A strong lensing model of the galaxy cluster PSZ1 G311.65-18.48
Clues on the presence and segregation of very massive stars in the Sunburst Lyman-continuum cluster at z = 2.37
Godzilla, a monster lurks in the Sunburst galaxy
High star cluster formation efficiency in the strongly lensed Sunburst Lyman-continuum galaxy at z = 2.37
Nitrogen-enriched, Highly Pressurized Nebular Clouds Surrounding a Super Star Cluster at Cosmic Noon
Slicing the cool circumgalactic medium along the major axis of a star-forming galaxy at z = 0.7
Small Region, Big Impact: Highly Anisotropic Lyman-continuum Escape from a Compact Starburst Region with Extreme Physical Properties
Statistical microlensing towards magnified high-redshift star clusters
The Cosmic Telescope That Lenses the Sunburst Arc, PSZ1 G311.65-18.48: Strong Gravitational Lensing Model and Source Plane Analysis
The impact of satellite trails on Hubble Space Telescope observations
Instrument
WFC3/IR, WFC3/UVIS
Temporal Coverage
2018-09-27T01:43:28Z/2019-04-30T15:56:51Z
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, Bayliss et al., 2019, 'Does the Brightest Strongly Lensed Galaxy Contain An AGN?', 1.0, European Space Agency, https://doi.org/10.5270/esa-uclaec5