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Paper Citation Record · LEDGER

The Evolution of Massive Stellar Multiplicity in the Field I. Numerical simulations, long-term evolution and final outcomes

As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:2412.14022.

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

pith.paper-citation-record.v1
2412.14022 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 5 of 5 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-10T06:31:04.303077+00:00

measured 5 of 5 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T14:45:42.434253Z

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

2
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 82e2da78-fc4b-4c4b-b55c-a0c4fd57c3cb · inbound

Stellar-mass black holes in young massive and open stellar clusters -- VI. Role of external galactic field cites this paper.

Stellar-mass black holes in young massive and open stellar clusters -- VI. Role of external galactic field The Evolution of Massive Stellar Multiplicity in the Field I. Numerical simulations, long-term evolution and final outcomes

Reference 7

Resolution
unresolved
no resolver link, observed 2026-08-07T14:45:42.434253Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T14:45:42.434253Z digest=sha256:38f663f7645be343b46553b4de65655211103fdc7f44a6b43ee87fd434880073

Observation 186963cc-c8f6-4d88-bd34-7dc8b5cfc16a · inbound

FROST-CLUSTERS -- II. Massive stars, binaries and triples boost supermassive black hole seed formation in assembling star clusters cites this paper.

FROST-CLUSTERS -- II. Massive stars, binaries and triples boost supermassive black hole seed formation in assembling star clusters The Evolution of Massive Stellar Multiplicity in the Field I. Numerical simulations, long-term evolution and final outcomes

Reference 199

Resolution
unresolved
no resolver link, observed 2026-08-07T10:50:57.460270Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T10:50:57.460270Z digest=sha256:b80a9d8ab20475ec6e137b03727e60de55f2092483d7d95d922b110f0520be4f

Observation ace604de-a9d3-4de4-918d-c3f5483e0973 · inbound

V407 Vul: a triple star system with an AM CVn detectable by gravitational wave observatories cites this paper.

V407 Vul: a triple star system with an AM CVn detectable by gravitational wave observatories The Evolution of Massive Stellar Multiplicity in the Field I. Numerical simulations, long-term evolution and final outcomes

Reference 67

Resolution
unresolved
no resolver link, observed 2026-08-01T02:17:55.091688Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T02:17:55.091688Z digest=sha256:2ed2996aece46b25aa7a3cfbdda062a7396280a8d22d477bd4d55379d49d33f5

Observation 8bed2140-648b-4b6e-b087-4deb887e45f5 · inbound

V407 Vul: a triple star system with an AM CVn detectable by gravitational wave observatories cites this paper.

V407 Vul: a triple star system with an AM CVn detectable by gravitational wave observatories The Evolution of Massive Stellar Multiplicity in the Field I. Numerical simulations, long-term evolution and final outcomes

Reference 211

Resolution
verified exact
local_arxiv, observed 2026-08-01T02:21:29.970591Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=arxiv_source observed=2026-08-01T02:17:55.440155Z digest=sha256:e99509a3a6911999295c29e09e25c0af94b5be224fcfee85e038ff8b7fc5bc69

Observation f33641a9-4bb8-4355-8a86-6345e2ad71b0 · inbound

The IACOB project XIX. Revisiting massive-star evolution with empirical TAMS constraints: updated models, overshoot calibration, and the population of blue supergiants cites this paper.

The IACOB project XIX. Revisiting massive-star evolution with empirical TAMS constraints: updated models, overshoot calibration, and the population of blue supergiants The Evolution of Massive Stellar Multiplicity in the Field I. Numerical simulations, long-term evolution and final outcomes

Reference 248

Resolution
unresolved
no resolver link, observed 2026-08-03T02:40:59.847547Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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