The file includes the NLTE abundance corrections (dex) for 6 subordinate lines Al I.
NLTE corrections are not provided for lines with EW(LTE) < 5 mA.
Everywhere, we use MARCS model atmospheres. Collisions with H I atoms are treated following Belyaev (2013, Astron. Astrophys. 560, A60).

Al1_NLTE_corrections_4500-6500_g3.0-4.5.dat
Teff = 4500 to 6500 K, log g = 3.0 to 4.5, [Fe/H] = 0 and -1. 

When using the data from Al1_dnlte_4000-5000_g0.5-2.5.dat in your research, cite please
Mashonkina, Belyaev, Shi, 2016, Astronomy Letters, 42, 366.