Responses of surface and underground scintillation detectors of Yakutsk array are calculated for showers initiated by primary particles with energy E0>=1.0E17 eV within the frameworks of QGSJet01 QGSIIJet-II-04, SIBYLL-2.1 and EPOS-LHC hadron interaction models. A new estimation of E0 is obtained with the use of various methods. The resulting energy is lower compared to the obtained with earlier method by factor ~1.33.
@article{arxiv.1408.6302,
title = {Revision of the energy calibration of the Yakutsk EAS array},
author = {A. V. Glushkov and M. I. Pravdin and A. Sabourov},
journal= {arXiv preprint arXiv:1408.6302},
year = {2015}
}