Exploring the Link between Extreme Coronal Line Emitters and Tidal Disruption Events
Galaxies with minimal or no activity from their nucleus can still exhibit significant coronal line (CL) emission, often exceeding the strength of typical narrow emission lines. Many of these CLs require ionization potentials of ≥100 eV, implying the need
Weiyu Ding +6 more
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DESI Spectroscopy of HETDEX Emission-line Candidates. I. Line Discrimination Validation
The Hobby–Eberly Dark Energy Experiment (HETDEX) is an untargeted spectroscopic galaxy survey that uses Ly α- emitting galaxies (LAEs) as tracers of 1.9 < z < 3.5 large-scale structure. Most detections consist of a single emission line, whose identity is
Martin Landriau +52 more
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Hunting for extremely metal-poor emission-line galaxies in the Sloan Digital Sky Survey: MMT and 3.5 m APO observations [PDF]
Y. I. Izotov, T. X. Thuan, N. G. Guseva
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We present a survey undertaken with the Atacama Large Millimeter/submillimeter Array (ALMA) to study the galaxies associated with a representative sample of 16 damped Ly α absorbers (DLAs) at z ≈ 4.1–4.5, using the [C ii ] 158 μ m ([C ii ]) line.
Marcel Neeleman +4 more
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Synthetic nebular emission from massive galaxies – II. Ultraviolet-line diagnostics of dominant ionizing sources [PDF]
Michaela Hirschmann +5 more
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Models of optical emission lines to investigate Narrow-Line Seyfert 1 galaxies in spectroscopic databases [PDF]
G. La Mura +8 more
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DOUBLE-PEAKED NARROW EMISSION-LINE GALAXIES FROM THE SLOAN DIGITAL SKY SURVEY. I. SAMPLE AND BASIC PROPERTIES [PDF]
Junqiang Ge +4 more
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Lyman Continuum Leakage from Massive Leaky Starbursts: A Different Class of Emitters?
The origin of Lyman continuum (LyC) photons responsible for reionizing the Universe remains largely unknown, with the fraction of escaping LyC photons from galaxies at z ∼ 6 to 12 still uncertain.
Namrata Roy +13 more
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Power-law Emission-line Wings and Radiation-driven Superwinds in Local Lyman Continuum Emitters
We investigate broad emission-line wings, reaching ≤800 km s ^−1 , observed in 26 galaxies with Lyman continuum (LyC) observations, primarily from the Low-redshift Lyman Continuum Survey.
Lena Komarova +29 more
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H‐like Iron Emission in Narrow‐Line Seyfert 1 Galaxies as a Temperature Diagnostic of Accretion Flows [PDF]
M. A. Bautista, L. Titarchuk
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