The manuscript referred to by M. Krumrey aimed to provide a basis for macromolecular crystallographers to determine the photon flux incident on, and hence dose absorbed by, a crystal during an experiment. Radiation damage is a pressing concern in macromolecular crystallography (MX), and it is important that a tool be provided to obtain the incident flux, to allow the dose metric to be used in ongoing studies. For this tool to be widely useful, an accuracy of $ 5-10% is required over an energy range 6-20 keV using commercially available devices.(i) We appreciate the significant contribution made by Krumrey and colleagues over the years to the now vast literature on calibrating photodiodes and other detectors; Krumrey & Tegeler (1992) was overlooked in the literature search during the preparation of the manuscript and we apologize for omitting it. As mentioned in the introduction of Krumrey & Tegeler (1992), the idea of tilting a detector to determine its thickness is an old one and we saw no reason to provide a specific reference for this. Also, the energy range used in their work (0.15-2.5 keV) meant that it was not obvious that it was immediately applicable to MX. The simple expression we used [equation (5), Owen et al. (2009)] is derived directly from the geometry of the diode, and the primary aim of the paper was to determine whether the behaviour of devices used could be explained considering only primary absorption. More sophisticated models including both charge-carrier recombination and diffusion (Gullikson et al., 1995;Lutz, 1999) were considered but found not to be well suited to the devices used.(ii) The neglect of Compton scattering is explicitly addressed in x1.4 of our paper, where we agree with Krumrey that photoelectric cross-section data alone can be used to calculate absorbed energy between 6 and 20 keV. As no attempt was made to calibrate the diodes at energies greater than 20 keV, we felt it was unnecessary to include Compton scattering, since the effect of omitting it contributed negligibly to the error in our flux calculations.(iii) We regret that we did not make Fig. 5 of our paper and its legend clear enough. The origin of the error bars is detailed in the legend of Fig. 5, and the size of these was determined from the r.m.s. scatter of ten experiments from the mutual mean; a pessimistic approach was taken and this scatter was not divided by ffiffiffiffiffi 10 p as is customary. The key point of interest is that the data and theory are superposed, not fitted to one another. We found it striking and satisfying that the average value (centre of each error bar) agreed very well with theoretical expectation (blue line).It is true that a scintillation device does not faithfully detect every incident photon, but the absorption of air and the front window, and the finite thickness of the scintillation crystal were all taken into account in this work, and the photon pile-up effects were both accounted for and minimized by keeping the count rate low. We did not take such factors as escape peaks int...