Discovery of Astrometric Accelerations by Dark Companions in the Globular Cluster o Centauri
Gaia Focused Product Release: Sources from Service Interface Function image analysis. Half a million new sources in omega Centauri
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
Multimass modelling of milky way globular clusters - II. Present-day black hole populations
No evidence for intermediate-mass black holes in the globular clusters o Cen and NGC 6624
The State-of-the-art HST Astro-photometric Analysis of the Core of o Centauri. II. Differential-reddening Map
The State-of-the-art HST Astro-photometric Analysis of the Core of o Centauri. III. The Main Sequences Multiple Populations Galore
The State-of-the-art HST Astro-photometric Analysis of the Core of o Centauri. I. The Catalog
Instrument
WFC3, WFC3/IR, WFC3/UVIS
Temporal Coverage
2010-12-12T21:21:12Z/2011-07-25T19:12:54Z
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, Kozhurina-Platais comma Vera, 2011, 'UVIS and IR Geometric Distortion Corrections', 1.0, European Space Agency, https://doi.org/10.5270/esa-5jsy0p4
