Nicole Drakos

Research Blog

Welcome to my Research Blog.

This is mostly meant to document what I am working on for myself, and to communicate with my colleagues. It is likely filled with errors!

This project is maintained by ndrakos

UV Properties

The main problem with the SED assignment is the UV properties (as shown, e.g., here).

MUV-Beta relation

Using the halo catalog generated earlier (as described here), the MUV-beta relation is:

FSPS parameters

There are six relevant parameters to make the SEDs (see this post)

Here is how the parameters vary in MUV-beta space:

Conclusions

Beta seems to depend strongly on the metallicity… Next, I will look into the metallicities of the galaxies more closely.


« Galaxy Sizes Part II
Metallicties »