A Census of Photometrically Selected Little Red Dots at 4 < z < 9 in JWST Blank Fields
An Atlas of Color-selected Quiescent Galaxies at z > 3 in Public JWST Fields
Dust in Little Red Dots
Even redder than we knew: Color and AV evolution up to z = 2.5 from JWST/NIRCam photometry
Morphology of Galaxies in JWST Fields: Initial Distribution and Evolution of Galaxy Morphology
The ALMA-CRISTAL survey: Resolved kinematic studies of main sequence star-forming galaxies at 4 < z < 6
The AURORA Survey: Multiple Balmer and Paschen Emission Lines for Individual Star-forming Galaxies at z = 1.5-4.4. I. A Diversity of Nebular Attenuation Curves and Evidence for Non-unity Dust Covering Fractions
The PANORAMIC Survey: Pure Parallel Wide Area Legacy Imaging with JWST/NIRCam
The Roles of Morphology and Environment on the Star Formation Rate-Stellar Mass Relation in COSMOS from 0 < z < 3.5
Instrument
WFC3/IR
Temporal Coverage
2018-03-08T02:40:23Z/2021-12-01T15:08:19Z
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, Suzuki et al., 2021, 'SUbaru Supernovae with Hubble Infrared (SUSHI)', 1.0, European Space Agency, https://doi.org/10.5270/esa-bcey5ty
Rights
Data hosted in the ESA Space Science Archives are distributed under the CC BY-NC 3.0 IGO license.