Over the last 15 years, the supernova community has endeavoured to identify progenitor stars of core-collapse supernovae in high resolution archival images of their galaxies.This review compiles results (from 1999 - 2013) in a distance limited sample and discusses the implications. The vast majority of the detections of progenitor stars are of type II-P, II-L or IIb with one type Ib progenitor system detected and many more upper limits for progenitors of Ibc supernovae (14). The data for these 45 supernovae progenitors illustrate a remarkable deficit of high luminosity stars above an apparent limit of Log L ~= 5.1 dex. For a typical Salpeter IMF, one would expect to have found 13 high luminosity and high mass progenitors. There is, possibly, only one object in this time and volume limited sample that is unambiguously high mass (the progenitor of SN2009ip). The possible biases due to the influence of circumstellar dust and sample selection methods are reviewed. It does not appear likely that these can explain the missing high mass progenitor stars. This review concludes that the observed populations of supernovae in the local Universe are not, on the whole, produced by high mass (M > ~18Msun) stars. Theoretical explosions of model stars also predict that black hole formation and failed supernovae tend to occur above M > ~18Msun. The models also suggest there are islands of explodability for stars in the 8-120Msun range. The observational constraints are quite consistent with the bulk of stars above M > ~18Msun collapsing to form black holes with no visible supernovae. (Abridged).
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