A test for skewed distributions of dark matter, and a possible detection in galaxy cluster Abell 3827
Coordinated Assembly of Brightest Cluster Galaxies
Dark matter dynamics in Abell 3827: new data consistent with standard cold dark matter
Geometric Support for Dark Matter by an Unaligned Einstein Ring in A3827
Much ado about no offset - characterizing the anomalous multiple-image configuration and the model-driven displacement between light and mass in the multiplane strong lens Abell 3827
The behaviour of dark matter associated with four bright cluster galaxies in the 10 kpc core of Abell 3827
The impact of satellite trails on Hubble Space Telescope observations
Instrument
ACS, ACS/WFC, WFC3, WFC3/IR, WFC3/UVIS
Temporal Coverage
2013-08-16T17:21:02Z/2013-10-06T08:53:37Z
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, Massey et al., 2014, 'Longevity of dark matter substructure in Abell 3827', 1.0, European Space Agency, https://doi.org/10.5270/esa-7ewc0i7