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Paper Citation Record · LEDGER

Stellar population synthesis models with a physically varying IMF

As of 10 August 2026, this Paper Citation Record lists 40 of 40 outbound references and 2 inbound Pith citation observations for arXiv:2502.03529.

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

pith.paper-citation-record.v1
2502.03529 v1

Coverage vector

measured 40 of 40 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links, observed 2026-08-09T04:41:45.431663Z

measured 42 of 42 standing notices

One-hop event checks from named stored sources.

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measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-07-12T13:23:49.728041Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-04T01:49:22.746476Z

Reference resolution

40 of 40 outbound references displayed

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External citation measurements

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Outbound references

Observation 8711d203-41d8-417b-b00e-d478f3d6621d · outbound

This paper cites J., Scott P., 2009, ARA&A, 47,.

Stellar population synthesis models with a physically varying IMF J., Scott P., 2009, ARA&A, 47,

Reference 1

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Stellar population synthesis models with a physically varying IMF Unresolved cited work

Reference 10

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Stellar population synthesis models with a physically varying IMF Unresolved cited work

Reference 11

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Observation 2d35a3a7-4dfe-4652-b98b-a70ac08bf226 · outbound

This paper cites The many tensions with dark-matter based models and implications on the nature of the Universe.

Stellar population synthesis models with a physically varying IMF The many tensions with dark-matter based models and implications on the nature of the Universe

Reference 37

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Observation a7b0a28b-8308-476c-8089-7e6318951add · outbound

This paper cites M., Tumlinson, J., et al.

Stellar population synthesis models with a physically varying IMF M., Tumlinson, J., et al

Reference 41

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Stellar population synthesis models with a physically varying IMF Unresolved cited work

Reference 44

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Stellar population synthesis models with a physically varying IMF Unresolved cited work

Reference 65

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Stellar population synthesis models with a physically varying IMF Unresolved cited work

Reference 71

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Stellar population synthesis models with a physically varying IMF Unresolved cited work

Reference 77

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Stellar population synthesis models with a physically varying IMF Unresolved cited work

Reference 95

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Observation 7eaf8d54-c876-484e-9cbb-102656334d67 · outbound

This paper cites 2003, MNRAS, 344, 1000 Calura, F., Recchi, S., Matteucci, F., & Kroupa, P.

Stellar population synthesis models with a physically varying IMF 2003, MNRAS, 344, 1000 Calura, F., Recchi, S., Matteucci, F., & Kroupa, P

Reference 127

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Observation 8560ee4a-f4d2-422e-aeac-9a39f90bc637 · outbound

This paper cites Effects of physical conditions on the stellar initial mass function: The low-metallicity star-forming region Sh 2-209.

Stellar population synthesis models with a physically varying IMF Effects of physical conditions on the stellar initial mass function: The low-metallicity star-forming region Sh 2-209

Reference 137

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Observation 637fd6b7-d0af-4ae5-abc4-e7c6db4fd59b · outbound

This paper cites B., Meurer, G.

Stellar population synthesis models with a physically varying IMF B., Meurer, G

Reference 157

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Stellar population synthesis models with a physically varying IMF Unresolved cited work

Reference 194

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Stellar population synthesis models with a physically varying IMF Unresolved cited work

Reference 212

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Stellar population synthesis models with a physically varying IMF Unresolved cited work

Reference 214

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Stellar population synthesis models with a physically varying IMF Unresolved cited work

Reference 229

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Reference 243

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This paper cites M., Driver, S.

Stellar population synthesis models with a physically varying IMF M., Driver, S

Reference 288

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Reference 365

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This paper cites S., 2012, LRR, 15,.

Stellar population synthesis models with a physically varying IMF S., 2012, LRR, 15,

Reference 455

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This paper cites G., & Villaume, A.

Stellar population synthesis models with a physically varying IMF G., & Villaume, A

Reference 486

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This paper cites 2020, A&A, 637, A68 Yan Z., Jeˇ r´ abkov´ a T., Kroupa P., 2021, A&A, 655, A19.

Stellar population synthesis models with a physically varying IMF 2020, A&A, 637, A68 Yan Z., Jeˇ r´ abkov´ a T., Kroupa P., 2021, A&A, 655, A19

Reference 524

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Reference 673

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Stellar population synthesis models with a physically varying IMF Conroy C., Gunn J

Reference 718

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Stellar population synthesis models with a physically varying IMF 2012, ApJ, 747, 72 Dabringhausen J., Kroupa P., 2023, MNRAS, 526,

Reference 839

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Stellar population synthesis models with a physically varying IMF J., Stanway E

Reference 1081

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Stellar population synthesis models with a physically varying IMF R., & Meyer, M

Reference 1331

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Reference 1491

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Reference 1496

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This paper cites 2001, MNRAS, 322, 231 Kroupa, P.

Stellar population synthesis models with a physically varying IMF 2001, MNRAS, 322, 231 Kroupa, P

Reference 1507

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This paper cites I., 2022, A&A, 660, A61.

Stellar population synthesis models with a physically varying IMF I., 2022, A&A, 660, A61

Reference 2301

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This paper cites Heger A., Fryer C.

Stellar population synthesis models with a physically varying IMF Heger A., Fryer C

Reference 3252

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Stellar population synthesis models with a physically varying IMF T., Gutermuth, R., Muzerolle, J., et al

Reference 3484

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Stellar population synthesis models with a physically varying IMF C., & Koopmans, L

Reference 4086

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Observation 60a0d3bd-b0f8-4630-958b-9fb461627a4a · outbound

This paper cites Scalo, J.

Stellar population synthesis models with a physically varying IMF Scalo, J

Reference 4168

Resolution
verified fuzzy
raw_fallback, observed 2026-08-09T04:41:45.961087Z

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.

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Observation 69d353db-861f-4510-9c82-8a88e9ee48bd · outbound

This paper cites an unresolved cited work.

Stellar population synthesis models with a physically varying IMF Unresolved cited work

Reference 4430

Resolution
unresolved
raw_fallback, observed 2026-08-09T04:41:45.855164Z

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.

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Observation 04080a5f-e246-4ab6-a3b1-5c8405893d91 · outbound

This paper cites R., Eldridge J.

Stellar population synthesis models with a physically varying IMF R., Eldridge J

Reference 4605

Resolution
verified fuzzy
raw_fallback, observed 2026-08-09T04:41:45.869995Z

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.

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Observation 4a7caafc-d3ff-4663-9bec-6c0cc5752bdf · outbound

This paper cites an unresolved cited work.

Stellar population synthesis models with a physically varying IMF Unresolved cited work

Reference 6005

Resolution
unresolved
raw_fallback, observed 2026-08-09T04:41:46.206909Z

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.

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Pith citing papers

Observation 5ec1c099-5259-4537-bf20-b295566655ae · inbound

Baryonic mass budgets in the central regions of the Bullet Cluster and their consistency with strong lensing in MOND cites this paper.

Baryonic mass budgets in the central regions of the Bullet Cluster and their consistency with strong lensing in MOND Stellar population synthesis models with a physically varying IMF

Reference 47

Resolution
verified exact
arxiv_id, observed 2026-07-04T01:49:22.748105Z

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.

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Observation c8ab673f-1d5c-4c65-b067-672dfac3b19e · inbound

Baryonic mass budgets in the central regions of the Bullet Cluster and their consistency with strong lensing in MOND cites this paper.

Baryonic mass budgets in the central regions of the Bullet Cluster and their consistency with strong lensing in MOND Stellar population synthesis models with a physically varying IMF

Reference 47

Resolution
unresolved
no resolver link, observed 2026-07-12T13:23:49.728041Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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