AStroLens: automatic strong-lens modelling of X-ray selected galaxy clusters
Cosmic-CoNN: A Cosmic-Ray Detection Deep-learning Framework, Data Set, and Toolkit
deepCR: Cosmic Ray Rejection with Deep Learning
Generalized model-independent characterization of strong gravitational lenses VIII. Automated multiband feature detection to constrain local lens properties
Hamiltons Object - a clumpy galaxy straddling the gravitational caustic of a galaxy cluster: constraints on dark matter clumping
Harnessing the Hubble Space Telescope Archives: A Catalog of 21,926 Interacting Galaxies
Non-parametric deprojection of NIKA SZ observations: Pressure distribution in the Planck-discovered cluster PSZ1 G045.85+57.71
The impact of satellite trails on Hubble Space Telescope observations
Instrument
ACS, ACS/WFC, WFC3, WFC3/IR
Temporal Coverage
2014-10-08T21:08:04Z/2015-10-01T15:27:01Z
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, Ebeling comma Harald, 2015, 'Beyond MACS: A Snapshot Survey of the Most Massive Clusters of Galaxies at z>0.5', 1.0, European Space Agency, https://doi.org/10.5270/esa-pz5k66s