activity
20052023
most citedANTARES: the first undersea neutrino telescope

629 citations · 1.1k across the 13 of their papers we have counts for

collaborators

13 papers

astro-ph.IM2023

Mechanical design of the optical modules intended for IceCube-Gen2

Yuya Makino

IceCube-Gen2 is an expansion of the IceCube neutrino observatory at the South Pole that aims to increase the sensitivity to high-energy neutrinos by an order of magnitude. To this…

astro-ph.HE2023

Performance Studies of the Acoustic Module for the IceCube Upgrade

Charlotte Benning, Jürgen Borowka, Christoph Günther +2

The IceCube Upgrade will augment the existing IceCube Neutrino Observatory by deploying 700 additional optical sensor modules and calibration devices within its center at a depth o…

astro-ph.IM2021★ 4 cited

A next-generation optical sensor for IceCube-Gen2

Vedant Basu, Aya Ishihara, Markus Dittmer +1

For the in-ice component of the next generation neutrino observatory at the South Pole, IceCube-Gen2, a new sensor module is being developed, which is an evolution of the D-Egg and…

physics.ins-det2014

Drilling deep in South Pole Ice

Timo Karg, Rolf Nahnhauer

To detect the tiny flux of ultra-high energy neutrinos from active galactic nuclei or from interactions of highest energy cosmic rays with the microwave background photons needs ta…

astro-ph.IM2014★ 4 cited

Introducing TAXI: a Transportable Array for eXtremely large area Instrumentation studies

T. Karg, A. Haungs, M. Kleifges +2

A common challenge in many experiments in high-energy astroparticle physics is the need for sparse instrumentation in areas of 100 km2 and above, often in remote and harsh environm…

astro-ph.IM2011★ 14 cited

Design and performance of the South Pole Acoustic Test Setup

Yasser Abdou, Karl-Heinz Becker, Jens Berdermann +32

The South Pole Acoustic Test Setup (SPATS) was built to evaluate the acoustic characteristics of the South Pole ice in the 10 kHz to 100 kHz frequency range, for the purpose of ass…

astro-ph.IM2011★ 629 cited

ANTARES: the first undersea neutrino telescope

ANTARES Collaboration

The ANTARES Neutrino Telescope was completed in May 2008 and is the first operational Neutrino Telescope in the Mediterranean Sea. The main purpose of the detector is to perform ne…

astro-ph2007★ 79 cited

The ANTARES Optical Beacon System

M. Ageron, ANTARES Collaboration

ANTARES is a neutrino telescope being deployed in the Mediterranean Sea. It consists of a three dimensional array of photomultiplier tubes that can detect the Cherenkov light induc…

astro-ph2006★ 174 cited

The data acquisition system for the ANTARES neutrino telescope

J. A. Aguilar, ANTARES collaboration

The ANTARES neutrino telescope is being constructed in the Mediterranean Sea. It consists of a large three-dimensional array of photo-multiplier tubes. The data acquisition system…

astro-ph2006★ 124 cited

First results of the Instrumentation Line for the deep-sea ANTARES neutrino telescope

J. A. Aguilar, ANTARES Collaboration

In 2005, the ANTARES Collaboration deployed and operated at a depth of 2500 m a so-called Mini Instrumentation Line equipped with Optical Modules (MILOM) at the ANTARES site. The v…

astro-ph2005★ 4 cited

Development of Acoustic Sensors for the ANTARES Experiment

Christopher Lindsay Naumann, Gisela Anton, Kay Graf +6

In order to study the possibility of acoustic detection of ultra-high energy neutrinos in water, our group is planning to deploy and operate an array of acoustic sensors using the…

physics.ins-det2005★ 89 cited

Study of Large Hemispherical Photomultiplier Tubes for the ANTARES Neutrino Telescope

The ANTARES Collaboration

The ANTARES neutrino telescope, to be immersed depth in the Mediterranean Sea, will consist of a 3 dimensional matrix of 900 large area photomultiplier tubes housed in pressure res…

astro-ph2005

Development of acoustic devices for ultra-high energy neutrino detectors

Timo Karg, Gisela Anton, Kay Graf +7

Acoustic neutrino detection is a promising approach to instrument the large detector volumes needed for the detection of the small neutrino fluxes expected at ultra-high energies (…