An HST/COS survey of molecular hydrogen in DLAs & sub-DLAs at z < 1: molecular fraction and excitation temperature
Atomic and molecular gas from the epoch of reionisation down to redshift 2
COS-Weak: probing the CGM using analogues of weak Mg II absorbers at z < 0.3
New Perspective on Galaxy Outflows from the First Detection of Both Intrinsic and Traverse Metal-line Absorption
Probing the dynamical state, baryon content, and multiphase nature of galaxy clusters with bright background QSOs
The COS/UVES Absorption Survey of the Magellanic Stream. III. Ionization, Total Mass, and Inflow Rate onto the Milky Way
The statistical properties of neutral gas at z < 1.65 from UV measurements of Damped Lyman Alpha systems
Instrument
COS, COS/FUV, COS/NUV
Temporal Coverage
2011-10-29T05:57:45Z/2013-05-19T05:09:44Z
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, Nestor comma Daniel B., 2014, 'A Survey of Atomic Hydrogen at 0.2 < z < 0.4', 1.0, European Space Agency, https://doi.org/10.5270/esa-8wcne1o