A gravitationally lensed supernova with an observable two-decade time delay
Cosmology with supernova Encore in the strong lensing cluster MACS J0138-2155: Photometry, cluster members, and lens mass model
Cosmology with supernova Encore in the strong lensing cluster MACS J0138-2155: Spectroscopy with MUSE
Resolving Quiescent Galaxies at z 2. II. Direct Measures of Rotational Support
Resolving Quiescent Galaxies at z 2. I. Search for Gravitationally Lensed Sources and Characterization of Their Structure, Stellar Populations, and Line Emission
The impact of satellite trails on Hubble Space Telescope observations
The PANORAMIC Survey: Pure Parallel Wide Area Legacy Imaging with JWST/NIRCam
The uncertain interstellar medium of high-redshift quiescent galaxies: Impact of methodology
UV Fluorescence Traces Gas and Lya Evolution in Protoplanetary Disks
Instrument
ACS, ACS/WFC, WFC3, WFC3/IR
Temporal Coverage
2016-07-18T23:14:50Z/2016-07-19T02:56:00Z
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, Newman et al., 2016, 'Resolving the Stellar Populations, Structure, and Kinematics of the NIR-Brightest Lensed Galaxy at z=2', 1.0, European Space Agency, https://doi.org/10.5270/esa-85agph5