Agnostic stacking of intergalactic doublet absorption: measuring the Ne VIII population
An HST/COS Observation of Broad Lya Emission and Associated Absorption Lines of the BL Lacertae Object H 2356-309
An HST/COS Survey of the Low-redshift Intergalactic Medium. I. Survey, Methodology, and Overall Results
Identifying Circumgalactic Medium Absorption in QSO Spectra: A Bayesian Approach
Identifying H I Emission and UV Absorber Associations near the Magellanic Stream
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
Probing the Southern Fermi Bubble in Ultraviolet Absorption Using Distant AGNs
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
The Signature of the Northern Galactic Center Region in Low-velocity UV Absorption
Instrument
COS, COS/FUV, COS/NUV
Temporal Coverage
2013-06-15T17:12:27Z/2013-06-20T00:05:25Z
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, Buote et al., 2014, 'UV Spectroscopy of the H 2356-309 Sightline: Confirming the X-ray WHIM Absorber and Testing the Structure Formation Theory', 1.0, European Space Agency, https://doi.org/10.5270/esa-ixihs9h