Closed-form analytic PDFs are derived for the ratio of projected separation to semimajor axis and for companion mass versus host acceleration, independent of all orbital elements when orientations are isotropic.
Title resolution pending
2 Pith papers cite this work, alongside 25 external citations. Polarity classification is still indexing.
2
Pith papers citing it
25
external citations · OpenAlex
years
2026 2representative citing papers
Tentative evidence for a super-Jupiter at 15-100 AU or brown dwarf at 20-170 AU in 51 Pegasi from RV curvature, but the signal is likely driven by Lick/Hamilton instrument drift.
citing papers explorer
-
Closed-Form Statistical Relations Between Projected Separation, Semimajor Axis, Companion Mass, and Host Acceleration
Closed-form analytic PDFs are derived for the ratio of projected separation to semimajor axis and for companion mass versus host acceleration, independent of all orbital elements when orientations are isotropic.
-
An Outer Giant Planet or Brown Dwarf in the 51 Pegasi System?
Tentative evidence for a super-Jupiter at 15-100 AU or brown dwarf at 20-170 AU in 51 Pegasi from RV curvature, but the signal is likely driven by Lick/Hamilton instrument drift.