The first search for extremely-high energy cosmogenic neutrinos with the IceCube Neutrino Observatory
IceCube Collaboration: R. Abbasi, Y. Abdou, T. Abu-Zayyad, J. Adams,, J. A. Aguilar, M. Ahlers, K. Andeen, J. Auffenberg, X. Bai, M. Baker, S. W., Barwick, R. Bay, J. L. Bazo Alba, K. Beattie, J. J. Beatty, S. Bechet, J. K., Becker, K.-H. Becker, M. L. Benabderrahmane

TL;DR
This paper reports the first search for extremely-high energy cosmogenic neutrinos using the partially constructed IceCube detector, setting upper limits on neutrino fluxes in the energy range of 3×10^7 to 3×10^9 GeV based on 242.1 days of data.
Contribution
It presents the first search for EHE neutrinos with IceCube and provides model-independent upper limits on neutrino fluxes in the specified energy range.
Findings
No signal events detected in the data.
Established a 90% confidence level upper limit on neutrino flux.
Set constraints on models predicting EHE neutrino fluxes.
Abstract
We report on the results of the search for extremely-high energy (EHE) neutrinos with energies above GeV obtained with the partially (30%) constructed IceCube in 2007. From the absence of signal events in the sample of 242.1 days of effective livetime, we derive a 90% C.L. model independent differential upper limit based on the number of signal events per energy decade at GeV cm sec sr for neutrinos in the energy range from to GeV.
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