Far-ultraviolet Spectra of Main-sequence O Stars at Extremely Low Metallicity
METAL-Z: Measuring Dust Depletion in Low-metallicity Dwarf Galaxies
Optically thick structure in early B-type supergiant stellar winds at low metallicities
The Ionizing Spectra of Extremely Metal-poor O Stars: Constraints from the Only H II Region in Leo P
X-Shooting ULLYSES: Massive stars at low metallicity. I. Project description
X-Shooting ULLYSES: Massive stars at low metallicity: V. Effect of metallicity on surface abundances of O stars
Instrument
COS, COS/FUV, COS/NUV
Temporal Coverage
2020-04-11T07:17:33Z/2020-06-26T12:06:03Z
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, Chisholm et al., 2020, 'Constraining the Stellar Astrophysics Powering Cosmic Reionization: Spectral Templates of Extremely Low-metallicity Main-sequence O-stars', 1.0, European Space Agency, https://doi.org/10.5270/esa-sbniq62