A blind CO detection of a distant red galaxy in the HS1700+64 protocluster.
An HST/WFC3-IR Morphological Survey of Galaxies at z = 1.5-3.6. I. Survey Description and Morphological Properties of Star-forming Galaxies
Constraints on the Assembly and Dynamics of Galaxies. I. Detailed Rest-frame Optical Morphologies on Kiloparsec Scale of z ~ 2 Star-forming Galaxies
Excess AGN activity in the z = 2.30 Protocluster in HS 1700+64
Harnessing the Hubble Space Telescope Archives: A Catalog of 21,926 Interacting Galaxies
High-resolution Imaging of PHIBSS z ~ 2 Main-sequence Galaxies in CO J = 1 - 0
Morphologies of Galaxies in and around a Protocluster at z = 2.300
Resolving a merger in a hyperluminous submillimeter galaxy at z = 2.82
The Azimuthal Dependence of Outflows and Accretion Detected Using O VI Absorption
The impact of satellite trails on Hubble Space Telescope observations
The KBSS-KCWI survey: the connection between extended Ly a haloes and galaxy azimuthal angle at z 2-3
The Lya Properties of Faint Galaxies at z ~ 2-3 with Systemic Redshifts and Velocity Dispersions from Keck-MOSFIRE
The realm of the galaxy protoclusters. A review
Two sub-millimetre bright protoclusters bounding the epoch of peak star-formation activity
Instrument
ACS, ACS/WFC
Temporal Coverage
2005-09-18T10:31:16Z/2005-09-23T02:57:29Z
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, Shapley comma Alice E., 2006, 'Imaging a Proto-cluster at z=2.3: The Morphology-Density Relation at High Redshift', 1.0, European Space Agency, https://doi.org/10.5270/esa-pefbk8y
