An HST/COS legacy survey of intervening Si III absorption in the extended gaseous halos of low-redshift galaxies
Evidence for a Rotational Component in the Circumgalactic Medium of Nearby Galaxies
Far-ultraviolet Spectroscopy of Active Galactic Nuclei with ASTROSAT/UVIT
Hot Gas in Galaxy Halos Traced by Coronal Broad Lya Absorbers
Measuring cosmic density of neutral hydrogen via stacking the DINGO-VLA data
New Measurements of the Lya Forest Continuum and Effective Optical Depth with LyCAN and DESI Y1 Data
Observations of a Magellanic Corona
Probing Large Galaxy Halos at Z ~ 0 with Automated Lya-absorption Matching
Probing the Southern Fermi Bubble in Ultraviolet Absorption Using Distant AGNs
Reporting a deficit of intrinsic N V absorbers in core-dominated radio-loud quasars
Signatures of gas flows - I. Connecting the kinematics of the H I circumgalactic medium to galaxy rotation
Studying the gaseous outskirts of galaxy groups with coherent Ly a absorption patterns
The H I Content of the Universe Over the Past 10 GYRS
The Signature of the Northern Galactic Center Region in Low-velocity UV Absorption
The Truncated Circumgalactic Medium of the Large Magellanic Cloud
Instrument
COS, COS/FUV, COS/NUV
Temporal Coverage
2012-11-07T07:39:07Z/2013-08-21T00:11:38Z
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, Jenkins, 2014, 'The Physical and Dynamical Properties of Gas that Molds the Fermi Bubbles', 1.0, European Space Agency, https://doi.org/10.5270/esa-p8fgkeb
Rights
Data hosted in the ESA Space Science Archives are distributed under the CC BY-NC 3.0 IGO license.