ARGOS at the LBT. Binocular laser guided ground-layer adaptive optics
PASSAGES: The Wide-ranging, Extreme Intrinsic Properties of Planck-selected, Lensed Dusty Star-forming Galaxies
Plancks dusty GEMS. III. A massive lensing galaxy with a bottom-heavy stellar initial mass function at z = 1.5
Plancks Dusty GEMS. VII. Atomic carbon and molecular gas in dusty starburst galaxies at z = 2 to 4
Plancks dusty GEMS. V. Molecular wind and clump stability in a strongly lensed star-forming galaxy at z = 2.2
PLCK G165.7+67.0: Analysis of a Massive Lensing Cluster in a Hubble Space Telescope Census of Submillimeter Giant Arcs Selected Using Planck/Herschel
Possible Ongoing Merger Discovered by Photometry and Spectroscopy in the Field of the Galaxy Cluster PLCK G165.7+67.0
Spectroscopy of the supernova H0pe host galaxy at redshift 1.78
The JWST Discovery of the Triply Imaged Type Ia Supernova H0pe and Observations of the Galaxy Cluster PLCK G165.7+67.0
Instrument
WFC3, WFC3/IR
Temporal Coverage
2015-12-25T17:54:18Z/2016-07-06T10:39:16Z
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, Frye et al., 2017, 'The Planck Dusty Gravitationally Enhanced subMillimeter Sources (GEMS)', 1.0, European Space Agency, https://doi.org/10.5270/esa-cu4y9b7
