A Comparison between the Stellar and Dynamical Masses of Six Globular Clusters
A Search for Black Hole Microlensing Signatures in Globular Cluster NGC 6656 (M22)
Exploring the formation environment and dynamics of multiple stellar populations in globular clusters through binary systems
Fast-moving stars around an intermediate-mass black hole in o Centauri
Gaia and Hubble Unveil the Kinematics of Stellar Populations in the Type II Globular Clusters o Centauri and M22
Hubble Space Telescope Proper Motion (HSTPROMO) Catalogs of Galactic Globular Cluster. II. Kinematic Profiles and Maps
Hubble Space Telescope Proper Motion (HSTPROMO) Catalogs of Galactic Globular Clusters. I. Sample Selection, Data Reduction, and NGC 7078 Results
Hubble Space Telescope Proper Motion (HSTPROMO) Catalogs of Galactic Globular Clusters. IV. Kinematic Profiles and Average Masses of Blue Straggler Stars
Kinematics of metallicity populations in Omega Centauri using the Gaia Focused Product Release and Hubble Space Telescope
Mass Loss of Different Stellar Populations in Globular Clusters: The Case of M4
Multimass modelling of milky way globular clusters - II. Present-day black hole populations
Multiple Stellar Populations of Globular Clusters from Homogeneous Ca by Photometry. I. M22 (NGC 6656)
Multi-wavelength Hubble Space Telescope Photometry of Stellar Populations in NGC 288
oMEGACat. III. Multiband Photometry and Metallicities Reveal Spatially Well-mixed Populations within o Centauris Half-light Radius
oMEGACat. II. Photometry and Proper Motions for 1.4 Million Stars in Omega Centauri and Its Rotation in the Plane of the Sky
oMEGACat. IV. Constraining the Ages of Omega Centauri Subgiant Branch Stars with HST and MUSE
oMEGACat. V. Helium Enrichment in o Centauri as a Function of Metallicity
oMEGACat. VI. Analysis of the Overall Kinematics of Omega Centauri in 3D: Velocity Dispersion, Kinematic Distance, Anisotropy, and Energy Equipartition
oMEGACat. VII. Tracing Interstellar and Intracluster Medium of o Centauri Using Sodium Absorptions
Survey of Multiple Populations in Globular Clusters among Very-low-mass Stars
The Hubble Space Telescope UV legacy survey of galactic globular clusters - XVI. The helium abundance of multiple populations
The impact of satellite trails on Hubble Space Telescope observations
Tracing oCentauris origins: Spatial and chemical signatures of its formation history
Validation of PSF models for HST and other space-based observations
Instrument
ACS, ACS/WFC, WFC3, WFC3/UVIS
Temporal Coverage
2010-11-10T10:40:20Z/2011-07-13T09:21:25Z
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, Lee et al., 2012, 'Globular clusters as galaxy building blocks', 1.0, European Space Agency, https://doi.org/10.5270/esa-zwl5a87