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This is a tutorial for RADMC-3D radiative transfer code. The aim of the tutorial is to create dust and line emission models of a T Tauri star.
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Fritz Alexander Francisco / OctoFishProject
MIT LicenseInterspecific collaboration: stereo calibration and 3D Habitat reconstruction/Tracking
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Analyzing result of queries II: "image gallery" browser for quantities. If scalar, a scatter plot (not really an image gallery), if more complex (e.g., band structure + DOS), think to nice visualization for comparisons and browsing.
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This is a fork of the ALCHEMIC astrochemical modelling code (Semenov et al. 2010). The code is adapted to model the chemical evolution of SPH trajectories from hydrodynamic molecular cloud simulations, using complex chemical networks.
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CLAPP / HermiteGF.jl
BSD 2-Clause "Simplified" LicenseUpdated -
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Example of machine learning for Hirshfeld ratios.
Attached to book chapter in Handbook of Materials Modeling
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Visualize the band structures and DOS from NOMAD.
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Florian Knoop / hilde
BSD Zero Clause LicenseUpdated