P. Gorham

Measurement of neutrino oscillation with KamLAND: Evidence of spectral distortion

We present results of a study of neutrino oscillation based on a 766 ton-year exposure of KamLAND to reactor anti-neutrinos. We observe 258 \nuebar\ candidate events with energies above 3.4 MeV compared to 365.2 events expected in the absence of neutrino oscillation. Accounting for 17.8 expected background events, the statistical significance for reactor \nuebar disappearance is 99.998%. The observed energy spectrum disagrees with the expected spectral shape in the absence of neutrino oscillation at 99.6% significance and prefers the distortion expected from \nuebar oscillation effects. A two-neutrino oscillation analysis of the KamLAND data gives \DeltaMSq = 7.9

Detecting radio emission from cosmic ray air showers and neutrinos with a digital radio telescope

^{+0.6}_{-0.5}\times10^{-5}

FORTE satellite constraints on ultrahigh energy cosmic particle fluxes

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Constraints on Cosmic Neutrino Fluxes from the Antarctic Impulsive Transient Antenna Experiment

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High sensitivity search for nu;e's from the sun and other sources at KamLAND.

. A global analysis of data from KamLAND and solar neutrino experiments yields \DeltaMSq = 7.9

Observations of the Askaryan Effect in Ice

^{+0.6}_{-0.5}\times10^{-5}

The Antarctic Impulsive Transient Antenna ultra-high energy neutrino detector: Design, performance, and sensitivity for the 2006–2007 balloon flight

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New Limits on the Ultrahigh Energy Cosmic Neutrino Flux from the ANITA Experiment

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Observation of ultrahigh-energy cosmic rays with the ANITA balloon-borne radio interferometer

and \ThetaParam = 0.40

Diffraction limited infrared images of the binary star T Tauri

^{+0.10}_{-0.07}