A GMOS/IFU Study of Jellyfish Galaxies in Massive Clusters
Exemplary Merging Clusters: Weak-lensing and X-Ray Analysis of the Double Radio Relic, Merging Galaxy Clusters MACS J1752.0+4440 and ZWCL 1856.8+6616
MC2: Mapping the Dark Matter Distribution of the Toothbrush Cluster RX J0603.3+4214 with Hubble Space Telescope and Subaru Weak Lensing
MC2: Multiwavelength and Dynamical Analysis of the Merging Galaxy Cluster ZwCl 0008.8+5215: An Older and Less Massive Bullet Cluster
Merging Cluster Collaboration: A Panchromatic Atlas of Radio Relic Mergers
Merging Cluster Collaboration: Optical and Spectroscopic Survey of a Radio-selected Sample of 29 Merging Galaxy Clusters
RELICS: Reionization Lensing Cluster Survey
The impact of satellite trails on Hubble Space Telescope observations
The ultraviolet continuum slopes of high-redshift galaxies: evidence for the emergence of dust-free stellar populations at z > 10
Instrument
ACS, ACS/WFC, WFC3, WFC3/UVIS
Temporal Coverage
2013-10-10T00:14:39Z/2014-10-26T04:19:35Z
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, Wittman comma David, 2015, 'Probing Dark Matter with a New Class of Merging Clusters', 1.0, European Space Agency, https://doi.org/10.5270/esa-h6982kc