Predicted UV properties of very metal-poor starburst galaxies
A&A, 523 (2010) A64
Published online: 2010-11-18
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The far-ultraviolet continuum slope as a Lyman Continuum escape estimator at high redshift
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A puzzling non-detection of [O III] and [C II] from a z ≈ 7.7 galaxy observed with ALMA
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Revealing the formation histories of the first stars with the cosmic near-infrared background
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Can nebular He II emission be explained by ultra-luminous X-ray sources?
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Ly α as a tracer of cosmic reionization in the SPHINX radiation-hydrodynamics cosmological simulation
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The evolution of rest-frame UV properties, Ly α EWs, and the SFR–stellar mass relation at z ∼ 2–6 for SC4K LAEs
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An analytic model for [O iii] fine structure emission from high redshift galaxies
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Identifying reionization-epoch galaxies with extreme levels of Lyman continuum leakage in James Webb Space Telescope surveys
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Lyman-αpolarization intensity mapping
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The impact of star formation sampling effects on the spectra of lensed z > 6 galaxies detectable with JWST
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When did Population III star formation end?
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Luminous Lyα Emitters with Very Blue UV-continuum Slopes at Redshift 5.7 ≤ z ≤ 6.6
Linhua Jiang, Seth H. Cohen, Rogier A. Windhorst, Eiichi Egami, Kristian Finlator, Daniel Schaerer and Fengwu SunThe Astrophysical Journal 889 (2) 90 (2020)
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Texas Spectroscopic Search for Lyα Emission at the End of Reionization. III. The Lyα Equivalent-width Distribution and Ionized Structures at z > 7
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The nature of CR7 revealed with MUSE: a young starburst powering extended Ly α emission at z = 6.6
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The impact of Lyα emission line heating and cooling on the cosmic dawn 21-cm signal
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Elevated ionizing photon production efficiency in faint high-equivalent-width Lyman-α emitters
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Exploring He II λ1640 emission line properties at z ∼2−4
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Lyman α-emitting galaxies in the epoch of reionization
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X-ray binaries as the origin of nebular He II emission in low-metallicity star-forming galaxies
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Extremely metal-poor galaxies with HST/COS: laboratories for models of low-metallicity massive stars and high-redshift galaxies
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The interstellar medium of dwarf galaxies: new insights from Machine Learning analysis of emission-line spectra
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The MUSE-Wide Survey: survey description and first data release
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Lyman-alpha as an Astrophysical and Cosmological Tool
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Submillimeter Signatures from Growing Supermassive Black Holes before Reionization
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Lyman-alpha as an Astrophysical and Cosmological Tool
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Resolved UV and [C ii] Structures of Luminous Galaxies within the Epoch of Reionization
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Constraints on the production and escape of ionizing radiation from the emission-line spectra of metal-poor star-forming galaxies
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Following the Cosmic Evolution of Pristine Gas. III. The Observational Consequences of the Unknown Properties of Population III Stars
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Dark Galaxy Candidates at Redshift ∼3.5 Detected with MUSE*
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Lyman continuum leakage versus quenching with the James Webb Space Telescope: the spectral signatures of quenched star formation activity in reionization-epoch galaxies
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Reionization in Technicolor
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Kiloparsec-scale gaseous clumps and star formation at z = 5–7
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Following the Cosmic Evolution of Pristine Gas. II. The Search for Pop III–bright Galaxies
Richard Sarmento, Evan Scannapieco and Seth CohenThe Astrophysical Journal 854 (1) 75 (2018)
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MUSE Spectroscopic Identifications of Ultra-faint Emission Line Galaxies with MUV ∼ −15*
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