Accurate radial velocity and metallicity of the Large Magellanic Cloud old globular clusters NGC 1928 and NGC 1939
A Cryogenic Liquid-Mirror Telescope on the Moon to Study the Early Universe
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
Is the SMC Bound to the LMC? The Hubble Space Telescope Proper Motion of the SMC
On the dynamics of the Small Magellanic Cloud through high-resolution ASKAP H I observations
Proper Motions of the Large Magellanic Cloud and Small Magellanic Cloud: Re-Analysis of Hubble Space Telescope Data
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 motions of the Magellanic Clouds and the nature of galactic dark matter
The Proper Motion of the Large Magellanic Cloud Using HST
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
ACS, ACS/HRC
Temporal Coverage
2002-08-26T09:38:46Z/2003-07-01T22:58:52Z
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, Alcock comma Charles R., 2003, 'Systemic and Internal Proper Motions of the Magellanic Clouds from Astrometry with ACS', 1.0, European Space Agency, https://doi.org/10.5270/esa-aatpd90