  We present a calculation of Bayes-factors for the digamma resonance
($\digamma$) versus the SM in light of ATLAS 8 TeV 20.3/fb, 13 TeV 3.2/fb and
13 TeV 15.4/fb data, sidestepping any difficulties in interpreting
significances in frequentist statistics. We matched, wherever possible,
parameterisations in the ATLAS analysis. We calculated that the plausibility of
the $\digamma$ versus the Standard Model increased by about eight in light of
the 8 TeV 20.3/fb and 13 TeV 3.2/fb ATLAS data, somewhat justifying interest in
$\digamma$ models. All told, however, in light of 15.4/fb data, the $\digamma$
was disfavoured by about 0.7.
