A First Look at Spatially Resolved Balmer Decrements at 1.0 < z < 2.4 from JWST NIRISS Slitless Spectroscopy
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
An Extremely Compact, Low-mass Galaxy on its Way to Quiescence at z = 5.2
A Steep Decline in the Galaxy Space Density beyond Redshift 9 in the CANUCS UV Luminosity Function
Bursty star formation and galaxy-galaxy interactions in low-mass galaxies 1 Gyr after the Big Bang
CANUCS: UV and ionizing properties of dwarf star-forming galaxies at z 5-7
Exposing Line Emission: The Systematic Differences of Measuring Galaxy Stellar Masses with JWST NIRCam Medium versus Wide Band Photometry
Insight from JWST/Near Infrared Camera into galaxy overdensities around bright Lyman-alpha emitters during reionization: implications for ionized bubbles at z 9
JWST catches the assembly of a z 5 ultra-low-mass galaxy
Spectroscopy from Photometry: A Population of Extreme Emission Line Galaxies at 1.7 z 6.7 Selected with JWST Medium Band Filters
The ALMA-ALPAKA survey. I. High-resolution CO and CI kinematics of star-forming galaxies at z = 0.5-3.5
When, where, and how star formation happens in a galaxy pair at cosmic noon using CANUCS JWST/NIRISS grism spectroscopy
LCDM not dead yet: massive high-z Balmer break galaxies are less common than previously reported
Instrument
ACS/WFC, WFC3/UVIS
Temporal Coverage
2021-10-13T16:38:23Z/2023-08-25T10:43:12Z
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, Bradac comma Marusa, 2023, 'The Final Frontier: HST and JWST Exploration of Galaxies Across Cosmic Epochs', 1.0, European Space Agency, https://doi.org/10.57780/esa-voexo3f