Free 10-minute demo · no account

Can this observation recover the known transit of WASP-12 b?

WASP-12 b is already known. You are not searching for a new planet. You are deciding whether this observation contains convincing evidence of its transit.

BUILD STATUS / INTERFACE PROTOTYPE

The interaction is complete, but this private build uses a transparent teaching dataset. Verified TransitSift measurements and frame exports will replace it before any public scientific claim is made.

TARGET / WASP-12 bTASK / RECOVER KNOWN TRANSIT

Stage 01 / 04

Review frame quality

TransitSift has flagged two groups for review. Its recommendation is evidence—not an answer. Keep or reject each group, then inspect the consequence.

Frames 042–06122:14–22:29
FWHM
2.7 px
Sky
812 ADU
Elong.
0.08
QC / nominal

Compact sources; stable sky.

Frames 062–08122:30–22:45
FWHM
2.9 px
Sky
826 ADU
Elong.
0.09
QC / nominal

Measurements agree with neighboring exposures.

Frames 082–10122:46–23:01
FWHM
6.2 px
Sky
1268 ADU
Elong.
0.13
FLAG / cloud

Elevated sky and broadened sources.

Frames 102–12123:02–23:17
FWHM
3.0 px
Sky
844 ADU
Elong.
0.10
QC / nominal

Nominal image quality.

Frames 122–14123:18–23:33
FWHM
3.8 px
Sky
861 ADU
Elong.
0.43
FLAG / trailing

Source elongation exceeds the review limit.

Frames 142–16123:34–23:49
FWHM
3.1 px
Sky
849 ADU
Elong.
0.11
QC / nominal

Stable background after transit egress.

Relative flux / normalized120 demonstration measurements
Light curve after the current frame-quality decisionsObserved depth 1.155%, uncertainty plus or minus 0.092%, with 120 accepted measurements. Rejected measurements are shown in red.0.9750.9850.9951.0050%25%50%75%100%OBSERVATION PROGRESSRELATIVE FLUX