A Comparison of UV and Optical Metallicities in Star-forming Galaxies
Extremely metal-poor galaxies with HST/COS: laboratories for models of low-metallicity massive stars and high-redshift galaxies
The Chemical Evolution of Carbon, Nitrogen, and Oxygen in Metal-poor Dwarf Galaxies
Instrument
COS, COS/FUV, COS/NUV
Temporal Coverage
2017-01-11T05:08:02Z/2017-05-26T12:49:13Z
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, Berg et al., 2018, 'The Evolution of C/O in Low Metallicity Dwarf Galaxies', 1.0, European Space Agency, https://doi.org/10.5270/esa-kmu8bxl