Accelerating galaxy winds during the big bang of starbursts
Diverse properties of Ly a emission in low-redshift compact star-forming galaxies with extremely high O III/O II ratios
Early Results from GLASS-JWST. XXII. Rest-frame UV-Optical Spectral Properties of Lya Emitting Galaxies at 3 < z < 6
On the Sizes of Ionized Bubbles Around Galaxies During the Reionization Epoch. The Spectral Shapes of the Lya Emission from Galaxies
Spectral Shapes of the Lya Emission from Galaxies. I. Blueshifted Emission and Intrinsic Invariance with Redshift
Spectral shapes of the Ly a emission from galaxies - II. The influence of stellar properties and nebular conditions on the emergent Ly a profiles
Instrument
COS, COS/FUV, COS/NUV
Temporal Coverage
2018-01-26T05:33:27Z/2019-02-25T12:14:39Z
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, Izotov comma Yuri I., 2019, 'Lyman alpha emission in nearby star-forming galaxies with the lowest metallicities and the highest [OIII]/[OII] ratios', 1.0, European Space Agency, https://doi.org/10.5270/esa-pnxy7do