Far-ultraviolet Spectra of Main-sequence O Stars at Extremely Low Metallicity
METAL-Z: Measuring Dust Depletion in Low-metallicity Dwarf Galaxies
Observations of Extremely Metal-poor O Stars: Weak Winds and Constraints for Evolution Models
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
The UV Legacy Library of Young Stars as Essential Standards (ULLYSES) Large Directors Discretionary Program with Hubble. I. Goals, Design, and Initial Results
X-Shooting ULLYSES: Massive stars at low metallicity. I. Project description
X-Shooting ULLYSES: Massive Stars at low metallicity: IX. Empirical constraints on mass-loss rates and clumping parameters for OB supergiants in the Large Magellanic Cloud
X-Shooting ULLYSES: Massive stars at low metallicity: V. Effect of metallicity on surface abundances of O stars
X-Shooting ULLYSES: Massive stars at low metallicity: VIII. Stellar and wind parameters of newly revealed stripped stars in Be binaries
X-Shooting ULLYSES: Massive stars at low metallicity: XIII. Testing the bi-stability jump in the Large Magellanic Cloud
Instrument
COS, COS/FUV, COS/NUV
Temporal Coverage
2020-04-11T08:53:32Z/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, 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