SNEWS: the SuperNova Early Warning System

@article{Antonioli1999SNEWSTS,
  title={SNEWS: the SuperNova Early Warning System},
  author={P. Antonioli and Richard Tresch Fienberg and Fabrice Fleurot and Yoshiyuki Fukuda and Walter Fulgione and Alec Habig and Jaret Heise and Arthur B. McDonald and Corrinne Mills and Toshio Namba and Leif J. Robinson and Kate Scholberg and Michael Schwendener and Roger W. Sinnott and Blake C. Stacey and Yoichiro Suzuki and R{\'e}da Tafirout and Carlo Francesco Vigorito and Brett Viren and Clarence J. Virtue and Antonino Zichichi},
  journal={New Journal of Physics},
  year={1999},
  volume={6},
  pages={114 - 114}
}
This paper provides a technical description of the SuperNova Early Warning System (SNEWS), an international network of experiments with the goal of providing an early warning of a galactic supernova. 

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References

SHOWING 1-10 OF 56 REFERENCES

Observation of a neutrino burst in coincidence with supernova 1987A in the Large Magellanic Cloud.

A burst of eight neutrino events preceding the optical detection of the supernova in the Large Magellanic cloud has been observed in a large underground water Cherenkov detector. The events span an

Observation of a neutrino burst from the supernova SN1987A.

A neutrono burst was observed in the KAMIOKANDE-II detector on 23 February during a time interval of 13 seconds and consisted of 11 electron events of energy 7.5 to 36 MeV with angles 18°±18° and 15°±27°.

On the Event Observed in the Mont Blanc Underground Neutrino Observatory during the Occurrence of Supernova 1987a

We discuss here the characteristics of the event detected in the Mont Blanc Underground Neutrino Observatory on February 23, 1987, consisting of 5 interactions recorded during 7s. The measured

Angular distribution of events from SN1987A.

Improved measurements of the event energies and energy uncertainties, relative times, triggering efficiencies, and angles from the presumed source are presented.

Observation in the Kamiokande-II detector of the neutrino burst from supernova SN1987A.

The nature of the single, observed neutrino burst coincides remarkably well with the elements of the current model of type-II supernovae and neutron-star formation.

The Sudbury Neutrino Observatory

A description is given of the proposed Sudbury Neutrino Observatory based on a 1000 tonne heavy water Cherenkov detector which is being designed. This detector would allow the measurement of
...