Absorption-line Abundances in the SMC-like Galaxy UGC 5282: Evidence of ISM Dilution from Inflows on Kiloparsec Scales
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
Diagnosing galactic feedback with line broadening in the low-redshift Lya forest
Nearby Galaxy Filaments and the Ly-alpha Forest: Confronting Simulations and the UV Background with Observations
Probing Large Galaxy Halos at Z ~ 0 with Automated Lya-absorption Matching
Small-scale Properties of Atomic Gas in Extended Disks of Galaxies
The effect of stellar and AGN feedback on the low-redshift Lyman a forest in the Sherwood simulation suite
The gas and stellar mass of low-redshift damped Lyman-a absorbers
The Signature of the Northern Galactic Center Region in Low-velocity UV Absorption
Instrument
COS, COS/FUV, COS/NUV
Temporal Coverage
2011-10-26T22:01:19Z/2013-03-11T13:24:12Z
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, Bowen comma David V., 2014, 'QSO Absorption Line Systems from Dwarf Galaxies', 1.0, European Space Agency, https://doi.org/10.5270/esa-4wb2e6g