The Advanced Spectrum Synthesis 3D Tool ASSET is introduced. ASSET allows for the accurate and fast calculation of spectra from 3D hydrodynamical models. To achieve the highest numerical accuracy 3(rd)-order Bezier interpolations are employed and all available information from the model grid with respect to the spacial and frequency resolution is exploited. ASSET is fully parallelized with OpenMP and MPI and highly optimized to run at about 25% of peak speed on workstations and clusters. The emergent flux for a single spectral line can be calculated from dozens of snapshots within a few minutes, and the whole spectrum (2 . 10(6) frequencies) can be calculated on a small cluster (a few hundred threads) within a day. The numerical methods, th...
We analyze synthetic neutral hydrogen (HI) absorption and emission spectral lines from a high-resolu...
We examine closely the solar center-to-limb variation of continua and lines and compare observations...
International audienceIn this paper we discuss three issues in the context of three-dimensional (3D)...
The Advanced Spectrum Synthesis 3D Tool ASSET is introduced. ASSET allows for the accurate and fast ...
We present a method for performing spectral synthesis based on 1D averages of 3D simulations of conv...
Context. High-precision stellar analyses require hydrodynamic 3D modeling. Such models predict chang...
Context. Recent developments in the three-dimensional (3D) spectral synthesis code Linfor3...
I describe recent progress in terms of 3D hydrodynamical model atmospheres and 3D line formation and...
The use of 3D hydrodynamical simulations of stellar surface convection for model atmospheres is comp...
Context. High-precision stellar analyses require hydrodynamic modeling to interpret chemical abundan...
Context. Tighter constraints on metal-poor stars we observe are needed to better understand the chem...
We describe a new software package that may be used to determine stellar and atomic parameters by ma...
International audienceContext. The surface structures and dynamics of cool stars are characterised b...
International audienceContext. Tighter constraints on metal-poor stars we observe are needed to bett...
Hydrodynamical simulations are increasingly able to accurately model physical systems on stellar, ga...
We analyze synthetic neutral hydrogen (HI) absorption and emission spectral lines from a high-resolu...
We examine closely the solar center-to-limb variation of continua and lines and compare observations...
International audienceIn this paper we discuss three issues in the context of three-dimensional (3D)...
The Advanced Spectrum Synthesis 3D Tool ASSET is introduced. ASSET allows for the accurate and fast ...
We present a method for performing spectral synthesis based on 1D averages of 3D simulations of conv...
Context. High-precision stellar analyses require hydrodynamic 3D modeling. Such models predict chang...
Context. Recent developments in the three-dimensional (3D) spectral synthesis code Linfor3...
I describe recent progress in terms of 3D hydrodynamical model atmospheres and 3D line formation and...
The use of 3D hydrodynamical simulations of stellar surface convection for model atmospheres is comp...
Context. High-precision stellar analyses require hydrodynamic modeling to interpret chemical abundan...
Context. Tighter constraints on metal-poor stars we observe are needed to better understand the chem...
We describe a new software package that may be used to determine stellar and atomic parameters by ma...
International audienceContext. The surface structures and dynamics of cool stars are characterised b...
International audienceContext. Tighter constraints on metal-poor stars we observe are needed to bett...
Hydrodynamical simulations are increasingly able to accurately model physical systems on stellar, ga...
We analyze synthetic neutral hydrogen (HI) absorption and emission spectral lines from a high-resolu...
We examine closely the solar center-to-limb variation of continua and lines and compare observations...
International audienceIn this paper we discuss three issues in the context of three-dimensional (3D)...