A gravitationally boosted MUSE survey for emission-line galaxies at z 5 behind the massive cluster RCS 0224
Assessing the sources of reionization: a spectroscopic case study of a 30x lensed galaxy at z 5 with Lya, C IV, Mg II, and Ne III
Properties of the brightest young stellar clumps in extremely lensed galaxies at redshifts 4 to 5
Resolving Clumpy versus Extended Lya in Strongly Lensed, High-redshift Lya Emitters
The impact of satellite trails on Hubble Space Telescope observations
Instrument
ACS/WFC, WFC3/IR
Temporal Coverage
2016-11-11T14:49:12Z/2016-11-17T14:39:22Z
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, Smit et al., 2017, 'Identifying z>12 galaxies with JWST: What sources produce strong UV emission lines?', 1.0, European Space Agency, https://doi.org/10.5270/esa-0hkktnc