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   	<dc:title>EIGER. VIII. First stars signatures in the connection between O I absorption and galaxies in the epoch of reionization</dc:title>
   	<dc:creator>Higginson, Jack</dc:creator>
   	<dc:creator>Bordoloi, Rongmon</dc:creator>
   	<dc:creator>Simcoe, Robert A.</dc:creator>
   	<dc:creator>Matthee, Jorryt J ; https://orcid.org/0000-0003-2871-127X</dc:creator>
   	<dc:creator>Kashino, Daichi</dc:creator>
   	<dc:creator>Mackenzie, Ruari</dc:creator>
   	<dc:creator>Kramarenko, Ivan ; https://orcid.org/0000-0001-5346-6048</dc:creator>
   	<dc:creator>Lilly, Simon J.</dc:creator>
   	<dc:creator>Eilers, Anna-Christina</dc:creator>
   	<dc:creator>Naidu, Rohan P.</dc:creator>
   	<dc:creator>Yue, Minghao</dc:creator>
   	<dc:subject>ddc:520</dc:subject>
   	<dc:description>We investigate the association between galaxies and neutral O I absorption systems at z ∼ 6, which trace metalenriched gas during the epoch of reionization. We identify 40 galaxies across six quasar fields, residing in 15
overdensities within 300 kpc of the background sight lines. Five O I absorption systems are associated with five of
these overdensities, yielding a covering fraction of
0.27 0.10
+0.13
within 300 kpc. The absorption occurs beyond typical
virial radii, indicating that the gas traces extended overdensity environments rather than individual galaxy halos,
unlike the z ∼ 0 circumgalactic medium (CGM), which is largely bound to halos. These galaxy-associated
absorbers account for ∼35% of all O I systems seen in blind quasar surveys, implying the remainder arise in
lower-mass galaxies below our detection threshold or in dense neutral intergalactic medium pockets. The CGM
around these galaxies contains ≳ 2 × 106 M⊙ of oxygen, comparable to the interstellar medium oxygen mass of
the galaxies themselves, suggesting that the surrounding environment holds as much metal mass as the galaxies.
All five galaxy-associated systems show significantly higher
log NCII NOI ( / )
ratios than absorbers lacking galaxy
associations. Furthermore, relative abundance ratios ([Si/O], [C/O]) reveal that four of the five exhibit
enrichment patterns consistent with Population III nucleosynthesis at the outskirts of galaxy overdensities. These
rare systems offer a unique window into the role of first-generation stars in shaping the early metal enrichment of
galaxies and their environments.</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/23115</dc:identifier>
   	<dc:identifier>https://research-explorer.ista.ac.at/download/23115/23136</dc:identifier>
   	<dc:source>Higginson J, Bordoloi R, Simcoe RA, et al. EIGER. VIII. First stars signatures in the connection between O I absorption and galaxies in the epoch of reionization. &lt;i&gt;The Astrophysical Journal&lt;/i&gt;. 2026;999(1). doi:&lt;a href=&quot;https://doi.org/10.3847/1538-4357/ae3e81&quot;&gt;10.3847/1538-4357/ae3e81&lt;/a&gt;</dc:source>
   	<dc:language>eng</dc:language>
   	<dc:relation>info:eu-repo/semantics/altIdentifier/doi/10.3847/1538-4357/ae3e81</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/2510.05220</dc:relation>
   	<dc:rights>info:eu-repo/semantics/openAccess</dc:rights>
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