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   	<dc:title>The Deepest GLIMPSE of a dense gas cocoon enshrouding a Little Red Dot</dc:title>
   	<dc:creator>Kokorev, Vasily</dc:creator>
   	<dc:creator>Chisholm, John</dc:creator>
   	<dc:creator>Naidu, Rohan P.</dc:creator>
   	<dc:creator>Fujimoto, Seiji</dc:creator>
   	<dc:creator>Atek, Hakim</dc:creator>
   	<dc:creator>Brammer, Gabriel</dc:creator>
   	<dc:creator>Finkelstein, Steven L.</dc:creator>
   	<dc:creator>Akins, Hollis B.</dc:creator>
   	<dc:creator>Berg, Danielle A.</dc:creator>
   	<dc:creator>Furtak, Lukas J.</dc:creator>
   	<dc:creator>Fei, Qinyue</dc:creator>
   	<dc:creator>Hsiao, Tiger Yu-Yang</dc:creator>
   	<dc:creator>Labbé, Ivo</dc:creator>
   	<dc:creator>Matthee, Jorryt J ; https://orcid.org/0000-0003-2871-127X</dc:creator>
   	<dc:creator>Muñoz, Julian B.</dc:creator>
   	<dc:creator>Oesch, Pascal A.</dc:creator>
   	<dc:creator>Pan, Richard</dc:creator>
   	<dc:creator>Rinaldi, Pierluigi</dc:creator>
   	<dc:creator>Saldana-Lopez, Alberto</dc:creator>
   	<dc:creator>Schaerer, Daniel</dc:creator>
   	<dc:creator>Volonteri, Marta</dc:creator>
   	<dc:creator>Zitrin, Adi</dc:creator>
   	<dc:subject>ddc:520</dc:subject>
   	<dc:description>The detection of strong Balmer breaks and absorption features in Little Red Dots (LRDs) suggests they host active galactic nuclei embedded within dense gas envelopes, potentially powered by super-Eddington accretion. We present GLIMPSE-17775, a luminous (Lbol ∼ 1045 erg s−1) LRD at z = 3.501 behind Abell S1063 (μ ∼ 2), observed with deep JWST/NIRCam and a ∼20 hr (80 hr delensed) NIRSpec G395M spectrum. The data reveal over 40 emission and absorption features, including a rich forest of low-ionization Fe ii lines and numerous broad hydrogen recombination transitions. We use this depth to test the dense-gas interpretation through five independent diagnostics. Nearly all permitted lines show exponential wings with consistent FWHM, a signature of Thomson scattering requiring ne ≳ 108 cm−3. Adopting this width yields MBH ∼ 106.7M⊙, a factor of 10 lower than Gaussian fits, and λEdd ∼ 1.8. Additional diagnostics support the same picture: a pronounced Balmer break (fν,4050/fν,3670 = 2.0 ± 0.1), enhanced He i λ7065 and λ10830 with P-Cygni absorption, Bowen-fluorescent O i λ8446–λ11290 emission requiring Lyβ pumping, and 16 Fe ii lines matching fluorescence models. These features indicate a dense (n ∼ 108 cm−3), partially ionized cocoon where scattering and fluorescence dominate line formation, providing strong evidence that at least some LRDs are powered by super-Eddington black hole growth in the early Universe.</dc:description>
   	<dc:publisher>IOP Publishing</dc:publisher>
   	<dc:date>2026</dc:date>
   	<dc:type>info:eu-repo/semantics/article</dc:type>
   	<dc:type>doc-type:article</dc:type>
   	<dc:type>article</dc:type>
   	<dc:type>http://purl.org/coar/resource_type/c_2df8fbb1</dc:type>
   	<dc:identifier>https://research-explorer.ista.ac.at/record/22296</dc:identifier>
   	<dc:identifier>https://research-explorer.ista.ac.at/download/22296/22313</dc:identifier>
   	<dc:source>Kokorev V, Chisholm J, Naidu RP, et al. The Deepest GLIMPSE of a dense gas cocoon enshrouding a Little Red Dot. &lt;i&gt;The Astrophysical Journal&lt;/i&gt;. 2026;1004(2). doi:&lt;a href=&quot;https://doi.org/10.3847/1538-4357/ae4ed7&quot;&gt;10.3847/1538-4357/ae4ed7&lt;/a&gt;</dc:source>
   	<dc:language>eng</dc:language>
   	<dc:relation>info:eu-repo/semantics/altIdentifier/doi/10.3847/1538-4357/ae4ed7</dc:relation>
   	<dc:relation>info:eu-repo/semantics/altIdentifier/issn/0004-637X</dc:relation>
   	<dc:relation>info:eu-repo/semantics/altIdentifier/e-issn/1538-4357</dc:relation>
   	<dc:relation>info:eu-repo/semantics/altIdentifier/arxiv/2511.07515</dc:relation>
   	<dc:rights>info:eu-repo/semantics/openAccess</dc:rights>
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