PT - JOURNAL ARTICLE AU - Simon Gunkel AU - Jes Rust AU - Torsten Wappler AU - Christoph Mayer AU - Oliver Niehuis AU - Bernhard Misof TI - A posteriori evaluation of molecular divergence dates using empirical estimates of time-heterogeneous fossilization rates AID - 10.1101/128314 DP - 2017 Jan 01 TA - bioRxiv PG - 128314 4099 - http://biorxiv.org/content/early/2017/04/18/128314.short 4100 - http://biorxiv.org/content/early/2017/04/18/128314.full AB - The application of molecular clock concepts in phylogenetics permits estimating the divergence times of clades with an incomplete fossil record. However, the reliability of this approach is disputed, because the resulting estimates are often inconsistent with different sets of fossils and other parameters (clock models and prior settings) in the analyses. Here, we present the λ statistic, a likelihood approach for a posteriori evaluating the reliability of estimated divergence times. The λ statistic is based on empirically derived fossilization rates and evaluates the fit of estimated divergence times to the fossil record. We tested the performance of this measure with simulated data sets. Furthermore, we applied it to the estimated divergence times of (i) Clavigeritae beetles of the family Staphylinidae and (ii) all extant insect orders. The reanalyzed beetle data supports the originally published results, but shows that several fossil calibrations used do not increase the reliability of the divergence time estimates. Analyses of estimated inter-ordinal insect divergences indicate that uniform priors with soft bounds marginally outperform log-normal priors on node ages. Furthermore, a posteriori evaluation of the original published analysis indicates that several inter-ordinal divergence estimates might be too young. The λ statistic allows the comparative evaluation of any clade divergence estimate derived from different calibration approaches. Consequently, the application of different algorithms, software tools, and calibration schemes can be empirically assessed.