A quantitative assessment of completeness correction methods and public release of a versatile simulation code
Brown Dwarf Candidates in the JADES and CEERS Extragalactic Surveys
HST Imaging of the Ionizing Radiation from a Star-forming Galaxy at z = 3.794
Hubble Imaging of the Ionizing Radiation from a Star-forming Galaxy at Z=3.2 with fesc>50%
MIDIS: JWST NIRCam and MIRI Unveil the Stellar Population Properties of Lya Emitters and Lyman-break Galaxies at z 3-7
MIDIS: Strong (Hb+O III) and Ha Emitters at Redshift z 7-8 Unveiled with JWST NIRCam and MIRI Imaging in the Hubble eXtreme Deep Field
The hidden side of cosmic star formation at z > 3. Bridging optically dark and Lyman-break galaxies with GOODS-ALMA
The Hubble Legacy Field GOODS-S Photometric Catalog
The impact of satellite trails on Hubble Space Telescope observations
The ultraviolet continuum slopes of high-redshift galaxies: evidence for the emergence of dust-free stellar populations at z > 10
Instrument
WFC3, WFC3/UVIS
Temporal Coverage
2015-10-07T16:00:55Z/2015-12-18T14:23:23Z
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, Vanzella et al., 2016, 'Unveiling the Lyman continuum morphology with HST', 1.0, European Space Agency, https://doi.org/10.5270/esa-wvz5ok4
