An excursion into the core of the cluster lens Abell 1689
Evolution of the UV upturn in cluster galaxies: Abell 1689
Probing the Stellar Populations and Star Formation History of Early-type Galaxies at 0 < z < 1.1 in the Rest-frame Ultraviolet
The Direct-method Oxygen Abundance of Typical Dwarf Galaxies at Cosmic High Noon
The Evolution of the Faint End of the UV Luminosity Function during the Peak Epoch of Star Formation (1 < z < 3)
The Hawaii SCUBA-2 Lensing Cluster Survey: Are Low-luminosity Submillimeter Galaxies Detected in the Rest-frame UV?
The impact of satellite trails on Hubble Space Telescope observations
The Ionizing Photon Production Efficiency (xion) of Lensed Dwarf Galaxies at z ~ 2
The origin of the observed Ly a EW distribution of dwarf galaxies at z 2
Ultra-faint Ultraviolet Galaxies at z ~ 2 behind the Lensing Cluster A1689: The Luminosity Function, Dust Extinction, and Star Formation Rate Density
Instrument
WFC3, WFC3/UVIS
Temporal Coverage
2010-12-11T09:11:02Z/2011-03-18T15:33:52Z
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, Siana et al., 2012, 'Ionizing Emission from the Faint Galaxies Responsible for Reionization', 1.0, European Space Agency, https://doi.org/10.5270/esa-lxg0g9o