ALMA constraints on star-forming gas in a prototypical z = 1.5 clumpy galaxy: the dearth of CO(5-4) emission from UV-bright clumps
A Remarkably Luminous Galaxy at z=11.1 Measured with Hubble Space Telescope Grism Spectroscopy
CEERS Key Paper. VIII. Emission-line Ratios from NIRSpec and NIRCam Wide-Field Slitless Spectroscopy at z > 2
CLEAR: Emission-line Ratios at Cosmic High Noon
CLEAR: Spatially Resolved Emission Lines and Active Galactic Nuclei at 0.6 < z < 1.3
CLEAR: Survey Overview, Data Analysis, and Products
CLEAR: The Gas-phase Metallicity Gradients of Star-forming Galaxies at 0.6 < z < 2.6
Exploring the Gas-phase Metallicity Gradients of Star-forming Galaxies at Cosmic Noon
Massive Dead Galaxies at z ~ 2 with HST Grism Spectroscopy. I. Star Formation Histories and Metallicity Enrichment
The Bursty Star Formation Histories of Low-mass Galaxies at 0.4 < z < 1 Revealed by Star Formation Rates Measured From Hb and FUV
The HDUV Survey: Six Lyman Continuum Emitter Candidates at z ~ 2 Revealed by HST UV Imaging
The impact of satellite trails on Hubble Space Telescope observations
The VANDELS survey: a measurement of the average Lyman-continuum escape fraction of star-forming galaxies at z = 3.5
Instrument
ACS, ACS/WFC, WFC3, WFC3/IR
Temporal Coverage
2015-02-11T10:46:43Z/2015-04-03T22:25:54Z
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, Oesch comma Pascal, 2016, 'A Spectroscopic Redshift for the Most Luminous Galaxy Candidate at z~10', 1.0, European Space Agency, https://doi.org/10.5270/esa-8yjgl0d