Paper Citation Record · LEDGER

[OII] as a Star Formation Rate Indicator

As of 22 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 6 inbound Pith citation observations for arXiv:astro-ph/0401172.

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

pith.paper-citation-record.v1
astro-ph/0401172 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 6 of 6 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-22T06:32:14.747728+00:00

measured 6 of 6 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-11T10:19:02.509217Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-10T02:16:42.228017Z

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 4e16523c-a6c4-4ad6-9cb0-e792d7a86cb2 · inbound

Inferring the role of binary neutron star mergers in r-process nucleosynthesis with multi-messenger observations using Cosmic Explorer and Einstein Telescope cites this paper.

Inferring the role of binary neutron star mergers in r-process nucleosynthesis with multi-messenger observations using Cosmic Explorer and Einstein Telescope [OII] as a Star Formation Rate Indicator

Reference 51

Resolution: verified exact; local_arxiv, observed 2026-05-25T03:55:19.653403Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

Observation c3e0fec0-9da7-45b9-9934-b46702ebfc8b · inbound

A Disappearing Act: Constraints From "Missing" Flares of Repeating Partial TDE Candidates cites this paper.

A Disappearing Act: Constraints From "Missing" Flares of Repeating Partial TDE Candidates [OII] as a Star Formation Rate Indicator

Reference 129

Resolution: verified exact; local_arxiv, observed 2026-06-28T02:01:29.708386Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

Observation 051a8165-3a6a-4afc-a961-67252fea1926 · inbound

GRB 250424A: A Case Study of Energy Injection with Multiwavelength Observations cites this paper.

GRB 250424A: A Case Study of Energy Injection with Multiwavelength Observations [OII] as a Star Formation Rate Indicator

Reference 111

Resolution: verified exact; local_arxiv, observed 2026-06-27T00:10:16.188453Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

Observation b70b9cb6-4d64-4512-93ae-fd6ab38152de · 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 [OII] as a Star Formation Rate Indicator

Reference 107

Resolution: verified exact; local_arxiv, observed 2026-07-10T02:16:42.229283Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

Observation e6675d14-e48a-45b3-a223-2695db574c5d · inbound

The chemodynamical signature of coherent metal-poor inflow and enriched recycled accretion in the cool circumgalactic medium cites this paper.

The chemodynamical signature of coherent metal-poor inflow and enriched recycled accretion in the cool circumgalactic medium [OII] as a Star Formation Rate Indicator

Reference 211

Resolution: unresolved; no resolver link, observed 2026-08-02T02:23:00.149661Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 9a65c0e1-d49c-4e76-a890-75c941a855c6 · inbound

An emerging baryon cycle in a galaxy 500 million years after the Big Bang cites this paper.

An emerging baryon cycle in a galaxy 500 million years after the Big Bang [OII] as a Star Formation Rate Indicator

Reference 85

Resolution: unresolved; no resolver link, observed 2026-08-11T10:19:02.509217Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.