Accelerating galaxy winds during the big bang of starbursts
A Close Relationship between Lya and Mg II in Green Pea Galaxies
Correlation between SFR Surface Density and Thermal Pressure of Ionized Gas in Local Analogs of High-redshift Galaxies
Direct T e Metallicity Calibration of R23 in Strong Line Emitters
Early Results from GLASS-JWST. XXII. Rest-frame UV-Optical Spectral Properties of Lya Emitting Galaxies at 3 < z < 6
Lya and UV Sizes of Green Pea Galaxies
Lya Profile, Dust, and Prediction of Lya Escape Fraction in Green Pea Galaxies
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 Compact UV Size of Green Pea Galaxies As Local Analogs of High-redshift Lya-Emitters
The Importance of Star Formation Intensity in Lya Escape from Green Pea Galaxies and Lyman Break Galaxy Analogs
The Lyman Alpha Spectral Database (LASD)
zELDA: fitting Lyman alpha line profiles using deep learning
Instrument
COS, COS/FUV, COS/NUV
Temporal Coverage
2015-09-27T21:14:04Z/2016-06-26T19:54:32Z
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, Malhotra et al., 2017, 'Lyman alpha escape in Green Pea galaxies (give peas a chance)', 1.0, European Space Agency, https://doi.org/10.5270/esa-zx41sps
