A Wide View of the Galactic Globular Cluster NGC 2808: Red Giant and Horizontal Branch Star Spatial Distributions
Constraining Globular Cluster Age Uncertainties using the IR Color-Magnitude Diagram
Flash Mixing on the White Dwarf Cooling Curve: Spectroscopic Confirmation in NGC 2808
New Observational Evidence of Flash Mixing on the White Dwarf Cooling Curve
Survey of Multiple Populations in Globular Clusters among Very-low-mass Stars
The impact of satellite trails on Hubble Space Telescope observations
The Infrared Eye of the Wide-Field Camera 3 on the Hubble Space Telescope Reveals Multiple Main Sequences of Very Low Mass Stars in NGC 2808
Instrument
STIS/CCD, STIS/FUV-MAMA, WFC3, WFC3/IR, WFC3/UVIS
Temporal Coverage
2010-09-01T14:53:51Z/2011-02-22T07:47:37Z
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, Brown comma Thomas M., 2012, 'The Formation Mechanisms of Extreme Horizontal Branch Stars', 1.0, European Space Agency, https://doi.org/10.5270/esa-ivav162