that the sub-PeV event 25 has a very large position uncertainty in Fig. \[fig:Galactic\] and have to be considered with some care.[]{data-label="fig:NeuOnly"}](f5.pdf){width="280pt"}

Neutrino PeV and sub-PeV events
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The median angular error values for the IceCube neutrino events are given in the Supplementary Material for @Aartsen14. Using these median angular errors, and assuming Gaussian statistics [see @Aartsen14a], we have produced a sky map with $2\!-\!\sigma$ contours (corresponding to about $86\%$ confidence in 2D Gaussian statistics) for the neutrino events in the vicinity of  (see Fig. \[fig:Galactic\]). As seen in this map, a source of neutrinos with a radius of $\sim 140$pc around  (black circle) can be associated with five neutrino events, including two PeV events. These are $2$, $14$ (PeV event “Bert"), $15$, $25$ and $35$ (PeV event “Big Bird").

Based on this sky map, we compared our model neutrino spectra from the  source with the fluxes in five IceCube energy bins corresponding to the five neutrinos within $2\!-\!\sigma$ of the source. This is shown in the Fig. \[fig:NeuOnly\]. A more precise comparison will require both more sophisticated models of the cloud distribution within a few hundred parsecs of  and a more accurate determination of the event positions.

![Map showing 