First constraints on small-scale non-Gaussianity from UV galaxy luminosity functions
First light and reionization epoch simulations (FLARES) X III: the lyman-continuum emission of high-redshift galaxies
Galaxy Stellar Mass Functions from z 10 to z 6 using the Deepest Spitzer/Infrared Array Camera Data: No Significant Evolution in the Stellar-to-halo Mass Ratio of Galaxies in the First Gigayear of Cosmic Time
Nature and Nurture? Comparing Lya Detections in UV-bright and Fainter O III+Hb Emitters at z 8 with Keck/MOSFIRE
Non-detection of post-eclipse changes in Ios Jupiter-facing atmosphere: Evidence for volcanic support?
The Ha Luminosity Function of Galaxies at z 4.5
UV Luminosity Functions at Redshifts z ~ 4 to z ~ 10: 10,000 Galaxies from HST Legacy Fields
Instrument
COS, COS/FUV, COS/NUV
Temporal Coverage
2011-12-05T06:49:41Z/2012-01-11T11:41:08Z
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, Green et al., 2013, 'COS-GTO: Io's Atmospheric Response to Eclipse', 1.0, European Space Agency, https://doi.org/10.5270/esa-ivq4bs0
