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Paper Citation Record · LEDGER

The Case for High Resolution Spectroscopy in the Ultraviolet

As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2504.00231.

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

pith.paper-citation-record.v1
2504.00231 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 3 of 3 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-11T06:34:44.6726+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-04T08:37:06.481111Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-06-30T16:04:53.056881Z

Reference resolution

0 of 0 outbound references displayed

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  • verified fuzzy0
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  • 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 f428ede7-4592-4455-858d-c65569ee5bc6 · inbound

The Synthetic Absorption Line Spectral Almanac (SALSA) cites this paper.

The Synthetic Absorption Line Spectral Almanac (SALSA) The Case for High Resolution Spectroscopy in the Ultraviolet

Reference 106

Resolution
unresolved
no resolver link, observed 2026-08-04T08:37:06.481111Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-04T08:37:06.481111Z digest=sha256:fd1ea9778d12e66a8c24ea808b766ec2ade408963429859f7b49aaa3ee0a4180

Observation fd60399f-6f93-4c70-9385-475e9ead4baf · inbound

The unique capabilities of HST for stellar physics: Probing Atmospheric Structure, Chromospheres, and Mass Loss of Evolved Stars cites this paper.

The unique capabilities of HST for stellar physics: Probing Atmospheric Structure, Chromospheres, and Mass Loss of Evolved Stars The Case for High Resolution Spectroscopy in the Ultraviolet

Reference 29

Resolution
verified exact
arxiv_id, observed 2026-05-25T05:36:40.206797Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

source=pdf_text observed=2026-05-25T05:32:07.261349Z digest=sha256:6b822e40415380849645729bd68d56a331bad7cb9983ed33b388d361a55cd801

Observation 0b7768aa-a07c-4865-9bbd-e614e4f61fc1 · inbound

The unique capabilities of HST for stellar physics: Probing Atmospheric Structure, Chromospheres, and Mass Loss of Evolved Stars cites this paper.

The unique capabilities of HST for stellar physics: Probing Atmospheric Structure, Chromospheres, and Mass Loss of Evolved Stars The Case for High Resolution Spectroscopy in the Ultraviolet

Reference 29

Resolution
verified exact
arxiv_id, observed 2026-06-30T16:04:53.058168Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

source=pdf_text observed=2026-06-30T15:57:50.423323Z digest=sha256:c4e9d72053e41d7b57db3b92c11236c6706a2243b9c6c0e9891cebd97f205503