opera experiment,
N. Agafonova et al.(OPERA),
Eur.Phys.J. C80 (2020) 699,arXiv:1912.11012.
[OPERA:2019soy]
Study of charged hadron multiplicities in charged-current neutrino-lead interactions in the OPERA detector,
N. Agafonova et al.(OPERA),
Eur.Phys.J. C78 (2018) 62,arXiv:1706.07930.
[OPERA:2017tas]
Study of neutrino interactions with the electronic detectors of the OPERA experiment,
N. Agafonova et al.(OPERA),
New J. Phys. 13 (2011) 053051,arXiv:1102.1882.
[OPERA:2011bgx]
The detection of neutrino interactions in the emulsion/lead target of the OPERA experiment,
N. Agafonova et al.(OPERA),
JINST 4 (2009) P06020,arXiv:0903.2973.
[Agafonova:2009kr]
Measurement of the neutrino velocity with the OPERA detector in the CNGS beam using the 2012 dedicated data,
T. Adam et al.(OPERA),
JHEP 01 (2013) 153,arXiv:1212.1276.
[OPERA:2012der]
The CNGS Neutrino Beam,
G. Giacomelli,
J. Phys. Conf. Ser. 116 (2008) 012004,arXiv:physics/0703247.
2nd Latin American School on Cosmic Rays and Astrophysics, Puebla, Mexico, 30th August - 8th September 2006. [Giacomelli:2007df]
The Angular Matching Method for the Muon Charge Sign Measurement in the OPERA Experiment,
N. Agafonova et al.(OPERA),
JINST 11 (2016) P07022,arXiv:1404.5933.
[OPERA:2014cdb]
Procedure for short-lived particle detection in the OPERA experiment and its application to charm decays,
N. Agafonova et al.(OPERA),
Eur.Phys.J. C74 (2014) 2986,arXiv:1404.4357.
[OPERA:2014fwn]
Momentum measurement by the Multiple Coulomb Scattering method in the OPERA lead emulsion target,
N. Agafonova et al.(OPERA),
New J. Phys. 14 (2012) 013026,arXiv:1106.6211.
[OPERA:2011aa]
First events from the CNGS neutrino beam detected in the OPERA experiment,
R. Acquafredda et al.(OPERA),
New J. Phys. 8 (2006) 303,arXiv:hep-ex/0611023.
[OPERA:2006oat]
The Nuclear Emulsion Technology and the Analysis of the OPERA Experiment Data,
Tsutomu Fukuda,
arXiv:0910.3274, 2009.DPF-2009, Detroit, MI, July 2009, eConf C090726. [Fukuda:2009mu]
The OPERA global readout and GPS distribution system,
J. Marteau(OPERA),
Nucl. Instrum. Meth. A617 (2010) 291-293,arXiv:0906.1494.
11th Pisa meeting on advanced detectors. [Marteau:2009ct]
Fast automated scanning of OPERA emulsion films,
G. Sirri,
Nucl. Phys. Proc. Suppl. 172 (2007) 324-326,arXiv:physics/0703068.
10th Topical Seminar on Innovative Particle and Radiation Detectors, 1-5 October 2006, Siena, Italy. [Sirri:2007hy]
The OPERA magnetic spectrometer,
M. Ambrosio et al.,
Ieee Trans. Nucl. Sci. 51 (2004) 975,arXiv:physics/0409137.
2003 IEEE-NSS conference, Portland, OR, USA, October 20-24, 2003. [Ambrosio:2004tm]
Sensitivity to $\vartheta_{13}$ of the CERN to Gran Sasso neutrino beam,
M. Komatsu, P. Migliozzi, F. Terranova,
J. Phys. G29 (2003) 443,arXiv:hep-ph/0210043. From the abstract:... a revised analysis of the OPERA $\nu_\mu \rightarrow \nu_e$ search is given. [Komatsu:2002sz]
OPERA: An appearance experiment to search for $\nu_\mu \to \nu_\tau$ oscillations in the CNGS beam. Experimental proposal,
M. Guler et al.(OPERA), 2000.CERN-SPSC-2000-028. [OPERA:2000zdf]
A long baseline $\nu_\tau$ appearance experiment in the CNGS beam from CERN to Gran Sasso. Progress report,
K. Kodama et al.(OPERA), 1999.CERN-SPSC-99-20. [OPERA:1999hzg]
Latest results of the OPERA experiment on nu-tau appearance in the CNGS neutrino beam,
N. Agafonova et al.(OPERA),
SciPost Phys.Proc. 1 (2019) 028,arXiv:1811.00095.
15th International Workshop on Tau Lepton Physics. [OPERA:2018fsq]
Results from the OPERA experiment,
Donato Di Ferdinando(OPERA),
arXiv:1608.01595, 2016.NuPhys2015 (London, 16-18 December 2015). [DiFerdinando:2016wbk]
Discovery of Tau Neutrino Appearance and Recent Results from OPERA,
T. Fukuda(OPERA),
Nuovo Cim. C39 (2017) 315,arXiv:1606.04632.
LaThuile2016, the XXXth Rencontres de Physique de la Vallee d'Aoste, March 6-12, 2016, La Thuile, Aosta Valley, Italy. [Fukuda:2016hfa]
A neutrino interaction with two vertices topology detected by OPERA,
Eduardo Medinaceli(OPERA),
arXiv:1604.08249, 2016.NuPhys2015 (London, 16-18 December 2015). [Medinaceli:2016vwh]
Search for Sterile Neutrinos at OPERA and other Long-Baseline Experiments,
Luca Stanco,
PoS EPS-HEP2015 (2016) 057,arXiv:1510.04151.
EPS2015, Vienna 22-29 July 2015. [Stanco:2015sua]
Opera Highlights,
Thomas Strauss(OPERA),
Acta Polytech. 53 (2013) 512-517,arXiv:1405.6847.
2012 Volcano Workshop: Frontier Objects in Astrophysics and Particle Physics. [Strauss:2013ivy]
Search for Neutrino Oscillations in Appearance Mode with the OPERA Experiment,
T. A. Dzhatdoev, V. L. Troshina(OPERA),
arXiv:1402.3861, 2014.HEPFT-2013. [Dzhatdoev:2014qsa]
Recent results of the OPERA experiment,
Fabio Pupilli(OPERA),
arXiv:1401.6776, 2014.14th ICATPP Conference, 23-27 September 2013, Villa Olmo - Como (Italy). [Pupilli:2014xua]
Study of Neutrino Oscillations in the OPERA Experiment,
Umut Kose(OPERA),
arXiv:1305.2513, 2013.Lake Louise Winter 2013 Conference, Banff, Alberta, Canada, 17-23 February 2013. [Kose:2013jca]
Search for $\nu_{\mu} \to \nu_{\tau}$ oscillations in appearance mode in the OPERA experiment,
Umut Kose,
arXiv:1106.3871, 2011.Les Rencontres de Physique de la Vallee D'Aoste (La Thuile, February 27-March 5 2011). [Kose:2011qw]
Search for $\nu_{\mu}\to\nu_{\tau}$ oscillations in appearance mode in the OPERA experiment,
L. S. Esposito(OPERA),
arXiv:1105.5239, 2011.WIN'11, Cape Town, South Africa, 31 January - 5 February 2011. [Esposito:2011as]
The OPERA experiment: a direct search of the $\nu_\mu \longrightarrow \nu_\tau$ oscillations,
J. Marteau,
arXiv:0910.3468, 2009.11th ICATPP Conference, Villa Olmo, Como, Italy, 5-9 October 2009. [Marteau:2009rj]
The OPERA experiment: on the way to the direct observation of $\nu_\mu \to \nu_\tau$ oscillation,
M. De Serio(OPERA),
arXiv:0910.0337, 2009.DPF-2009, Detroit, MI, July 2009. [DeSerio:2009vt]
The OPERA experiment: Preliminary results from the 2008 run,
Guillaume Lutter,
arXiv:0905.4521, 2009.Lake Louise Winter Institute 2009. [Lutter:2009ce]
OPERA: waiting for the tau,
Andrea Longhin(OPERA),
arXiv:0810.2664, 2008.XXVIII Physics in Collisions, Perugia, Italy, 25-28 June 2008. [Longhin:2008nf]
The OPERA Long Baseline Experiment: Status and First Results,
Dominique Duchesneau(OPERA),
arXiv:0810.2476, 2008.ICHEP08, Philadelphia, USA, July 2008. [Duchesneau:2008hj]
Observation of neutrino interactions in the OPERA detector,
Alberto Garfagnini, Ciro Pistillo,
Frascati Phys.Ser. 47 (2008) 121-132,arXiv:0805.3243.
[Garfagnini:2008bz]
OPERA first events from the CNGS neutrino beam,
J. Marteau(OPERA),
arXiv:0706.1699, 2007.XLIInd Rencontres de Moriond session, La Thuile, 10-17 March 2007. [Marteau:2007uf]
The Opera Experiment,
G. Giacomelli, M. Giorgini(OPERA),
arXiv:physics/0609045, 2006.Vulcano Workshop 2006, Frontier Objects in Astrophysics and Particle Physics, Vulcano, Italy, May 2006. [Giacomelli:2006xn]
Searching for neutrino oscillations with OPERA,
N. Savvinov(OPERA),
arXiv:hep-ex/0602010, 2006.XII Lomonosov conference on Elementary Particle Physics. [Savvinov:2006pb]
The OPERA experiment,
H. Pessard et al.(OPERA),
arXiv:hep-ex/0504033, 2005.32nd International Conference on High-Energy Physics (ICHEP 04), Beijing, China, 16-22 Aug 2004. [Pessard:2004kv]
OPERA experiment,
M. Komatsu,
Nucl. Instrum. Meth. A503 (2003) 124-126.3rd International Workshop on Neutrino Factory based on Muon Storage Rings (NuFACT'01), Tsukuba, Japan, 24-30 May 2001. [Komatsu:2003zn]
OPERA : A Search for $\nu_\mu \rightarrow \nu_\tau$ in the CNGS beam from CERN to Gran Sasso,
P. Strolin, 2002.Neutrinos to Gran Sasso, Padua University, 25 March 2002.http://www.pd.infn.it/~laveder/cngspd/trasparenze/Strolin.pdf.
[Strolin-Padova2002]
It is possible to perform a cross search between the various pages of Neutrino Unbound.
This is useful if you want to show the common elements that appear
in the listings of two (or more) different topics or experiments.