(First person named usually indicates the lead.)
The skeleton of the paper is available on Overleaf.
Writing assignments:
- (HW): Introduction
- (GDZ): Uncertainties in the Atomic Data
- (NS/DVD/DS): Inference
- (HW/FR): Test Cases
- (GDZ/HW): EIS Observations
- (AF/CB): Covariance Structure
- (HW): Discussion of Future work
- (HW): Conclusions
(HW/NS): Test case #1: Blind test with specific ne, ds, with default CHIANTI model.
(HW/NS): Test case #2: Use FR's MHD model to blind test the solver.
(DS; NS): There are still a handful of cases that are causing problems with the Hessian calculations, but working on that. But after that, the codes will be uploaded to the repository.
(HW): Check that all 10^6 combinations have LS solutions.
(DVD/NS/DS/JC): How does the data analyst extract the "best" (ne, ds) solution from the posteriors? What is "the" solution they should put into their analysis?
(MW; HW) How well do the "best" (ne, ds) solutions fit the data?
(HW; GDZ): Add Fe XIII 196.5 and 209.6 A lines to the list of intensities.
(HW; GDZ): Add EIS data from 20061225_225013.
(VK): Track paper development. Put outline into Overleaf and update periodically.
ambiguous state: