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Between 2011 March and 2014 August Swift responded to 20 triggers from theIceCube neutrino observatory, observing the IceCube 50% confidence error circlein X-rays, typically within 5 hours of the trigger. No confirmed counterparthas been detected. We describe the Swift follow up strategy and data analysisand present the results of the campaign. We discuss the challenges ofdistinguishing the X-ray counterpart to a neutrino trigger from serendipitousuncatalogued X-ray sources in the error circle, and consider the implicationsof our results for future strategies for multi-messenger astronomy, withparticular reference to the follow up of gravitational wave triggers from theadvanced-era detectors.

Swift follow-up of IceCube triggers, and implications for the Advanced-LIGO era