Paper Citation Record · LEDGER

Why Wide Jupiter-Mass Binary-Objects Cannot Form

As of 17 August 2026, this Paper Citation Record lists 24 of 24 outbound references and 0 inbound Pith citation observations for arXiv:2507.11786.

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

pith.paper-citation-record.v1
2507.11786 v1

Coverage vector

measured 24 of 24 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links, observed 2026-08-06T17:11:32.171566Z

measured 24 of 24 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-17T06:30:58.91139+00:00

measured 0 of 0 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links

measured 0 of 1 external citation measurements

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

Source: cited_works

Reference resolution

24 of 24 outbound references displayed

verified exact2
verified fuzzy5
unresolved13
parse uncertain0
malformed identifier1
metadata mismatch3

External citation measurements

No source-named external measurement is stored.

Outbound references

Observation 05988e54-b1ed-4889-bc9f-948bdadd2f36 · outbound

This paper cites Jupiter Mass Binary Objects in the Trapezium Cluster.

Why Wide Jupiter-Mass Binary-Objects Cannot Form Jupiter Mass Binary Objects in the Trapezium Cluster

Reference 1

Resolution: unresolved; no resolver link, observed 2026-08-06T17:11:32.067933Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 2760aa20-cffa-46b5-9946-0f7833aafac5 · outbound

This paper cites Floating binary planets from ejections during close stellar encounters.

Why Wide Jupiter-Mass Binary-Objects Cannot Form Floating binary planets from ejections during close stellar encounters

Reference 2

Resolution: metadata mismatch; local_arxiv, observed 2026-08-06T17:11:32.481680Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

Observation 112ce383-43bc-4730-b087-e911c1736a48 · outbound

This paper cites SciPost Astronomy3(1), 001 (2024) https: //doi.org/10.21468/SciPostAstro.3.1.001.

Why Wide Jupiter-Mass Binary-Objects Cannot Form SciPost Astronomy3(1), 001 (2024) https: //doi.org/10.21468/SciPostAstro.3.1.001

Reference 3

Resolution: verified exact; doi, observed 2026-08-06T17:11:32.245792Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

Observation e288e8e0-654f-4928-afcb-183a27cdb1f6 · outbound

This paper cites Free-Floating Planets, Survivor Planets, Captured Planets and Binary Planets from Stellar Flybys.

Why Wide Jupiter-Mass Binary-Objects Cannot Form Free-Floating Planets, Survivor Planets, Captured Planets and Binary Planets from Stellar Flybys

Reference 4

Resolution: unresolved; no resolver link, observed 2026-08-06T17:11:32.083322Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 4cd5dcb9-9276-49be-af50-cdeb6a568ee0 · outbound

This paper cites MNRAS 322, 231–246 (2001).

Why Wide Jupiter-Mass Binary-Objects Cannot Form MNRAS 322, 231–246 (2001)

Reference 5

Resolution: verified fuzzy; raw_fallback, observed 2026-08-06T17:11:32.552674Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

Observation 485d2239-692f-42c1-b51c-c1098985f51d · outbound

This paper cites ApJ 492, 540–553 (1998) https://doi.org/10.

Why Wide Jupiter-Mass Binary-Objects Cannot Form ApJ 492, 540–553 (1998) https://doi.org/10

Reference 6

Resolution: verified fuzzy; raw_fallback, observed 2026-08-06T17:11:32.541142Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

Observation 7cd26bcd-4228-46bd-89cf-709ece337d8a · outbound

This paper cites I - Numerical experiments for equal masses.

Why Wide Jupiter-Mass Binary-Objects Cannot Form I - Numerical experiments for equal masses

Reference 7

Resolution: unresolved; no resolver link, observed 2026-08-06T17:11:32.097362Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 4099930f-55ec-4239-ae0a-be4cafa07a83 · outbound

This paper cites AJ 95, 1755 (1988) https://doi.org/10.1086/114773.

Why Wide Jupiter-Mass Binary-Objects Cannot Form AJ 95, 1755 (1988) https://doi.org/10.1086/114773

Reference 8

Resolution: unresolved; no resolver link, observed 2026-08-06T17:11:32.102319Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7da1c2c4-0ff9-4d00-8fb8-f00b1e46aad9 · outbound

This paper cites Size distribution of circumstellar disks in the Trapezium cluster.

Why Wide Jupiter-Mass Binary-Objects Cannot Form Size distribution of circumstellar disks in the Trapezium cluster

Reference 9

Resolution: metadata mismatch; local_arxiv, observed 2026-08-06T17:11:32.451386Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

Observation ac7d8108-8876-4f88-b6fb-5009d1d0c8e6 · outbound

This paper cites Measurement of Circumstellar Disk Sizes in the Upper Scorpius OB Association with ALMA.

Why Wide Jupiter-Mass Binary-Objects Cannot Form Measurement of Circumstellar Disk Sizes in the Upper Scorpius OB Association with ALMA

Reference 10

Resolution: unresolved; no resolver link, observed 2026-08-06T17:11:32.111280Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 8c5a030b-76bf-4a27-a7cd-9fda73e1cebe · outbound

This paper cites Formation of wide-orbit giant planets in protoplanetary disks with a decreasing pebble flux.

Why Wide Jupiter-Mass Binary-Objects Cannot Form Formation of wide-orbit giant planets in protoplanetary disks with a decreasing pebble flux

Reference 11

Resolution: metadata mismatch; local_arxiv, observed 2026-08-06T17:11:32.422082Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

Observation a09ff9bf-ae84-4091-b9f1-8add91f016dd · outbound

This paper cites Computer Physics Communications 184, 456–468 (2013) https://doi.

Why Wide Jupiter-Mass Binary-Objects Cannot Form Computer Physics Communications 184, 456–468 (2013) https://doi

Reference 12

Resolution: unresolved; no resolver link, observed 2026-08-06T17:11:32.119831Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 5f985052-013a-46a0-89ca-ed66d17cb675 · outbound

This paper cites MNRAS 71, 460–470 (1911) 7.

Why Wide Jupiter-Mass Binary-Objects Cannot Form MNRAS 71, 460–470 (1911) 7

Reference 13

Resolution: verified fuzzy; raw_fallback, observed 2026-08-06T17:11:32.530430Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

Observation e71656b5-4e96-4fbd-ac77-2cee26e2147a · outbound

This paper cites The minimum mass for star formation, and the origin of binary brown dwarfs.

Why Wide Jupiter-Mass Binary-Objects Cannot Form The minimum mass for star formation, and the origin of binary brown dwarfs

Reference 14

Resolution: unresolved; no resolver link, observed 2026-08-06T17:11:32.128826Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation b6f58008-6d30-4a36-9181-eed426f7cbc0 · outbound

This paper cites ALMA Observations of Circumstellar Disks in the Upper Scorpius OB Association.

Why Wide Jupiter-Mass Binary-Objects Cannot Form ALMA Observations of Circumstellar Disks in the Upper Scorpius OB Association

Reference 15

Resolution: unresolved; no resolver link, observed 2026-08-06T17:11:32.133154Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 4f5685be-92c0-4360-8c36-c3b9e46ad5dd · outbound

This paper cites Zenodo (2018).

Why Wide Jupiter-Mass Binary-Objects Cannot Form Zenodo (2018)

Reference 16

Resolution: malformed identifier; doi_truncated, observed 2026-08-06T17:11:32.214384Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

Observation ffdbcde9-60ae-4986-a764-73a10fef8443 · outbound

This paper cites The dynamical evolution of fractal star clusters: the survival of substructure.

Why Wide Jupiter-Mass Binary-Objects Cannot Form The dynamical evolution of fractal star clusters: the survival of substructure

Reference 17

Resolution: unresolved; no resolver link, observed 2026-08-06T17:11:32.142200Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 272823e2-6536-4bdf-a3b4-db20decfd365 · outbound

This paper cites Computing in Science Engineering 13(2), 22–30 (2011) https://doi.org/10.1109/MCSE.2011.37.

Why Wide Jupiter-Mass Binary-Objects Cannot Form Computing in Science Engineering 13(2), 22–30 (2011) https://doi.org/10.1109/MCSE.2011.37

Reference 18

Resolution: unresolved; no resolver link, observed 2026-08-06T17:11:32.146759Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c20176e4-b053-4473-a334-c70496122277 · outbound

This paper cites Chaos in self-gravitating many-body systems: Lyapunov time dependence of $N$ and the influence of general relativity.

Why Wide Jupiter-Mass Binary-Objects Cannot Form Chaos in self-gravitating many-body systems: Lyapunov time dependence of $N$ and the influence of general relativity

Reference 19

Resolution: verified exact; local_arxiv, observed 2026-08-06T17:11:32.372011Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

Observation f05fc701-2d9e-4833-9ef0-1cafb97a9896 · outbound

This paper cites Computing in Science and Engineering 9, 90–95 (2007) https://doi.org/10.1109/MCSE.2007.55.

Why Wide Jupiter-Mass Binary-Objects Cannot Form Computing in Science and Engineering 9, 90–95 (2007) https://doi.org/10.1109/MCSE.2007.55

Reference 20

Resolution: unresolved; no resolver link, observed 2026-08-06T17:11:32.155721Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 4dd07dea-2900-46ae-ad05-e2034012902c · outbound

This paper cites CreateSpace, Scotts Valley, CA (2009).

Why Wide Jupiter-Mass Binary-Objects Cannot Form CreateSpace, Scotts Valley, CA (2009)

Reference 21

Resolution: unresolved; no resolver link, observed 2026-08-06T17:11:32.159834Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation eb464f44-4ca2-4362-be19-78eaf8db9b80 · outbound

This paper cites A&A 309, 179–196 (1996).

Why Wide Jupiter-Mass Binary-Objects Cannot Form A&A 309, 179–196 (1996)

Reference 22

Resolution: verified fuzzy; raw_fallback, observed 2026-08-06T17:11:32.509730Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

Observation dbacf13f-2633-4536-9030-66dff9b110dd · outbound

This paper cites http://www.scipy.org/.

Why Wide Jupiter-Mass Binary-Objects Cannot Form http://www.scipy.org/

Reference 23

Resolution: verified fuzzy; raw_fallback, observed 2026-08-06T17:11:32.495949Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

Observation e0f30d9c-6d2f-4e76-ae1a-7d04b4758ba3 · outbound

This paper cites Dissection of an open star cluster: spectroscopy.

Why Wide Jupiter-Mass Binary-Objects Cannot Form Dissection of an open star cluster: spectroscopy

Reference 24

Resolution: unresolved; no resolver link, observed 2026-08-06T17:11:32.171566Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Pith citing papers

No inbound Pith citation observations are available.