NLTE abundance correction

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    • Atmosphere model
    plane-parallel 1D MAFAGS-OS

    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) 2000:13000 A

    H lines
    O lines
    Mn 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: Bergemann et al. 2021
    • Mn: Bergemann et al. 2019
    • Co: Bergemann, Pickering, & Gehren 2010, MNRAS, 401, 1334 with collisional data from Voronov et al. 2022

    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