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
Luminous Lya Emitters with Very Blue UV-continuum Slopes at Redshift 5.7 <= z <= 6.6
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
Instrument
WFC3/IR
Temporal Coverage
2017-11-12T00:50:48Z/2018-11-26T21:17:07Z
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, Jiang et al., 2018, 'Spectroscopically-Confirmed z > 6 Galaxies with Extremely Blue UV Slopes: Possible Pop III dominated targets for JWST spectroscopy', 1.0, European Space Agency, https://doi.org/10.5270/esa-eg5226q
Rights
Data hosted in the ESA Space Science Archives are distributed under the CC BY-NC 3.0 IGO license.