Extremely metal-poor galaxies with HST/COS: laboratories for models of low-metallicity massive stars and high-redshift galaxies
High-mass X-ray binaries in nearby metal-poor galaxies: on the contribution to nebular He II emission
Modeling the High-energy Ionizing Output from Simple Stellar and X-Ray Binary Populations
Shining a Light on the Connections between Galactic Outflows Seen in Absorption and Emission Lines
Instrument
COS, COS/FUV, COS/NUV
Temporal Coverage
2017-06-24T03:56:49Z/2018-03-10T03:07:09Z
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, Stark, 2019, 'Extremely Metal Poor Galaxies with HST/COS: Completing the Groundwork for JWST', 1.0, European Space Agency, https://doi.org/10.5270/esa-smpqtzc
Rights
Data hosted in the ESA Space Science Archives are distributed under the CC BY-NC 3.0 IGO license.