List of Tables

1 The line parameter and default frequency point arrangements for line transitions
2 Selection of plot symbols available for the use in PLXY
3 Fundamental constants used in TMAP
4 TMAP uses the following values as solar abundances^a (Asplund et al. 2009; Maiorca et al. 2014; Grevesse et al. 2015; Scott et al. 2015b,a).
5 Steps to calculate a NLTE model with PRO2
6 Example for ATOMS2 jobs in the case of LTE (LTE2, left) and NLTE (PRO2, right) model-atmosphere calculations.
7 Example for SETF2 jobs in the case of LTE (LTE2, left) and NLTE (PRO2, right) model-atmosphere calculations.

All Users of the Tübingen
NLTE Model-Atmosphere Package
are reminded to be careful
at the creation and / or modification
of the atomic data files.

Although ATOMS2, SETF2, PRO2, and LINE1 check these files partly for consistency, small errors here can have large influence on the resulting model atmospheres.

All programs terminate in the case of fatal errors but can give only warnings when the input is ambiguous. The neglection of these warnings may be fatal!

For PRO2 and LINE1 output options are existing to print the model atoms and atomic data read by these programs. They should be used for checks — not only at the first time when the program is running with new or modified data!

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