Early Results from GLASS-JWST. IV. Spatially Resolved Metallicity in a Low-mass z 3 Galaxy with NIRISS
First Census of Gas-phase Metallicity Gradients of Star-forming Galaxies in Overdense Environments at Cosmic Noon
The Mass-Metallicity Relation at Cosmic Noon in Overdense Environments: First Results from the MAMMOTH-Grism HST Slitless Spectroscopic Survey
What boost galaxy mergers in two massive galaxy protoclusters at z = 2.24?
Instrument
WFC3/IR
Temporal Coverage
2020-11-15T21:40:16Z/2022-11-13T06:03:06Z
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, Wang et al., 2023, 'WFC3 Spectroscopy of the Most Massive Galaxy Protoclusters at Cosmic Noon', 1.0, European Space Agency, https://doi.org/10.5270/esa-wkj5ar2