Accurate radial velocity and metallicity of the Large Magellanic Cloud old globular clusters NGC 1928 and NGC 1939
A likely runaway star cluster in the outer disc of the Large Magellanic Cloud
An estimate of the mass of the Milky Way from the Magellanic Stream
First Gaia Local Group Dynamics: Magellanic Clouds Proper Motion and Rotation
Gaia Early Data Release 3. Structure and properties of the Magellanic Clouds
On the dynamics of the Small Magellanic Cloud through high-resolution ASKAP H I observations
The ALMA REBELS Survey: dust continuum detections at z > 6.5
The ALMA REBELS survey: obscured star formation in massive Lyman-break galaxies at z= 4-8 revealed by the IRX-b and M relations
The impact of satellite trails on Hubble Space Telescope observations
The Proper Motion Field of the Small Magellanic Cloud: Kinematic Evidence for Its Tidal Disruption
Third-epoch Magellanic Cloud Proper Motions. I. Hubble Space Telescope/WFC3 Data and Orbit Implications
Third-epoch Magellanic Cloud Proper Motions. II. The Large Magellanic Cloud Rotation Field in Three Dimensions
Instrument
WFC3, WFC3/UVIS
Temporal Coverage
2009-10-21T19:41:40Z/2010-07-24T06:58:22Z
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, Kallivayalil et al., 2011, 'Continued Proper Motions of the Magellanic Clouds: Orbits, Internal Kinematics, and Distance', 1.0, European Space Agency, https://doi.org/10.5270/esa-7sqo3fq