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   	<dc:title>The evolution of low-ionization electron densities in galaxies across cosmic epochs</dc:title>
   	<dc:creator>Stephenson, Mabel G.</dc:creator>
   	<dc:creator>Chisholm, John</dc:creator>
   	<dc:creator>Saldana-Lopez, A.</dc:creator>
   	<dc:creator>Matthee, Jorryt J ; https://orcid.org/0000-0003-2871-127X</dc:creator>
   	<dc:creator>Henry, Alaina</dc:creator>
   	<dc:creator>Naidu, Rohan P.</dc:creator>
   	<dc:creator>Flury, Sophia R.</dc:creator>
   	<dc:creator>Hutchison, Taylor A.</dc:creator>
   	<dc:creator>Finkelstein, Steven L.</dc:creator>
   	<dc:creator>Guseva, Natalia G.</dc:creator>
   	<dc:creator>Izotov, Yuri I.</dc:creator>
   	<dc:creator>Marques-Chaves, Rui</dc:creator>
   	<dc:creator>Oesch, Pascal A.</dc:creator>
   	<dc:creator>Reddy, Naveen A.</dc:creator>
   	<dc:creator>Schaerer, Daniel</dc:creator>
   	<dc:subject>ddc:520</dc:subject>
   	<dc:description>We investigate the low-ionization electron density in the interstellar medium (ISM) of galaxies across 0 &lt; z &lt; 8,
derived with the [O II] λλ3727, 3730 and [S II] λλ6718, 6733 doublets, using both deep JWST/NIRCam/grism
and NIRSpec/MSA spectroscopy. Along with ancillary density samples from the literature at 0 &lt; z &lt; 6, we
assemble three samples containing a total of 703 galaxies spanning 3.7 &lt; z &lt; 7.8 at 〈z〉 ∼ 5.6; 691 galaxies in the
luminosity-complete NIRCam/grism programs CONGRESS and FRESCO at 〈z〉 ∼ 4.3 and ∼5.3, respectively;
and 12 galaxies with high-resolution NIRSpec/MSA spectra from the GO 1871 and GLASS programs. We find
median electron densities of ne[S II] = + 463 203 cm 281 3
for CONGRESS, ne[S II] = + 301 206 cm 388 3
for FRESCO, and
ne[O II] = + 202 102 cm 145 3
for the NIRSpec/MSA sample. The median low-ionization ne increases from z = 0 to 4,
in agreement with previous studies and those using JWST observations. However, beyond z ∼ 4 median ne begins
to deviate from a monotonically increasing evolution with z. We find a positive, but shallow, correlation between
O32 (a proxy for the ionization parameter) and ne, while also confirming a positive correlation between O32 and z.
We suggest that these trends are possibly due to an evolving ISM gas density and ionization structure, and
propose a toy model where the gas clumping evolves with z to explain the observed density and ionization
variations.</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/23200</dc:identifier>
   	<dc:identifier>https://research-explorer.ista.ac.at/download/23200/23202</dc:identifier>
   	<dc:source>Stephenson MG, Chisholm J, Saldana-Lopez A, et al. The evolution of low-ionization electron densities in galaxies across cosmic epochs. &lt;i&gt;The Astrophysical Journal&lt;/i&gt;. 2026;1010(2). doi:&lt;a href=&quot;https://doi.org/10.3847/1538-4357/ae9eb7&quot;&gt;10.3847/1538-4357/ae9eb7&lt;/a&gt;</dc:source>
   	<dc:language>eng</dc:language>
   	<dc:relation>info:eu-repo/semantics/altIdentifier/doi/10.3847/1538-4357/ae9eb7</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/2608.23846</dc:relation>
   	<dc:rights>info:eu-repo/semantics/openAccess</dc:rights>
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