Accelerating galaxy winds during the big bang of starbursts
Early Results from GLASS-JWST. XXII. Rest-frame UV-Optical Spectral Properties of Lya Emitting Galaxies at 3 < z < 6
Kinematics and Optical Depth in the Green Peas: Suppressed Superwinds in Candidate LyC Emitters
Neutral Gas Properties and Lya Escape in Extreme Green Pea Galaxies
New Insights on Lya and Lyman Continuum Radiative Transfer in the Greenest Peas
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
The Lyman Alpha Spectral Database (LASD)
The origin of the escape of Lyman a and ionizing photons in Lyman continuum emitters
zELDA: fitting Lyman alpha line profiles using deep learning
Instrument
COS, COS/FUV, COS/NUV
Temporal Coverage
2015-12-02T15:56:18Z/2017-02-02T22:13:02Z
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, Jaskot et al., 2018, 'LyC, Ly-alpha, and Low Ions in Green Peas: Diagnostics of Optical Depth, Geometry, and Outflows', 1.0, European Space Agency, https://doi.org/10.5270/esa-84l6xtl
