ALMA Lensing Cluster Survey: Hubble Space Telescope and Spitzer Photometry of 33 Lensed Fields Built with CHArGE
ALMA Lensing Cluster Survey: Properties of Millimeter Galaxies Hosting X-Ray-detected Active Galactic Nuclei
Constraints on the Hubble constant from supernova Refsdals reappearance
Determining Cosmological-model-independent H 0 with Gravitationally Lensed Supernova Refsdal
GAUSSN: Bayesian time-delay estimation for strongly lensed supernovae
Insight from JWST/Near Infrared Camera into galaxy overdensities around bright Lyman-alpha emitters during reionization: implications for ionized bubbles at z 9
Searching for Highly Magnified Stars at Cosmological Distances: Discovery of a Redshift 0.94 Blue Supergiant in Archival Images of the Galaxy Cluster MACS J0416.1-2403
The ALMA-ALPAKA survey. I. High-resolution CO and CI kinematics of star-forming galaxies at z = 0.5-3.5
The impact of satellite trails on Hubble Space Telescope observations
The Magnificent Five Images of Supernova Refsdal: Time Delay and Magnification Measurements
Instrument
ACS, ACS/WFC, WFC3, WFC3/IR, WFC3/UVIS
Temporal Coverage
2016-11-28T17:34:35Z/2017-01-23T16:51:53Z
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, Kelly comma Patrick, 2017, 'A Hidden Potential Counterimage of a Highly Magnified Star at Redshift z=1.49', 1.0, European Space Agency, https://doi.org/10.5270/esa-pcv092f