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Paper Citation Record · LEDGER

Indicators of star formation: 4000 Angstrom break and Balmer lines

As of 14 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 6 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.

pith.paper-citation-record.v1
astro-ph/9703067 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 2026-08-14T06:32:32.682623+00:00

measured 6 of 6 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-14T04:18:57.122699Z

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

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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.

source=arxiv_source observed=2026-08-08T23:42:57.018804Z digest=sha256:5e70e34c0bf37a8d3652247f93a9ed848a9e239a421b9fe6b079c860955dc8cc

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 2026-08-14T06:32:32.682623+00:00.

source=arxiv_source observed=2026-05-14T18:18:38.368482Z digest=sha256:6fbb10febd70783d03902e253115f40b39134a865cf177f3be3b30eeaa5967ff

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 2026-08-14T06:32:32.682623+00:00.

source=pdf_text observed=2026-07-11T11:50:26.030339Z digest=sha256:8a79c168b4ef31073259491cd9daf8f6c18b3721d5dddb56de015b37d71d52b4

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 2026-08-14T06:32:32.682623+00:00.

source=pdf_text observed=2026-06-28T13:47:59.860576Z digest=sha256:3d2b3bde0a0e804cf9058ee9559921660bbc214afd5979f81b695bf1c4a1e28d

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.

source=pdf_text observed=2026-08-02T12:35:30.231106Z digest=sha256:208212aa45771cecb63a46a69b31e2b2c36ac2ab109f34a4d01fee034fbb1c01

Observation 970e25e6-a1c6-4c64-a4d1-0c0be2513a2e · inbound

CORN -- Chronometers of Relic Nature I: The first estimate of the expansion rate of the Universe using compact relic galaxies cites this paper.

CORN -- Chronometers of Relic Nature I: The first estimate of the expansion rate of the Universe using compact relic galaxies Indicators of star formation: 4000 Angstrom break and Balmer lines

Reference 6

Resolution
unresolved
no resolver link, observed 2026-08-14T04:18:57.122699Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T04:18:57.122699Z digest=sha256:e5ca1e9e297642794dbbc1d9fb497155e8757336df0beef6495a974b48d22fc6