Are Ultra-faint Galaxies at z = 6-8 Responsible for Cosmic Reionization? Combined Constraints from the Hubble Frontier Fields Clusters and Parallels
First light and reionization epoch simulations (FLARES) X III: the lyman-continuum emission of high-redshift galaxies
Frontier Fields: High-redshift Predictions and Early Results
New Constraints on the Faint End of the UV Luminosity Function at z ~ 7-8 Using the Gravitational Lensing of the Hubble Frontier Fields Cluster A2744
The ASTRODEEP Frontier Fields catalogues. I. Multiwavelength photometry of Abell-2744 and MACS-J0416
The extreme faint end of the UV luminosity function at z ~ 6 through gravitational telescopes: a comprehensive assessment of strong lensing uncertainties
The production of ionizing photons in UV-faint z ~ 3-7 galaxies
Instrument
STIS, STIS/CCD
Temporal Coverage
2009-06-04T22:48:03Z/2009-08-03T06:48:21Z
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.
