  We study the status of the reactor antineutrino anomaly in light of recent
reactor flux models obtained with the conversion and summation methods. We
present a new improved calculation of the IBD yields of the standard
Huber-Mueller (HM) model and those of the new models. We show that the reactor
rates and the fuel evolution data are consistent with the predictions of the
Kurchatov Institute (KI) conversion model and with those of the Estienne-Fallot
(EF) summation model, leading to a plausible robust demise of the reactor
antineutrino anomaly. We show that the results of several goodness of fit tests
favor the KI and EF models over other models that we considered. We also
discuss the implications of the new reactor flux models for short-baseline
neutrino oscillations due to active-sterile oscillations. We show that reactor
data give upper bounds on active-sterile neutrino mixing that are not very
different for the reactor flux models under consideration and are in tension
with the large mixing required by the Gallium anomaly that has been refreshed
by the recent results of the BEST experiment.
