Color–magnitude diagram of likely members of Crius 224 (black circles) including TOI 2076 (red star) compared to isochrones from PARSEC. The green lines are random samples from the MCMC posterior. Circles are colored by their outlier probability (mixture weight). We show 125 Myr (red dashed) and 500 Myr (blue dashed) lines for reference. The lack of pre-main-sequence M dwarfs rules out ages ≲150 Myr, while higher ages are ruled out by the A star HD 153808.