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
COS-Weak: probing the CGM using analogues of weak Mg II absorbers at z < 0.3
Discovery of multiphase cold accretion in a massive galaxy at z = 0.7
Halo Mass Dependence of H I and O VI Absorption: Evidence for Differential Kinematics
MAGIICAT VI. The Mg II Intragroup Medium Is Kinematically Complex
Quenched Cold Accretion of a Large-scale Metal-poor Filament due to Virial Shocking in the Halo of a Massive z = 0.7 Galaxy
Relationship between the Metallicity of the Circumgalactic Medium and Galaxy Orientation
The Azimuthal Dependence of Outflows and Accretion Detected Using O VI Absorption
The Highly Ionized Circumgalactic Medium is Kinematically Uniform around Galaxies
The Impact of the Group Environment on the O VI Circumgalactic Medium
The Relationship between Galaxy ISM and Circumgalactic Gas Metallicities
Instrument
COS, COS/FUV, COS/NUV
Temporal Coverage
2010-05-26T09:11:35Z/2010-06-26T05:57:33Z
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, Churchill comma Christopher W., 2011, 'Detailed Probing of a 3000 km/s Ly-alpha + Metal Line Absorption Complex Near Two Galaxies at z=0.67', 1.0, European Space Agency, https://doi.org/10.5270/esa-444udrc