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
Identifying Circumgalactic Medium Absorption in QSO Spectra: A Bayesian Approach
Jet feedback and the photon underproduction crisis in SIMBA
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
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, COS/NUV
Temporal Coverage
2013-04-26T05:48:27Z/2013-12-23T19:11:35Z
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, Stocke comma John Thomas, 2014, 'Probing Weak Intergalactic Absorption with Flaring Blazar Spectra 2', 1.0, European Space Agency, https://doi.org/10.5270/esa-p8yyxwz
