An Atlas of Color-selected Quiescent Galaxies at z > 3 in Public JWST Fields
A Spectroscopic Redshift Measurement for a Luminous Lyman Break Galaxy at z = 7.730 Using Keck/MOSFIRE
A z = 1.85 galaxy group in CEERS: Evolved, dustless, massive intra-halo light and a brightest group galaxy in the making
Extremely Small Sizes for Faint z ~ 2-8 Galaxies in the Hubble Frontier Fields: A Key Input for Establishing Their Volume Density and UV Emissivity
Morphology of Galaxies in JWST Fields: Initial Distribution and Evolution of Galaxy Morphology
Newly Discovered Bright z ~ 9-10 Galaxies and Improved Constraints on Their Prevalence Using the Full CANDELS Area
The impact of satellite trails on Hubble Space Telescope observations
The missing light of the Hubble Ultra Deep Field
The Roles of Morphology and Environment on the Star Formation Rate-Stellar Mass Relation in COSMOS from 0 < z < 3.5
Instrument
ACS, ACS/WFC, WFC3, WFC3/IR
Temporal Coverage
2014-11-15T19:25:34Z/2015-07-09T23:51:18Z
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, 2015, 'A Complete Census of the Bright z~9-10 Galaxies in the CANDELS Data Set', 1.0, European Space Agency, https://doi.org/10.5270/esa-jyi7qnx