Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Indicators of star formation: 4000 Angstrom break and Balmer lines
As of 9 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:astro-ph/9703067.
A citation records a reference. It does not transfer a finding from one paper to another.
Coverage vector
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-09T06:31:02.800959+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-08T23:42:57.018804Z
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
14
pith, observed 2026-08-05T02:28:24.338817Z
Outbound references
No outbound reference observations are available for this paper version.
Pith citing papers
Observation 5274bc21-7911-4721-9e1c-c45eb9f5d10c · inbound
AT 2018dyk: tidal disruption event or active galactic nucleus? Follow-up observations of an extreme coronal line emitter with the Dark Energy Spectroscopic Instrument cites this paper.
AT 2018dyk: tidal disruption event or active galactic nucleus? Follow-up observations of an extreme coronal line emitter with the Dark Energy Spectroscopic Instrument Indicators of star formation: 4000 Angstrom break and Balmer lines
Reference 99
- Resolution
- unresolved
- no resolver link, observed 2026-08-08T23:42:57.018804Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 53616d0b-748f-4f47-a88f-c7676de6188d · inbound
First Light And Reionization Epoch Simulations (FLARES) XXI: The UV Indices of Galaxies in the Early Universe cites this paper.
First Light And Reionization Epoch Simulations (FLARES) XXI: The UV Indices of Galaxies in the Early Universe Indicators of star formation: 4000 Angstrom break and Balmer lines
Reference 224
- Resolution
- verified exact
- local_arxiv, observed 2026-05-14T18:19:23.240335Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.
Observation 7576aab7-ebfd-46c7-8533-4687409e3c33 · inbound
Inside-Out vs. Outside-In Quenching of MaNGA Galaxies: Dependence on Stellar Mass and Environment cites this paper.
Inside-Out vs. Outside-In Quenching of MaNGA Galaxies: Dependence on Stellar Mass and Environment Indicators of star formation: 4000 Angstrom break and Balmer lines
Reference 7
- Resolution
- metadata mismatch
- local_arxiv, observed 2026-06-28T17:02:23.683157Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.
Observation b4f01a43-b9d4-4877-8274-e0c1aebae214 · inbound
Towards Unbreaking the Universe: MINERVA Measurements of Color Gradients in Massive Quiescent Galaxies Can Help Ease Too-Early Star Formation Tensions cites this paper.
Towards Unbreaking the Universe: MINERVA Measurements of Color Gradients in Massive Quiescent Galaxies Can Help Ease Too-Early Star Formation Tensions Indicators of star formation: 4000 Angstrom break and Balmer lines
Reference 101
- Resolution
- verified exact
- local_arxiv, observed 2026-06-28T14:32:18.785245Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.
Observation 52b82a80-091c-41a2-b214-42139eff1138 · inbound
Towards Unbreaking the Universe: MINERVA Measurements of Color Gradients in Massive Quiescent Galaxies Can Help Ease Too-Early Star Formation Tensions cites this paper.
Towards Unbreaking the Universe: MINERVA Measurements of Color Gradients in Massive Quiescent Galaxies Can Help Ease Too-Early Star Formation Tensions Indicators of star formation: 4000 Angstrom break and Balmer lines
Reference 101
- Resolution
- unresolved
- no resolver link, observed 2026-08-02T12:35:30.231106Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.