A lack of evolution in the very bright end of the galaxy luminosity function from z 8 to 10
A Mass-dependent Slope of the Galaxy Size-Mass Relation out to z ~ 3: Further Evidence for a Direct Relation between Median Galaxy Size and Median Halo Mass
COSMOS-DASH: The Evolution of the Galaxy Size-Mass Relation since z ~ 3 from New Wide-field WFC3 Imaging Combined with CANDELS/3D-HST
HST Imaging of the Brightest z ~ 8-9 Galaxies from UltraVISTA: The Extreme Bright End of the UV Luminosity Function
The Roles of Morphology and Environment on the Star Formation Rate-Stellar Mass Relation in COSMOS from 0 < z < 3.5
Instrument
WFC3, WFC3/IR
Temporal Coverage
2017-03-27T21:33:55Z/2017-03-29T21:34:02Z
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, Bouwens comma Rychard, 2017, 'Confirmation of ultra-luminous z~9 galaxies', 1.0, European Space Agency, https://doi.org/10.5270/esa-leyd8du