Characterizing SN Observations with the Roman ST Prism
- Given an embedding (c1, c2, & c2), phase, redshift, and Roman ST exposure time, can we recover the original c1, c2, and c3?
- Use
embed2spec
but also need Roman prism specific characteristics. - Use
???
to fit Roman prism spectra for expected embedding parameters
Create a new conda
environment with
conda env create -f environment.yml
and activate it
conda activate embed2roman
The environment can be updated via conda env update -f environment.yml
.
- embed2roman.py - WIP - produce Roman prism-like 1D spectra for a collection of embedding parameters.
- analysis.py - WIP - Do we fit the same embedding parameters we used?