Agnostic stacking of intergalactic doublet absorption: measuring the Ne VIII population
A new multifield determination of the galaxy luminosity function at z = 7-9 incorporating the 2012 Hubble Ultra-Deep Field imaging
An HST/COS Survey of the Low-redshift Intergalactic Medium. I. Survey, Methodology, and Overall Results
A Redshift-independent Efficiency Model: Star Formation and Stellar Masses in Dark Matter Halos at z 4
Can early dark energy be probed by the high-redshift galaxy abundance?
Digging into the Ultraviolet Luminosity Functions of Galaxies at High Redshifts: Galaxies Evolution, Reionization, and Cosmological Parameters
Extreme ultraviolet quasar colours from GALEX observations of the SDSS DR14Q catalogue
First constraints on small-scale non-Gaussianity from UV galaxy luminosity functions
First light and reionization epoch simulations (FLARES) X III: the lyman-continuum emission of high-redshift galaxies
Galaxy Stellar Mass Functions from z 10 to z 6 using the Deepest Spitzer/Infrared Array Camera Data: No Significant Evolution in the Stellar-to-halo Mass Ratio of Galaxies in the First Gigayear of Cosmic Time
HST-COS Observations of AGNs. II. Extended Survey of Ultraviolet Composite Spectra from 159 Active Galactic Nuclei
HST-COS Observations of AGNs. I. Ultraviolet Composite Spectra of the Ionizing Continuum and Emission Lines
Identifying Circumgalactic Medium Absorption in QSO Spectra: A Bayesian Approach
Mining circumgalactic baryons in the low-redshift universe
Nature and Nurture? Comparing Lya Detections in UV-bright and Fainter O III+Hb Emitters at z 8 with Keck/MOSFIRE
Ne v emission from a faint epoch of reionization-era galaxy: evidence for a narrow-line intermediate-mass black hole
On the connection between the metal-enriched intergalactic medium and galaxies: an O VI-galaxy cross-correlation study at z < 1
Redshift space three-point correlation function of IGM at z < 0.48
Reporting a deficit of intrinsic N V absorbers in core-dominated radio-loud quasars
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
Testing the near-far connection with FIRE simulations: inferring the stellar mass function of the proto-Local Group at z > 6 using the fossil record of present-day galaxies
The Brightest of Reionizing Galaxies Survey: Constraints on the Bright End of the z ~ 8 Luminosity Function
The Ha Luminosity Function of Galaxies at z 4.5
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 Opacity of the Intergalactic Medium Measured along Quasar Sightlines at z ~ 6
The Physical Properties of Luminous z 8 Galaxies and Implications for the Cosmic Star Formation Rate Density from 0.35 deg2 of (Pure-)Parallel HST Observations
The power spectrum of the Lyman-a Forest at z < 0.5
The role of black hole feedback on galaxy star formation and the degeneracy with halo quenching
The size and shape of the Milky Way disc and halo from M-type brown dwarfs in the BoRG survey
The UV luminosity functions of bright z > 8 galaxies: determination from 0.41 deg2 of HST observations along 300 independent sightlines
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
UV Luminosity Functions at Redshifts z ~ 4 to z ~ 10: 10,000 Galaxies from HST Legacy Fields
Instrument
COS, COS/FUV, WFC3, WFC3/IR, WFC3/UVIS
Temporal Coverage
2010-01-07T17:12:41Z/2010-06-02T19:16:10Z
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.
