A Redshift-independent Efficiency Model: Star Formation and Stellar Masses in Dark Matter Halos at z 4
A spectroscopically confirmed z = 1.327 galaxy-scale deflector magnifying a z ~ 8 Lyman-break galaxy in the Brightest of Reionizing Galaxies survey
Bright z ~ 9 Galaxies in Parallel: The Bright End of the Rest-frame UV Luminosity Function from HST Parallel Programs
Correcting the z ~ 8 Galaxy Luminosity Function for Gravitational Lensing Magnification Bias
Galaxy Candidates at z ~ 10 in Archival Data from the Brightest of Reionizing Galaxies (BORGz8) Survey
Hubble Space Telescope Observations of Field Ultracool Dwarfs at High Galactic Latitude
Milky Way Red Dwarfs in the BoRG Survey; Galactic Scale-height and the Distribution of Dwarf Stars in WFC3 Imaging
Overdensities of Y-dropout Galaxies from the Brightest-of-Reionizing Galaxies Survey: A Candidate Protocluster at Redshift z 8
Probing Very Bright End of Galaxy Luminosity Function at z >~ 7 Using Hubble Space Telescope Pure Parallel Observations
SuperBoRG: Exploration of Point Sources at z ~ 8 in HST Parallel Fields
SuperBoRG: Search for the Brightest of Reionizing Galaxies and Quasars in HST Parallel Imaging Data
The Bright-end Galaxy Candidates at z ~ 9 from 79 Independent HST Fields
The Brightest of Reionizing Galaxies Survey: Constraints on the Bright End of the z ~ 8 Luminosity Function
The Brightest of Reionizing Galaxies Survey: Design and Preliminary Results
The impact of satellite trails on Hubble Space Telescope observations
The Luminosity Function at z ~ 8 from 97 Y-band Dropouts: Inferences about Reionization
The missing light of the Hubble Ultra Deep Field
The Physical Properties of Luminous z 8 Galaxies and Implications for the Cosmic Star Formation Rate Density from 0.35 deg2 of (Pure-)Parallel HST Observations
The Sizes of z ~ 9-10 Galaxies Identified in the Brightest of Reionizing Galaxies (BoRG) Survey
The UV Luminosity Function of Star-forming Galaxies via Dropout Selection at Redshifts z ~ 7 and 8 from the 2012 Ultra Deep Field Campaign
The UV luminosity functions of bright z > 8 galaxies: determination from 0.41 deg2 of HST observations along 300 independent sightlines
Instrument
WFC3, WFC3/IR, WFC3/UVIS
Temporal Coverage
2010-01-05T15:43:54Z/2010-11-25T01:23:57Z
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, Yan et al., 2010, 'Search for Very High-z Galaxies with WFC3 Pure Parallel', 1.0, European Space Agency, https://doi.org/10.5270/esa-pqjsi8g