...
- generate draft of research proposal by end of today.
- intro about SFR vs. redshift
- observable proxies for SFR (emission line EW)
- why study this in high mass clusters, previous work.
- Why is SPT sample special?
- highest-mass clusters across wide range of redshifts
- existing spectroscopic data that includes some emission line galaxies
- independent x-ray mass estimates for many of these clusters.
- we can therefore explore the redshift dependence of SFR in the most extreme cluster environments, across 0.2<z<1.
- write quick summary of key papers, including a clip out of key plots.
- arrange meetings with 1) jonathan ruel, 2) matt bayliss to talk about Gemini and Magellan existing spectroscopy.
Test.