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.
CITATION STYLE
Evans, P. A., Osborne, J. P., Kennea, J. A., Smith, M., Palmer, D. M., Gehrels, N., … Stasik, A. (2015). Swift follow-up of IceCube triggers, and implications for the advanced-LIGO era. Monthly Notices of the Royal Astronomical Society, 448(3), 2210–2223. https://doi.org/10.1093/mnras/stv136
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