Andromedas Parachute: Time Delays and Hubble Constant
A Taxonomy for the Configurations of Quadruply Lensed Quasars
Even Simpler Modeling of Quadruply Lensed Quasars (and Random Quartets) Using Witts Hyperbola
First black hole mass estimation for the quadruple lensed system WGD2038-4008
Gaia GraL: Gaia DR2 gravitational lens systems - VIII. A radio census of lensed systems
Gravitational Lens System PS J0147+4630 (Andromedas Parachute): Main Lensing Galaxy and Optical Variability of the Quasar Images
Is every strong lens model unhappy in its own way? Uniform modelling of a sample of 13 quadruply+ imaged quasars
STRIDES: a 3.9 per cent measurement of the Hubble constant from the strong lens system DES J0408-5354
STRIDES: automated uniform models for 30 quadruply imaged quasars
TDCOSMO. IX. Systematic comparison between lens modelling software programs: Time-delay prediction for WGD 2038-4008
TDCOSMO. X. Automated modeling of nine strongly lensed quasars and comparison between lens-modeling software
TDCOSMO. XI. New lensing galaxy redshift and velocity dispersion measurements from Keck spectroscopy of eight lensed quasar systems
TDCOSMO: XVI. Measurement of the Hubble constant from the lensed quasar WGD 2038-4008
The impact of satellite trails on Hubble Space Telescope observations
What Makes Quadruply Lensed Quasars Quadruple?
Instrument
WFC3/IR, WFC3/UVIS
Temporal Coverage
2017-08-29T12:19:21Z/2018-08-15T14:19:39Z
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, Treu comma Tommaso L., 2019, 'Probing the dark universe with quadruply imaged quasars', 1.0, European Space Agency, https://doi.org/10.5270/esa-7mrf0bg
