ZEU-ICE

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2019-12-10
13:12
OpenAccess [PUBDB-2019-04940] Report

Annual Report 2018 [VH-NG-1202]
[2018]
3 pp. () [10.3204/PUBDB-2019-04940]  GO
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2019-12-10
13:10
OpenAccess [PUBDB-2019-04939] Report

Annual Report 2017 [VH-NG-1202]
[2017]
3 pp. () [10.3204/PUBDB-2019-04939]  GO
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2019-12-02
16:15
Embargoed OpenAccess [PUBDB-2019-04674] Journal Article
et al
Neutrino vertex reconstruction with in-ice radio detectors using surface reflections and implications for the neutrino energy resolution
Ultra high energy neutrinos (E >1016:5 eV) are eciently measured via radiosignals following a neutrino interaction in ice. An antenna placed O(15 m) below the icesurface will measure two signals for the vast majority of events (90% at E=1018 eV): adirect pulse and a second delayed pulse from a reection o the ice surface. [...]
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2019-11-20
09:44
arXiv [PUBDB-2019-04316] Report/Journal Article

Reconstructing the cosmic-ray energy from the radio signal measured in one single station
[arXiv:1905.11185]
Short radio pulses can be measured from showers of both high-energy cosmic rays and neutrinos. While commonly several antenna stations are needed to reconstruct the energy of an air shower, we describe a novel method that relies on the radio signal measured in one antenna station only. [...]
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2019-11-18
17:05
[PUBDB-2019-04289] Journal Article
et al
Search for Sources of Astrophysical Neutrinos Using Seven Years of IceCube Cascade Events
Low-background searches for astrophysical neutrino sources anywhere in the sky can be performed using cascade events induced by neutrinos of all flavors interacting in IceCube with energies as low as ~1 TeV. Previously we showed that, even with just two years of data, the resulting sensitivity to sources in the southern sky is competitive with IceCube and ANTARES analyses using muon tracks induced by charge current muon neutrino interactions—especially if the neutrino emission follows a soft energy spectrum or originates from an extended angular region. [...]
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2019-11-18
16:54
OpenAccess [PUBDB-2019-04288] Journal Article
et al
GROWTH on S190425z: Searching Thousands of Square Degrees to Identify an Optical or Infrared Counterpart to a Binary Neutron Star Merger with the Zwicky Transient Facility and Palomar Gattini-IR
The third observing run by LVC has brought the discovery of many compact binary coalescences. Following the detection of the first binary neutron star merger in this run (LIGO/Virgo S190425z), we performed a dedicated follow-up campaign with the Zwicky Transient Facility (ZTF) and Palomar Gattini-IR telescopes. [...]
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2019-11-18
16:48
[PUBDB-2019-04287] Journal Article
et al
Transient processing and analysis using AMPEL: alert management, photometry, and evaluation of light curves
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2019-10-31
10:32
OpenAccess [PUBDB-2019-03849] Journal Article
et al
NuRadioReco: a reconstruction framework for radio neutrino detectors
While the radio detection of cosmic rays has advanced to a standard method in astroparticle physics, the radio detection of neutrinos is just about to start its full bloom. The successes of pilot-arrays have to be accompanied by the development of modern and flexible software tools to ensure rapid progress in reconstruction algorithms and data processing. [...]
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2019-10-21
16:20
OpenAccess [PUBDB-2019-03715] Report/Journal Article
et al
Investigation of Two Fermi -LAT Gamma-Ray Blazars Coincident with High-energy Neutrinos Detected by IceCube
[arXiv:1901.10806]
After the identification of the gamma-ray blazar TXS 0506+056 as the first compelling IceCube neutrino source candidate, we perform a systematic analysis of all high-energy neutrino events satisfying the IceCube realtime trigger criteria. We find one additional known gamma-ray source, the blazar GB6J1040+0617, in spatial coincidence with a neutrino in this sample. [...]
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2019-07-29
14:53
OpenAccess [PUBDB-2019-02863] Report/Journal Article
et al
Search for transient optical counterparts to high-energy IceCube neutrinos with Pan-STARRS1
[arXiv:1901.11080]
In order to identify the sources of the observed diffuse high-energy neutrino flux, it is crucial to discover their electromagnetic counterparts. To increase the sensitivity of detecting counterparts of transient or variable sources by telescopes with a limited field of view, IceCube began releasing alerts for single high-energy (E$_ν$ >  60 TeV) neutrino detections with sky localisation regions of order 1° radius in 2016. [...]
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