Agnostic stacking of intergalactic doublet absorption: measuring the Ne VIII population
An HST/COS Survey of the Low-redshift Intergalactic Medium. I. Survey, Methodology, and Overall Results
COS-Weak: probing the CGM using analogues of weak Mg II absorbers at z < 0.3
Detection of low-metallicity warm plasma in a galaxy overdensity environment at z ~ 0.2
Identifying Circumgalactic Medium Absorption in QSO Spectra: A Bayesian Approach
Mining circumgalactic baryons in the low-redshift universe
Role of ionizing background and galactic feedback in the redshift space clustering of O VI absorbers in hydrodynamical simulations
SuperBoRG: Exploration of Point Sources at z ~ 8 in HST Parallel Fields
SuperBoRG: Search for the Brightest of Reionizing Galaxies and Quasars in HST Parallel Imaging Data
The Brightest of Reionizing Galaxies Survey: Constraints on the Bright End of the z ~ 8 Luminosity Function
The impact of satellite trails on Hubble Space Telescope observations
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
Ultraviolet Emission-line Correlations in HST/COS Spectra of Active Galactic Nuclei: Single-epoch Black Hole Masses
Instrument
COS, COS/FUV, COS/NUV, WFC3, WFC3/IR, WFC3/UVIS
Temporal Coverage
2011-04-14T19:57:37Z/2011-04-25T14:00:10Z
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, Green comma James Carswell, 2012, 'COS-GTO: Great Wall Tomography - Part 2', 1.0, European Space Agency, https://doi.org/10.5270/esa-e0bflfu
