J. Braun
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View article: Constraints on the Correlation of IceCube Neutrinos with Tracers of Large-Scale Structure
Constraints on the Correlation of IceCube Neutrinos with Tracers of Large-Scale Structure Open
The IceCube Neutrino Observatory has observed extragalactic astrophysical neutrinos with an apparently isotropic distribution. Only a small fraction of the observed astrophysical neutrinos can be explained by known sources. Neutrino produc…
View article: Quantification of galacturonic acid in pectin-containing samples using a stable isotope dilution approach and LC-MS
Quantification of galacturonic acid in pectin-containing samples using a stable isotope dilution approach and LC-MS Open
Reliable quantification of galacturonic acids (GalA) is essential for understanding the structural and functional properties of pectin-containing materials. However, conventional photometric methods often suffer from low reproducibility, l…
View article: Seasonal Variations of the Atmospheric Muon Neutrino Spectrum measured with IceCube
Seasonal Variations of the Atmospheric Muon Neutrino Spectrum measured with IceCube Open
This study presents an energy-dependent analysis of seasonal variations in the atmospheric muon neutrino spectrum, using 11.3 years of data from the IceCube Neutrino Observatory. By leveraging a novel spectral unfolding method, we explore …
View article: Quantification of Total Uronic Acids in Pectin-Containing Samples Using a Stable Isotope Dilution Approach and Lc-Ms
Quantification of Total Uronic Acids in Pectin-Containing Samples Using a Stable Isotope Dilution Approach and Lc-Ms Open
View article: Search for an eV-Scale Sterile Neutrino Using Improved High-Energy <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:msub><mml:mrow><mml:mi>ν</mml:mi></mml:mrow><mml:mrow><mml:mi>μ</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math> Event Reconstruction in IceCube
Search for an eV-Scale Sterile Neutrino Using Improved High-Energy Event Reconstruction in IceCube Open
This Letter presents the result of a 3+1 sterile neutrino search using 10.7 yr of IceCube data. We analyze atmospheric muon neutrinos that traverse the Earth with energies ranging from 0.5 to 100 TeV, incorporating significant improvements…
View article: The High-Altitude Water Cherenkov (HAWC) observatory in México: The primary detector
The High-Altitude Water Cherenkov (HAWC) observatory in México: The primary detector Open
View article: POS0299 EFFECT OF SECUKINUMAB ON RADIOGRAPHIC PROGRESSION AND INFLAMMATION IN SACROILIAC JOINTS AND SPINE IN PATIENTS WITH NON-RADIOGRAPHIC AXIAL SPONDYLOARTHRITIS: 2-YEAR IMAGING OUTCOMES FROM A PHASE III RANDOMISED TRIAL
POS0299 EFFECT OF SECUKINUMAB ON RADIOGRAPHIC PROGRESSION AND INFLAMMATION IN SACROILIAC JOINTS AND SPINE IN PATIENTS WITH NON-RADIOGRAPHIC AXIAL SPONDYLOARTHRITIS: 2-YEAR IMAGING OUTCOMES FROM A PHASE III RANDOMISED TRIAL Open
View article: POS0531 ABATACEPT DELAYS THE DEVELOPMENT OF RA– CLINICAL RESULTS AFTER 18 MONTHS FROM THE RANDOMIZED, PLACEBO-CONTROLLED ARIAA STUDY IN RA-AT RISK PATIENTS
POS0531 ABATACEPT DELAYS THE DEVELOPMENT OF RA– CLINICAL RESULTS AFTER 18 MONTHS FROM THE RANDOMIZED, PLACEBO-CONTROLLED ARIAA STUDY IN RA-AT RISK PATIENTS Open
View article: POS0974 LOW DOSE COMPUTED TOMOGRAPHY HOUNSFIELD UNITS: A RELIABLE METHODOLOGY FOR ASSESSING CHANGES IN VERTEBRAL BONE DENSITY IN RADIOGRAPHIC AXIAL SPONDYLOARTHRITIS
POS0974 LOW DOSE COMPUTED TOMOGRAPHY HOUNSFIELD UNITS: A RELIABLE METHODOLOGY FOR ASSESSING CHANGES IN VERTEBRAL BONE DENSITY IN RADIOGRAPHIC AXIAL SPONDYLOARTHRITIS Open
View article: Non-standard neutrino interactions in IceCube
Non-standard neutrino interactions in IceCube Open
Non-standard neutrino interactions (NSI) may arise in various types of new physics. Their existence would change the potential that atmospheric neutrinos encounter when traversing Earth matter and hence alter their oscillation behavior. Th…
View article: Neutrino Education, Outreach, and Communications Activities: Captivating Examples from IceCube
Neutrino Education, Outreach, and Communications Activities: Captivating Examples from IceCube Open
The IceCube Neutrino Observatory at the South Pole has tremendous emotional appeal---the extreme Antarctic environment coupled with the aura of a pioneering experiment that explores the universe in a new way. However, as with most cutting-…
View article: Search for Quantum Gravity Using Astrophysical Neutrino Flavour with IceCube
Search for Quantum Gravity Using Astrophysical Neutrino Flavour with IceCube Open
Along their long propagation from production to detection, neutrino states undergo quantum interference which converts their types, or flavours. High-energy astrophysical neutrinos, first observed by the IceCube Neutrino Observatory, are k…
View article: Cosmic-Ray Studies with the Surface Instrumentation of IceCube
Cosmic-Ray Studies with the Surface Instrumentation of IceCube Open
IceCube is a cubic-kilometer Cherenkov detector installed in deep ice at the geographic South Pole. IceCube’s surface array, IceTop, measures the electromagnetic signal and mainly low-energy muons from extensive air showers above several 1…
View article: Reconstruction of Neutrino Events in IceCube using Graph Neural Networks
Reconstruction of Neutrino Events in IceCube using Graph Neural Networks Open
The IceCube Neutrino Observatory is a cubic-kilometer scale neutrino detector embedded in the\nAntarctic ice of the South Pole. In the near future, the detector will be augmented by extensions,\nsuch as the IceCube Upgrade and the planned …
View article: A Search for Neutrino Sources with Cascade Events in IceCube
A Search for Neutrino Sources with Cascade Events in IceCube Open
IceCube has discovered a flux of astrophysical neutrinos, and more recently has used muon-neutrino datasets to present evidence for one source; a flaring blazar known as TXS 0506+056. However, the sources responsible for the majority of th…
View article: Search for secluded dark matter with 6 years of IceCube data
Search for secluded dark matter with 6 years of IceCube data Open
The IceCube neutrino observatory--installed in the Antarctic ice--is the largest neutrino telescope to date. It consists of 5,160 photomultiplier-tubes spread among 86 vertical strings making a total detector volume of more than a cubic ki…
View article: A model-independent analysis of neutrino flares detected in IceCube from X-ray selected blazars
A model-independent analysis of neutrino flares detected in IceCube from X-ray selected blazars Open
Blazars are among the most powerful steady sources in the Universe. Multi-messenger searches for blazars have traditionally focused on their gamma-ray emission, which can be produced simultaneously with neutrinos in photohadronic interacti…
View article: First air-shower measurements with the prototype station of the IceCube surface enhancement
First air-shower measurements with the prototype station of the IceCube surface enhancement Open
IceTop, the surface array of the IceCube Neutrino Observatory, consists of 162 ice-Cherenkov tanks distributed over an area of 1km$^2$. Besides being used as a veto for the in-ice neutrino detector, IceTop is a powerful cosmic-ray detector…
View article: New flux limit in the low relativistic regime for magnetic monopoles at IceCube
New flux limit in the low relativistic regime for magnetic monopoles at IceCube Open
Magnetic monopoles are hypothetical particles that carry magnetic charge. Depending on their velocity, different light production mechanisms exist to facilitate detection. In this work, a previously unused light production mechanism, lumin…
View article: Probing neutrino emission at GeV energies from compact binary mergers with the IceCube Neutrino Observatory
Probing neutrino emission at GeV energies from compact binary mergers with the IceCube Neutrino Observatory Open
The advent of multi-messenger astronomy has allowed for new types of source searches by neutrino detectors. We present the results of the search for 0.5-100 GeV astrophysical neutrinos detected with IceCube and emitted from compact binary …
View article: Cosmic ray spectrum from 250 TeV to 10 PeV using IceTop
Cosmic ray spectrum from 250 TeV to 10 PeV using IceTop Open
We report here an extension of the measurement of the all-particle cosmic-ray spectrum with IceTop to lower energy. The new measurement gives full coverage of the knee region of the spectrum and reduces the gap in energy between previous I…
View article: Search for sub-TeV neutrino emission from transient sources with three years of IceCube data.
Search for sub-TeV neutrino emission from transient sources with three years of IceCube data. Open
Since the discovery of a flux of high-energy astrophysical neutrinos, searches for their origins have focused primarily at TeV-PeV energies. Compared to sub-TeV searches, high-energy searches benefit from an increase in the neutrino cross …
View article: FRI0521 EARLY RECOGNITION OF PATIENTS WITH AXIAL SPONDYLOARTHRITIS BY USING A PRACTICAL REFERRAL SYSTEM – EVALUATION OF THE RECENTLY PROPOSED 2-STEP STRATEGY
FRI0521 EARLY RECOGNITION OF PATIENTS WITH AXIAL SPONDYLOARTHRITIS BY USING A PRACTICAL REFERRAL SYSTEM – EVALUATION OF THE RECENTLY PROPOSED 2-STEP STRATEGY Open
View article: Constraining the <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mover accent="true"><mml:mi>p</mml:mi><mml:mo stretchy="false">¯</mml:mo></mml:mover><mml:mo stretchy="false">/</mml:mo><mml:mi>p</mml:mi></mml:math> ratio in TeV cosmic rays with observations of the Moon shadow by HAWC
Constraining the ratio in TeV cosmic rays with observations of the Moon shadow by HAWC Open
An indirect measurement of the antiproton flux in cosmic rays is possible as\nthe particles undergo deflection by the geomagnetic field. This effect can be\nmeasured by studying the deficit in the flux, or shadow, created by the Moon as\ni…
View article: Data acquisition architecture and online processing system for the HAWC gamma-ray observatory
Data acquisition architecture and online processing system for the HAWC gamma-ray observatory Open
View article: HAWC Contributions to the 34th International Cosmic Ray Conference (ICRC2015)
HAWC Contributions to the 34th International Cosmic Ray Conference (ICRC2015) Open
List of proceedings from the HAWC Collaboration presented at the 34th International Cosmic Ray Conference, 30 July - 6 August 2015, The Hague, The Netherlands.
View article: Measurement of the Atmospheric<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:msub><mml:mi>ν</mml:mi><mml:mi>e</mml:mi></mml:msub></mml:math>Spectrum with IceCube
Measurement of the AtmosphericSpectrum with IceCube Open
We present a measurement of the atmospheric νe spectrum at energies between 0.1 and 100 TeV using data from the first year of the complete IceCube detector. Atmospheric νe originate mainly from the decays of kaons produced in cosmic-ray ai…