Stream-orbit misalignment II: A new algorithm to constrain the Galactic potential
Jason L. Sanders, James Binney

TL;DR
This paper introduces a new angle-action based algorithm for constraining the Galactic potential using tidal streams without assuming they delineate orbits, demonstrating its effectiveness with simulations and Gaia-like data.
Contribution
The paper presents a novel method that accurately constrains the Galactic potential from tidal streams without progenitor mass assumptions, improving upon previous orbit-fitting techniques.
Findings
Method successfully recovers potential parameters from simulations.
Averaged data can constrain potential with Gaia-like observational errors.
Potential parameters are accurately recovered within observational error margins.
Abstract
In the first of these two papers we demonstrated that assuming streams delineate orbits can lead to order one errors in potential parameters for realistic Galactic potentials. Motivated by the need for an improvement on orbit-fitting, we now present an algorithm for constraining the Galactic potential using tidal streams without assuming that streams delineate orbits. This approach is independent of the progenitor mass so is valid for all observed tidal streams. The method makes heavy use of angle-action variables and seeks the potential which recovers the expected correlations in angle space. We demonstrate that the method can correctly recover the parameters of a simple two-parameter logarithmic potential by analysing an N-body simulation of a stream. We investigate the magnitude of the errors in observational data for which the method can still recover the correct potential and…
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