Repository logo
Log in(current)
Repository logoMIT Open ScholarshipDSpace@MIT
  1. Home
  2. MIT Open Access Articles
  3. MIT Open Access Articles
  4. All-sky Search for Time-integrated Neutrino Emission from Astrophysical Sources with 7 yr of IceCube Data

All-sky Search for Time-integrated Neutrino Emission from Astrophysical Sources with 7 yr of IceCube Data

Thumbnail Image
Download
Name

Aartsen-2017-All-sky search for time-integrate.pdf

Size

1.31 MB

Format

Adobe PDF

Checksum (MD5)

f57ed87780908fa7b47704dcf9ad56de

Author(s)
Arguelles Delgado, Carlos A
•
Axani, Spencer Nicholas
•
Collin, G. H.
•
Conrad, Janet Marie
•
Jones, Benjamin James Poyner
•
Moulai, Marjon H.
Date Issued
January 2017
Journal
The Astrophysical Journal
Publisher
IOP Publishing
Citation
Aartsen, M. G. et al. “All-Sky Search for Time-Integrated Neutrino Emission from Astrophysical Sources with 7 Yr of IceCube Data.” The Astrophysical Journal 835.2 (2017): 151. © 2017 The American Astronomical Society
Version
Final published version
Abstract
Since the recent detection of an astrophysical flux of high-energy neutrinos, the question of its origin has not yet fully been answered. Much of what is known about this flux comes from a small event sample of high neutrino purity, good energy resolution, but large angular uncertainties. In searches for point-like sources, on the other hand, the best performance is given by using large statistics and good angular reconstructions. Track-like muon events produced in neutrino interactions satisfy these requirements. We present here the results of searches for point-like sources with neutrinos using data acquired by the IceCube detector over 7 yr from 2008 to 2015. The discovery potential of the analysis in the northern sky is now significantly below E[superscript 2][subscript nu]φ/ dE[subscript nu] = 10[superscript −12] TeV cm[superscript −2] s[superscript −1], on average 38% lower than the sensitivity of the previously published analysis of 4 yr exposure. No significant clustering of neutrinos above background expectation was observed, and implications for prominent neutrino source candidates are discussed.
MIT Department
Massachusetts Institute of Technology. Department of Physics
Massachusetts Institute of Technology. Laboratory for Nuclear Science
Terms of Use
Article is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use.
Persistent DSpace Link
http://hdl.handle.net/1721.1/109516
DOI of Published Version
https://doi.org/10.3847/1538-4357/835/2/151
Repository logo
PrivacyPermissionsAccessibilityContact us
Repository logo
Notify us about copyright concerns.