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tokens: This work was supported by a Marie Curie Fellowship and the NASA grants NNX13AI63G / NNX14AQ31G. We thank J.P. Wuelser for providing us with the absolute calibration of IRIS and its temporal evolution. We are very grateful to S. Couvidat for creating hmi.Ic _ 45s _ nrt data for this flare and to P. Scherrer for his explanations of the details of HMI. We thank A. Sainz Dalda for comments on the manuscript and J. Kašparová for her help with adapting the MALI code to account for non-thermal hydrogen collisional rates. We acknowledge helpful discussions that took place at ISSI. S.K. acknowledges the support by the Swiss National Science Foundation (200021-140308), by the European Commission through HESPE (FP7-SPACE-2010-263086), and through NASA contract NAS 5-98033 for RHESSI . P.H. was supported by the FP7 project F-CHROMA under the EC contract no. 606862, by the project RVO:67985815, and by the grant P209/12/1652 of the Grant agency of the Czech Republic.