The grid of the NLTE abundance corrections for lines of Eu II.
Everywhere, we use MARCS model atmospheres. Collisions with H I atoms are treated with the Drawinian rates scaled by S_H = 0.1.

Eu2_NLTE_corrections_4500-5000_g1.0-2.5.dat
includes equivalent widths EW_LTE (mA) and NLTE abundance corrections (dex) for lines of Eu II in the metal-poor model atmospheres. No NLTE corrections are given for lines with EW(LTE) < 5 mA.

When using the data from Eu2_NLTE_corrections_4500-5000_g1.0-2.5.dat in your research, cite please
Mashonkina, Christlieb, 2014, A&A, 565, A123.