Three-dimensional simulations of an 27 solar-mass progenitor (2002 series of Alex Heger)
Model computed using the Lattimer&Swesty (K=220 MeV) equation of state and the neutrino transport employs 12 energy bins.
Model published in ApJ 770 (2013) 66 and arXiv:1303.6269
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The following data is available
Movie: Time-evolution of the IceCube detection rate on a sky-plot of observer directions
for the 27 M_sun supernova progenitor at 10 kpc.
The rate has been computed for the un-oscillated electron antineutrino
flux (i.e., assuming no flavor conversions):
When making use of data from this website, please
cite the data archive by giving the weblink and the corresponding
publication, if existent.
We made all possible efforts to ensure the correctness of the
data in this archive. Errors, however, cannot be excluded.
If any are found, we would appreciate being informed.
