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Paper Citation Record · LEDGER

Origin of the 6.85 micron band near young stellar objects: The ammonium ion (NH4+) revisited

As of 12 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:astro-ph/0212230.

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

pith.paper-citation-record.v1
astro-ph/0212230 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 2 of 2 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-12T06:34:41.77262+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-11T15:58:18.737484Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-06-29T01:02:55.266072Z

Reference resolution

0 of 0 outbound references displayed

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

External citation measurements

No source-named external measurement is stored.

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 607279b2-2469-4f22-be24-f4b4823645c3 · inbound

The Dust Mineralogy of Interstellar Comet 3I/ATLAS from JWST/MIRI Observations cites this paper.

The Dust Mineralogy of Interstellar Comet 3I/ATLAS from JWST/MIRI Observations Origin of the 6.85 micron band near young stellar objects: The ammonium ion (NH4+) revisited

Reference 179

Resolution
metadata mismatch
local_arxiv, observed 2026-06-29T01:02:55.267523Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:74a996c664aa28f9b512b3113cedbaa436d1e331a84faf2379c3397498389f14

Observation 7a6b3330-e188-4f24-bf89-84930c3e7bcc · inbound

Dust production in the harsh environment of Sgr A* - MIRI/JWST observation of the O-rich asymptotic giant branch star IRS~3 cites this paper.

Dust production in the harsh environment of Sgr A* - MIRI/JWST observation of the O-rich asymptotic giant branch star IRS~3 Origin of the 6.85 micron band near young stellar objects: The ammonium ion (NH4+) revisited

Reference 50

Resolution
unresolved
no resolver link, observed 2026-08-11T15:58:18.737484Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-11T15:58:18.737484Z digest=sha256:3857ff0597bd0e22dee89fe47666f8d8ff61cdb82abe66ee89dbf3a5dee6cd8e