NLTE abundance corrections (dex) for lines of Fe I, Ca I, Ti I, and Ti II in the grid of MARCS model atmospheres.

Select the line and interpolate for given Teff, log g, and element abundance ([X/H] - a). a = 0.4 for lines of Ca I, Ti I, Ti II in the [Fe/H]<=-1 stars. Otherwise, a = 0.0.

Species Wavelength Teff log g [X/H]
(
..
)		 (4000 ..
....
)		 (0.5 .. 2.5) (-4.0 .. 0.0)
 

In case of using these data in your studies, cite please Mashonkina, Sitnova, Pakhomov, 2016, Astronomy Letters, 42, 606

Grids of the NLTE abundance corrections for lines of Na I, Mg I, Ca I, Ca II, Ti II, Fe I, Zn I, Zn II, Sr II, and Ba II in the extended stellar parameter range are available at https://spectrum.inasan.ru/nLTE2

Bibliography of model atoms for non-LTE line-formation calculations is available on https://non-lte.com/bibliography.html