Characterizing circumgalactic gas around massive ellipticals at z ~ 0.4 - I. Initial results
Characterizing circumgalactic gas around massive ellipticals at z ~ 0.4 - II. Physical properties and elemental abundances
Cool circumgalactic gas of passive galaxies from cosmological inflow
Probing the physicochemical properties of the Leo Ring and the Leo I group
The Cosmic Ultraviolet Baryon Survey: Empirical Characterization of Turbulence in the Cool Circumgalactic Medium
Warm-hot gas in X-ray bright galaxy clusters and the H I-deficient circumgalactic medium in dense environments
Instrument
COS, COS/FUV, COS/NUV
Temporal Coverage
2014-12-20T11:08:25Z/2015-11-09T23:24:24Z
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, Tejos comma Nicolas, 2016, 'Characterizing the cool and warm-hot intergalactic medium in clusters at z < 0.4', 1.0, European Space Agency, https://doi.org/10.5270/esa-cnrrhbq