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262:. The detection principles of the two projects are very similar, although ANTARES only points toward the Southern Hemisphere. Thanks to its location in the Mediterranean Sea, ANTARES is more sensitive to neutrinos with energies below 100 TeV in the southern sky, a region that includes many galactic sources. ANTARES will detect neutrinos from high energy origin, particularly in the range from 10 to 10
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organisms. Results from these instruments, while also important for the calibration of the detector, will be shared with ocean science institutes involved in the ANTARES collaboration. While the ANTARES detector contains an acoustic positioning system for the alignment of the free-floating detector
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tubes. Each one has 75 optical modules and is about 350 meters long. They are anchored at the bottom of the sea at a depth of about 2.5 km, roughly 70 meters apart from each other. When neutrinos enter the southern hemisphere of the earth, they usually continue traveling directly through it.
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were deployed in 2005. The first string of photomultiplier tubes was moved into place in
February 2006. In September 2006 the second line was successfully connected. Lines 3, 4 and 5 were deployed at the end of 2006 and connected in January 2007. This was an important step that made Antares the
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from cosmic origins in the
Southern Hemisphere. Of particular interest would be the detection of astrophysical point sources of neutrinos, possibly in correlation with observations in other bands (such as gamma rays sources observed by the
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emitted as the muon passes through the water. The detection techniques used discriminate between the signature of "upward-going muons", a muon neutrino that has had interactions with matter below the detector (the
381:, which will comprise 6 converted ANTARES storeys with hydrophones to evaluate the possibility for acoustic detection of neutrinos in the deep sea. The first 3 of these acoustic storeys have been included in the
224:). Lines 6, 7, 8, 9, and 10 were deployed between March and early November 2007 and connected in December 2007 and January 2008. From May 2008 the detector has been running in its complete 12-line configuration.
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The construction of ANTARES was completed on May 30, 2008, two years after the first string was deployed. Initial testing began in 2000. Equipment indirectly related to the detector such as a
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Adrián-MartĂnez, S.; et al. (2014). "Searches for point-like and extended neutrino sources close to the galactic center using the ANTARES neutrino telescope".
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profilers and instrumentation for the measurement of light transmission and sound velocity. Also, a camera system has been installed for automatic tracking of
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Apart from this astro-particle physics aspect, the ANTARES telescope may also tackle some fundamental problems in particle physics, such as the search for
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Using 6 years of data, a search of the galactic center for point sources of neutrinos found none. Atmospheric neutrino oscillations were also measured.
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telescope, which are both in early design stages. The data taking of ANTARES was finished in
February 2022, after 16 years of continuous operation.
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In addition to the main optical detector for cosmic neutrinos, the ANTARES experiment also houses a number of instruments for the study of the
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Adrián-MartĂnez, S.; et al. (2012). "Measurement of atmospheric neutrino oscillations with the ANTARES neutrino telescope".
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that detects neutrinos from both hemispheres. The experiment is a recognized
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muon. ANTARES works by its photomultiplier tubes detecting the
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The array contains a set of twelve separate vertical strings of
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An artist illustration of the
Antares neutrino detector and the
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The first neutrino detections were reported in Feb 2007.
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309:being outside the energy range of ANTARES) or the
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472:. — The ANTARES Collaboration official web-site.
651:Neutrino detectors, experiments, and facilities
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116:from cosmic origins in the direction of the
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254:The ANTARES project complements the
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485:The Astrophysical Journal Letters
415:"Recognized Experiments at CERN"
385:, the other 3 on the 12th line.
449:The CERN Experimental Programme
97:residing 2.5 km under the
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419:The CERN Scientific Committees
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692:Lederman–Schwartz–Steinberger
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1431:List of neutrino experiments
256:IceCube Neutrino Observatory
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159:On rare occasions, a few
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205:bioluminescent organisms
203:-40 in the sea salt and
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421:. CERN. Archived from
235:, currently using the
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470:The ANTARES adventure
360:environment, such as
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1462:Particle experiments
746:Neutrino oscillation
383:instrumentation line
211:Construction history
183:neutrino telescopes
93:earch project) is a
1416:Kamioka Observatory
563:2012PhLB..714..224A
508:2014ApJ...786L...5A
179:In contrast to the
169:Cherenkov radiation
118:Southern Hemisphere
89:byss environmental
33: /
611:Record for ANTARES
335:magnetic monopoles
250:Experimental goals
139:telescope and the
63:For the star, see
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1452:Mediterranean Sea
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1173:Heidelberg-Moscow
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897:ICARUS (Fermilab)
540:Physics Letters B
101:off the coast of
99:Mediterranean Sea
95:neutrino detector
16:Neutrino Detector
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42:42.800; 6.167
1380:NEMO Project
1138:Double Chooz
1045:Construction
789:
777:Astronomical
665:Cowan–Reines
596:ANTARES home
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453:. Retrieved
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427:. Retrieved
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986:KamLAND-Zen
885:Accelerator
763:(divided by
658:Discoveries
615:INSPIRE-HEP
370:sea current
331:nuclearites
321:and at the
292:dark matter
231:institute,
217:seismometer
197:radioactive
165:high energy
40: /
1446:Categories
1203:Kamiokande
1158:Gargamelle
1062:Baikal-GVD
917:NA61/SHINE
902:MicroBooNE
455:21 January
429:21 January
401:References
296:neutralino
260:Antarctica
181:South Pole
1358:Cancelled
1178:Homestake
1128:Cuoricino
1092:SuperNEMO
912:MiniBooNE
761:Operating
554:1206.0645
499:1402.6182
492:(1): L5.
241:submarine
201:potassium
199:isotopes
1404:See also
1349:WATCHMAN
1299:JEM-EUSO
1282:Proposed
1268:Soudan 2
1258:SciBooNE
991:MAJORANA
941:Collider
861:Daya Bay
805:Borexino
767:neutrino
579:26970978
524:31685649
389:See also
368:probes,
362:salinity
358:deep sea
305:(normal
111:neutrino
81:eutrino
1329:Nucifer
1148:EXO-200
1101:Retired
1057:ARIANNA
953:SND@LHC
907:MINERνA
866:KamLAND
854:Reactor
820:IceCube
790:ANTARES
769:source)
765:primary
751:SN 1987
559:Bibcode
504:Bibcode
379:AMADEUS
341:Results
301:in the
285:Namibia
244:Nautile
233:IFREMER
189:IceCube
141:Italian
126:IceCube
120:of the
71:ANTARES
65:Antares
57:Nautile
25:42°48′N
1426:SNOLAB
1370:LAGUNA
1314:LEGEND
1233:MINOS+
1208:KARMEN
1183:ICARUS
1153:GALLEX
1108:AMANDA
1087:KM3NeT
1027:KATRIN
1001:PandaX
876:STEREO
736:τ
731:ν
709:μ
704:ν
677:ν
577:
522:
451:. CERN
366:oxygen
270:- 100
185:AMANDA
150:Design
137:NESTOR
107:France
103:Toulon
28:6°10′E
1395:BOREX
1334:P-ONE
1304:GRAND
1289:CUPID
1248:OPERA
1228:MINOS
1223:MACRO
1163:GERDA
1133:DONUT
1118:Chooz
1032:WITCH
1020:Other
1011:XMASS
981:CUORE
976:COBRA
971:AMoRE
948:FASER
892:ANNIE
845:SNEWS
830:NEVOD
800:BDUNT
785:ANITA
719:DONUT
575:S2CID
549:arXiv
520:S2CID
494:arXiv
395:P-ONE
174:Earth
134:Greek
122:Earth
1421:LNGS
1339:SBND
1319:LENA
1294:nEXO
1273:Utah
1253:RICE
1243:NEMO
1238:NARC
1218:LSND
1188:IGEX
1143:ERPM
1123:CNGS
1113:CDHS
1082:JUNO
1072:DUNE
1067:BEST
1006:SNO+
996:NEXT
963:0νββ
927:NuMI
922:NOvA
871:RENO
835:SAGE
815:HALO
810:BUST
457:2020
431:2020
364:and
319:CDMS
315:DAMA
281:HESS
276:flux
266:(10
187:and
161:muon
144:NEMO
130:CERN
114:flux
1390:SOX
1344:UNO
1309:INO
1263:SNO
1213:KGF
1198:K2K
1193:IMB
1168:GNO
1052:ARA
932:T2K
825:LVD
795:ASD
613:on
567:doi
545:714
512:doi
490:786
333:or
323:LHC
303:Sun
272:TeV
268:GeV
258:in
237:ROV
91:RES
1448::
573:.
565:.
557:.
543:.
518:.
510:.
502:.
488:.
447:.
417:.
337:.
317:,
246:.
105:,
742:)
721:(
715:)
694:(
688:)
682:e
667:(
643:e
636:t
629:v
581:.
569::
561::
551::
526:.
514::
506::
496::
459:.
433:.
87:A
83:T
79:N
75:A
73:(
67:.
59:.
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