Notes from discussion with Marcio and Shannon - cc @shanosborne, @obi-wan76
SI defocus models
Pupil shear and pupil distortions.
- To the extent that pupil distortions are in the SIAF, this will be automatically handed by @shanosborne's new code for applying distortions.
- Same for the pupil rotations mostly. The default per each SI was taken from the SIAF a while ago, and hard-coded into webbpsf_core.
- Pupil shear/offsets. Doesn't matter for imaging modes with clear pupils. Does matter for modes with additional pupil obscurations inside the SIs, in particular the NIRCam and MIRI coronagraph modes. See Table 19 of Aronstein's WFE report.
SI WFE Zernikes
- Were there any changes to WFE maps over the past ~ year since @mperrin imported them into webbpsf? As of June 2017, Aronstein told Perrin that the WFE maps had not changed since the late 2016 delivery. Probably no change since but should verify.
Pupil Map resolution for large FOV PSFs, and incoherent scattered light
- Marcio can put his existing info on very large FOV PSFs and scattered light into a report or JDox page. Turns out JStans and Holler already have plans for such a JDox page, and we can assist as needed but otherwise let them do it. Lightsey is working to extend scattered light to MIRI wavelengths.
- (As discussed previously w/ Marcio and JStans, large FOV PSFs needs better sampling). Consider setting up a better supported mode for WebbPSF to use 2048 squared OPDs instead of 1024, for better sampling of the segment gaps (and thus better modeling of the diffraction spikes).
- Incoherent scattered light
Other
Notes from discussion with Marcio and Shannon - cc @shanosborne, @obi-wan76
SI defocus models
Pupil shear and pupil distortions.
__init__functions to setoptions[pupil_shift_x],options[pupil_shift_y]to the values from the report.SI WFE Zernikes
Pupil Map resolution for large FOV PSFs, and incoherent scattered light
Other