A morphological analysis of the galaxy cluster XLSSC 122 at z = 1.98
An Active Galaxy Cluster Merger at Cosmic Noon Revealed by JWST Weak Lensing and Multiwavelength Probes
Exploring the Masses of the Two Most Distant Gravitational Lensing Clusters at Cosmic Noon
Intracluster light in the core of z 2 galaxy proto-clusters
Lessons on early structure formation from a mature galaxy cluster observed at cosmic noon
Obscured star formation in clusters at z = 1.6-2.0: massive galaxy formation and the reversal of the star formation-density relation
Quiescent galaxies in a virialized cluster at redshift 2: evidence for accelerated size growth
Spectroscopic confirmation of a mature galaxy cluster at a redshift of 2
The XXL survey. XLIX. Linking the members star formation histories to the cluster mass assembly in the z = 1.98 galaxy cluster XLSSC 122
XLSSC 122 caught in the act of growing up: Spatially resolved SZ observations of a z = 1.98 galaxy cluster
Instrument
WFC3/IR
Temporal Coverage
2017-11-04T07:54:48Z/2018-01-13T03:41:59Z
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, Canning et al., 2018, 'HST Grism observations of the highest-z massive galaxy cluster', 1.0, European Space Agency, https://doi.org/10.5270/esa-9xgcpcf
Rights
Data hosted in the ESA Space Science Archives are distributed under the CC BY-NC 3.0 IGO license.