3D hydrodynamic simulations for the formation of the Local Group satellite planes
First Gaia Dynamics of the Andromeda System: DR2 Proper Motions, Orbits, and Rotation of M31 and M33
Implications of the Milky Way Travel Velocity for Dynamical Mass Estimates of the Local Group
Isotropic at the Break? 3D Kinematics of Milky Way Halo Stars in the Foreground of M31
Solo dwarfs - III. Exploring the orbital origins of isolated Local Group galaxies with Gaia Data Release 2
Sum of the masses of the Milky Way and M31: A likelihood-free inference approach
The impact of satellite trails on Hubble Space Telescope observations
The M31 Velocity Vector. I. Hubble Space Telescope Proper-motion Measurements
The M31 Velocity Vector. II. Radial Orbit toward the Milky Way and Implied Local Group Mass
The outskirts of M33: Tidally induced distortions versus signatures of gas accretion
The Velocity Anisotropy of Distant Milky Way Halo Stars from Hubble Space Telescope Proper Motions
Instrument
ACS, ACS/WFC, WFC3, WFC3/UVIS
Temporal Coverage
2010-01-08T06:35:17Z/2010-08-31T21:24:24Z
Version
1.0
Mission Description
Launched in 1990, the NASA/ESA Hubble Space Telescope remains the premier UV and visible light telescope in orbit. With well over 1.6 million observations from 10 different scientific instruments, the ESA Hubble Science Archive is a treasure trove of astronomical data to be exploited.
European Space Agency, van der Marel et al., 2011, 'The First Proper Motion Measurement for M31: Dynamics and Mass of the Local Group', 1.0, European Space Agency, https://doi.org/10.5270/esa-y3azy2w