Claims

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As of snapshot 27745 under ledger-default@0.3.0.

Claim	Type	Assessment	Score	Review checks	References
The study found no evidence of a massive outer planetary companion or wide stellar binary companion to GJ 3090, and reported that this disfavors gravitational-perturbation explanations for the planet’s retrograde orbit.	OBSERVATIONAL	Supported	0.8581	1 of 4	66
Six NIRPS/HARPS transit observations yielded a 3D orbital obliquity of 136^{+24}_{-18} degrees for the sub-Neptune GJ 3090 b, establishing it as a retrograde planet around an M dwarf in the study.	QUANTITATIVE	Supported	0.8808	1 of 4	60