Context. In analyses of stellar spectra and colours, and for the analysis of integrated light from galaxies, a homogeneous grid of model atmospheres of late-type stars and corresponding flux spectra is needed.

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A grid of MARCS model atmospheres for late-type stars | Synapse

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Gustafsson et al. (Thu,) studied this question.

synapsesocial.com/papers/6a078fcbc9983f2ec4c64235 https://doi.org/https://doi.org/10.1051/0004-6361:200809724

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