Paper Citation Record · LEDGER

Dynamically derived morphology from the recurrence patterns of close binary stars using Kepler data

As of 8 August 2026, this Paper Citation Record lists 44 of 44 outbound references and 0 inbound Pith citation observations for arXiv:2506.04111.

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

pith.paper-citation-record.v1
2506.04111 v2

Coverage vector

measured 44 of 44 reference resolution

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Pith citing papers itemized under the disclosed page cap.

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Source: cited_works

Reference resolution

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External citation measurements

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Outbound references

Observation d0f41dce-c703-451b-8066-df7727e759a1 · outbound

This paper cites write newline.

Dynamically derived morphology from the recurrence patterns of close binary stars using Kepler data write newline

Reference 1

Resolution: unresolved; no resolver link, observed 2026-08-07T10:52:41.109146Z

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Unavailable: canonical work link unavailable.

Observation be8cd69c-7615-4270-a2ce-1d187365968e · outbound

This paper cites an unresolved cited work.

Dynamically derived morphology from the recurrence patterns of close binary stars using Kepler data Unresolved cited work

Reference 2

Resolution: unresolved; raw_fallback, observed 2026-08-07T10:52:49.052028Z

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Observation 68cad5b3-3cf2-4675-b0b1-572749520f60 · outbound

This paper cites an unresolved cited work.

Dynamically derived morphology from the recurrence patterns of close binary stars using Kepler data Unresolved cited work

Reference 3

Resolution: unresolved; raw_fallback, observed 2026-08-07T10:52:49.038839Z

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Observation f2c19726-1638-4a8a-91d9-8ba4607a030e · outbound

This paper cites an unresolved cited work.

Dynamically derived morphology from the recurrence patterns of close binary stars using Kepler data Unresolved cited work

Reference 4

Resolution: unresolved; no resolver link, observed 2026-08-07T10:52:41.303055Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation b71bd454-c7ff-4c45-b53b-6c3dac293fae · outbound

This paper cites an unresolved cited work.

Dynamically derived morphology from the recurrence patterns of close binary stars using Kepler data Unresolved cited work

Reference 5

Resolution: verified exact; doi, observed 2026-08-07T10:52:46.597498Z

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Observation 6fc9d094-7996-4b59-b2d9-2ef27873663f · outbound

This paper cites B., Klagyivik P., 2015, @doi [Monthly Notices of the Royal Astronomical Society] 10.1093/mnras/stv2530 , 455, 4136.

Dynamically derived morphology from the recurrence patterns of close binary stars using Kepler data B., Klagyivik P., 2015, @doi [Monthly Notices of the Royal Astronomical Society] 10.1093/mnras/stv2530 , 455, 4136

Reference 6

Resolution: unresolved; no resolver link, observed 2026-08-07T10:52:41.455329Z

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Observation 3bb0616b-c992-4b13-b079-02b20e4e61ff · outbound

This paper cites J., et al., 2010, @doi [Science] 10.1126/science.1185402 , https://ui.adsabs.harvard.edu/abs/2010Sci...327..977B 327, 977.

Dynamically derived morphology from the recurrence patterns of close binary stars using Kepler data J., et al., 2010, @doi [Science] 10.1126/science.1185402 , https://ui.adsabs.harvard.edu/abs/2010Sci...327..977B 327, 977

Reference 7

Resolution: unresolved; no resolver link, observed 2026-08-07T10:52:41.527560Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 15622680-aa2e-4bc8-8e1d-f4abf3a7a78d · outbound

This paper cites an unresolved cited work.

Dynamically derived morphology from the recurrence patterns of close binary stars using Kepler data Unresolved cited work

Reference 8

Resolution: unresolved; no resolver link, observed 2026-08-07T10:52:41.622514Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e74517a6-79c3-4a21-8fcf-e6dabd66321d · outbound

This paper cites an unresolved cited work.

Dynamically derived morphology from the recurrence patterns of close binary stars using Kepler data Unresolved cited work

Reference 9

Resolution: unresolved; raw_fallback, observed 2026-08-07T10:52:49.026569Z

Source-reported events for the cited work

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Observation 2e6adccd-b064-46bf-bf5e-f9143106d528 · outbound

This paper cites F., et al., 2015, @doi [Chaos: An Interdisciplinary Journal of Nonlinear Science] 10.1063/1.4934554 , 25, 113101.

Dynamically derived morphology from the recurrence patterns of close binary stars using Kepler data F., et al., 2015, @doi [Chaos: An Interdisciplinary Journal of Nonlinear Science] 10.1063/1.4934554 , 25, 113101

Reference 10

Resolution: verified exact; doi, observed 2026-08-07T10:52:46.264572Z

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Observation 276bb5a5-bb36-4272-964a-9a98c7eb5c01 · outbound

This paper cites O., Ruelle D., et al., 1995, World Scientific Series on Nonlinear Science Series A, 16, 441.

Dynamically derived morphology from the recurrence patterns of close binary stars using Kepler data O., Ruelle D., et al., 1995, World Scientific Series on Nonlinear Science Series A, 16, 441

Reference 11

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T10:52:49.013341Z

Source-reported events for the cited work

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Observation ff363619-23b1-44b4-a5e4-30f6ca685558 · outbound

This paper cites an unresolved cited work.

Dynamically derived morphology from the recurrence patterns of close binary stars using Kepler data Unresolved cited work

Reference 12

Resolution: unresolved; raw_fallback, observed 2026-08-07T10:52:48.999449Z

Source-reported events for the cited work

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Observation c46c4235-9a52-4741-86d2-ab1c3b4539d4 · outbound

This paper cites an unresolved cited work.

Dynamically derived morphology from the recurrence patterns of close binary stars using Kepler data Unresolved cited work

Reference 13

Resolution: unresolved; raw_fallback, observed 2026-08-07T10:52:48.984744Z

Source-reported events for the cited work

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Observation 836e126a-91b4-4f00-9da5-aa0f3a9ca56d · outbound

This paper cites V., Misra R., Ambika G., 2019, @doi [Chaos: An Interdisciplinary Journal of Nonlinear Science] 10.1063/1.5120739 , 29, 113112.

Dynamically derived morphology from the recurrence patterns of close binary stars using Kepler data V., Misra R., Ambika G., 2019, @doi [Chaos: An Interdisciplinary Journal of Nonlinear Science] 10.1063/1.5120739 , 29, 113112

Reference 14

Resolution: verified exact; doi, observed 2026-08-07T10:52:46.001935Z

Source-reported events for the cited work

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Observation 773047f8-da9c-4ff0-a87e-91af70994d88 · outbound

This paper cites V., Misra R., Ambika G., 2020, @doi [Communications in Nonlinear Science and Numerical Simulation] https://doi.org/10.1016/j.cnsns.2019.104988 , 80, 104988.

Dynamically derived morphology from the recurrence patterns of close binary stars using Kepler data V., Misra R., Ambika G., 2020, @doi [Communications in Nonlinear Science and Numerical Simulation] https://doi.org/10.1016/j.cnsns.2019.104988 , 80, 104988

Reference 15

Resolution: unresolved; no resolver link, observed 2026-08-07T10:52:42.239774Z

Source-reported events for the cited work

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Observation 169d47ab-2f65-4d97-8026-1778203220ef · outbound

This paper cites P., Misra R., Ambika G., 2011, @doi [Research in Astronomy and Astrophysics] 10.1088/1674-4527/11/1/004 , https://ui.adsabs.harvard.edu/abs/2011RAA....11...71H 11, 71.

Dynamically derived morphology from the recurrence patterns of close binary stars using Kepler data P., Misra R., Ambika G., 2011, @doi [Research in Astronomy and Astrophysics] 10.1088/1674-4527/11/1/004 , https://ui.adsabs.harvard.edu/abs/2011RAA....11...71H 11, 71

Reference 16

Resolution: verified exact; doi, observed 2026-08-07T10:52:45.794234Z

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Observation c3b63c85-9109-481d-b31c-cd16f1f40f3c · outbound

This paper cites J., 1992, in , Breakthroughs in statistics: Methodology and distribution.

Dynamically derived morphology from the recurrence patterns of close binary stars using Kepler data J., 1992, in , Breakthroughs in statistics: Methodology and distribution

Reference 17

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T10:52:48.970795Z

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Observation bb56b3c8-f00c-40fd-ba26-3ba30c9aaf9c · outbound

This paper cites an unresolved cited work.

Dynamically derived morphology from the recurrence patterns of close binary stars using Kepler data Unresolved cited work

Reference 18

Resolution: unresolved; raw_fallback, observed 2026-08-07T10:52:48.957991Z

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Observation 62327e5b-7d41-4a4c-996f-509904030704 · outbound

This paper cites F., Caballero-Nieves S.

Dynamically derived morphology from the recurrence patterns of close binary stars using Kepler data F., Caballero-Nieves S

Reference 19

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T10:52:48.945181Z

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Observation fed15546-9a3d-41f5-af81-0137e5b2037a · outbound

This paper cites an unresolved cited work.

Dynamically derived morphology from the recurrence patterns of close binary stars using Kepler data Unresolved cited work

Reference 20

Resolution: unresolved; raw_fallback, observed 2026-08-07T10:52:48.869543Z

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Observation 24ad1d4e-0459-4d9b-a806-263ed8eef15d · outbound

This paper cites an unresolved cited work.

Dynamically derived morphology from the recurrence patterns of close binary stars using Kepler data Unresolved cited work

Reference 21

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Observation accdea6f-9d5e-49f7-a840-079244dccc59 · outbound

This paper cites an unresolved cited work.

Dynamically derived morphology from the recurrence patterns of close binary stars using Kepler data Unresolved cited work

Reference 22

Resolution: unresolved; no resolver link, observed 2026-08-07T10:52:42.844450Z

Source-reported events for the cited work

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Observation 514f3b93-9280-4148-a0d4-751b71e31c6e · outbound

This paper cites A., Welsh W.

Dynamically derived morphology from the recurrence patterns of close binary stars using Kepler data A., Welsh W

Reference 23

Resolution: unresolved; no resolver link, observed 2026-08-07T10:52:42.915173Z

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Observation 7c868f2b-d319-462a-8eb0-c6b295dfb0e1 · outbound

This paper cites an unresolved cited work.

Dynamically derived morphology from the recurrence patterns of close binary stars using Kepler data Unresolved cited work

Reference 24

Resolution: unresolved; raw_fallback, observed 2026-08-07T10:52:48.705361Z

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Observation 7293e76a-3966-40dd-ab79-d247513f640a · outbound

This paper cites P., Mukhopadhyay B., Ambika G., Kembhavi A.

Dynamically derived morphology from the recurrence patterns of close binary stars using Kepler data P., Mukhopadhyay B., Ambika G., Kembhavi A

Reference 25

Resolution: verified exact; doi, observed 2026-08-07T10:52:45.523411Z

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Observation 999273b4-7f97-4e11-9af1-2a5ee7f5c9f0 · outbound

This paper cites P., Ambika G., Kembhavi A.

Dynamically derived morphology from the recurrence patterns of close binary stars using Kepler data P., Ambika G., Kembhavi A

Reference 26

Resolution: verified exact; doi, observed 2026-08-07T10:52:45.383530Z

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Observation ee134acf-27db-416d-9cb5-ff7c4096000a · outbound

This paper cites K., 2022, @doi [ ] 10.1007/s10509-022-04050-9 , https://ui.adsabs.harvard.edu/abs/2022Ap&SS.367...19M 367, 19.

Dynamically derived morphology from the recurrence patterns of close binary stars using Kepler data K., 2022, @doi [ ] 10.1007/s10509-022-04050-9 , https://ui.adsabs.harvard.edu/abs/2022Ap&SS.367...19M 367, 19

Reference 27

Resolution: verified exact; doi, observed 2026-08-07T10:52:45.195576Z

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Observation e7e3011c-7de0-46e6-8941-2a60e9a2fba1 · outbound

This paper cites H., Crutchfield J.

Dynamically derived morphology from the recurrence patterns of close binary stars using Kepler data H., Crutchfield J

Reference 28

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T10:52:48.527876Z

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Observation 2b507f03-7c79-4b78-94c2-d0b8f6d319d8 · outbound

This paper cites G., Burger D.

Dynamically derived morphology from the recurrence patterns of close binary stars using Kepler data G., Burger D

Reference 29

Resolution: verified exact; doi, observed 2026-08-07T10:52:45.000501Z

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Observation d96c5f94-7516-4722-baa1-534774e1aca8 · outbound

This paper cites A., Boyd P.

Dynamically derived morphology from the recurrence patterns of close binary stars using Kepler data A., Boyd P

Reference 30

Resolution: verified exact; doi, observed 2026-08-07T10:52:44.852094Z

Source-reported events for the cited work

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Observation 90f93a29-5556-446d-8370-c349d002a3c1 · outbound

This paper cites H., 2007, Numerical recipes 3rd edition: The art of scientific computing.

Dynamically derived morphology from the recurrence patterns of close binary stars using Kepler data H., 2007, Numerical recipes 3rd edition: The art of scientific computing

Reference 31

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T10:52:48.409823Z

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Observation 7f22e77f-440b-4227-b5a8-522cc6eb258f · outbound

This paper cites an unresolved cited work.

Dynamically derived morphology from the recurrence patterns of close binary stars using Kepler data Unresolved cited work

Reference 32

Resolution: unresolved; no resolver link, observed 2026-08-07T10:52:43.545219Z

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Observation e6f3af7b-ba45-4fa2-9364-4b968184955e · outbound

This paper cites M., S \'a nchez-Fern \'a ndez C., Gim \'e nez \'A ., 2006, @doi [ ] 10.1051/0004-6361:20052830 , https://ui.adsabs.harvard.edu/abs/2006A&A...446..395S 446, 395.

Dynamically derived morphology from the recurrence patterns of close binary stars using Kepler data M., S \'a nchez-Fern \'a ndez C., Gim \'e nez \'A ., 2006, @doi [ ] 10.1051/0004-6361:20052830 , https://ui.adsabs.harvard.edu/abs/2006A&A...446..395S 446, 395

Reference 33

Resolution: unresolved; no resolver link, observed 2026-08-07T10:52:43.599042Z

Source-reported events for the cited work

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Observation dbee06cb-4f9c-43ab-b74e-c5d92f3be6ca · outbound

This paper cites W., 2011, IEEE Signal processing magazine, 28, 111.

Dynamically derived morphology from the recurrence patterns of close binary stars using Kepler data W., 2011, IEEE Signal processing magazine, 28, 111

Reference 34

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T10:52:48.180947Z

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Observation 618cbfff-6523-475e-9669-eaf9396570bd · outbound

This paper cites N., 2003, in Meyers R.

Dynamically derived morphology from the recurrence patterns of close binary stars using Kepler data N., 2003, in Meyers R

Reference 35

Resolution: verified exact; doi, observed 2026-08-07T10:52:44.708406Z

Source-reported events for the cited work

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Observation eb224f64-9ba4-4992-b88c-fb93850e0cd6 · outbound

This paper cites H., 1982, The Physical Universe.

Dynamically derived morphology from the recurrence patterns of close binary stars using Kepler data H., 1982, The Physical Universe

Reference 36

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T10:52:47.918608Z

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Observation 741f0e56-88db-4a87-ab26-1dd1088eb0e0 · outbound

This paper cites W., et al., 2011, @doi [ ] 10.1088/0004-6256/142/5/160 , https://ui.adsabs.harvard.edu/abs/2011AJ....142..160S 142, 160.

Dynamically derived morphology from the recurrence patterns of close binary stars using Kepler data W., et al., 2011, @doi [ ] 10.1088/0004-6256/142/5/160 , https://ui.adsabs.harvard.edu/abs/2011AJ....142..160S 142, 160

Reference 37

Resolution: unresolved; no resolver link, observed 2026-08-07T10:52:43.898399Z

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Observation ab65c727-5280-4f3b-b00c-7daa860633c9 · outbound

This paper cites an unresolved cited work.

Dynamically derived morphology from the recurrence patterns of close binary stars using Kepler data Unresolved cited work

Reference 38

Resolution: verified exact; doi, observed 2026-08-07T10:52:44.490651Z

Source-reported events for the cited work

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Observation 19565f79-dcbf-4751-a39b-7c812371bf81 · outbound

This paper cites Springer Berlin Heidelberg, Berlin, Heidelberg, pp 366--381.

Dynamically derived morphology from the recurrence patterns of close binary stars using Kepler data Springer Berlin Heidelberg, Berlin, Heidelberg, pp 366--381

Reference 39

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T10:52:47.721914Z

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Observation b0bb96d0-2879-4134-977d-47010cd0dc1a · outbound

This paper cites an unresolved cited work.

Dynamically derived morphology from the recurrence patterns of close binary stars using Kepler data Unresolved cited work

Reference 40

Resolution: unresolved; raw_fallback, observed 2026-08-07T10:52:47.528957Z

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Observation 96e31846-9dcd-4d10-846b-23c1aa9f5e49 · outbound

This paper cites an unresolved cited work.

Dynamically derived morphology from the recurrence patterns of close binary stars using Kepler data Unresolved cited work

Reference 41

Resolution: unresolved; raw_fallback, observed 2026-08-07T10:52:47.305102Z

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Observation 9ead580a-58b3-4cb1-b1f3-aa341ad244c6 · outbound

This paper cites @esa (Ref.

Dynamically derived morphology from the recurrence patterns of close binary stars using Kepler data @esa (Ref

Reference 42

Resolution: unresolved; no resolver link, observed 2026-08-07T10:52:44.199354Z

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Observation 2353e071-76be-414b-b001-e6cad3753bd3 · outbound

This paper cites an unresolved cited work.

Dynamically derived morphology from the recurrence patterns of close binary stars using Kepler data Unresolved cited work

Reference 43

Resolution: unresolved; no resolver link, observed 2026-08-07T10:52:44.262385Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 2292aecb-bfd9-4c7a-87ef-fab2143fe352 · outbound

This paper cites =ʄGȝoWhDsZSg>S.

Dynamically derived morphology from the recurrence patterns of close binary stars using Kepler data =ʄGȝoWhDsZSg>S

Reference 44

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T10:52:47.051894Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Pith citing papers

No inbound Pith citation observations are available.