- Sarah Kendrew mentions for MIRI: some info on strange persistence issues. Perhaps this would mean not using certain TA filters, but not there yet. This might be an issue in particular for phase-curves; still under investigation (see: shadow region).
- Brian Brooks:
- Information about timing (timing offset between detectors, timestamps on headers versus timestamps on the data, etc.) — probably this should be its own page.
- Another thing: example science programs. Might be good to update? This is coming, he has a meeting next week on this.
- Everett Schlawin: some systematics. Offsets between overall transit depths on different instruments?
- Nikolay Nikolov : we might want to put a JDox article to outline this? No solution right now. Nestor Espinoza things this might also be an analysis detail (e.g., limb darkening, stellar activity, say). Nikolay Nikolov mentions he can identify targets for which there's many
- Brian Brooks mentions on how to mitigate a guide star failure from FGS. Michael Regan mentions there's nothing to do this — Brian Brooks mentions this might be something to discuss in JDox too? Sarah Kendrew: nothing you can do, but most common reason visits can be skipped. Perhaps then explain the algorithm for FGS guide star acquisition describing the process (and what might fail, based on Cycle 1).
Nestor Espinoza's summary (above, plus points in meeting slides):
- JDox TSO timing (time-stamps) page.
- Update JDox to have information on instrument systematics: (a) ramps, (b) persistence (e.g., MIRI's shadow region), (c) 1/f noise, (d) perhaps some word on transit depth updates.
- Contact MO/FGS folks so guide star acquisiton process is explained (instead of having to explain it via e-mails), as well as possible ways in which a visit might fail or be skipped.
- Have a look at example TSO programs (pending on Brian Brooks' meeting next week).
- NIRCam: information about DHS & TSO's (no timescales, but general information for observers).
- NIRISS/SOSS: information about trace/wavelength solution changes and how to solve it.
- NIRSpec: backgrounds? 1/f noise (e.g., NSClean)?
- MIRI: backgrounds?