This page keeps track of tilt events observed on TSO datasets. We identify  tilt events from TSOs based on different metrics (flux variations, FWHM, etc.) and change those to  based on WFS analyses/feedback.

Relevant information before reading the table below:

2022

DateTargetPID / ObsInstrument(s) used for detectionDetection methodStatusComments
2022-05-02Transit of HAT-P-14b1442 / 1NIRcam SW/LW + FGS

Flux "jump" (in NIRCam and FGS), FWHM "jump", centroid "jump"

See Schlawin+2022. Event at about 2459701.94 JD. Event identified to be on C6 and C1 segments.
2022-06-08Transit of HAT-P-14b1541 / 1NIRISS/SOSSFlux "bumps" (both in Order 1 and 2), FWHM

This seems to be a different tilt event flavor, with a trend in the FWHM rather than a jump in it. Various analyses done by Nestor Espinoza. It doesn't appear on FGS telemetry flux count.

2022-06-21Transit of WASP-96b2734 / 2NIRISS/SOSS (+ FGS?)FWHM "jump", but no apparent impact on white-light photometry.

This event didn't produce a measurable flux "bump", but it shows a clear FWHM "jump" signature. FGS shows what appears to be a small (500 ppm) flux jump at 2459751.86 JD — but the BJD TDB time for the event in SOSS is about 2459751.88 — so a 30-min difference.

2022-07-30Transit of WASP-39b1366 / 3NIRSpec/BOTS G395H + FGSFlux "jump", FWHM "jump", centroid "jump".


2022-08-11Eclipse of WASP-18b1366 / 21NIRISS/SOSS + FGSFlux "jump", FWHM "jump", centroid "jump".

Tilt event seems to be very small, suggesting (again) SOSS is very sensitive to these. FWHM jump is obvious in the data. Event likely on B6 segment.