Evidence item

The search becomes less sensitive to higher true companion masses for lower-inclination companions. 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:b187a640ef1ddef4afd56dfa6090728325aec1885720c49199b5c801ecc9ebf9

As i_c is reduced, the mass limits become less stringent since a larger true companion mass is required to produce the same observed RV semi-amplitude.