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Paper Citation Record · LEDGER

Reconstructing the star formation history of the Milky Way disc(s) from chemical abundances

As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 6 inbound Pith citation observations for arXiv:1410.3829.

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

pith.paper-citation-record.v1
1410.3829 v2

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 2026-08-11T06:34:44.6726+00:00

measured 6 of 6 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-10T05:52:04.711957Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-09T20:56:34.152342Z

Reference resolution

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External citation measurements

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Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation abf67dc8-9948-4b90-b6c2-0b9f1a9020f2 · inbound

Vertical Structure and Dynamics of a Galactic Disk cites this paper.

Vertical Structure and Dynamics of a Galactic Disk Reconstructing the star formation history of the Milky Way disc(s) from chemical abundances

Reference 281

Resolution
unresolved
no resolver link, observed 2026-08-06T20:44:22.766154Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 9804ff25-697d-40c7-8e08-255891bd3f47 · inbound

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations cites this paper.

Is the composition of the Solar atmosphere unusual, and if so, why? Possible interpretations Reconstructing the star formation history of the Milky Way disc(s) from chemical abundances

Reference 156

Resolution
unresolved
no resolver link, observed 2026-08-05T10:57:04.990347Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation a7d03113-f1d3-416e-be92-752337c908e4 · inbound

Milky Way's warped disc traced by AGB stars cites this paper.

Milky Way's warped disc traced by AGB stars Reconstructing the star formation history of the Milky Way disc(s) from chemical abundances

Reference 141

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verified exact
local_arxiv, observed 2026-06-27T19:01:08.540208Z

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

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Observation 795e00cd-e631-47a7-8444-0d9ba3a029e8 · inbound

Introducing AuriGLOBES: The effects of compressive tides, compact object-induced mass loss, and size evolution on modelling globular clusters cites this paper.

Introducing AuriGLOBES: The effects of compressive tides, compact object-induced mass loss, and size evolution on modelling globular clusters Reconstructing the star formation history of the Milky Way disc(s) from chemical abundances

Reference 134

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verified exact
local_arxiv, observed 2026-07-01T01:45:14.192991Z

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

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Observation e8d62bf2-10ae-4bb8-9ff2-f94813a2bb1a · inbound

Unveiling the Milky Way with a Gaia DR3 census of OB-type stars within 2 kpc. I. Tracing local Galactic structure, massive star-forming regions and core-collapse supernova progenitors cites this paper.

Unveiling the Milky Way with a Gaia DR3 census of OB-type stars within 2 kpc. I. Tracing local Galactic structure, massive star-forming regions and core-collapse supernova progenitors Reconstructing the star formation history of the Milky Way disc(s) from chemical abundances

Reference 197

Resolution
verified exact
local_arxiv, observed 2026-07-09T20:56:34.153688Z

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.

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Observation 5ed58f49-1113-4fb6-9323-3522750213d1 · inbound

Tracing the early Milky Way thin disc with the Gaia-ESO Survey cites this paper.

Tracing the early Milky Way thin disc with the Gaia-ESO Survey Reconstructing the star formation history of the Milky Way disc(s) from chemical abundances

Reference 94

Resolution
unresolved
no resolver link, observed 2026-08-10T05:52:04.711957Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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