The ANTARES detector

[0710.0527] The ANTARES detector background sources and

Oct 02,2007 The ANTARES detector#0183;The ANTARES Collaboration is deploying a large neutrino detector at a depth of 2475 m in the Mediterranean Sea,40 km off shore from La Seyne-sur-Mer in South France.The construction of this 12-line detector with 75 phototubes per line will be completed early 2008.Data taking has begun since April 2005 with an instrumentation line also equipped with optical modules.The first 5 detector Why Scientists Sank a Telescope Into the Deepest Parts of Dec 19,2016 The ANTARES detector#0183;An illustration of the Antares neutrino detector.Fran The ANTARES detector#231;ois Montanet/CC BY-SA 2.0 FR.In 2006,scientists working on the ANTARES neutrino telescope found themselves facing aThe positioning system of the ANTARES NeutrinoThe ANTARES detector consists of 885 optical modules arranged in a three dimensional array over twelve detection lines.The inter-line spacing is 60-70m.Typi-cally,the lines have a height of about 450m and carry 25 storeys.Each storey is a support structure

The Antares detector - ScienceDirect

Aug 01,2013 The ANTARES detector#0183;1.Introduction.The Antares telescope is a large area water Cherenkov detector meant to perform neutrino Astronomy in the deep Mediterranean sea.Among many other considerations,the detector has been designed to be efficient to the detection of neutrinos emitted by high energy sources such as active galactic nuclei,gamma ray bursts,micro-quasars or supernova remnants.The Antares detector - NASA/ADSAug 01,2013 The ANTARES detector#0183;The Antares detector Creusot,A.Abstract.The Antares Neutrino Telescope is the first operational Neutrino Telescope in the Mediterranean Sea.It has been completed in May 2008 and is meant to perform neutrino astronomy via a large three-dimensional array of photo-multiplier tubes.This note describes the design,the construction and the The Antares And Km3Net Neutrino Telescopes Status And The ANTARES detector has been operating continuously since 2007 in the Mediterranean Sea,demonstrating the feasibility of an undersea neutrino telescope.It

The Antares And Km3Net Neutrino Telescopes Status And

The ANTARES detector has been operating continuously since 2007 in the Mediterranean Sea,demonstrating the feasibility of an undersea neutrino telescope.ItThe ANTARES detector background sources and effectsS.Escoffier,ANTARES background sources and effects ICRC 07,Merida Standard trigger Old trigger N local coincidences anywhere inside the detector For N=5,accidental trigger rate increases as f 10 Problem Online Data filter Level 1 Trigger (L1) Look for local coincidences (2/3 OMs in the same storey) or Charge The ANTARES detectorgt; 3 p.e.on a The ANTARES detector background sources and effectsS.Escoffier,ANTARES background sources and effects ICRC 07,Merida Standard trigger Old trigger N local coincidences anywhere inside the detector For N=5,accidental trigger rate increases as f 10 Problem Online Data filter Level 1 Trigger (L1) Look for local coincidences (2/3 OMs in the same storey) or Charge The ANTARES detectorgt; 3 p.e.on a

The ANTARES detector background sources and effects

30TH INTERNATIONAL COSMIC RAY CONFERENCE The ANTARES detector background sources and effects on detector performance S.ESCOFFIER1 ON BEHALF OF THE ANTARES COLLABORATION 1Centre de Physique des Particules de Marseille,CNRS/IN2P3 163,av.de Luminy,Case 902,13288 Marseille Cedex 09,FranceThe ANTARES Detector Electronics and Readout30TH INTERNATIONAL COSMIC RAY CONFERENCE The ANTARES Detector Electronics and Readout M.CIRCELLA1 ON BEHALF OF THE ANTARES COLLABORATION 1Istituto Nazionale di Fisica Nucleare (INFN) Sezione di Bari,via Amendola 173,I-70126 Bari,Italy [email protected] Abstract ANTARES is a large volume,deep-sea neutrino telescope currently under construction offThe ANTARES Detector Electronics and Readout - COREThe ANTARES Detector Electronics and Readout .By M.Circella and for the ANTARES Collaboration.Abstract.In this paper,we illustrate the main features of the electronics and data acquisition systems of the ANTARES apparatus,a large volume,deep-sea neutrino telescope under construction in the Mediterranean Sea off the coast of Toulon

Some results are removed in response to a notice of local law requirement.For more information,please see here.Previous123456Next(PDF) The ANTARES detector Annarita Margiotta -

Academia.edu is a platform for academics to share research papers.Some results are removed in response to a notice of local law requirement.For more information,please see here.12345Next[0710.0527] The ANTARES detector background sourcesOct 02,2007 The ANTARES detector#0183;The ANTARES Collaboration is deploying a large neutrino detector at a depth of 2475 m in the Mediterranean Sea,40 km off shore from La Seyne-sur-Mer in South France.The construction of this 12-line detector with 75 phototubes per line will be completed early 2008.Data taking has begun since April 2005 with an instrumentation line also equipped with optical modules.The first 5 detector Some results are removed in response to a notice of local law requirement.For more information,please see here.

Search for Exotic Physics with the ANTARES Detector

THE ANTARES DETECTOR The ANTARES detector has reached its nominal size in May 2008.The 884 Optical Modules (OM) are deployed on twelve vertical lines in the Western Mediterranean,at depths between 2050 and 2400 meters.The OMs,consisting of a glass sphere housing a 10 Hamamatsu photomultiplier (PMT) [1],are arranged by triplet per storey Register - AntaresAuto-Tune Pro,Auto-Tune Artist,Auto-Tune EFX+,Auto-Tune Access and Auto-Key all use WIBU Codemeter for authorization.These plugins do not require a hardware key,and can be activated using AntaresNeutrino astrophysics with the ANTARES Cherenkov detector Nov 13,2013 The ANTARES detector#0183;The ANTARES neutrino telescope is currently the largest operating water Cherenkov detector and the largest neutrino detector in the Northern Hemisphere.The detector array consists of 12 detector lines holding a total of 885 Optical Modules and is located in the Mediterranean Sea at a depth of about 2500 m.Its scientific target is the detection of ultra-high energy cosmic neutrinos

Neutrino Telescope Is Born On The Floor Of The

Apr 08,2006 The ANTARES detector#0183;The Antares telescope is a neutrino detector which has two main goals high-energy astronomy and the search for dark matter.Neutrinos hardly interact with matter at all.Detector design - ANTARESSchematic of the detector at the Antares site Arrangement of the twelve lines on the sea bed The basic unit of the detector is the optical module,consisting of a photomultiplier tube,various sensors,and the associated electronics,housed in a pressure-resistant glass sphere.Detector design - ANTARESSchematic of the detector at the Antares site Arrangement of the twelve lines on the sea bed The basic unit of the detector is the optical module,consisting of a photomultiplier tube,various sensors,and the associated electronics,housed in a pressure-resistant glass sphere.

Cited by 7Publish Year 2009Author Annarita MargiottaImages of the ANTARES detector

imagesThe ANTARES Detector SpringerLinkJun 23,2015 The ANTARES detector#0183;The ANTARES 1 detector (Ageron et al.2011) is a pilot project to demonstrate that underwater neutrino telescopes are feasible and that they can operate for several years in the sea water at great depths.The ANTARES detector is located near Toulon,France.The coordinates are \(42^\circ 50'\) N and \(6^\circ 10'\) E.Its location makes it sensitive to a large part of the southern sky Cited by 2Publish Year 2007Author S.EscoffierAntares Auto-Key The Automatic Key Detection Plug-InThe Auto-Key automatic key detection plug-in detects the song key of any audio file and effortlessly sends those parameters to all instances of Auto-Tune in a DAW with a single button click.It significantly improves music production workflow for producers,songwritersCited by 1Publish Year 2013Author A.CreusotThe ANTARES detector - ScienceDirectMay 01,2009 The ANTARES detector#0183;The ANTARES collaboration concluded the construction of a high energy neutrino telescope under the Mediterranean Sea,40 km off the French coast.The complete detector is a 3-dimensional array of 12 lines equipped with 900 photomultipliers,installed at a depth of 2475 m.

Cited by 1Publish Year 2013Author A.CreusotThe ANTARES Detector Electronics and Readout - NASA/ADS

The ANTARES collaboration is building an underwater neutrino telescope at 2500 m depth in the Mediterranean Sea.The experiment aims to detect high- energy cosmic neutrinos using a 3D array of 900 photomultipliers distributed along 12 lines.5 such lines have been operational since January 2007.The PMTs collect the Cherenkov light induced by neutrino-produced charged particles in the water.Cited by 1Publish Year 2008Author M.CircellaDetector design - ANTARESSchematic of the detector at the Antares site Arrangement of the twelve lines on the sea bed The basic unit of the detector is the optical module,consisting of a photomultiplier tube,various sensors,and the associated electronics,housed in a pressure-resistant glass sphere.Author Vladimir KulikovskiyPublish Year 2015(PDF) The Antares DetectorANTARES consists of a three-dimensional array of photosensitive devices that measure Cherenkov light induced by charged particles produced by high energy neutrinos interacting in the detector

Author Annarita MargiottaTHE ANTARES DETECTOR The Identification of Dark Matter

The ANTARES Collaboration is building an underwater neutrino telescope in the Mediterranean Sea,at a depth of 2500 m,40 km offshore from Toulon (France).The main goal of the detector is the search for high energy neutrinos from possible Galactic and extra-Galactic sources as well as from the decay of neutralinos and other exotic particles.Acoustic Particle Detection with the ANTARES Detector Mar 18,2010 The ANTARES detector#0183;The (Antares Modules for Acoustic Detection Under the Sea) AMADEUS system within the (Astronomy with a Neutrino Telescope and Abyss environmental RESsearch) ANTARES neutrino telescope is designed to investigate detection techniques for acoustic signals produced by particle cascades.While passing through a liquid a cascade deposits energy and produces a measurableAcoustic Particle Detection with the ANTARES Detector The ANTARES detector#0183;The ANTARES detector is deployed 40 km offshore from Toulon,France (\(42^\circ 48'\hbox {N}\),\(6^\circ 10'\hbox {E}\)) anchored at a depth of about 2475 m.The telescope detects the Cherenkov light stimulated in the medium by relativistic particles by means of a three dimensional grid of optical modules (OMs),pressure resistant glass spheres each containing one \(10^{\prime \prime

ANTARES home page

Click on the ANTARES logo at any time to come back to this page .Original design Th.S.Background picture Stars at the Galactic Center from the Spitzer Space Telescope's infrared cameras - Image Credit NASA,JPL-Caltech,Susan Stolovy (SSC/Caltech) et al.Antares undersea view,Credit (PDF) The ANTARES detector background sources andThe ANTARES Collaboration is deploying a large neutrino detector at a depth of 2475 m in the Mediterranean Sea,40 km off shore from La Seyne-sur-Mer in South France.

[0710.0527] The ANTARES detector background sources and

Oct 02,2007 The ANTARES detector#0183;The ANTARES Collaboration is deploying a large neutrino detector at a depth of 2475 m in the Mediterranean Sea,40 km off shore from La Seyne-sur-Mer in South France.The construction of this 12-line detector with 75 phototubes per line will be completed early 2008.Data taking has begun since April 2005 with an instrumentation line also equipped with optical modules.The first 5 detector Why Scientists Sank a Telescope Into the Deepest Parts of Dec 19,2016 The ANTARES detector#0183;An illustration of the Antares neutrino detector.Fran The ANTARES detector#231;ois Montanet/CC BY-SA 2.0 FR.In 2006,scientists working on the ANTARES neutrino telescope found themselves facing aThe positioning system of the ANTARES NeutrinoThe ANTARES detector consists of 885 optical modules arranged in a three dimensional array over twelve detection lines.The inter-line spacing is 60-70m.Typi-cally,the lines have a height of about 450m and carry 25 storeys.Each storey is a support structure

The Antares detector - ScienceDirect

Aug 01,2013 The ANTARES detector#0183;1.Introduction.The Antares telescope is a large area water Cherenkov detector meant to perform neutrino Astronomy in the deep Mediterranean sea.Among many other considerations,the detector has been designed to be efficient to the detection of neutrinos emitted by high energy sources such as active galactic nuclei,gamma ray bursts,micro-quasars or supernova remnants.The Antares detector - NASA/ADSAug 01,2013 The ANTARES detector#0183;The Antares detector Creusot,A.Abstract.The Antares Neutrino Telescope is the first operational Neutrino Telescope in the Mediterranean Sea.It has been completed in May 2008 and is meant to perform neutrino astronomy via a large three-dimensional array of photo-multiplier tubes.This note describes the design,the construction and the The Antares And Km3Net Neutrino Telescopes Status And The ANTARES detector has been operating continuously since 2007 in the Mediterranean Sea,demonstrating the feasibility of an undersea neutrino telescope.It

The Antares And Km3Net Neutrino Telescopes Status And

The ANTARES detector has been operating continuously since 2007 in the Mediterranean Sea,demonstrating the feasibility of an undersea neutrino telescope.ItThe ANTARES detector background sources and effectsS.Escoffier,ANTARES background sources and effects ICRC 07,Merida Standard trigger Old trigger N local coincidences anywhere inside the detector For N=5,accidental trigger rate increases as f 10 Problem Online Data filter Level 1 Trigger (L1) Look for local coincidences (2/3 OMs in the same storey) or Charge The ANTARES detectorgt; 3 p.e.on a The ANTARES detector background sources and effectsS.Escoffier,ANTARES background sources and effects ICRC 07,Merida Standard trigger Old trigger N local coincidences anywhere inside the detector For N=5,accidental trigger rate increases as f 10 Problem Online Data filter Level 1 Trigger (L1) Look for local coincidences (2/3 OMs in the same storey) or Charge The ANTARES detectorgt; 3 p.e.on a

The ANTARES detector background sources and effects

30TH INTERNATIONAL COSMIC RAY CONFERENCE The ANTARES detector background sources and effects on detector performance S.ESCOFFIER1 ON BEHALF OF THE ANTARES COLLABORATION 1Centre de Physique des Particules de Marseille,CNRS/IN2P3 163,av.de Luminy,Case 902,13288 Marseille Cedex 09,FranceThe ANTARES Detector Electronics and Readout30TH INTERNATIONAL COSMIC RAY CONFERENCE The ANTARES Detector Electronics and Readout M.CIRCELLA1 ON BEHALF OF THE ANTARES COLLABORATION 1Istituto Nazionale di Fisica Nucleare (INFN) Sezione di Bari,via Amendola 173,I-70126 Bari,Italy [email protected] Abstract ANTARES is a large volume,deep-sea neutrino telescope currently under construction offThe ANTARES Detector Electronics and Readout - COREThe ANTARES Detector Electronics and Readout .By M.Circella and for the ANTARES Collaboration.Abstract.In this paper,we illustrate the main features of the electronics and data acquisition systems of the ANTARES apparatus,a large volume,deep-sea neutrino telescope under construction in the Mediterranean Sea off the coast of Toulon

Some results are removed in response to a notice of local law requirement.For more information,please see here.Previous123456Next(PDF) The ANTARES detector Annarita Margiotta -

Academia.edu is a platform for academics to share research papers.Some results are removed in response to a notice of local law requirement.For more information,please see here.12345Next[0710.0527] The ANTARES detector background sourcesOct 02,2007 The ANTARES detector#0183;The ANTARES Collaboration is deploying a large neutrino detector at a depth of 2475 m in the Mediterranean Sea,40 km off shore from La Seyne-sur-Mer in South France.The construction of this 12-line detector with 75 phototubes per line will be completed early 2008.Data taking has begun since April 2005 with an instrumentation line also equipped with optical modules.The first 5 detector Some results are removed in response to a notice of local law requirement.For more information,please see here.

Search for Exotic Physics with the ANTARES Detector

THE ANTARES DETECTOR The ANTARES detector has reached its nominal size in May 2008.The 884 Optical Modules (OM) are deployed on twelve vertical lines in the Western Mediterranean,at depths between 2050 and 2400 meters.The OMs,consisting of a glass sphere housing a 10 Hamamatsu photomultiplier (PMT) [1],are arranged by triplet per storey Register - AntaresAuto-Tune Pro,Auto-Tune Artist,Auto-Tune EFX+,Auto-Tune Access and Auto-Key all use WIBU Codemeter for authorization.These plugins do not require a hardware key,and can be activated using AntaresNeutrino astrophysics with the ANTARES Cherenkov detector Nov 13,2013 The ANTARES detector#0183;The ANTARES neutrino telescope is currently the largest operating water Cherenkov detector and the largest neutrino detector in the Northern Hemisphere.The detector array consists of 12 detector lines holding a total of 885 Optical Modules and is located in the Mediterranean Sea at a depth of about 2500 m.Its scientific target is the detection of ultra-high energy cosmic neutrinos

Neutrino Telescope Is Born On The Floor Of The

Apr 08,2006 The ANTARES detector#0183;The Antares telescope is a neutrino detector which has two main goals high-energy astronomy and the search for dark matter.Neutrinos hardly interact with matter at all.Detector design - ANTARESSchematic of the detector at the Antares site Arrangement of the twelve lines on the sea bed The basic unit of the detector is the optical module,consisting of a photomultiplier tube,various sensors,and the associated electronics,housed in a pressure-resistant glass sphere.Detector design - ANTARESSchematic of the detector at the Antares site Arrangement of the twelve lines on the sea bed The basic unit of the detector is the optical module,consisting of a photomultiplier tube,various sensors,and the associated electronics,housed in a pressure-resistant glass sphere.

Cited by 7Publish Year 2009Author Annarita MargiottaImages of the ANTARES detector

imagesThe ANTARES Detector SpringerLinkJun 23,2015 The ANTARES detector#0183;The ANTARES 1 detector (Ageron et al.2011) is a pilot project to demonstrate that underwater neutrino telescopes are feasible and that they can operate for several years in the sea water at great depths.The ANTARES detector is located near Toulon,France.The coordinates are \(42^\circ 50'\) N and \(6^\circ 10'\) E.Its location makes it sensitive to a large part of the southern sky Cited by 2Publish Year 2007Author S.EscoffierAntares Auto-Key The Automatic Key Detection Plug-InThe Auto-Key automatic key detection plug-in detects the song key of any audio file and effortlessly sends those parameters to all instances of Auto-Tune in a DAW with a single button click.It significantly improves music production workflow for producers,songwritersCited by 1Publish Year 2013Author A.CreusotThe ANTARES detector - ScienceDirectMay 01,2009 The ANTARES detector#0183;The ANTARES collaboration concluded the construction of a high energy neutrino telescope under the Mediterranean Sea,40 km off the French coast.The complete detector is a 3-dimensional array of 12 lines equipped with 900 photomultipliers,installed at a depth of 2475 m.

Cited by 1Publish Year 2013Author A.CreusotThe ANTARES Detector Electronics and Readout - NASA/ADS

The ANTARES collaboration is building an underwater neutrino telescope at 2500 m depth in the Mediterranean Sea.The experiment aims to detect high- energy cosmic neutrinos using a 3D array of 900 photomultipliers distributed along 12 lines.5 such lines have been operational since January 2007.The PMTs collect the Cherenkov light induced by neutrino-produced charged particles in the water.Cited by 1Publish Year 2008Author M.CircellaDetector design - ANTARESSchematic of the detector at the Antares site Arrangement of the twelve lines on the sea bed The basic unit of the detector is the optical module,consisting of a photomultiplier tube,various sensors,and the associated electronics,housed in a pressure-resistant glass sphere.Author Vladimir KulikovskiyPublish Year 2015(PDF) The Antares DetectorANTARES consists of a three-dimensional array of photosensitive devices that measure Cherenkov light induced by charged particles produced by high energy neutrinos interacting in the detector

Author Annarita MargiottaTHE ANTARES DETECTOR The Identification of Dark Matter

The ANTARES Collaboration is building an underwater neutrino telescope in the Mediterranean Sea,at a depth of 2500 m,40 km offshore from Toulon (France).The main goal of the detector is the search for high energy neutrinos from possible Galactic and extra-Galactic sources as well as from the decay of neutralinos and other exotic particles.Acoustic Particle Detection with the ANTARES Detector Mar 18,2010 The ANTARES detector#0183;The (Antares Modules for Acoustic Detection Under the Sea) AMADEUS system within the (Astronomy with a Neutrino Telescope and Abyss environmental RESsearch) ANTARES neutrino telescope is designed to investigate detection techniques for acoustic signals produced by particle cascades.While passing through a liquid a cascade deposits energy and produces a measurableAcoustic Particle Detection with the ANTARES Detector The ANTARES detector#0183;The ANTARES detector is deployed 40 km offshore from Toulon,France (\(42^\circ 48'\hbox {N}\),\(6^\circ 10'\hbox {E}\)) anchored at a depth of about 2475 m.The telescope detects the Cherenkov light stimulated in the medium by relativistic particles by means of a three dimensional grid of optical modules (OMs),pressure resistant glass spheres each containing one \(10^{\prime \prime

ANTARES home page

Click on the ANTARES logo at any time to come back to this page .Original design Th.S.Background picture Stars at the Galactic Center from the Spitzer Space Telescope's infrared cameras - Image Credit NASA,JPL-Caltech,Susan Stolovy (SSC/Caltech) et al.Antares undersea view,Credit (PDF) The ANTARES detector background sources andThe ANTARES Collaboration is deploying a large neutrino detector at a depth of 2475 m in the Mediterranean Sea,40 km off shore from La Seyne-sur-Mer in South France.

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