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Paper Citation Record · LEDGER

Redshift Evolution of the Electron Density in the ISM at $z\sim 0-9$ Uncovered with JWST/NIRSpec Spectra and Line-Spread Function Determinations

As of 18 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 8 inbound Pith citation observations for arXiv:2301.06811.

A citation records a reference. It does not transfer a finding from one paper to another.

pith.paper-citation-record.v1
2301.06811 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 8 of 8 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-17T06:30:58.91139+00:00

measured 8 of 8 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-16T04:26:10.108576Z

measured 1 of 1 external citation measurements

A source-named dated measurement, never combined with another source.

Source: pith, observed 2026-08-05T02:28:24.338817Z

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
  • unresolved0
  • parse uncertain0
  • malformed identifier0
  • metadata mismatch0

External citation measurements

7
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 2428c343-00b1-46e9-9933-b445635f24fb · inbound

Direct T_e-based Metallicities of z=2-9 Galaxies with JWST/NIRSpec: Empirical Metallicity Calibrations Applicable from Reionization to Cosmic Noon cites this paper.

Direct T_e-based Metallicities of z=2-9 Galaxies with JWST/NIRSpec: Empirical Metallicity Calibrations Applicable from Reionization to Cosmic Noon Redshift Evolution of the Electron Density in the ISM at $z\sim 0-9$ Uncovered with JWST/NIRSpec Spectra and Line-Spread Function Determinations

Reference 40

Resolution
verified exact
arxiv_id, observed 2026-05-24T09:59:18.525089Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

source=arxiv_source observed=2026-05-24T09:57:11.896883Z digest=sha256:6b4429ec8f27a405c8cb20b463a999708bbc45825551ce9de465acc633902cd5

Observation e70ebee0-23a3-4cab-b203-97d1265a44d7 · inbound

CAPERS-LRD-z9: A Gas Enshrouded Little Red Dot Hosting a Broad-line AGN at z=9.288 cites this paper.

CAPERS-LRD-z9: A Gas Enshrouded Little Red Dot Hosting a Broad-line AGN at z=9.288 Redshift Evolution of the Electron Density in the ISM at $z\sim 0-9$ Uncovered with JWST/NIRSpec Spectra and Line-Spread Function Determinations

Reference 67

Resolution
unresolved
no resolver link, observed 2026-08-15T23:32:33.834373Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-15T23:32:33.834373Z digest=sha256:257b2090791651889ff80bcdcd3ab9d827dc029f1920bb02771a26aae87a8647

Observation fdea9e1c-7606-40c0-9e5a-a2573088c026 · inbound

Deep Spectroscopic Follow-Up of Maisie's Galaxy -- A Typical Galaxy in the Early Universe cites this paper.

Deep Spectroscopic Follow-Up of Maisie's Galaxy -- A Typical Galaxy in the Early Universe Redshift Evolution of the Electron Density in the ISM at $z\sim 0-9$ Uncovered with JWST/NIRSpec Spectra and Line-Spread Function Determinations

Reference 115

Resolution
metadata mismatch
local_arxiv, observed 2026-07-10T02:16:42.242447Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:1edcf7184ca363d93dc22143818f3b68cc5600517ff7d7d45fba92952383ed3f

Observation 08f5c82f-7601-4bc9-aa8a-3db696b60f3b · inbound

ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs cites this paper.

ATLAS. II. Extremely High Incidence of Balmer Line Absorption with Predominant Blueshifts in LRDs: Statistical Insights through Comparison with Type 1 AGNs Redshift Evolution of the Electron Density in the ISM at $z\sim 0-9$ Uncovered with JWST/NIRSpec Spectra and Line-Spread Function Determinations

Reference 58

Resolution
unresolved
no resolver link, observed 2026-08-01T00:25:30.417725Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T00:25:30.417725Z digest=sha256:7d2139b17f91ccc5c619bf0926baff51904ce3e7858e8454df3dcef8abe1eaa1

Observation 1a06c2b1-a8fe-46a3-a5f4-b755d1a3997b · inbound

Breathing Fire: Hot Dust in the Big Three Dragons at z = 7.15 cites this paper.

Breathing Fire: Hot Dust in the Big Three Dragons at z = 7.15 Redshift Evolution of the Electron Density in the ISM at $z\sim 0-9$ Uncovered with JWST/NIRSpec Spectra and Line-Spread Function Determinations

Reference 235

Resolution
unresolved
no resolver link, observed 2026-08-12T00:39:29.951637Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-12T00:39:29.951637Z digest=sha256:cd3c197f51eb88e63cd509299822da8195fca3f3e80bd9b038a15d7177bbccec

Observation 2a795de9-406d-49eb-88d1-278921291811 · inbound

Unveiling and Characterising Ubiquitous Nitrogen Enhancement in $6 \leq z \leq 10$ Galaxies with JWST Spectroscopy cites this paper.

Unveiling and Characterising Ubiquitous Nitrogen Enhancement in $6 \leq z \leq 10$ Galaxies with JWST Spectroscopy Redshift Evolution of the Electron Density in the ISM at $z\sim 0-9$ Uncovered with JWST/NIRSpec Spectra and Line-Spread Function Determinations

Reference 188

Resolution
unresolved
no resolver link, observed 2026-08-14T04:17:47.529704Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T04:17:47.529704Z digest=sha256:6491fcb8d40ddb573757c5ad8c6d44bcd4e6f3daa503c3a5f264c0115205d42f

Observation 8b903814-dc09-450a-b3c0-4995d1ca4f4c · inbound

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics cites this paper.

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics Redshift Evolution of the Electron Density in the ISM at $z\sim 0-9$ Uncovered with JWST/NIRSpec Spectra and Line-Spread Function Determinations

Reference 233

Resolution
unresolved
no resolver link, observed 2026-08-16T00:12:18.635850Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:12:18.635850Z digest=sha256:d958f77c7bcb01199be8b6cd80c585ba21d27b66dc8279ae00963695089e650c

Observation c0428adb-a30a-406a-bc0c-7ec3fb55f1f9 · inbound

SPURS: Massive Stars, Dense Gas, and Ly$\alpha$ Escape in GN-z11 at $z = 10.6$ cites this paper.

SPURS: Massive Stars, Dense Gas, and Ly$\alpha$ Escape in GN-z11 at $z = 10.6$ Redshift Evolution of the Electron Density in the ISM at $z\sim 0-9$ Uncovered with JWST/NIRSpec Spectra and Line-Spread Function Determinations

Reference 144

Resolution
unresolved
no resolver link, observed 2026-08-16T04:26:10.108576Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T04:26:10.108576Z digest=sha256:9830ec948d55238e1fe37259206aa1fc560cd91b8975918000dd0f1b976a6b4e