3D tomography of the giant Lya nebulae of z 3-5 radio-loud AGN
A galaxy populations study of a radio-selected protocluster at z ~ 3.1
Are we seeing accretion flows in a 250 kpc Lya halo at z = 3?
Evidence for powerful AGN winds at high redshift: dynamics of galactic outflows in radio galaxies during the Quasar Era
High redshift Lya halos
OIII emitters in the field of the MRC0316-257 protocluster
The impact of satellite trails on Hubble Space Telescope observations
The Nascent Red Sequence at z ~ 2
The realm of the galaxy protoclusters. A review
Instrument
ACS, ACS/WFC, NICMOS, NICMOS/NIC3
Temporal Coverage
2004-12-14T07:07:49Z/2005-01-21T08:35:33Z
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, Miley et al., 2006, 'Imaging a protocluster at z=3.1: Effects of environment and evolution on galaxy populations in the early universe', 1.0, European Space Agency, https://doi.org/10.5270/esa-lx01of3