Constraining the Milky Way potential with a 6-D phase-space map of the GD-1 stellar stream
Sergey E. Koposov (1,2,3), Hans-Walter Rix (1), David W. Hogg (1,4), ((1) Max Planck Institute for Astronomy, Heidelberg, Germany, (2) Institute, of Astronomy, Cambridge, UK, (3) Sternberg Astronomical Institute, Moscow,, Russia, (4) New York University, New York, USA)

TL;DR
This study uses a detailed 6-D phase-space map of the GD-1 stellar stream to tightly constrain the Milky Way's circular velocity and potential flattening near 15 kpc, improving understanding of the galaxy's mass distribution.
Contribution
It provides the first comprehensive 6-D phase-space map of GD-1 and derives new constraints on the Milky Way's circular velocity and potential flattening at large radii.
Findings
Constraints on the circular velocity at the Sun's radius: 224 ± 13 km/s.
The potential flattening parameter q_Φ=0.87^{+0.07}_{-0.04}.
Weak constraints on halo flattening, q_{Φ,halo}>0.89 at 90% confidence.
Abstract
The narrow GD-1 stream of stars, spanning 60 deg on the sky at a distance of ~10 kpc from the Sun and ~15 kpc from the Galactic center, is presumed to be debris from a tidally disrupted star cluster that traces out a test-particle orbit in the Milky Way halo. We combine SDSS photometry, USNO-B astrometry, and SDSS and Calar Alto spectroscopy to construct a complete, empirical 6-dimensional phase-space map of the stream. We find that an eccentric orbit in a flattened isothermal potential describes this phase-space map well. Even after marginalizing over the stream orbital parameters and the distance from the Sun to the Galactic center, the orbital fit to GD-1 places strong constraints on the circular velocity at the Sun's radius V_c=224 \pm 13 km/s and total potential flattening q_\Phi=0.87^{+0.07}_{-0.04}. When we drop any informative priors on V_c the GD-1 constraint becomes V_c=221…
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