Analysing resolved stellar populations using Gaia data and theoretical models (V)

4 Abril 2022, 11:00 • André Maria da Silva Dias Moitinho de Almeida

# Clusters parameter determination - going further (II)

- Using parallaxes to constrain distance

- Maximum likelihood distance from parallax

- Dicussion the differences between the various distance estimates made

- Discuss extension of maximum likelihood fit to all parameters