Meeting 3: 31st May 2022
Dust & SED fitting

AGENDA:

• Dust modeling in SED fitting
  (Samir Salim) - 15 minutes

• A Bayesian Population Model for Dust Attenuation
  (Gautam Nagaraj) - 10 minutes

• The effect of dust on the morphology of resolved galaxies
  (Lamiya Mowla) - 10 minutes

• Open discussion on Dust & SED fitting
  30 minutes

• Informal gathering
  Wonderme/Gathertown - 30 minutes