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Searches for neutrinos from cosmic-ray interactions in the Sun using seven years of IceCube data
IceCube Collaboration, M. G. Aartsen, M. Ackermann +358
Cosmic-ray interactions with the solar atmosphere are expected to produce particle showers which in turn produce neutrinos from weak decays of mesons. These solar atmospheric neutr…
Pulse Shape Particle Identification by a Single Large Hemispherical Photo-Multiplier Tube
S. Samani, S. Mandalia, C. Argüelles +8
In neutrino experiments, hemispherical photomultiplier tubes (PMTs) are often used to cover large surfaces or volumes to maximize the photocathode coverage with a minimum number of…
Searching for new physics with profile likelihoods: Wilks and beyond
Sara Algeri, Jelle Aalbers, Knut Dundas Morå +1
Particle physics experiments use likelihood ratio tests extensively to compare hypotheses and to construct confidence intervals. Often, the null distribution of the likelihood rati…
Constraints on Neutrino Emission from Nearby Galaxies Using the 2MASS Redshift Survey and IceCube
IceCube Collaboration, M. G. Aartsen, M. Ackermann +354
The distribution of galaxies within the local universe is characterized by anisotropic features. Observatories searching for the production sites of astrophysical neutrinos can tak…
A Method to Determine the Electric Field of Liquid Argon Time Projection Chambers Using a UV Laser System and its Application in MicroBooNE
MicroBooNE collaboration, C. Adams, M. Alrashed +187
Liquid argon time projection chambers (LArTPCs) are now a standard detector technology for making accelerator neutrino measurements, due to their high material density, precise tra…
Reconstruction and Measurement of (100) MeV Energy Electromagnetic Activity from Decays in the MicroBooNE LArTPC
MicroBooNE collaboration, C. Adams, M. Alrashed +186
We present results on the reconstruction of electromagnetic (EM) activity from photons produced in charged current interactions with final state s. We employ a fully-aut…