Follow steps similar to those in Example 1.5 to analyse the Gaia catalogue data of NGC 3201 in Clustermancer, and analyse the sample images in Afterglow Access. Note that Afterglow photometry can be skipped entirely, as you did in the case of IC 2948 and M67. However, due to the density and number of stars in the cluster, you will likely need to go through multiple iterations of field star removal, archive fetching up to a limited radius, refinement of field star removal parameters, and subsequent archive fetching, before you can add all cluster stars out to the cluster’s full radius. Once you’ve isolated the stars in the cluster, complete your isochrone analysis using what you’ve learned above. When you have completed your analysis, enter the isochrone model parameters into this form.
Make sure to download your HR diagram(s) with isochrone fits, and save your Results Summary CSV when your analysis is complete.
cosmiCave.org 