  Neutrino events from IceCube have recently been associated with multiple
astrophysical sources. Interestingly, these likely detections represent three
distinct astrophysical source types: active galactic nuclei (AGN), blazars, and
tidal disruption events (TDE). Here we compute the expected contributions of
AGNs, blazars and TDEs to the overall cosmic neutrino flux detected by IceCube
based on the associated events, IceCube's sensitivity, and the source types'
astrophysical properties. We find that, despite being the most commonly
identified sources, blazars cannot contribute more than 11% of the total flux
(90% credible level), consistent with existing limits from stacked searches. On
the other hand, we find that either AGNs or TDEs could contribute more than 50%
of the total flux (90% credible level), although stacked searches further limit
the TDE contribution to $\lesssim 30%$. We also find that so-far unknown source
types contribute at least 10% of the total cosmic flux with a probability of
80%. We assemble a pie chart that shows the most likely fractional contribution
of each source type to IceCube's total neutrino flux.
