posted on 2015-04-27, 15:20authored byP. A. Evans, J. P. Osborne, J. A. Kennea, M. Smith, D. M. Palmer, N. Gehrels, J. M. Gelbord, A. Homeier, M. Voge, N. L. Strotjohann, D. F. Cowen, S. Boeser, M. Kowalski, A. Stasik
Between 2011 March and 2014 August Swift responded to 20 triggers from the IceCube neutrino observatory, observing the IceCube 50 per cent confidence error circle in X-rays, typically within 5 h of the trigger. No confirmed counterpart has been detected. We describe the Swift follow-up strategy and data analysis and present the results of the campaign. We discuss the challenges of distinguishing the X-ray counterpart to a neutrino trigger from serendipitous uncatalogued X-ray sources in the error circle, and consider the implications of our results for future strategies for multimessenger astronomy, with particular reference to the follow-up of gravitational wave triggers from the advanced-era detectors.
Funding
PAE and JPO acknowledge UK Space Agency support. JMG gratefully acknowledges the
support from NASA under award NNH13CH61C.
History
Citation
Monthly Notices of the Royal Astronomical Society, 2015, 448 (3), pp. 2210-2223 (14)
Author affiliation
/Organisation/COLLEGE OF SCIENCE AND ENGINEERING/Department of Physics and Astronomy
Version
VoR (Version of Record)
Published in
Monthly Notices of the Royal Astronomical Society
Publisher
Oxford University Press (OUP), Royal Astronomical Society