MPS-ATLAS: A fast all-in-one code for synthesising stellar spectra
V. Witzke, A. I. Shapiro, M. Cernetic, R. V. Tagirov, N. M. Kostogryz,, L. S. Anusha, Y. C. Unruh, S. K. Solanki, R. L. Kurucz

TL;DR
MPS-ATLAS is a new, efficient, all-in-one code for synthesizing stellar spectra that combines atmosphere modeling, spectral synthesis, and opacity calculations, significantly improving speed and flexibility over existing tools.
Contribution
It introduces a fast, flexible, and integrated code based on ATLAS9 that enhances stellar spectral synthesis with parallel computation and customizable line lists.
Findings
Code is substantially faster than existing tools.
Validated against ATLAS9, PHOENIX, and observations.
Supports different elemental compositions easily.
Abstract
Context. Stellar spectral synthesis is essential for various applications, ranging from determining stellar parameters to comprehensive stellar variability calculations. New observational resources as well as advanced stellar atmosphere modelling, taking three dimensional (3D) effects from radiative magnetohydrodynamics calculations into account, require a more efficient radiative transfer. Aims. For accurate, fast and flexible calculations of opacity distribution functions (ODFs), stellar atmospheres and stellar spectra we developed an efficient code building on the well-established ATLAS9 code. The new code also paves the way for an easy and fast access to different elemental compositions in stellar calculations. Methods. For the generation of ODF tables we further developed the well-established DFSYNTHE code by implementing additional functionality, and a speed-up by employing a…
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Taxonomy
TopicsStellar, planetary, and galactic studies · Astrophysics and Star Formation Studies · Atmospheric Ozone and Climate
