IceCube Data for Neutrino Point-Source Searches Years 2008-2018
arXiv:2101.09836 · doi:10.21234/CPKQ-K003
Abstract
IceCube has performed several all-sky searches for point-like neutrino sources using track-like events, including a recent time-integrated analysis using 10 years of IceCube data. This paper accompanies the public data release of these neutrino candidates detected by IceCube between April 6, 2008 and July 8, 2018. The selection includes through-going tracks, primarily due to muon neutrino candidates, that reach the detector from all directions, as well as neutrino track events that start within the instrumented volume. An updated selection and reconstruction for data taken after April 2012 slightly improves the sensitivity of the sample. While more than 80% of the sample overlaps between the old and new versions, differing events can lead to changes relative to the previous 7 year event selection. An a posteriori estimate of the significance of the 2014-2015 TXS flare is reported with an explanation of observed discrepancies with previous results. This public data release, which includes 10 years of data and binned detector response functions for muon neutrino signal events, shows improved sensitivity in generic time-integrated point source analyses and should be preferred over previous releases.
arXiv commentSee https://icecube.wisc.edu/science/data/PS-IC40-IC86_VII for the associated data release files. For the associated time-integrated analysis results, see Phys. Rev. Lett. 124, 051103 (2020) (also available at arXiv:1910.08488)
Cited by in corpus (29)
- Search for High-Energy Neutrino Emission from Radio-Bright AGN
- Neutrinos from the Brightest Gamma-Ray Burst?
- Constraints on the models of the origin of high-energy astrophysical neutrinos
- Is the high-energy neutrino event IceCube-200530A associated with a hydrogen-rich superluminous supernova?
- High-energy neutrinos from X-rays flares of blazars frequently observed by the Swift X-Ray Telescope
- GB6 J2113+1121: A multi-wavelength flaring gamma-ray blazar temporally and spatially coincident with the neutrino event IceCube-191001A
- Neutrino propagation in the Earth and emerging charged leptons with
- Optically Informed Searches of High-Energy Neutrinos from Interaction-Powered Supernovae
- Near-future discovery of point sources of ultra-high-energy neutrinos
- IceCube constraints on Violation of Equivalence Principle
- Search for spatial coincidence between IceCube neutrinos and radio pulsars
- Constraints on Hadronic Contribution to LHAASO Sources with Neutrino Observations
- A Search for Coincident Neutrino Emission from Fast Radio Bursts with Seven Years of IceCube Cascade Events
- Monte Carlo simulations of neutrino and charged lepton propagation in the Earth with nuPyProp
- A stacked search for spatial coincidences between IceCube neutrinos and radio pulsars
- Searching New Particles at Neutrino Telescopes with Quantum-Gravitational Decoherence
- Radio astronomy locates the neutrino origin in bright blazars
- Insights from leptohadronic modelling of the brightest blazar flare
- Is Fermi 1544-0649 a misaligned blazar? discovering the jet structure with VLBI
- The Spectra of IceCube Neutrino (SIN) candidate sources -- IV. Spectral energy distributions and multi-wavelength variability
- All-Sky Search for Transient Astrophysical Neutrino Emission with 10 Years of IceCube Cascade Events
- A hierarchical Bayesian approach to point source analysis in high-energy neutrino telescopes
- Time-integrated constraint on neutrino flux of CHIME fast radio burst sources with 10-year IceCube point-source data
- Seeking Neutrino Emission from AGN through Temporal and Spatial Cross Correlation
- A relook at the GZK Neutrino-Photon Connection: Impact of Extra-galactic Radio Background & UHECR properties
- Searching for Dark Matter Annihilation with IceCube and P-ONE
- Fast Identification of Transients: Applying Expectation Maximization to Neutrino Data
- Predictions for dimuon production in high-energy neutrino-proton collisions using the color dipole model
- toise: a framework to describe the performance of high-energy neutrino detectors