Accelerating galaxy winds during the big bang of starbursts
A Semi-analytical Line Transfer Model to Interpret the Spectra of Galaxy Outflows
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
The impact of satellite trails on Hubble Space Telescope observations
The Lyman Alpha Spectral Database (LASD)
zELDA: fitting Lyman alpha line profiles using deep learning
Instrument
COS, COS/FUV, COS/NUV, WFC3, WFC3/UVIS
Temporal Coverage
2011-02-17T19:27:16Z/2011-10-21T07:03:03Z
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, Scarlata et al., 2012, 'The escape of Lya photons in star-forming galaxies', 1.0, European Space Agency, https://doi.org/10.5270/esa-7euklbg