We present our NextGen Model Atmosphere grid for low mass stars for effective temperatures larger than 3000 { K } .
These LTE models are calculated with the same basic model assumptions and input physics as the VLMS part of the NextGen grid so that the complete grid can be used , e.g. , for consistent stellar evolution calculations and for internally consistent analysis of cool star spectra .
This grid is also the starting point for a large grid of detailed NLTE model atmospheres for dwarfs and giants ( Hauschildt et al , in preparation ) .
The models were calculated from 3000 { K } to 10000 { K } ( in steps of 200 { K } ) for 3.5 \leq \log ( g ) \leq 5.5 ( in steps of 0.5 ) and metallicities of -4.0 \leq [ { M / H } ] \leq 0.0 .

We discuss the results of the model calculations and compare our results to the Kurucz 1994 grid .
Some comparisons to standard stars like Vega and the Sun are presented and compared with detailed NLTE calculations .