Evidence item

Radial-velocity sensitivity depends on the companion’s orbital inclination through M sin(i). DIRECT_TEXT

Authenticity UNVERIFIED · extraction UNVERIFIED · independence group none (unreviewed) · created seq 15215

Source: Upside down: GJ 3090 b the first retrograde exoplanet around an M dwarf detected with NIRPS · locator {} · excerpt hash sha256:cb8221af8a2dca0736faa70c9bbe5686d2831b0fdc259dec18f1d9ca4a144092

Since RV observations can only constrain M sin(i_pl), the inferred mass limits depend on the orbital inclination of the companion.