COOL-LAMPS. VI. Lens Model and New Constraints on the Properties of COOL J1241+2219, a Bright z = 5 Lyman Break Galaxy and its z = 1 Cluster Lens
GalWeight Application: A Publicly Available Catalog of Dynamical Parameters of 1800 Galaxy Clusters from SDSS-DR13, (GalWCat19)
HST/WFC3 Grism Observations of z 1 Clusters: Evidence for Rapid Outside-in Environmental Quenching from Spatially Resolved Ha Maps
MAGAZ3NE: High Stellar Velocity Dispersions for Ultramassive Quiescent Galaxies at z 3
Resolving CO (2-1) in z ~ 1.6 Gas-rich Cluster Galaxies with ALMA: Rotating Molecular Gas Disks with Possible Signatures of Gas Stripping
The GOGREEN and GCLASS surveys: first data release
The GOGREEN Survey: A deep stellar mass function of cluster galaxies at 1.0 < z < 1.4 and the complex nature of satellite quenching
The GOGREEN Survey: Evidence of an Excess of Quiescent Disks in Clusters at 1.0
Instrument
WFC3/IR
Temporal Coverage
2018-03-27T11:10:00Z/2019-06-06T21:55:34Z
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, Wilson et al., 2019, 'The GOGREEN Survey: The Relationship between Quenching, Morphological Transformation and Size Growth of Satellite Galaxies', 1.0, European Space Agency, https://doi.org/10.5270/esa-sibitnu