adrn / chemical-torus-imaging

Archived!

This repository is archived, and the paper is published! Future work will use the totoro package for executing inferences, and separate repositories for specific projects.

Orbital Torus Imaging

chemical-torus-imaging's Issues

Describe dashed lines in figures 7/8 captions

Add plot of "bad" abundances

We pick 8 abundance ratios to show in Figure 2. These were hand-selected, but there are others that we deem "bad" for various reasons. We could show these and mention that a better thing to do would be to jointly fit a calibration model and what we do here.

Run on GALAH DR3

Optimize over all (or more) potential parameters

Right now, we do mdisk, zsun, vzun, but we could also vary disk scale height, and other parameters!

Reorganize discussion section and add subsection headings

The discussion section is currently a giant pile of TODO's. We should organize what is there into a set of subsections that address our assumptions, and add subsections for other discussion topics (like comparing to eDF modeling vs. bovy & rix and etc.). This issue is only to set up the subheadings!

Add plot of abundances vs. Jz

Restrict to the 8 elements shown in Figure 2. Highlight that different elements are sensitive to different ranges of Jz. Stronger gradients are better.

Change blue marker in Figure 6 to red??

Add R-z panel to Figure 1

As suggested by Chris

Submit to SDSS collaboration

If the EC request is accepted, submit to the SDSS collaboration for the 3 week review period.
https://internal.sdss.org/collaboration/projects/browse/select/id%3D769

Do the same inference with theta_r instead

Vary the disk mass and halo mass and do the same thing for theta_r

split joint results figure into two figures

fig 1: v_sun vs m/m
fig 2: z_sun vs m/m and z_sun vs v_sun
This is for the cosmology plots.