Accelerating galaxy winds during the big bang of starbursts
Accurately predicting the escape fraction of ionizing photons using rest-frame ultraviolet absorption lines
A Systematic Study of Galactic Outflows via Fluorescence Emission: Implications for Their Size and Structure
Chemodynamics of green pea galaxies - I. Outflows and turbulence driving the escape of ionizing photons and chemical enrichment
Constraining the Metallicities, Ages, Star Formation Histories, and Ionizing Continua of Extragalactic Massive Star Populations
Discovery of a Low-redshift Damped Lya System in a Foreground Extended Disk Using a Starburst Galaxy Background Illuminator
Do galaxies that leak ionizing photons have extreme outflows?
Early Results from GLASS-JWST. XXII. Rest-frame UV-Optical Spectral Properties of Lya Emitting Galaxies at 3 < z < 6
Fast Outflows Identified in Early Star-forming Galaxies at z = 5-6
Haro 11: The Spatially Resolved Lyman Continuum Sources
Haro 11 - Untying the knots of the nuclear starburst
Identifying H I Emission and UV Absorber Associations near the Magellanic Stream
Indirect Evidence for Escaping Ionizing Photons in Local Lyman Break Galaxy Analogs
Lyman-I+- spectral properties of five newly discovered Lyman continuum emitters
Lyman-a spectral properties of five newly discovered Lyman continuum emitters
Lya and UV Sizes of Green Pea Galaxies
Lya Profile, Dust, and Prediction of Lya Escape Fraction in Green Pea Galaxies
Metal-enriched galactic outflows shape the mass-metallicity relationship
Neutral ISM, Lya, and Lyman-continuum in the Nearby Starburst Haro11
On the Sizes of Ionized Bubbles Around Galaxies During the Reionization Epoch. The Spectral Shapes of the Lya Emission from Galaxies
O VI Emission Imaging of a Galaxy with the Hubble Space Telescope: a Warm Gas Halo Surrounding the Intense Starburst SDSS J115630.63+500822.1
Scaling Relations Between Warm Galactic Outflows and Their Host Galaxies
Shining a light on galactic outflows: photoionized outflows
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
Synthetic Absorption Lines from Simulations of Multiphase Gas in Galactic Winds
The Compact UV Size of Green Pea Galaxies As Local Analogs of High-redshift Lya-Emitters
The Implications of Extreme Outflows from Extreme Starbursts
The Importance of Star Formation Intensity in Lya Escape from Green Pea Galaxies and Lyman Break Galaxy Analogs
The Lyman Alpha Spectral Database (LASD)
The Magellan Evolution of Galaxies Spectroscopic and Ultraviolet Reference Atlas (MegaSaura). II. Stacked Spectra
The mass and momentum outflow rates of photoionized galactic outflows
The Source of Leaking Ionizing Photons from Haro11: Clues from HST/COS Spectroscopy of Knots A, B, and C
The Systematic Properties of the Warm Phase of Starburst-Driven Galactic Winds
Using Lyman-a to detect galaxies that leak Lyman continuum
VLT/X-Shooter Spectroscopy of Lyman Break Analogs: Direct-method O/H Abundances and Nitrogen Enhancements
zELDA: fitting Lyman alpha line profiles using deep learning
Instrument
COS, COS/FUV, COS/NUV
Temporal Coverage
2012-10-16T20:50:46Z/2013-07-23T17:43:35Z
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, Heckman comma Timothy M., 2014, 'UV Spectroscopy of Lyman Break Galaxy Analogs: A Local Window on the Early Universe', 1.0, European Space Agency, https://doi.org/10.5270/esa-syxmon6
