Paper Citation Record · LEDGER

Characterisation of all known multiple stellar systems within 10 pc

As of 11 August 2026, this Paper Citation Record lists 15 of 15 outbound references and 1 inbound Pith citation observation for arXiv:2605.04094.

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

pith.paper-citation-record.v1
2605.04094 v1

Coverage vector

measured 15 of 15 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links, observed 2026-05-09T20:28:59.523387Z

measured 16 of 16 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 1 of 1 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-07-31T12:52:33.107420Z

measured 0 of 1 external citation measurements

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

Source: cited_works

Reference resolution

15 of 15 outbound references displayed

verified exact1
verified fuzzy8
unresolved2
parse uncertain0
malformed identifier4
metadata mismatch0

External citation measurements

No source-named external measurement is stored.

Outbound references

Observation 4972a5fb-dced-427c-b212-96a62dc85e3a · outbound

This paper cites A., Levy S.

Characterisation of all known multiple stellar systems within 10 pc A., Levy S

Reference 1

Resolution: verified exact; doi, observed 2026-05-09T20:37:32.339216Z

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.

Observation 08030a7a-9cc1-4b90-ad58-3c0ef5b984a7 · outbound

This paper cites J., et al., 2000, AJ, 119, 906 Ségransan D., Delfosse X., Forveille T., Beuzit J.

Characterisation of all known multiple stellar systems within 10 pc J., et al., 2000, AJ, 119, 906 Ségransan D., Delfosse X., Forveille T., Beuzit J

Reference 2

Resolution: verified fuzzy; raw_fallback, observed 2026-05-24T12:16:12.407202Z

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.

Observation 7b22f904-8dab-464c-a2cf-6263a724a52c · outbound

This paper cites 1 Tokovinin A., 2023, in Docobo J.

Characterisation of all known multiple stellar systems within 10 pc 1 Tokovinin A., 2023, in Docobo J

Reference 3

Resolution: verified fuzzy; raw_fallback, observed 2026-05-24T12:16:12.410367Z

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.

Observation 3cf61156-ea23-4fcb-abb8-9b402093f26e · outbound

This paper cites 1 Tokovinin A., 2024, in Docobo J.

Characterisation of all known multiple stellar systems within 10 pc 1 Tokovinin A., 2024, in Docobo J

Reference 4

Resolution: verified fuzzy; raw_fallback, observed 2026-05-24T12:16:12.400907Z

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.

Observation 14716923-2e5e-4394-a5cb-3f1daac958e6 · outbound

This paper cites an unresolved cited work.

Characterisation of all known multiple stellar systems within 10 pc Unresolved cited work

Reference 5

Resolution: unresolved; raw_fallback, observed 2026-05-24T12:16:12.403699Z

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.

Observation f289d12a-a5cb-4e5d-a0be-0acce35165e3 · outbound

This paper cites 1995, 1998).

Characterisation of all known multiple stellar systems within 10 pc 1995, 1998)

Reference 6

Resolution: verified fuzzy; raw_fallback, observed 2026-05-24T12:16:12.383787Z

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.

Observation 2358d174-4928-42e8-83d8-491c8da0dd0b · outbound

This paper cites (1999) with adaptive optics at an angular separation of 0.620arcsec.

Characterisation of all known multiple stellar systems within 10 pc (1999) with adaptive optics at an angular separation of 0.620arcsec

Reference 7

Resolution: verified fuzzy; raw_fallback, observed 2026-05-24T12:16:12.380670Z

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.

Observation 757fc7ae-42f4-4d84-8a4b-eabfdf6a31f4 · outbound

This paper cites In fact, it appears to be single based on extremely precise astrometry fromGaia(e.g., Kervella et al.

Characterisation of all known multiple stellar systems within 10 pc In fact, it appears to be single based on extremely precise astrometry fromGaia(e.g., Kervella et al

Reference 8

Resolution: verified fuzzy; raw_fallback, observed 2026-05-24T12:16:12.373110Z

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.

Observation d0c0b3ce-0748-4155-a81a-8bc09293ccb5 · outbound

This paper cites defini- tive.

Characterisation of all known multiple stellar systems within 10 pc defini- tive

Reference 9

Resolution: verified fuzzy; raw_fallback, observed 2026-05-24T12:16:12.396492Z

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.

Observation 59ff377b-4b96-433a-84ce-63b9fc2f101d · outbound

This paper cites The primary component, HD 152751, has an M3.0V spectral type (Reid et al.

Characterisation of all known multiple stellar systems within 10 pc The primary component, HD 152751, has an M3.0V spectral type (Reid et al

Reference 10

Resolution: verified fuzzy; raw_fallback, observed 2026-05-24T12:16:12.376738Z

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.

Observation db4db3d2-7bf3-47a3-ad9b-f696e8cf8541 · outbound

This paper cites 1999), with inner and outer orbital periods of 2.965 and 627 days, respec- tively,andacombinedmassofroughlyonesolarmass(Mazehetal.

Characterisation of all known multiple stellar systems within 10 pc 1999), with inner and outer orbital periods of 2.965 and 627 days, respec- tively,andacombinedmassofroughlyonesolarmass(Mazehetal

Reference 11

Resolution: malformed identifier; raw_fallback, observed 2026-05-24T12:16:12.387831Z

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.

Observation 01074a21-42d4-45cb-8bf3-7abb8e09de57 · outbound

This paper cites We refrain from tabulating stars with ‘GJ’ identifier≥9000, as they were not part of any Gliese or Gliese-Jahreiss catalogues.

Characterisation of all known multiple stellar systems within 10 pc We refrain from tabulating stars with ‘GJ’ identifier≥9000, as they were not part of any Gliese or Gliese-Jahreiss catalogues

Reference 12

Resolution: malformed identifier; raw_fallback, observed 2026-05-24T12:16:12.392375Z

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.

Observation 716b9df5-0ab3-4625-a57a-f694dd3c2e80 · outbound

This paper cites González-Payo et al.Table C2: Individual components in all multiple systems at𝑑 <10pc(continued).

Characterisation of all known multiple stellar systems within 10 pc González-Payo et al.Table C2: Individual components in all multiple systems at𝑑 <10pc(continued)

Reference 13

Resolution: malformed identifier; arxiv_id, observed 2026-05-11T15:11:08.369073Z

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.

Observation 93446f07-dccd-48f9-80d3-618e6a0ef9af · outbound

This paper cites González-Payo et al.Table C3: Pairs in all multiple systems at𝑑 <10pc(continued).

Characterisation of all known multiple stellar systems within 10 pc González-Payo et al.Table C3: Pairs in all multiple systems at𝑑 <10pc(continued)

Reference 14

Resolution: malformed identifier; arxiv_id, observed 2026-05-11T15:11:08.380586Z

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.

Observation 2a7446ec-a8a2-4181-9d2b-7f4c31e22b35 · outbound

This paper cites an unresolved cited work.

Characterisation of all known multiple stellar systems within 10 pc Unresolved cited work

Reference 15

Resolution: unresolved; raw_fallback, observed 2026-05-24T12:16:12.369158Z

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.

Pith citing papers

Observation 5fbcedf1-08e2-4071-b29f-6e35296e2129 · inbound

Identification of unresolved binaries in the VVV b294 tile: A Pro-Am collaboration using the Virtual Observatory cites this paper.

Identification of unresolved binaries in the VVV b294 tile: A Pro-Am collaboration using the Virtual Observatory Characterisation of all known multiple stellar systems within 10 pc

Reference 81

Resolution: unresolved; no resolver link, observed 2026-07-31T12:52:33.107420Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.