Atmosphere model
plane-parallel 1D MAFAGS-OS spherical 1D MARCS spherical 1D RSG-MARCS coverage

Input stellar parameters (please use the same format, maximal number of stars 82)

example: Star_name(!unique per line!) Teff log(g) [Fe/H] Vmic

Input from a file? select file:

Input of spectral lines and element code: example: 4571.1 12.01 (maximal number of lines 99)

Linelist (spectral interval)

H lines
O lines
Mg lines
Si lines
Ca I lines
Ca II lines
Ti lines
Ti II lines
Cr lines
Mn lines
Fe lines
Fe II lines
Co lines

Scaling factors used in NLTE calculations with DETAIL
chemical abundances in atmospheric models

If you find the datasets useful, we kindly ask you to provide a reference to the following studies:

 O:  Sitnova, Mashonkina, Ryabchikova 2013, AstL, 39, 126S
 Mg (IR): Bergemann, Kudritzki, Gazak et al. 2015, ApJ, 804, 113
 Mg (optical): Bergemann, Collet, Amarsi et al. 2017, ApJ, 847, 15
 Si: Bergemann, Kudritzki, Plez et al. 2013, ApJ, 764, 115
 Ca: Mashonkina, L.; Korn, A. J.; Przybilla, N. 2007, A&A, 461, 261M
 Ti: Bergemann 2011, MNRAS, 413, 2184
 Cr: Bergemann, M., Cescutti, G. A&A, 522, A9, 13 pp.
 Mn: Bergemann & Gehren 2008, A&A, 492, 823
 Fe, Ti (IR):  Bergemann, Kudritzki, Plez et al. 2012, ApJ, 751, 156
 Fe (optical): Bergemann, Lind, Collet et al. 2012, MNRAS, 427, 1
 Co: Bergemann, Pickering, & Gehren 2010, MNRAS, 401, 1334

BibTex Citation
you can also use this service with NLTE abundance corrections by L. Mashonkina or INSPECT database

Output with plots (NLTE and LTE profiles)?