First observation of the cosmic ray shadow of the Moon and the Sun with KM3NeT/ORCA

S. Aiello; A. Albert; S. Alves Garre; Z. Aly; A. Ambrosone; F. Ameli; M. Andre; M. Anghinolfi; M. Anguita; M. Ardid; S. Ardid; J. Aublin; C. Bagatelas; L. Bailly-Salins; B. Baret; S. Basegmez du Pree; Y. Becherini; M. Bendahman; F. Benfenati; E. Berbee; V. Bertin; S. Biagi; M. Boettcher; M. Bou Cabo; J. Boumaaza; M. Bouta; M. Bouwhuis; C. Bozza; H. BrÃÂ¢nzaş; R. Bruijn; J. Brunner; R. Bruno; E. Buis; R. Buompane; J. Busto; B. Caiffi; D. Calvo; S. Campion; A. Capone; F. Carenini; V. Carretero; P. Castaldi; S. Celli; L. Cerisy; M. Chabab; N. Chau; A. Chen; R. Cherkaoui El Moursli; S. Cherubini; Miroslav Filipovic; null et al

First observation of the cosmic ray shadow of the Moon and the Sun with KM3NeT/ORCA

S. Aiello, A. Albert, S. Alves Garre, Z. Aly, A. Ambrosone, F. Ameli, M. Andre, M. Anghinolfi, M. Anguita, M. Ardid, S. Ardid, J. Aublin, C. Bagatelas, L. Bailly-Salins, B. Baret, S. Basegmez du Pree, Y. Becherini, M. Bendahman, F. Benfenati, E. BerbeeV. Bertin, S. Biagi, M. Boettcher, M. Bou Cabo, J. Boumaaza, M. Bouta, M. Bouwhuis, C. Bozza, H. BrÃÂ¢nzaş, R. Bruijn, J. Brunner, R. Bruno, E. Buis, R. Buompane, J. Busto, B. Caiffi, D. Calvo, S. Campion, A. Capone, F. Carenini, V. Carretero, P. Castaldi, S. Celli, L. Cerisy, M. Chabab, N. Chau, A. Chen, R. Cherkaoui El Moursli, S. Cherubini, Miroslav Filipovic, et al

Western Sydney University

Research output: Contribution to journal › Article › peer-review

10 Citations (Scopus)

Abstract

This article reports the first observation of the Moon and the Sun shadows in the sky distribution of cosmic-ray induced muons measured by the KM3NeT/ORCA detector. The analysed data-taking period spans from February 2020 to November 2021, when the detector had 6 Detection Units deployed at the bottom of the Mediterranean Sea, each composed of 18 Digital Optical Modules. The shadows induced by the Moon and the Sun were detected at their nominal position with a statistical significance of 4.2 Ïƒ and 6.2 Ïƒ , and an angular resolution of Ïƒres= 0. 49 âˆ˜ and Ïƒres= 0. 66 âˆ˜ , respectively, consistent with the prediction of 0. 53 âˆ˜ from simulations. This early result confirms the effectiveness of the detector calibration, in time, position and orientation and the accuracy of the event direction reconstruction. This also demonstrates the performance and the competitiveness of the detector in terms of pointing accuracy and angular resolution.

Original language	English
Article number	344
Number of pages	9
Journal	European Physical Journal C
Volume	83
Issue number	4
Publication status	Published - Apr 2023

Bibliographical note

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© 2023, The Author(s).

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Notes

WIP in RD

Cite this

Aiello, S., Albert, A., Alves Garre, S., Aly, Z., Ambrosone, A., Ameli, F., Andre, M., Anghinolfi, M., Anguita, M., Ardid, M., Ardid, S., Aublin, J., Bagatelas, C., Bailly-Salins, L., Baret, B., Basegmez du Pree, S., Becherini, Y., Bendahman, M., Benfenati, F., ... et al (2023). First observation of the cosmic ray shadow of the Moon and the Sun with KM3NeT/ORCA. European Physical Journal C, 83(4), Article 344.

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title = "First observation of the cosmic ray shadow of the Moon and the Sun with KM3NeT/ORCA",

abstract = "This article reports the first observation of the Moon and the Sun shadows in the sky distribution of cosmic-ray induced muons measured by the KM3NeT/ORCA detector. The analysed data-taking period spans from February 2020 to November 2021, when the detector had 6 Detection Units deployed at the bottom of the Mediterranean Sea, each composed of 18 Digital Optical Modules. The shadows induced by the Moon and the Sun were detected at their nominal position with a statistical significance of 4.2 {\"I}ƒ and 6.2 {\"I}ƒ , and an angular resolution of {\"I}ƒres= 0. 49 {\^a}ˆ˜ and {\"I}ƒres= 0. 66 {\^a}ˆ˜ , respectively, consistent with the prediction of 0. 53 {\^a}ˆ˜ from simulations. This early result confirms the effectiveness of the detector calibration, in time, position and orientation and the accuracy of the event direction reconstruction. This also demonstrates the performance and the competitiveness of the detector in terms of pointing accuracy and angular resolution.",

author = "S. Aiello and A. Albert and {Alves Garre}, S. and Z. Aly and A. Ambrosone and F. Ameli and M. Andre and M. Anghinolfi and M. Anguita and M. Ardid and S. Ardid and J. Aublin and C. Bagatelas and L. Bailly-Salins and B. Baret and {Basegmez du Pree}, S. and Y. Becherini and M. Bendahman and F. Benfenati and E. Berbee and V. Bertin and S. Biagi and M. Boettcher and {Bou Cabo}, M. and J. Boumaaza and M. Bouta and M. Bouwhuis and C. Bozza and H. Br{\~A}{\^A}¢nza{\c s} and R. Bruijn and J. Brunner and R. Bruno and E. Buis and R. Buompane and J. Busto and B. Caiffi and D. Calvo and S. Campion and A. Capone and F. Carenini and V. Carretero and P. Castaldi and S. Celli and L. Cerisy and M. Chabab and N. Chau and A. Chen and {Cherkaoui El Moursli}, R. and S. Cherubini and Miroslav Filipovic and {et al}",

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Aiello, S, Albert, A, Alves Garre, S, Aly, Z, Ambrosone, A, Ameli, F, Andre, M, Anghinolfi, M, Anguita, M, Ardid, M, Ardid, S, Aublin, J, Bagatelas, C, Bailly-Salins, L, Baret, B, Basegmez du Pree, S, Becherini, Y, Bendahman, M, Benfenati, F, Berbee, E, Bertin, V, Biagi, S, Boettcher, M, Bou Cabo, M, Boumaaza, J, Bouta, M, Bouwhuis, M, Bozza, C, BrÃÂ¢nzaş, H, Bruijn, R, Brunner, J, Bruno, R, Buis, E, Buompane, R, Busto, J, Caiffi, B, Calvo, D, Campion, S, Capone, A, Carenini, F, Carretero, V, Castaldi, P, Celli, S, Cerisy, L, Chabab, M, Chau, N, Chen, A, Cherkaoui El Moursli, R, Cherubini, S, Filipovic, M & et al 2023, 'First observation of the cosmic ray shadow of the Moon and the Sun with KM3NeT/ORCA', European Physical Journal C, vol. 83, no. 4, 344.

TY - JOUR

T1 - First observation of the cosmic ray shadow of the Moon and the Sun with KM3NeT/ORCA

AU - Aiello, S.

AU - Albert, A.

AU - Alves Garre, S.

AU - Aly, Z.

AU - Ambrosone, A.

AU - Ameli, F.

AU - Andre, M.

AU - Anghinolfi, M.

AU - Anguita, M.

AU - Ardid, M.

AU - Ardid, S.

AU - Aublin, J.

AU - Bagatelas, C.

AU - Bailly-Salins, L.

AU - Baret, B.

AU - Basegmez du Pree, S.

AU - Becherini, Y.

AU - Bendahman, M.

AU - Benfenati, F.

AU - Berbee, E.

AU - Bertin, V.

AU - Biagi, S.

AU - Boettcher, M.

AU - Bou Cabo, M.

AU - Boumaaza, J.

AU - Bouta, M.

AU - Bouwhuis, M.

AU - Bozza, C.

AU - BrÃÂ¢nzaş, H.

AU - Bruijn, R.

AU - Brunner, J.

AU - Bruno, R.

AU - Buis, E.

AU - Buompane, R.

AU - Busto, J.

AU - Caiffi, B.

AU - Calvo, D.

AU - Campion, S.

AU - Capone, A.

AU - Carenini, F.

AU - Carretero, V.

AU - Castaldi, P.

AU - Celli, S.

AU - Cerisy, L.

AU - Chabab, M.

AU - Chau, N.

AU - Chen, A.

AU - Cherkaoui El Moursli, R.

AU - Cherubini, S.

AU - Filipovic, Miroslav

AU - et al, null

PY - 2023/4

Y1 - 2023/4

N2 - This article reports the first observation of the Moon and the Sun shadows in the sky distribution of cosmic-ray induced muons measured by the KM3NeT/ORCA detector. The analysed data-taking period spans from February 2020 to November 2021, when the detector had 6 Detection Units deployed at the bottom of the Mediterranean Sea, each composed of 18 Digital Optical Modules. The shadows induced by the Moon and the Sun were detected at their nominal position with a statistical significance of 4.2 Ïƒ and 6.2 Ïƒ , and an angular resolution of Ïƒres= 0. 49 âˆ˜ and Ïƒres= 0. 66 âˆ˜ , respectively, consistent with the prediction of 0. 53 âˆ˜ from simulations. This early result confirms the effectiveness of the detector calibration, in time, position and orientation and the accuracy of the event direction reconstruction. This also demonstrates the performance and the competitiveness of the detector in terms of pointing accuracy and angular resolution.

AB - This article reports the first observation of the Moon and the Sun shadows in the sky distribution of cosmic-ray induced muons measured by the KM3NeT/ORCA detector. The analysed data-taking period spans from February 2020 to November 2021, when the detector had 6 Detection Units deployed at the bottom of the Mediterranean Sea, each composed of 18 Digital Optical Modules. The shadows induced by the Moon and the Sun were detected at their nominal position with a statistical significance of 4.2 Ïƒ and 6.2 Ïƒ , and an angular resolution of Ïƒres= 0. 49 âˆ˜ and Ïƒres= 0. 66 âˆ˜ , respectively, consistent with the prediction of 0. 53 âˆ˜ from simulations. This early result confirms the effectiveness of the detector calibration, in time, position and orientation and the accuracy of the event direction reconstruction. This also demonstrates the performance and the competitiveness of the detector in terms of pointing accuracy and angular resolution.

UR - https://hdl.handle.net/1959.7/uws:72004

UR - http://www.scopus.com/inward/record.url?scp=85156205426&partnerID=8YFLogxK

M3 - Article

SN - 1434-6044

VL - 83

JO - European Physical Journal C

JF - European Physical Journal C

IS - 4

M1 - 344

ER -

First observation of the cosmic ray shadow of the Moon and the Sun with KM3NeT/ORCA

Abstract

Bibliographical note

Open Access - Access Right Statement

Notes

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