This repository was archived by the owner on Sep 11, 2024. It is now read-only.

Description
- Plot stretch vs spectral features and look for trends (re Sullivan 2010).
- Follow up on correlation we see with trend with Si feature strength and high/low SFR (in histograms). Read Maoz 2014 paper regarding this. This trend could be explained by the delay time distribution and/or correlation between star formation rate and galaxy age. Include this story as a part of the paper.