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
HST/COS Observations of the Warm Ionized Gaseous Halo of NGC 891
Identifying Circumgalactic Medium Absorption in QSO Spectra: A Bayesian Approach
Improving blazar redshift constraints with the edge of the Ly a forest: 1ES 1553+113 and implications for observations of the WHIM
Measurement of redshift-space two- and three-point correlation of Lya absorbers at 1.7 < z < 3.5: implications on evolution of the physical properties of IGM
On the Redshift of the Very High Energy Blazar 3C 66A
Role of ionizing background and galactic feedback in the redshift space clustering of O VI absorbers in hydrodynamical simulations
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
Temporal Coverage
2012-11-08T13:56:51Z/2012-11-08T17:51:34Z
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, Furniss comma Amy Kathryn, 2013, 'Determining the Redshift of the Blazar 3C 66A for Studies of the Extragalactic Background Light', 1.0, European Space Agency, https://doi.org/10.5270/esa-q8thmdk