Speaker
Zoe Rhiannon Jones
(Tartu Observatory)
Description
We explore the relationships between the cosmic environments of galaxies and their own physical properties through large-scale statistics, with the ultimate goal of being able to predict a galaxy's most likely cosmic environment from its SED and properties alone. To do so, we are developing a tool to compare the SEDs of large samples of galaxies in order to find similarity between them. We present our method and preliminary results.