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Paper Citation Record · LEDGER

Nucleosynthesis in Chandrasekhar Mass Models for Type Ia Supernovae and Constraints on Progenitor Systems and Burning-Front Propagation

As of 17 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 9 inbound Pith citation observations for arXiv:astro-ph/0002337.

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

pith.paper-citation-record.v1
astro-ph/0002337 v1

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measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 9 of 9 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-16T06:30:59.297886+00:00

measured 9 of 9 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-16T00:12:18.526961Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-01T05:15:24.697343Z

Reference resolution

0 of 0 outbound references displayed

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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 d95f2a83-a364-4f30-a653-d3588439b0b7 · inbound

The Simulated Oxygen Shortage (SOS): Mapping the Missing OVI in Simulated Dwarf Galaxies to Subgrid Physics cites this paper.

The Simulated Oxygen Shortage (SOS): Mapping the Missing OVI in Simulated Dwarf Galaxies to Subgrid Physics Nucleosynthesis in Chandrasekhar Mass Models for Type Ia Supernovae and Constraints on Progenitor Systems and Burning-Front Propagation

Reference 102

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verified exact
local_arxiv, observed 2026-05-19T15:47:38.389966Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

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Observation 1843fb05-e75c-4428-9a06-7f4b1a68a96f · inbound

Grain-size evolution and rapid dust growth in high-redshift galaxies cites this paper.

Grain-size evolution and rapid dust growth in high-redshift galaxies Nucleosynthesis in Chandrasekhar Mass Models for Type Ia Supernovae and Constraints on Progenitor Systems and Burning-Front Propagation

Reference 40

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verified exact
local_arxiv, observed 2026-06-28T00:51:27.421621Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

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Observation 371c6faf-85e3-4cd8-9da1-acb3a3dd4d84 · inbound

JWST Absorption-Line Analysis of UV-Bright Galaxies at $z=7.2-10.6$: Early Chemical Enrichment Traced by C, O, Mg, Al, Si, and Fe cites this paper.

JWST Absorption-Line Analysis of UV-Bright Galaxies at $z=7.2-10.6$: Early Chemical Enrichment Traced by C, O, Mg, Al, Si, and Fe Nucleosynthesis in Chandrasekhar Mass Models for Type Ia Supernovae and Constraints on Progenitor Systems and Burning-Front Propagation

Reference 64

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verified exact
local_arxiv, observed 2026-06-27T18:01:08.221740Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

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Observation 1689a731-43b3-43de-8767-c27f2b1ace7e · inbound

The Sc, Ti, and V Abundance Discrepancy: Testing High-Mass IMF Variation and Massive-Star Rotation cites this paper.

The Sc, Ti, and V Abundance Discrepancy: Testing High-Mass IMF Variation and Massive-Star Rotation Nucleosynthesis in Chandrasekhar Mass Models for Type Ia Supernovae and Constraints on Progenitor Systems and Burning-Front Propagation

Reference 76

Resolution
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local_arxiv, observed 2026-07-01T05:15:24.699955Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

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Observation e4641ea5-d4cc-438e-ba39-a6bd61c794a4 · inbound

RABBITS IV: Stellar feedback and SMBH merging time-scales in the sub-Milky Way mass regime cites this paper.

RABBITS IV: Stellar feedback and SMBH merging time-scales in the sub-Milky Way mass regime Nucleosynthesis in Chandrasekhar Mass Models for Type Ia Supernovae and Constraints on Progenitor Systems and Burning-Front Propagation

Reference 91

Resolution
unresolved
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Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 7039531a-d0eb-4099-9280-26102ef400bc · inbound

Chemical Evolution of Galaxies: Past, Present and Future cites this paper.

Chemical Evolution of Galaxies: Past, Present and Future Nucleosynthesis in Chandrasekhar Mass Models for Type Ia Supernovae and Constraints on Progenitor Systems and Burning-Front Propagation

Reference 108

Resolution
unresolved
no resolver link, observed 2026-08-01T22:19:57.614428Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 446a322e-535e-487a-a501-be402c3bf7f4 · inbound

Chemical Abundances and Globular Clusters of Milky Way Dwarf Galaxies cites this paper.

Chemical Abundances and Globular Clusters of Milky Way Dwarf Galaxies Nucleosynthesis in Chandrasekhar Mass Models for Type Ia Supernovae and Constraints on Progenitor Systems and Burning-Front Propagation

Reference 61

Resolution
unresolved
no resolver link, observed 2026-08-15T14:56:15.832890Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 327f7194-229c-469a-a03a-3bcfc85e483e · inbound

Kings of the Milky Way: A Homogeneous Gaia DR3 Analysis of King Open Clusters and the Galactic Disc Metallicity Gradient cites this paper.

Kings of the Milky Way: A Homogeneous Gaia DR3 Analysis of King Open Clusters and the Galactic Disc Metallicity Gradient Nucleosynthesis in Chandrasekhar Mass Models for Type Ia Supernovae and Constraints on Progenitor Systems and Burning-Front Propagation

Reference 255

Resolution
unresolved
no resolver link, observed 2026-08-12T00:23:45.947839Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation ed92ac76-166e-440a-84c5-734f5a06b352 · inbound

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics cites this paper.

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics Nucleosynthesis in Chandrasekhar Mass Models for Type Ia Supernovae and Constraints on Progenitor Systems and Burning-Front Propagation

Reference 210

Resolution
unresolved
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Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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