An HST/COS survey of molecular hydrogen in DLAs & sub-DLAs at z < 1: molecular fraction and excitation temperature
Cloud-by-cloud multiphase investigation of the circumgalactic medium of low-redshift galaxies
Cold parsec-scale gas in a zabs ~ 0.1 sub-damped Lyman a with disparate H2 and 21-cm absorption
COS-Weak: probing the CGM using analogues of weak Mg II absorbers at z < 0.3
Discovery of extremely low-metallicity circumgalactic gas at z = 0.5 towards Q0454-220
Halo Mass Dependence of H I and O VI Absorption: Evidence for Differential Kinematics
Hubble Space Telescope Observations of Sub-damped Lya Absorbers at z < 0.5, and Implications for Galaxy Chemical Evolution
Probing the interstellar dust in galaxies over >10 Gyr of cosmic history
The COS/UVES Absorption Survey of the Magellanic Stream. III. Ionization, Total Mass, and Inflow Rate onto the Milky Way
Instrument
COS, COS/FUV, COS/NUV
Temporal Coverage
2012-03-10T20:30:18Z/2012-08-13T21:46:55Z
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, Kulkarni et al., 2013, 'Sub-damped Lyman-alpha Absorbers at z < 0.6: An Unexplored Terrain in the Quest for Cosmic Metals', 1.0, European Space Agency, https://doi.org/10.5270/esa-48s02xi