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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:c8463b467bb260810cf859365ece1a71d9b1f410883c49e2989e168e9ba629b3

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=sha256:61b49705562f7768ffc1020816a1e22c9ac573711ab8ed2a45c4fd3cfe8726f1

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=sha256:3810f20965331a56af9008c7661678da7ddada3fc97d5ef13240e1272684ba49

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:a3d162c9e25eb8707a4a898855dad6f3c7e88fbe06fa6b1645c628d7b984775a

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:cced9f1408179b67657e61ddb6f80db3f8fc94507a0c8cbe1595de392c314f62

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:e609f243b3e8d32b5aa3ffa3ab17a3ad11d81ffdebf38ea035d4eb522cc50790

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:a707cbad19244f394fb60b76fcf5adea0ea683f2a7432f8db233cc0593065b8c

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:a4f09224dc02d1b6e7fc4caf46202ce6ddec004d0c9efe3ebd0a7188f117ebbc