Ngā tūemi rite

• M3DIS -- A grid of 3D radiation-hydrodynamics stellar atmosphere models for stellar surveys. II. Carbon-enhanced metal-poor stars
  mā: Eitner, Philipp, me ētahi atu.
  I whakaputaina: (2025)
• Solar carbon abundance from 3D non-LTE modelling of the diagnostic lines of the CH molecule
  mā: Hoppe, Richard, me ētahi atu.
  I whakaputaina: (2025)
• 3D Non-LTE radiation transfer: theory and applications to stars, exoplanets, and kilonovae
  mā: Bergemann, Maria, me ētahi atu.
  I whakaputaina: (2025)
• A grid of self-consistent MSG (MARCS-StaticWeather-GGchem) cool stellar, sub-stellar, and exoplanetary model atmospheres
  mā: Jørgensen, Uffe G., me ētahi atu.
  I whakaputaina: (2024)
• A method to derive self-consistent NLTE astrophysical parameters for 4 million high-resolution 4MOST stellar spectra in half a day with invertible neural networks
  mā: Ksoll, Victor F., me ētahi atu.
  I whakaputaina: (2026)