Characterizing circumgalactic gas around massive ellipticals at z 0.4 - III. The galactic environment of a chemically pristine Lyman limit absorber
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
The Cosmic Ultraviolet Baryon Survey: Empirical Characterization of Turbulence in the Cool Circumgalactic Medium
Instrument
COS, COS/FUV, COS/NUV
Temporal Coverage
2016-03-30T16:28:43Z/2017-01-06T02:10:14Z
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, Chen comma Hsiao-Wen, 2018, 'Characterizing Circumgalactic Gas around Passive Galaxies', 1.0, European Space Agency, https://doi.org/10.57780/esa-59y7m24