Agnostic stacking of intergalactic doublet absorption: measuring the Ne VIII population
A Massive Runaway Star from 30 Doradus
An HST/COS Survey of the Low-redshift Intergalactic Medium. I. Survey, Methodology, and Overall Results
Commissioning of the cosmic origins spectrograph on the Hubble Space Telescope: an overview of COS servicing mission observatory verification
Diagnosing galactic feedback with line broadening in the low-redshift Lya forest
Identifying Circumgalactic Medium Absorption in QSO Spectra: A Bayesian Approach
Mining circumgalactic baryons in the low-redshift universe
Nearby Galaxy Filaments and the Ly-alpha Forest: Confronting Simulations and the UV Background with Observations
Redshift space three-point correlation function of IGM at z < 0.48
Role of ionizing background and galactic feedback in the redshift space clustering of O VI absorbers in hydrodynamical simulations
The effect of stellar and AGN feedback on the low-redshift Lyman a forest in the Sherwood simulation suite
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 VLT-FLAMES Tarantula Survey. XVII. Physical and wind properties of massive stars at the top of the main sequence
Tracing the Cosmic Metal Evolution in the Low-redshift Intergalactic Medium
Instrument
COS/FUV, COS/NUV
Temporal Coverage
2009-07-20T17:55:33Z/2009-08-25T11:49:41Z
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, Hartig comma George, 2009, 'COS FUV Optics Alignment and Focus', 1.0, European Space Agency, https://doi.org/10.5270/esa-a41b8yw
