A Compact High Velocity Cloud near the Magellanic Stream: Metallicity and Small-scale Structure
Agnostic stacking of intergalactic doublet absorption: measuring the Ne VIII population
An HST/COS survey of molecular hydrogen in DLAs & sub-DLAs at z < 1: molecular fraction and excitation temperature
An HST/COS Survey of the Low-redshift Intergalactic Medium. I. Survey, Methodology, and Overall Results
An Ultraviolet Survey of Low-redshift Partial Lyman-limit Systems with the HST Cosmic Origins Spectrograph
COS-Weak: probing the CGM using analogues of weak Mg II absorbers at z < 0.3
HST/COS Detection of Deuterated Molecular Hydrogen in a Damped Lya System at z = 0.18
HST/COS Observations of Thirteen New He II Quasars
Identifying Circumgalactic Medium Absorption in QSO Spectra: A Bayesian Approach
Identifying H I Emission and UV Absorber Associations near the Magellanic Stream
New Measurements of the Lya Forest Continuum and Effective Optical Depth with LyCAN and DESI Y1 Data
On the connection between the metal-enriched intergalactic medium and galaxies: an O VI-galaxy cross-correlation study at z < 1
Reporting a deficit of intrinsic N V absorbers in core-dominated radio-loud quasars
Role of ionizing background and galactic feedback in the redshift space clustering of O VI absorbers in hydrodynamical simulations
The COS/UVES Absorption Survey of the Magellanic Stream. III. Ionization, Total Mass, and Inflow Rate onto the Milky Way
The Low-redshift Intergalactic Medium as Seen in Archival Legacy HST/STIS and FUSE Data
The Metagalactic Ionizing Background: A Crisis in UV Photon Production or Incorrect Galaxy Escape Fractions?
The power spectrum of the Lyman-a Forest at z < 0.5
Tracing the Cosmic Metal Evolution in the Low-redshift Intergalactic Medium
Instrument
COS, COS/FUV, COS/NUV
Temporal Coverage
2011-06-23T16:36:32Z/2011-06-29T23:32:03Z
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.
