NLTE effects on Fe I/II in the atmospheres of FGK stars and application   to abundance analysis of their spectra
  We describe the first results from our project aimed at large-scale calculations of NLTE abundance corrections for important astrophysical atoms and ions. In this paper, the focus is on Fe which is a proxy of stellar metallicity and is commonly used to derive effective temperature and gravity. We present a small grid of NLTE abundance corrections for Fe I lines and discuss how NLTE effects influence determination of effective temperature, surface gravity, and metallicity for late-type stars. 
Maria Bergemann, Karin Lind, Remo Collet, and Martin Asplund
astro-ph.SR astro-ph.GA