NLTE abundance correction

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    • 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: StarID (one 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)

    -- For O, Mn and Co lines in the interval 2000:13000 A, please use this update

    Linelist (spectral interval in Å)

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

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

    References
    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)?

    webmaster: This service is developed by MPIA