Observational Bias and Young Massive Cluster Characterisation II. Can Gaia accurately observe young clusters and associations?

Field-of-View for synthetic Gaia observations of clusters Orion-type-3, Orion-type-5.5 and Wd2-type presented in Buckner et al. (2023). Files contain both simulation and field stars along the Line-of-Sight (l = 270^o, b = 0^o) for the clusters when placed at 500pc, 2500pc and 4300pc distances. The original simulation files are included for reference. Included README files provide more detailed descriptions of the files.