Erin M. May

la0 and lo0 are flipped in the spherical harmonics brightness model

1

la0 results in longitude offsets and vice versa  

### Instrument NIRSpec (Stages 1-3) ### What is your suggestion? Just like the title: allow users to supply custom bad pixel mask in Stage 1. ### Error traceback output _No...

Enable modeling of starspots with both Fleck and Starry

10

Exactly what the title says - Adds fleck for starspot modeling, modifies starry code to allow starspots (not recommended, very slow...). Adds a plot to show starspots for fleck. This...

[Bug]: If a user marks a column as saturated in every group in S1, the column is still used in S3

3

### FAQ check - [X] Yes, I checked the FAQ and my question has not been addressed. ### Instrument NIRSpec (Stages 1-3) ### What happened? From a chat with @gianninapr...

Enables custom bad pixel masks (S1), user supplied wavelength files (S4), adds joint white light curve fitting parameters to docs (S5)

1

Addressed #638 and also enables users to supply a wavelength file in S4 for pre-computed bins. Also adds joint white light curve fitting to docs and demo ecf to address...