Automated galaxy-galaxy strong lens modelling: No lens left behind
Detecting low-mass haloes with strong gravitational lensing I: the effect of data quality and lensing configuration
Low-mass halo perturbations in strong gravitational lenses at redshift z ~ 0.5 are consistent with CDM
Resolving on 100 pc scales the UV-continuum in Lyman-a emitters between redshift 2 and 3 with gravitational lensing
Rest-frame UV properties of luminous strong gravitationally lensed Lya emitters from the BELLS GALLERY Survey
Scanning for dark matter subhaloes in Hubble Space Telescope imaging of 54 strong lenses
The BOSS Emission-line Lens Survey. III. Strong Lensing of Lya Emitters by Individual Galaxies
The BOSS Emission-line Lens Survey. IV. Smooth Lens Models for the BELLS GALLERY Sample
The BOSS Emission-line Lens Survey. V. Morphology and Substructure of Lensed Lya Emitters at Redshift Z 2.5 in the BELLS GALLERY
The impact of satellite trails on Hubble Space Telescope observations
Using deep Residual Networks to search for galaxy-Ly a emitter lens candidates based on spectroscopic selection
Instrument
WFC3, WFC3/UVIS
Temporal Coverage
2015-11-16T08:32:10Z/2016-05-07T00:21:19Z
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, Bolton et al., 2016, 'Quantifying Cold Dark Matter Substructure with a Qualitatively New Gravitational Lens Sample', 1.0, European Space Agency, https://doi.org/10.5270/esa-rkn6a4y