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
GLACiAR, an Open-Source Python Tool for Simulations of Source Recovery and Completeness in Galaxy Surveys
Observational determination of the galaxy bias from cosmic variance with a random pointing survey: clustering of z ~ 2 galaxies from Hubbles BoRG survey
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 Cosmic Web around the Brightest Galaxies during the Epoch of Reionization
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 Sizes of z ~ 9-10 Galaxies Identified in the Brightest of Reionizing Galaxies (BoRG) Survey
Instrument
WFC3, WFC3/IR, WFC3/UVIS
Temporal Coverage
2012-11-14T19:19:40Z/2012-11-17T05:33:54Z
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, Trenti et al., 2013, 'Unveiling the structure of the farthest galaxy protocluster: WFC3 imaging of a z~8 galaxy overdensity', 1.0, European Space Agency, https://doi.org/10.5270/esa-72reta5