No guaranteed neutrino astronomy without (enough) double bang tau and downward HESE muon tracks: An update version

IceCube Neutrino Astronomy is considered. The tau neutrino flavor paucity and the asymmetry for the tracks suggest a dominant atmospheric charm noise. The correlated cascades and tracks asymmetry with relevant statistics enforce the charm noise dominance in the data. The charm signal may explain at once the absence of correlation for the tracks data with the galactic plane and with known brightest gamma sources.
Comment: 16 pages, 4 figure , Questions and Discussion; new sections and new updated arguments