Absorption Line Search through Three Local Group Dwarf Galaxy Halos
COS-Weak: probing the CGM using analogues of weak Mg II absorbers at z < 0.3
Fast Outflowing Warm Absorbers in Narrow-line Seyfert 1 Galaxy PG 1001+054 Revealed by HST/COS Spectra
New Measurements of the Lya Forest Continuum and Effective Optical Depth with LyCAN and DESI Y1 Data
Probing Large Galaxy Halos at Z ~ 0 with Automated Lya-absorption Matching
Reporting a deficit of intrinsic N V absorbers in core-dominated radio-loud quasars
The COS-legacy survey of C IV absorbers: properties and origins of the intervening systems
Instrument
COS, COS/FUV, COS/NUV
Temporal Coverage
2014-04-13T04:49:33Z/2014-11-23T11:32:22Z
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, Bregman, 2015, 'The Missing Baryons Around Nearby Dwarf Galaxies', 1.0, European Space Agency, https://doi.org/10.5270/esa-dnmru71
Rights
Data hosted in the ESA Space Science Archives are distributed under the CC BY-NC 3.0 IGO license.