The Evolution of Low-ionization Electron Densities in Galaxies across Cosmic Epochs

Abstract We investigate the low-ionization electron density in the interstellar medium (ISM) of galaxies across 0 < z < 8, derived with the [O ii ] λλ 3727, 3730 and [S ii ] λλ 6718, 6733 doublets, using both deep JWST/NIRCam/grism and NIRSpec/MSA spectroscopy. Along with ancillary density samples from the literature at 0 < z < 6, we assemble three samples containing a total of 703 galaxies spanning 3.7 < z < 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 n e [S ii ] = 46 3 − 203 + 281 cm − 3 for CONGRESS, n e [S ii ] = 30 1 − 206 + 388 cm − 3 for FRESCO, and n e [O ii ] = 20 2 − 102 + 145 cm − 3 for the NIRSpec/MSA sample. The median low-ionization n e increases from z = 0 to 4, in agreement with previous studies and those using JWST observations. However, beyond z ∼ 4 median n e begins to deviate from a monotonically increasing evolution with z . We find a positive, but shallow, correlation between O 32 (a proxy for the ionization parameter) and n e , while also confirming a positive correlation between O 32 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.

Authors

Institutions

Publication Details

Journal
The Astrophysical Journal
Published
2026-10-15
DOI
https://doi.org/10.3847/1538-4357/ae9eb7
Primary Topic
Galaxies: Formation, Evolution, Phenomena
Type
article
Field-Weighted Citation Impact
0.00

Funders

Controls
|||
ALL TIME
JAN
FEB
MAR
APR
MAY
JUN
JUL
AUG
SEP
OCT
article

The Evolution of Low-ionization Electron Densities in Galaxies across Cosmic Epochs

Mabel G. Stephenson, R. Marques-Chaves, Jorryt Matthee, Sophia R. Flury et al.
The Astrophysical Journal
Galaxies: Formation, Evolution, Phenomena
article

The Evolution of Low-ionization Electron Densities in Galaxies across Cosmic Epochs

Mabel G. Stephenson, R. Marques-Chaves, Jorryt Matthee, Sophia R. Flury, N. G. Guseva, Alaina Henry, Rohan P. Naidu, Naveen A. Reddy, Alberto Saldana-Lopez, Y. I. Izotov, Steven L. Finkelstein, Pascal A. Oesch, Daniel Schaerer, Taylor A. Hutchison, 0000-0003-4717-0376
article en

Abstract

Abstract We investigate the low-ionization electron density in the interstellar medium (ISM) of galaxies across 0 < z < 8, derived with the [O ii ] λλ 3727, 3730 and [S ii ] λλ 6718, 6733 doublets, using both deep JWST/NIRCam/grism and NIRSpec/MSA spectroscopy. Along with ancillary density samples from the literature at 0 < z < 6, we assemble three samples containing a total of 703 galaxies spanning 3.7 < z < 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 n e [S ii ] = 46 3 − 203 + 281 cm − 3 for CONGRESS, n e [S ii ] = 30 1 − 206 + 388 cm − 3 for FRESCO, and n e [O ii ] = 20 2 − 102 + 145 cm − 3 for the NIRSpec/MSA sample. The median low-ionization n e increases from z = 0 to 4, in agreement with previous studies and those using JWST observations. However, beyond z ∼ 4 median n e begins to deviate from a monotonically increasing evolution with z . We find a positive, but shallow, correlation between O 32 (a proxy for the ionization parameter) and n e , while also confirming a positive correlation between O 32 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.

The Astrophysical JournalVol. 1010(2)
University of California, Riverside (US), University of Geneva (CH), University of Copenhagen (DK), Centre National de la Recherche Scientifique (FR), Space Telescope Science Institute (US), Goddard Space Flight Center (US), National Academy of Sciences of Ukraine (UA), Institute of Science and Technology Austria (AT), Stockholm University (SE), Massachusetts Institute of Technology (US), University of Maryland, College Park (US), The University of Texas at Austin (US), University of Edinburgh (GB)
National Science Foundation, National Aeronautics and Space Administration, Oak Ridge Associated Universities, Space Telescope Science Institute, National Research Foundation, Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung, Danmarks Grundforskningsfond, Knut och Alice Wallenbergs Stiftelse, Goddard Space Flight Center, Staatssekretariat für Bildung, Forschung und Innovation
Openalex Percentile: Top 33%
Galaxies: Formation, Evolution, Phenomena
AI Navigator

Ask Laika to Summarize, Analyze, and Connect papers live on the map.

Summarize Papers & Methodologies

Extract key findings, datasets, and comparative methods across publications.

Benchmark Rankings & Visual Analytics

Rank top research institutions, authors, funders, topics, and journals by Field-Weighted Citation Impact (FWCI) and paper volume with instant charts.

Connect Distant Disciplines

Bridge topological clusters on the map to find hidden collaborative intersections.