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Time calibration with atmospheric muon tracks in the ANTARES neutrino telescope

The ANTARES experiment consists of an array of photomultipliers distributed along 12 lines and located deep underwater in the Mediterranean Sea. It searches for astrophysical neutrinos collecting the Cherenkov light induced by the charged particles, mainly muons, produced in neutrino interactions ar...

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Detalles Bibliográficos
Autores principales: Adrián-Martínez, S., Albert, A., André, M., Anton, G., Ardid, M., Aubert, J.-J., Baret, B., Barrios-Martí, J., Basa, S., Bertin, V., Biagi, S., Bogazzi, C., Bormuth, R., Bou-Cabo, M., Bouwhuis, M.C., Bruijn, R., Brunner, J., Busto, J., Capone, A., Caramete, L., Carr, J., Chiarusi, T., Circella, M., Coniglione, R., Costantini, H., Coyle, P., Creusot, A., Dekeyser, I., Deschamps, A., De Bonis, G., Distefano, C., Donzaud, C., Dornic, D., Drouhin, D., Dumas, A., Eberl, T., Elsässer, D., Enzenhöfer, A., Fehn, K., Felis, I., Fermani, P., Flaminio, V., Folger, F., Fusco, L.A., Galatà, S., Gay, P., Geißelsöder, S., Geyer, K., Giordano, V., Gleixner, A., Gracia-Ruiz, R., Gómez-González, J.P., Graf, K., van Haren, H., Heijboer, A.J., Hello, Y., Hernández-Rey, J.J., Herrero, A., Hößl, J., Hofestädt, J., Hugon, C., James, C.W., de Jong, M., Kadler, M., Kalekin, O., Katz, U., Kießling, D., Kooijman, P., Kouchner, A., Kreykenbohm, I., Kulikovskiy, V., Lahmann, R., Lambard, G., Lattuada, D., Lefèvre, D., Leonora, E., Loucatos, S., Mangano, S., Marcelin, M., Margiotta, A., Marinelli, A., Martínez-Mora, J.A., Martini, S., Mathieu, A., Michael, T., Migliozzi, P., Moussa, A., Mueller, C., Neff, M., Nezri, E., Păvălaş, G.E., Pellegrino, C., Perrina, C., Piattelli, P., Popa, V., Pradier, T., Racca, C., Riccobene, G., Richter, R., Roensch, K., Rostovtsev, A., Saldaña, M., Samtleben, D.F.E., Sánchez-Losa, A., Sanguineti, M., Sapienza, P., Schmid, J., Schnabel, J., Schulte, S., Schüssler, F., Seitz, T., Sieger, C., Spurio, M., Steijger, J.J.M., Stolarczyk, Th., Taiuti, M., Tamburini, C., Trovato, A., Tselengidou, M., Tönnis, C., Turpin, D., Vallage, B., Vallée, C., Van Elewyck, V., Visser, E., Vivolo, D., Wagner, S., Wilms, J., Zornoza, J.D., Zúñiga, J.
Lenguaje:eng
Publicado: 2015
Materias:
Acceso en línea:https://dx.doi.org/10.1016/j.astropartphys.2016.02.001
http://cds.cern.ch/record/2034613
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author Adrián-Martínez, S.
Albert, A.
André, M.
Anton, G.
Ardid, M.
Aubert, J.-J.
Baret, B.
Barrios-Martí, J.
Basa, S.
Bertin, V.
Biagi, S.
Bogazzi, C.
Bormuth, R.
Bou-Cabo, M.
Bouwhuis, M.C.
Bruijn, R.
Brunner, J.
Busto, J.
Capone, A.
Caramete, L.
Carr, J.
Chiarusi, T.
Circella, M.
Coniglione, R.
Costantini, H.
Coyle, P.
Creusot, A.
Dekeyser, I.
Deschamps, A.
De Bonis, G.
Distefano, C.
Donzaud, C.
Dornic, D.
Drouhin, D.
Dumas, A.
Eberl, T.
Elsässer, D.
Enzenhöfer, A.
Fehn, K.
Felis, I.
Fermani, P.
Flaminio, V.
Folger, F.
Fusco, L.A.
Galatà, S.
Gay, P.
Geißelsöder, S.
Geyer, K.
Giordano, V.
Gleixner, A.
Gracia-Ruiz, R.
Gómez-González, J.P.
Graf, K.
van Haren, H.
Heijboer, A.J.
Hello, Y.
Hernández-Rey, J.J.
Herrero, A.
Hößl, J.
Hofestädt, J.
Hugon, C.
James, C.W.
de Jong, M.
Kadler, M.
Kalekin, O.
Katz, U.
Kießling, D.
Kooijman, P.
Kouchner, A.
Kreykenbohm, I.
Kulikovskiy, V.
Lahmann, R.
Lambard, G.
Lattuada, D.
Lefèvre, D.
Leonora, E.
Loucatos, S.
Mangano, S.
Marcelin, M.
Margiotta, A.
Marinelli, A.
Martínez-Mora, J.A.
Martini, S.
Mathieu, A.
Michael, T.
Migliozzi, P.
Moussa, A.
Mueller, C.
Neff, M.
Nezri, E.
Păvălaş, G.E.
Pellegrino, C.
Perrina, C.
Piattelli, P.
Popa, V.
Pradier, T.
Racca, C.
Riccobene, G.
Richter, R.
Roensch, K.
Rostovtsev, A.
Saldaña, M.
Samtleben, D.F.E.
Sánchez-Losa, A.
Sanguineti, M.
Sapienza, P.
Schmid, J.
Schnabel, J.
Schulte, S.
Schüssler, F.
Seitz, T.
Sieger, C.
Spurio, M.
Steijger, J.J.M.
Stolarczyk, Th.
Taiuti, M.
Tamburini, C.
Trovato, A.
Tselengidou, M.
Tönnis, C.
Turpin, D.
Vallage, B.
Vallée, C.
Van Elewyck, V.
Visser, E.
Vivolo, D.
Wagner, S.
Wilms, J.
Zornoza, J.D.
Zúñiga, J.
author_facet Adrián-Martínez, S.
Albert, A.
André, M.
Anton, G.
Ardid, M.
Aubert, J.-J.
Baret, B.
Barrios-Martí, J.
Basa, S.
Bertin, V.
Biagi, S.
Bogazzi, C.
Bormuth, R.
Bou-Cabo, M.
Bouwhuis, M.C.
Bruijn, R.
Brunner, J.
Busto, J.
Capone, A.
Caramete, L.
Carr, J.
Chiarusi, T.
Circella, M.
Coniglione, R.
Costantini, H.
Coyle, P.
Creusot, A.
Dekeyser, I.
Deschamps, A.
De Bonis, G.
Distefano, C.
Donzaud, C.
Dornic, D.
Drouhin, D.
Dumas, A.
Eberl, T.
Elsässer, D.
Enzenhöfer, A.
Fehn, K.
Felis, I.
Fermani, P.
Flaminio, V.
Folger, F.
Fusco, L.A.
Galatà, S.
Gay, P.
Geißelsöder, S.
Geyer, K.
Giordano, V.
Gleixner, A.
Gracia-Ruiz, R.
Gómez-González, J.P.
Graf, K.
van Haren, H.
Heijboer, A.J.
Hello, Y.
Hernández-Rey, J.J.
Herrero, A.
Hößl, J.
Hofestädt, J.
Hugon, C.
James, C.W.
de Jong, M.
Kadler, M.
Kalekin, O.
Katz, U.
Kießling, D.
Kooijman, P.
Kouchner, A.
Kreykenbohm, I.
Kulikovskiy, V.
Lahmann, R.
Lambard, G.
Lattuada, D.
Lefèvre, D.
Leonora, E.
Loucatos, S.
Mangano, S.
Marcelin, M.
Margiotta, A.
Marinelli, A.
Martínez-Mora, J.A.
Martini, S.
Mathieu, A.
Michael, T.
Migliozzi, P.
Moussa, A.
Mueller, C.
Neff, M.
Nezri, E.
Păvălaş, G.E.
Pellegrino, C.
Perrina, C.
Piattelli, P.
Popa, V.
Pradier, T.
Racca, C.
Riccobene, G.
Richter, R.
Roensch, K.
Rostovtsev, A.
Saldaña, M.
Samtleben, D.F.E.
Sánchez-Losa, A.
Sanguineti, M.
Sapienza, P.
Schmid, J.
Schnabel, J.
Schulte, S.
Schüssler, F.
Seitz, T.
Sieger, C.
Spurio, M.
Steijger, J.J.M.
Stolarczyk, Th.
Taiuti, M.
Tamburini, C.
Trovato, A.
Tselengidou, M.
Tönnis, C.
Turpin, D.
Vallage, B.
Vallée, C.
Van Elewyck, V.
Visser, E.
Vivolo, D.
Wagner, S.
Wilms, J.
Zornoza, J.D.
Zúñiga, J.
author_sort Adrián-Martínez, S.
collection CERN
description The ANTARES experiment consists of an array of photomultipliers distributed along 12 lines and located deep underwater in the Mediterranean Sea. It searches for astrophysical neutrinos collecting the Cherenkov light induced by the charged particles, mainly muons, produced in neutrino interactions around the detector. Since at energies of $\sim$10 TeV the muon and the incident neutrino are almost collinear, it is possible to use the ANTARES detector as a neutrino telescope and identify a source of neutrinos in the sky starting from a precise reconstruction of the muon trajectory. To get this result, the arrival times of the Cherenkov photons must be accurately measured. A to perform time calibrations with the precision required to have optimal performances of the instrument is described. The reconstructed tracks of the atmospheric muons in the ANTARES detector are used to determine the relative time offsets between photomultipliers. Currently, this method is used to obtain the time calibration constants for photomultipliers on different lines at a precision level of 0.5 ns. It has also been validated for calibrating photomultipliers on the same line, using a system of LEDs and laser light devices.
id cern-2034613
institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2015
record_format invenio
spelling cern-20346132023-03-14T19:31:23Zdoi:10.1016/j.astropartphys.2016.02.001http://cds.cern.ch/record/2034613engAdrián-Martínez, S.Albert, A.André, M.Anton, G.Ardid, M.Aubert, J.-J.Baret, B.Barrios-Martí, J.Basa, S.Bertin, V.Biagi, S.Bogazzi, C.Bormuth, R.Bou-Cabo, M.Bouwhuis, M.C.Bruijn, R.Brunner, J.Busto, J.Capone, A.Caramete, L.Carr, J.Chiarusi, T.Circella, M.Coniglione, R.Costantini, H.Coyle, P.Creusot, A.Dekeyser, I.Deschamps, A.De Bonis, G.Distefano, C.Donzaud, C.Dornic, D.Drouhin, D.Dumas, A.Eberl, T.Elsässer, D.Enzenhöfer, A.Fehn, K.Felis, I.Fermani, P.Flaminio, V.Folger, F.Fusco, L.A.Galatà, S.Gay, P.Geißelsöder, S.Geyer, K.Giordano, V.Gleixner, A.Gracia-Ruiz, R.Gómez-González, J.P.Graf, K.van Haren, H.Heijboer, A.J.Hello, Y.Hernández-Rey, J.J.Herrero, A.Hößl, J.Hofestädt, J.Hugon, C.James, C.W.de Jong, M.Kadler, M.Kalekin, O.Katz, U.Kießling, D.Kooijman, P.Kouchner, A.Kreykenbohm, I.Kulikovskiy, V.Lahmann, R.Lambard, G.Lattuada, D.Lefèvre, D.Leonora, E.Loucatos, S.Mangano, S.Marcelin, M.Margiotta, A.Marinelli, A.Martínez-Mora, J.A.Martini, S.Mathieu, A.Michael, T.Migliozzi, P.Moussa, A.Mueller, C.Neff, M.Nezri, E.Păvălaş, G.E.Pellegrino, C.Perrina, C.Piattelli, P.Popa, V.Pradier, T.Racca, C.Riccobene, G.Richter, R.Roensch, K.Rostovtsev, A.Saldaña, M.Samtleben, D.F.E.Sánchez-Losa, A.Sanguineti, M.Sapienza, P.Schmid, J.Schnabel, J.Schulte, S.Schüssler, F.Seitz, T.Sieger, C.Spurio, M.Steijger, J.J.M.Stolarczyk, Th.Taiuti, M.Tamburini, C.Trovato, A.Tselengidou, M.Tönnis, C.Turpin, D.Vallage, B.Vallée, C.Van Elewyck, V.Visser, E.Vivolo, D.Wagner, S.Wilms, J.Zornoza, J.D.Zúñiga, J.Time calibration with atmospheric muon tracks in the ANTARES neutrino telescopeDetectors and Experimental TechniquesThe ANTARES experiment consists of an array of photomultipliers distributed along 12 lines and located deep underwater in the Mediterranean Sea. It searches for astrophysical neutrinos collecting the Cherenkov light induced by the charged particles, mainly muons, produced in neutrino interactions around the detector. Since at energies of $\sim$10 TeV the muon and the incident neutrino are almost collinear, it is possible to use the ANTARES detector as a neutrino telescope and identify a source of neutrinos in the sky starting from a precise reconstruction of the muon trajectory. To get this result, the arrival times of the Cherenkov photons must be accurately measured. A to perform time calibrations with the precision required to have optimal performances of the instrument is described. The reconstructed tracks of the atmospheric muons in the ANTARES detector are used to determine the relative time offsets between photomultipliers. Currently, this method is used to obtain the time calibration constants for photomultipliers on different lines at a precision level of 0.5 ns. It has also been validated for calibrating photomultipliers on the same line, using a system of LEDs and laser light devices.The ANTARES experiment consists of an array of photomultipliers distributed along 12 lines and located deep underwater in the Mediterranean Sea. It searches for astrophysical neutrinos collecting the Cherenkov light induced by the charged particles, mainly muons, produced in neutrino interactions around the detector. Since at energies of ∼10 TeV the muon and the incident neutrino are almost collinear, it is possible to use the ANTARES detector as a neutrino telescope and identify a source of neutrinos in the sky starting from a precise reconstruction of the muon trajectory. To get this result, the arrival times of the Cherenkov photons must be accurately measured. A to perform time calibrations with the precision required to have optimal performances of the instrument is described. The reconstructed tracks of the atmospheric muons in the ANTARES detector are used to determine the relative time offsets between photomultipliers. Currently, this method is used to obtain the time calibration constants for photomultipliers on different lines at a precision level of 0.5 ns. It has also been validated for calibrating photomultipliers on the same line, using a system of LEDs and laser light devices.The ANTARES experiment consists of an array of photomultipliers distributed along 12 lines and located deep underwater in the Mediterranean Sea. It searches for astrophysical neutrinos collecting the Cherenkov light induced by the charged particles, mainly muons, produced in neutrino interactions around the detector. Since at energies of $\sim$10 TeV the muon and the incident neutrino are almost collinear, it is possible to use the ANTARES detector as a neutrino telescope and identify a source of neutrinos in the sky starting from a precise reconstruction of the muon trajectory. To get this result, the arrival times of the Cherenkov photons must be accurately measured. A to perform time calibrations with the precision required to have optimal performances of the instrument is described. The reconstructed tracks of the atmospheric muons in the ANTARES detector are used to determine the relative time offsets between photomultipliers. Currently, this method is used to obtain the time calibration constants for photomultipliers on different lines at a precision level of 0.5 ns. It has also been validated for calibrating photomultipliers on the same line, using a system of LEDs and laser light devices.arXiv:1507.04182oai:cds.cern.ch:20346132015-07-15
spellingShingle Detectors and Experimental Techniques
Adrián-Martínez, S.
Albert, A.
André, M.
Anton, G.
Ardid, M.
Aubert, J.-J.
Baret, B.
Barrios-Martí, J.
Basa, S.
Bertin, V.
Biagi, S.
Bogazzi, C.
Bormuth, R.
Bou-Cabo, M.
Bouwhuis, M.C.
Bruijn, R.
Brunner, J.
Busto, J.
Capone, A.
Caramete, L.
Carr, J.
Chiarusi, T.
Circella, M.
Coniglione, R.
Costantini, H.
Coyle, P.
Creusot, A.
Dekeyser, I.
Deschamps, A.
De Bonis, G.
Distefano, C.
Donzaud, C.
Dornic, D.
Drouhin, D.
Dumas, A.
Eberl, T.
Elsässer, D.
Enzenhöfer, A.
Fehn, K.
Felis, I.
Fermani, P.
Flaminio, V.
Folger, F.
Fusco, L.A.
Galatà, S.
Gay, P.
Geißelsöder, S.
Geyer, K.
Giordano, V.
Gleixner, A.
Gracia-Ruiz, R.
Gómez-González, J.P.
Graf, K.
van Haren, H.
Heijboer, A.J.
Hello, Y.
Hernández-Rey, J.J.
Herrero, A.
Hößl, J.
Hofestädt, J.
Hugon, C.
James, C.W.
de Jong, M.
Kadler, M.
Kalekin, O.
Katz, U.
Kießling, D.
Kooijman, P.
Kouchner, A.
Kreykenbohm, I.
Kulikovskiy, V.
Lahmann, R.
Lambard, G.
Lattuada, D.
Lefèvre, D.
Leonora, E.
Loucatos, S.
Mangano, S.
Marcelin, M.
Margiotta, A.
Marinelli, A.
Martínez-Mora, J.A.
Martini, S.
Mathieu, A.
Michael, T.
Migliozzi, P.
Moussa, A.
Mueller, C.
Neff, M.
Nezri, E.
Păvălaş, G.E.
Pellegrino, C.
Perrina, C.
Piattelli, P.
Popa, V.
Pradier, T.
Racca, C.
Riccobene, G.
Richter, R.
Roensch, K.
Rostovtsev, A.
Saldaña, M.
Samtleben, D.F.E.
Sánchez-Losa, A.
Sanguineti, M.
Sapienza, P.
Schmid, J.
Schnabel, J.
Schulte, S.
Schüssler, F.
Seitz, T.
Sieger, C.
Spurio, M.
Steijger, J.J.M.
Stolarczyk, Th.
Taiuti, M.
Tamburini, C.
Trovato, A.
Tselengidou, M.
Tönnis, C.
Turpin, D.
Vallage, B.
Vallée, C.
Van Elewyck, V.
Visser, E.
Vivolo, D.
Wagner, S.
Wilms, J.
Zornoza, J.D.
Zúñiga, J.
Time calibration with atmospheric muon tracks in the ANTARES neutrino telescope
title Time calibration with atmospheric muon tracks in the ANTARES neutrino telescope
title_full Time calibration with atmospheric muon tracks in the ANTARES neutrino telescope
title_fullStr Time calibration with atmospheric muon tracks in the ANTARES neutrino telescope
title_full_unstemmed Time calibration with atmospheric muon tracks in the ANTARES neutrino telescope
title_short Time calibration with atmospheric muon tracks in the ANTARES neutrino telescope
title_sort time calibration with atmospheric muon tracks in the antares neutrino telescope
topic Detectors and Experimental Techniques
url https://dx.doi.org/10.1016/j.astropartphys.2016.02.001
http://cds.cern.ch/record/2034613
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AT kalekino timecalibrationwithatmosphericmuontracksintheantaresneutrinotelescope
AT katzu timecalibrationwithatmosphericmuontracksintheantaresneutrinotelescope
AT kießlingd timecalibrationwithatmosphericmuontracksintheantaresneutrinotelescope
AT kooijmanp timecalibrationwithatmosphericmuontracksintheantaresneutrinotelescope
AT kouchnera timecalibrationwithatmosphericmuontracksintheantaresneutrinotelescope
AT kreykenbohmi timecalibrationwithatmosphericmuontracksintheantaresneutrinotelescope
AT kulikovskiyv timecalibrationwithatmosphericmuontracksintheantaresneutrinotelescope
AT lahmannr timecalibrationwithatmosphericmuontracksintheantaresneutrinotelescope
AT lambardg timecalibrationwithatmosphericmuontracksintheantaresneutrinotelescope
AT lattuadad timecalibrationwithatmosphericmuontracksintheantaresneutrinotelescope
AT lefevred timecalibrationwithatmosphericmuontracksintheantaresneutrinotelescope
AT leonorae timecalibrationwithatmosphericmuontracksintheantaresneutrinotelescope
AT loucatoss timecalibrationwithatmosphericmuontracksintheantaresneutrinotelescope
AT manganos timecalibrationwithatmosphericmuontracksintheantaresneutrinotelescope
AT marcelinm timecalibrationwithatmosphericmuontracksintheantaresneutrinotelescope
AT margiottaa timecalibrationwithatmosphericmuontracksintheantaresneutrinotelescope
AT marinellia timecalibrationwithatmosphericmuontracksintheantaresneutrinotelescope
AT martinezmoraja timecalibrationwithatmosphericmuontracksintheantaresneutrinotelescope
AT martinis timecalibrationwithatmosphericmuontracksintheantaresneutrinotelescope
AT mathieua timecalibrationwithatmosphericmuontracksintheantaresneutrinotelescope
AT michaelt timecalibrationwithatmosphericmuontracksintheantaresneutrinotelescope
AT migliozzip timecalibrationwithatmosphericmuontracksintheantaresneutrinotelescope
AT moussaa timecalibrationwithatmosphericmuontracksintheantaresneutrinotelescope
AT muellerc timecalibrationwithatmosphericmuontracksintheantaresneutrinotelescope
AT neffm timecalibrationwithatmosphericmuontracksintheantaresneutrinotelescope
AT nezrie timecalibrationwithatmosphericmuontracksintheantaresneutrinotelescope
AT pavalasge timecalibrationwithatmosphericmuontracksintheantaresneutrinotelescope
AT pellegrinoc timecalibrationwithatmosphericmuontracksintheantaresneutrinotelescope
AT perrinac timecalibrationwithatmosphericmuontracksintheantaresneutrinotelescope
AT piattellip timecalibrationwithatmosphericmuontracksintheantaresneutrinotelescope
AT popav timecalibrationwithatmosphericmuontracksintheantaresneutrinotelescope
AT pradiert timecalibrationwithatmosphericmuontracksintheantaresneutrinotelescope
AT raccac timecalibrationwithatmosphericmuontracksintheantaresneutrinotelescope
AT riccobeneg timecalibrationwithatmosphericmuontracksintheantaresneutrinotelescope
AT richterr timecalibrationwithatmosphericmuontracksintheantaresneutrinotelescope
AT roenschk timecalibrationwithatmosphericmuontracksintheantaresneutrinotelescope
AT rostovtseva timecalibrationwithatmosphericmuontracksintheantaresneutrinotelescope
AT saldanam timecalibrationwithatmosphericmuontracksintheantaresneutrinotelescope
AT samtlebendfe timecalibrationwithatmosphericmuontracksintheantaresneutrinotelescope
AT sanchezlosaa timecalibrationwithatmosphericmuontracksintheantaresneutrinotelescope
AT sanguinetim timecalibrationwithatmosphericmuontracksintheantaresneutrinotelescope
AT sapienzap timecalibrationwithatmosphericmuontracksintheantaresneutrinotelescope
AT schmidj timecalibrationwithatmosphericmuontracksintheantaresneutrinotelescope
AT schnabelj timecalibrationwithatmosphericmuontracksintheantaresneutrinotelescope
AT schultes timecalibrationwithatmosphericmuontracksintheantaresneutrinotelescope
AT schusslerf timecalibrationwithatmosphericmuontracksintheantaresneutrinotelescope
AT seitzt timecalibrationwithatmosphericmuontracksintheantaresneutrinotelescope
AT siegerc timecalibrationwithatmosphericmuontracksintheantaresneutrinotelescope
AT spuriom timecalibrationwithatmosphericmuontracksintheantaresneutrinotelescope
AT steijgerjjm timecalibrationwithatmosphericmuontracksintheantaresneutrinotelescope
AT stolarczykth timecalibrationwithatmosphericmuontracksintheantaresneutrinotelescope
AT taiutim timecalibrationwithatmosphericmuontracksintheantaresneutrinotelescope
AT tamburinic timecalibrationwithatmosphericmuontracksintheantaresneutrinotelescope
AT trovatoa timecalibrationwithatmosphericmuontracksintheantaresneutrinotelescope
AT tselengidoum timecalibrationwithatmosphericmuontracksintheantaresneutrinotelescope
AT tonnisc timecalibrationwithatmosphericmuontracksintheantaresneutrinotelescope
AT turpind timecalibrationwithatmosphericmuontracksintheantaresneutrinotelescope
AT vallageb timecalibrationwithatmosphericmuontracksintheantaresneutrinotelescope
AT valleec timecalibrationwithatmosphericmuontracksintheantaresneutrinotelescope
AT vanelewyckv timecalibrationwithatmosphericmuontracksintheantaresneutrinotelescope
AT vissere timecalibrationwithatmosphericmuontracksintheantaresneutrinotelescope
AT vivolod timecalibrationwithatmosphericmuontracksintheantaresneutrinotelescope
AT wagners timecalibrationwithatmosphericmuontracksintheantaresneutrinotelescope
AT wilmsj timecalibrationwithatmosphericmuontracksintheantaresneutrinotelescope
AT zornozajd timecalibrationwithatmosphericmuontracksintheantaresneutrinotelescope
AT zunigaj timecalibrationwithatmosphericmuontracksintheantaresneutrinotelescope