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Paper Citation Record · LEDGER

Does IRS13 require an intermediate-mass black hole?

As of 18 August 2026, this Paper Citation Record lists 100 of 288 outbound references and 0 inbound Pith citation observations for arXiv:2608.10117.

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

pith.paper-citation-record.v1
2608.10117 v1

Coverage vector

measured 100 of 288 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links, observed 2026-08-14T04:17:26.184350Z

measured 100 of 100 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

100 of 288 outbound references displayed

  • verified exact13
  • verified fuzzy0
  • unresolved86
  • parse uncertain1
  • malformed identifier0
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External citation measurements

No source-named external measurement is stored.

Outbound references

Observation 2976191e-617f-4d7b-a4f9-bfdee3c532d3 · outbound

This paper cites Intermediate-Mass Black Holes in Early Globular Clusters.

Does IRS13 require an intermediate-mass black hole? Intermediate-Mass Black Holes in Early Globular Clusters

Reference 1

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Observation edcdb1a5-04a6-459f-ae90-5f05963024f7 · outbound

This paper cites IMBH Progenitors from Stellar Collisions in Dense Star Clusters.

Does IRS13 require an intermediate-mass black hole? IMBH Progenitors from Stellar Collisions in Dense Star Clusters

Reference 2

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Observation d47820e3-1114-45df-be34-35d7c84aea02 · outbound

This paper cites The formation of massive black holes through collision runaway in dense young star clusters.

Does IRS13 require an intermediate-mass black hole? The formation of massive black holes through collision runaway in dense young star clusters

Reference 3

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Unavailable: canonical work link unavailable.

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Observation 87cc1c56-9c1d-42bf-9ade-c8b1d941e09b · outbound

This paper cites NBODY6++GPU: Ready for the gravitational million-body problem.

Does IRS13 require an intermediate-mass black hole? NBODY6++GPU: Ready for the gravitational million-body problem

Reference 4

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Unavailable: canonical work link unavailable.

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Observation 57967709-28cd-4175-a21d-79e9af7f2bb0 · outbound

This paper cites an unresolved cited work.

Does IRS13 require an intermediate-mass black hole? Unresolved cited work

Reference 5

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Unavailable: canonical work link unavailable.

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Observation ef1ffe22-8aec-40b4-b745-df3df66d7d90 · outbound

This paper cites AGAMA: Action-based galaxy modelling architecture.

Does IRS13 require an intermediate-mass black hole? AGAMA: Action-based galaxy modelling architecture

Reference 6

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Observation 29b58af9-36aa-412e-97cb-6b9df032c49f · outbound

This paper cites an unresolved cited work.

Does IRS13 require an intermediate-mass black hole? Unresolved cited work

Reference 7

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Unavailable: canonical work link unavailable.

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Observation eb460102-c7e3-4c51-a8e8-94023e112b64 · outbound

This paper cites an unresolved cited work.

Does IRS13 require an intermediate-mass black hole? Unresolved cited work

Reference 8

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Unavailable: canonical work link unavailable.

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Observation 3c31ebef-f932-4f3f-aa3c-07e53db1c3f2 · outbound

This paper cites an unresolved cited work.

Does IRS13 require an intermediate-mass black hole? Unresolved cited work

Reference 10

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Unavailable: canonical work link unavailable.

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Observation 1ca962c0-b264-4854-8378-91bdb29a7612 · outbound

This paper cites an unresolved cited work.

Does IRS13 require an intermediate-mass black hole? Unresolved cited work

Reference 11

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Unavailable: canonical work link unavailable.

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Observation c6974c1f-111b-44e9-af2c-d0cc4041d3b0 · outbound

This paper cites an unresolved cited work.

Does IRS13 require an intermediate-mass black hole? Unresolved cited work

Reference 12

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Observation 5e8f1af0-60be-4092-ac80-95fb6a886dbd · outbound

This paper cites an unresolved cited work.

Does IRS13 require an intermediate-mass black hole? Unresolved cited work

Reference 13

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Observation 3399696d-f97b-4041-930e-34fe17c02941 · outbound

This paper cites , keywords =.

Does IRS13 require an intermediate-mass black hole? , keywords =

Reference 14

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verified exact
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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.

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Observation ce46c18a-502a-4789-9977-73a5e0fce922 · outbound

This paper cites and Hut, P.

Does IRS13 require an intermediate-mass black hole? and Hut, P

Reference 15

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Unavailable: canonical work link unavailable.

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Observation e19344ec-c00d-4ec0-b620-6782f9d74cb4 · outbound

This paper cites Journal of Computational Physics , year = 1973, volume = 12, pages =.

Does IRS13 require an intermediate-mass black hole? Journal of Computational Physics , year = 1973, volume = 12, pages =

Reference 16

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Observation b129454d-f2e1-49c9-90f5-4a8197b14c8b · outbound

This paper cites an unresolved cited work.

Does IRS13 require an intermediate-mass black hole? Unresolved cited work

Reference 17

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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.

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Observation c1e7966d-2719-46c7-84b4-fb67bcad11ea · outbound

This paper cites an unresolved cited work.

Does IRS13 require an intermediate-mass black hole? Unresolved cited work

Reference 18

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verified exact
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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.

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Observation f9251a38-ed97-4e38-a63b-cd8dcac00a7f · outbound

This paper cites and Aarseth, S.

Does IRS13 require an intermediate-mass black hole? and Aarseth, S

Reference 19

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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.

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Observation c588af1a-a373-47f7-887e-c255a8aa9179 · outbound

This paper cites , eprint =.

Does IRS13 require an intermediate-mass black hole? , eprint =

Reference 21

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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.

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Observation 2a17ff3a-9d51-4425-8e7b-3b967519dbc7 · outbound

This paper cites IAU Symposium , volume = 174, pages =.

Does IRS13 require an intermediate-mass black hole? IAU Symposium , volume = 174, pages =

Reference 22

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Observation c5160da1-ebf7-4e57-8002-8d9f851637e0 · outbound

This paper cites , eprint =.

Does IRS13 require an intermediate-mass black hole? , eprint =

Reference 25

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Observation 3b5f1e22-15ce-4866-8a92-345300561764 · outbound

This paper cites On The Maximum Mass of Stellar Black Holes.

Does IRS13 require an intermediate-mass black hole? On The Maximum Mass of Stellar Black Holes

Reference 27

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Observation 151f3a47-74b2-4679-bd0c-79cf15430a75 · outbound

This paper cites 2008 , publisher=.

Does IRS13 require an intermediate-mass black hole? 2008 , publisher=

Reference 28

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Observation a4447f93-f0c9-4808-8bd0-374436a7bf95 · outbound

This paper cites , keywords =.

Does IRS13 require an intermediate-mass black hole? , keywords =

Reference 29

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Observation 28433972-b5bb-4d05-a2e1-b6838bd0c5b0 · outbound

This paper cites , archivePrefix = "arXiv", eprint =.

Does IRS13 require an intermediate-mass black hole? , archivePrefix = "arXiv", eprint =

Reference 30

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Observation cfcf767f-3d3a-4f8c-8223-386210810580 · outbound

This paper cites Constraining the initial conditions of young stellar clusters by studying their binary populations.

Does IRS13 require an intermediate-mass black hole? Constraining the initial conditions of young stellar clusters by studying their binary populations

Reference 31

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Observation 915a6e57-f56a-4e02-8165-558ae610d2ce · outbound

This paper cites , keywords =.

Does IRS13 require an intermediate-mass black hole? , keywords =

Reference 32

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Observation a7c35216-5321-4e38-a2f1-8ec2ea365b25 · outbound

This paper cites an unresolved cited work.

Does IRS13 require an intermediate-mass black hole? Unresolved cited work

Reference 33

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Observation bfa59f3b-984f-4949-b68e-2caa45ddf900 · outbound

This paper cites an unresolved cited work.

Does IRS13 require an intermediate-mass black hole? Unresolved cited work

Reference 34

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Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 534a6c5a-876b-48dd-8841-645d2d11da7e · outbound

This paper cites Mass segregation and fractal substructure in young massive clusters – I.

Does IRS13 require an intermediate-mass black hole? Mass segregation and fractal substructure in young massive clusters – I

Reference 35

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unresolved
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Observation 95074b9c-cceb-489d-b344-223b17c4d68f · outbound

This paper cites Neutron stars and millisecond pulsars in star clusters: implications for the diffuse $\gamma$-radiation from the Galactic Centre.

Does IRS13 require an intermediate-mass black hole? Neutron stars and millisecond pulsars in star clusters: implications for the diffuse $\gamma$-radiation from the Galactic Centre

Reference 36

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Observation ed12da13-9930-425b-b926-66672f775be4 · outbound

This paper cites A MODEST review.

Does IRS13 require an intermediate-mass black hole? A MODEST review

Reference 37

Resolution
verified exact
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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.

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Observation 078970b0-a1ac-4408-9e51-5f2c9b0d0a4c · outbound

This paper cites The hunt for self-similar core collapse.

Does IRS13 require an intermediate-mass black hole? The hunt for self-similar core collapse

Reference 38

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Observation d7dd9ea0-e607-408f-b782-6a8453855c4e · outbound

This paper cites , keywords =.

Does IRS13 require an intermediate-mass black hole? , keywords =

Reference 39

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Observation 76795f11-7b14-49c6-b6cb-0c7d43742b8b · outbound

This paper cites Do star clusters form in a completely mass-segregated way?.

Does IRS13 require an intermediate-mass black hole? Do star clusters form in a completely mass-segregated way?

Reference 40

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unresolved
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Source-reported events for the cited work

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Observation b4375de4-2efd-4c6a-8224-5b374ad58425 · outbound

This paper cites Primordial mass segregation of star clusters: The role of binary stars.

Does IRS13 require an intermediate-mass black hole? Primordial mass segregation of star clusters: The role of binary stars

Reference 41

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unresolved
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Source-reported events for the cited work

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Observation 4f998c30-ddab-4961-90b8-51891a70ac18 · outbound

This paper cites Primordial mass segregation of star clusters with primordial binaries.

Does IRS13 require an intermediate-mass black hole? Primordial mass segregation of star clusters with primordial binaries

Reference 42

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unresolved
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Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 9a988636-1e40-46aa-a1be-b21b05538da6 · outbound

This paper cites VizieR Online Data Catalog , keywords =.

Does IRS13 require an intermediate-mass black hole? VizieR Online Data Catalog , keywords =

Reference 43

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Observation e737446a-fe29-4fba-ac25-e6e95ddcdd1a · outbound

This paper cites Planets, Stars and Stellar Systems.

Does IRS13 require an intermediate-mass black hole? Planets, Stars and Stellar Systems

Reference 44

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unresolved
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Observation 3e1aea10-2add-4f77-a88e-e304865d3c15 · outbound

This paper cites an unresolved cited work.

Does IRS13 require an intermediate-mass black hole? Unresolved cited work

Reference 45

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unresolved
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Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T04:17:25.842089Z digest=sha256:803adf3db22bc870feee15bfcf25ec6f10c4e3724b6fcb9a186fd9750d3f9821

Observation d479dadf-d5a6-4577-9ee9-321d26627f1d · outbound

This paper cites ArXiv e-prints , archivePrefix = "arXiv", eprint =.

Does IRS13 require an intermediate-mass black hole? ArXiv e-prints , archivePrefix = "arXiv", eprint =

Reference 46

Resolution
unresolved
no resolver link, observed 2026-08-14T04:17:25.848624Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T04:17:25.848624Z digest=sha256:e9507e6151d263204f60ef14b4db50d2a32ec3691f5968e6fbcb62fd3ab7dccb

Observation d3a3e317-9d4f-49a5-b2da-e34492eeb1ce · outbound

This paper cites VizieR Online Data Catalog , keywords =.

Does IRS13 require an intermediate-mass black hole? VizieR Online Data Catalog , keywords =

Reference 47

Resolution
unresolved
no resolver link, observed 2026-08-14T04:17:25.853531Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T04:17:25.853531Z digest=sha256:c8a9aada6707e3c1a0c4217afc7921f9f53b386cd5dbbf3aee68082fd2d8aa0e

Observation 5d525874-72b1-41a5-9756-51d90bc14472 · outbound

This paper cites The Fourth US Naval Observatory CCD Astrograph Catalog (UCAC4).

Does IRS13 require an intermediate-mass black hole? The Fourth US Naval Observatory CCD Astrograph Catalog (UCAC4)

Reference 48

Resolution
unresolved
no resolver link, observed 2026-08-14T04:17:25.858722Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T04:17:25.858722Z digest=sha256:385f23590181bd78b52d8ed9426807446584243ed523394ae8d79812c1623337

Observation df5e12cf-103a-43bb-83a7-306141bc405c · outbound

This paper cites Protostars and Planets VI , archivePrefix = "arXiv", eprint =.

Does IRS13 require an intermediate-mass black hole? Protostars and Planets VI , archivePrefix = "arXiv", eprint =

Reference 49

Resolution
unresolved
no resolver link, observed 2026-08-14T04:17:25.864128Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T04:17:25.864128Z digest=sha256:74b31b9f0ac95e133b2a9e0d91cd104bd6246d38111fd34bc6f254a5c2613773

Observation a553c6ab-7b3b-4c9b-89a8-f8926b19f59b · outbound

This paper cites Fibers in the NGC1333 proto-cluster.

Does IRS13 require an intermediate-mass black hole? Fibers in the NGC1333 proto-cluster

Reference 50

Resolution
unresolved
no resolver link, observed 2026-08-14T04:17:25.869448Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T04:17:25.869448Z digest=sha256:5f5e0b1f5c6b704df6b0344bb7b49a379d2b16b698f9c1c0aac88e4aa796c8b1

Observation d6ff73e9-1a14-440d-909a-a4e6ca6dc137 · outbound

This paper cites An ALMA study of the Orion Integral Filament: I. Evidence for narrow fibers in a massive cloud.

Does IRS13 require an intermediate-mass black hole? An ALMA study of the Orion Integral Filament: I. Evidence for narrow fibers in a massive cloud

Reference 51

Resolution
unresolved
no resolver link, observed 2026-08-14T04:17:25.875173Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T04:17:25.875173Z digest=sha256:31823445b029e5653d7d66b0af1815f9275910b9603469ea8bc1d91504dd9d5d

Observation 8bb34547-9062-435a-9fed-aa88caface13 · outbound

This paper cites , keywords =.

Does IRS13 require an intermediate-mass black hole? , keywords =

Reference 52

Resolution
unresolved
no resolver link, observed 2026-08-14T04:17:25.880346Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T04:17:25.880346Z digest=sha256:b9cb3700984c278db5c8b7fcf42d15791ac2b7dc91ad035659dd4ea4250bcfee

Observation 79ecc729-d089-45fa-bd7a-2acd616c93ee · outbound

This paper cites , keywords =.

Does IRS13 require an intermediate-mass black hole? , keywords =

Reference 53

Resolution
unresolved
no resolver link, observed 2026-08-14T04:17:25.885148Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T04:17:25.885148Z digest=sha256:de2459b2a76bf583371444db7f66b84af87374144c71062f55626bf998343956

Observation 31bf34d4-e40a-424f-85af-a5e9f36c3b2a · outbound

This paper cites doi:10.1515/crll.1965.218.204 , issn =.

Does IRS13 require an intermediate-mass black hole? doi:10.1515/crll.1965.218.204 , issn =

Reference 54

Resolution
unresolved
no resolver link, observed 2026-08-14T04:17:25.889852Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T04:17:25.889852Z digest=sha256:ea693b67b061bb18f26fcb92894f78a99d987b89b6b055bc850279506db9f202

Observation 5e86bc47-83b6-4e33-a574-cce546db4e97 · outbound

This paper cites Celestial Mechanics , keywords =.

Does IRS13 require an intermediate-mass black hole? Celestial Mechanics , keywords =

Reference 55

Resolution
unresolved
no resolver link, observed 2026-08-14T04:17:25.896322Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T04:17:25.896322Z digest=sha256:8dbcafe608fd41ecf0f5ad157781b754793792e0750fb41feb39b3c3b69fd180

Observation ebb2ce7e-f989-4800-88c2-8c84af3570b6 · outbound

This paper cites Celestial Mechanics and Dynamical Astronomy , keywords =.

Does IRS13 require an intermediate-mass black hole? Celestial Mechanics and Dynamical Astronomy , keywords =

Reference 56

Resolution
unresolved
no resolver link, observed 2026-08-14T04:17:25.901972Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T04:17:25.901972Z digest=sha256:44de9dd2b902ecf58955b49589c6eaeb5c2d68f0c7032b62f904fd3fd2c27aae

Observation 26967f6b-f32d-46a4-a1c1-59973108b746 · outbound

This paper cites Celestial Mechanics and Dynamical Astronomy , keywords =.

Does IRS13 require an intermediate-mass black hole? Celestial Mechanics and Dynamical Astronomy , keywords =

Reference 57

Resolution
unresolved
no resolver link, observed 2026-08-14T04:17:25.906791Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T04:17:25.906791Z digest=sha256:3e3585db6776739b193ac953676dda6fa958aa61ba0437253d80b6dde4653303

Observation 63e3e15b-a8c9-4e02-bf08-0d635138ed20 · outbound

This paper cites 1950", month =.

Does IRS13 require an intermediate-mass black hole? 1950", month =

Reference 58

Resolution
unresolved
no resolver link, observed 2026-08-14T04:17:25.911720Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T04:17:25.911720Z digest=sha256:0cf09b899c297ef14e6d731cf0f7afb4e15b916fb8568503d918e4375a527454

Observation f92f6c80-6b78-4401-9b43-bbfdb625ac5e · outbound

This paper cites I - The hybrid code.

Does IRS13 require an intermediate-mass black hole? I - The hybrid code

Reference 59

Resolution
verified exact
doi, observed 2026-08-14T04:19:06.798301Z

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.

source=arxiv_source observed=2026-08-14T04:17:25.916692Z digest=sha256:809e7aea53592b3345a32caa7dc96996adbfd82c053c009e72f3982b06713c82

Observation 4f4d2f5a-d5de-4ef9-af81-6e9e4f5b09a2 · outbound

This paper cites 1971", month =.

Does IRS13 require an intermediate-mass black hole? 1971", month =

Reference 60

Resolution
unresolved
no resolver link, observed 2026-08-14T04:17:25.921733Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T04:17:25.921733Z digest=sha256:20544a593ee6c6c7cf3d9bfbe8a3b29ec23db827e5a72c8b6ff7e8c5b164e44f

Observation 44f4b79e-0eca-44b9-86d3-ddca2cd1b845 · outbound

This paper cites 1971", month =.

Does IRS13 require an intermediate-mass black hole? 1971", month =

Reference 61

Resolution
unresolved
no resolver link, observed 2026-08-14T04:17:25.928377Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T04:17:25.928377Z digest=sha256:844b17b32273b15c0ce6fe6ba788760ad60664d461c1b4323032af76531586db

Observation d329df0e-3f09-463d-a497-fb6e50ce3285 · outbound

This paper cites 1973", month =.

Does IRS13 require an intermediate-mass black hole? 1973", month =

Reference 62

Resolution
unresolved
no resolver link, observed 2026-08-14T04:17:25.933412Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T04:17:25.933412Z digest=sha256:9714d5b11ef4ef741393a61a21cdf93b74ab46a316b73375c7cf0a93ef582b54

Observation 2222b5a3-b2e4-4d9d-be25-62f7c1a7231f · outbound

This paper cites 1972", month =.

Does IRS13 require an intermediate-mass black hole? 1972", month =

Reference 63

Resolution
verified exact
doi, observed 2026-08-14T04:19:06.736463Z

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.

source=arxiv_source observed=2026-08-14T04:17:25.938629Z digest=sha256:c0dc10919d64b301212052d7b7dbdd1d7175bafbe07c9fed2ceee52eb34c0ef8

Observation 7804a4ec-407e-4e96-9d9d-c1932b2b08dd · outbound

This paper cites II - Distribution of the orbital elements in an unbiased sample.

Does IRS13 require an intermediate-mass black hole? II - Distribution of the orbital elements in an unbiased sample

Reference 64

Resolution
unresolved
no resolver link, observed 2026-08-14T04:17:25.943570Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T04:17:25.943570Z digest=sha256:ea87e07e8fa732b89c572a6a622035a9e657e943d1997469f265b7c949d96d2f

Observation e2129112-ce19-46ab-aeef-e7d55074b756 · outbound

This paper cites A Survey of Stellar Families: Multiplicity of Solar-Type Stars.

Does IRS13 require an intermediate-mass black hole? A Survey of Stellar Families: Multiplicity of Solar-Type Stars

Reference 65

Resolution
unresolved
no resolver link, observed 2026-08-14T04:17:25.948748Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T04:17:25.948748Z digest=sha256:62530d18961493eca394009593fb5d0f9e22fe2a7a0ebced5d4011513e138506

Observation e1dd90be-9f04-4def-8cc9-f45be7258e5e · outbound

This paper cites Interrupted Stellar Encounters in Star Clusters.

Does IRS13 require an intermediate-mass black hole? Interrupted Stellar Encounters in Star Clusters

Reference 66

Resolution
unresolved
no resolver link, observed 2026-08-14T04:17:25.954728Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T04:17:25.954728Z digest=sha256:1d0bea20c12a7e8e71d3fa0f8054b479cc36ef30afaf82cddbc2349f3c7cb427

Observation c79bdaaa-8fc9-48b0-8e71-defea5f94e75 · outbound

This paper cites Small-N collisional dynamics II: Roaming the realm of not-so-small-N.

Does IRS13 require an intermediate-mass black hole? Small-N collisional dynamics II: Roaming the realm of not-so-small-N

Reference 67

Resolution
unresolved
no resolver link, observed 2026-08-14T04:17:25.960101Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T04:17:25.960101Z digest=sha256:9b48ab9c9f9e463d7452fc2a70e3b5d85ec54dec0b9d37b0138c9d8b24d23fdc

Observation d02ebf96-af6f-4db0-b072-5228347168d0 · outbound

This paper cites an unresolved cited work.

Does IRS13 require an intermediate-mass black hole? Unresolved cited work

Reference 68

Resolution
unresolved
no resolver link, observed 2026-08-14T04:17:25.965807Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T04:17:25.965807Z digest=sha256:26c974e78f6887796b9759459bfeba1aee115a0f59047d49ed0d25c02e2fc4f0

Observation 9a7aa640-86ff-4087-9fd2-6b62fdc425fb · outbound

This paper cites 1942", month =.

Does IRS13 require an intermediate-mass black hole? 1942", month =

Reference 69

Resolution
unresolved
no resolver link, observed 2026-08-14T04:17:25.971306Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T04:17:25.971306Z digest=sha256:8a7a1216041b79773d9927852ce9cbd65c2089a480ba6020833ac7d6470db15b

Observation fd7b60b7-219e-48a9-9b80-b365c4c53864 · outbound

This paper cites 1943", month =.

Does IRS13 require an intermediate-mass black hole? 1943", month =

Reference 70

Resolution
unresolved
no resolver link, observed 2026-08-14T04:17:25.976549Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T04:17:25.976549Z digest=sha256:2c3ba099f6f1f4b079d1d5dfeb49730269817f48c56f2e9daa06c69330662159

Observation efe153f7-7d85-42ed-b5f6-2c24a5f8ddd0 · outbound

This paper cites , keywords =.

Does IRS13 require an intermediate-mass black hole? , keywords =

Reference 71

Resolution
unresolved
no resolver link, observed 2026-08-14T04:17:25.981722Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T04:17:25.981722Z digest=sha256:51481446c1b175c42ad92003a2755eeaec24da816b5980888992719bd236a6d8

Observation 2305f554-5fa7-41ca-b43e-39e1ee19afee · outbound

This paper cites an unresolved cited work.

Does IRS13 require an intermediate-mass black hole? Unresolved cited work

Reference 72

Resolution
unresolved
no resolver link, observed 2026-08-14T04:17:25.986640Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T04:17:25.986640Z digest=sha256:8611e57cfedf474004f496258f2076b92ba7c740592f711e43923f823fbface3

Observation 7d746f31-80e2-4c9f-a12c-c570f531e4f7 · outbound

This paper cites an unresolved cited work.

Does IRS13 require an intermediate-mass black hole? Unresolved cited work

Reference 73

Resolution
unresolved
no resolver link, observed 2026-08-14T04:17:25.991087Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T04:17:25.991087Z digest=sha256:5811ead8a29b865e7b0665a55ecd351054543167f861a242253c1d495b6eb93d

Observation 6b6dd85c-dee4-4cef-9943-4d16e93da5f8 · outbound

This paper cites an unresolved cited work.

Does IRS13 require an intermediate-mass black hole? Unresolved cited work

Reference 74

Resolution
unresolved
no resolver link, observed 2026-08-14T04:17:25.995919Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T04:17:25.995919Z digest=sha256:d540adc7ae103a2bd4d13d63c76d0cad4ed204a389f27ae1b3931da52bb86348

Observation 0d243b98-9cd7-4ab6-8ce0-380e3acc077f · outbound

This paper cites , eprint =.

Does IRS13 require an intermediate-mass black hole? , eprint =

Reference 75

Resolution
unresolved
no resolver link, observed 2026-08-14T04:17:26.001388Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T04:17:26.001388Z digest=sha256:3240a74c48d9e788fe1214f36c7d53e315b8fbb8e8f684ade3e7bb60ace8bf63

Observation 03a86a62-a9de-40e8-8b7f-b5df2e0c3b67 · outbound

This paper cites and Kroupa, P.

Does IRS13 require an intermediate-mass black hole? and Kroupa, P

Reference 77

Resolution
unresolved
no resolver link, observed 2026-08-14T04:17:26.012195Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T04:17:26.012195Z digest=sha256:1fe671e6685eb494a47ac3b4b47e0296eb1f532b9f3f5ddc9dc16dc6f8e0b631

Observation aee69bd1-e614-4af4-8651-bb85b034ed5d · outbound

This paper cites , archivePrefix = "arXiv", eprint =.

Does IRS13 require an intermediate-mass black hole? , archivePrefix = "arXiv", eprint =

Reference 78

Resolution
unresolved
no resolver link, observed 2026-08-14T04:17:26.016927Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T04:17:26.016927Z digest=sha256:7589734b3148267b3428c2b1bb8193705702741ebbe9de5bba254ad2b7333e76

Observation 2ce3680c-6f57-4faa-b810-f129c617e1c4 · outbound

This paper cites , archivePrefix = "arXiv", eprint =.

Does IRS13 require an intermediate-mass black hole? , archivePrefix = "arXiv", eprint =

Reference 79

Resolution
verified exact
doi, observed 2026-08-14T04:19:06.541882Z

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.

source=arxiv_source observed=2026-08-14T04:17:26.022111Z digest=sha256:7bed0de1696180129c57301fc71774a32be0e175fca9436c9c797a2196be3c1e

Observation 3b4a927c-c28d-4c59-b018-81751cb315cd · outbound

This paper cites , archivePrefix = "arXiv", eprint =.

Does IRS13 require an intermediate-mass black hole? , archivePrefix = "arXiv", eprint =

Reference 80

Resolution
unresolved
no resolver link, observed 2026-08-14T04:17:26.026942Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T04:17:26.026942Z digest=sha256:62c942d5db36dc298b2b7910cf1b83c2bce00f3090f69ed3f17a5be52abb890c

Observation ce7dd534-7765-4d5c-a8cc-70279bb151dc · outbound

This paper cites , archivePrefix = "arXiv", eprint =.

Does IRS13 require an intermediate-mass black hole? , archivePrefix = "arXiv", eprint =

Reference 81

Resolution
unresolved
no resolver link, observed 2026-08-14T04:17:26.032417Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T04:17:26.032417Z digest=sha256:54464e9df9554caa103221a77e883a7198d579d0dbe62aacea58464cb8534fa8

Observation f6f9a050-e17c-4146-b537-741448374c59 · outbound

This paper cites II - Distribution of the orbital elements in an unbiased sample.

Does IRS13 require an intermediate-mass black hole? II - Distribution of the orbital elements in an unbiased sample

Reference 82

Resolution
unresolved
no resolver link, observed 2026-08-14T04:17:26.037827Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T04:17:26.037827Z digest=sha256:0ec22672130d4a55dd8e853cab40ade12ad46fed589145d1e32dbc270cfb3da4

Observation 5ff4a327-2dcb-4d5b-a398-aba365d0bd3c · outbound

This paper cites an unresolved cited work.

Does IRS13 require an intermediate-mass black hole? Unresolved cited work

Reference 83

Resolution
unresolved
no resolver link, observed 2026-08-14T04:17:26.043197Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T04:17:26.043197Z digest=sha256:d80379c6a4edddd1bd0f6d12ca527f9c6ba24bd8b9197995aeefc9097a315bd0

Observation 864c7b64-ec01-462a-b456-8becee264c3a · outbound

This paper cites , year = 2006, month = jul, volume = 646, pages =.

Does IRS13 require an intermediate-mass black hole? , year = 2006, month = jul, volume = 646, pages =

Reference 84

Resolution
verified exact
doi, observed 2026-08-14T04:19:06.303569Z

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.

source=arxiv_source observed=2026-08-14T04:17:26.048711Z digest=sha256:df0b964225c38702326b9199bcffea35a47e314b28c214a7e47925a68b61fd6e

Observation 67aeb483-b813-4f6d-96a1-86e99f740418 · outbound

This paper cites New low-mass stellar companions of the exoplanet host stars HD 125612 and HD 212301.

Does IRS13 require an intermediate-mass black hole? New low-mass stellar companions of the exoplanet host stars HD 125612 and HD 212301

Reference 85

Resolution
verified exact
doi, observed 2026-08-14T04:19:06.196574Z

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.

source=arxiv_source observed=2026-08-14T04:17:26.071137Z digest=sha256:df8a47fa1c9f7d2ef9fa3c661271289c7c6697fa2bff0925659da8046aa6d424

Observation ed857d44-8f5b-4895-a214-ea121fa8ae21 · outbound

This paper cites A& A , year = 2012, month = jun, volume = 542, pages =.

Does IRS13 require an intermediate-mass black hole? A& A , year = 2012, month = jun, volume = 542, pages =

Reference 86

Resolution
unresolved
no resolver link, observed 2026-08-14T04:17:26.077235Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T04:17:26.077235Z digest=sha256:ed1b180cd4f229c876136d4c8022fb5c78e8e52c48be26685b6426cbeef0776b

Observation 6984ae46-7c2c-4795-aaab-917fc2fc9be5 · outbound

This paper cites an unresolved cited work.

Does IRS13 require an intermediate-mass black hole? Unresolved cited work

Reference 87

Resolution
unresolved
no resolver link, observed 2026-08-14T04:17:26.082421Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T04:17:26.082421Z digest=sha256:73bf2947d512bce38c4e761388edecdf06504b1e2d47dfcb94b662719b76d253

Observation b34804d8-0395-4089-814f-acaf7d6763e2 · outbound

This paper cites an unresolved cited work.

Does IRS13 require an intermediate-mass black hole? Unresolved cited work

Reference 88

Resolution
unresolved
no resolver link, observed 2026-08-14T04:17:26.087924Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T04:17:26.087924Z digest=sha256:c3055ef15c2cd18be14c29eebba01e072cdd309cb99f954168266a18c48319f9

Observation 3c4c9018-e002-4d89-aed2-4a798fa80cf8 · outbound

This paper cites , archivePrefix = "arXiv", eprint =.

Does IRS13 require an intermediate-mass black hole? , archivePrefix = "arXiv", eprint =

Reference 89

Resolution
verified exact
doi, observed 2026-08-14T04:17:28.387500Z

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.

source=arxiv_source observed=2026-08-14T04:17:26.092695Z digest=sha256:0002ee53d71efbb87a9beb8e6f38ad05014b1c7c6db1fcf97da9d2db310bd059

Observation f4107137-3817-4d0f-a1f4-73ab0bf58901 · outbound

This paper cites , year = 1962, month = nov, volume = 67, pages =.

Does IRS13 require an intermediate-mass black hole? , year = 1962, month = nov, volume = 67, pages =

Reference 90

Resolution
unresolved
no resolver link, observed 2026-08-14T04:17:26.097652Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T04:17:26.097652Z digest=sha256:bbf6a1941d00568d12426916558203ef2bee291daf4bad5650856e45b6e0cef5

Observation 4cf69540-7bc7-4889-8501-4886a51cee45 · outbound

This paper cites , year = 1962, month = oct, volume = 9, pages =.

Does IRS13 require an intermediate-mass black hole? , year = 1962, month = oct, volume = 9, pages =

Reference 91

Resolution
unresolved
no resolver link, observed 2026-08-14T04:17:26.102438Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T04:17:26.102438Z digest=sha256:7bef53c803e29d00193dfdd1dbc9fef6c151c8a81304d77f0961a659e5efa568

Observation 36a3b66e-7353-431f-8b9a-8b8996a9d9a4 · outbound

This paper cites , keywords =.

Does IRS13 require an intermediate-mass black hole? , keywords =

Reference 92

Resolution
unresolved
no resolver link, observed 2026-08-14T04:17:26.107097Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T04:17:26.107097Z digest=sha256:971c284c8e33a4959447987a8974b31c487abffe1b66c550d54d11bd9cde6c74

Observation 85df680f-deef-4ce9-8355-42ea49b069fe · outbound

This paper cites , year = 1996, month = oct, volume = 282, pages =.

Does IRS13 require an intermediate-mass black hole? , year = 1996, month = oct, volume = 282, pages =

Reference 93

Resolution
unresolved
no resolver link, observed 2026-08-14T04:17:26.111609Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T04:17:26.111609Z digest=sha256:bef215c78f23f2ceb689f807b3ebbc27b41d5fb74f3199f7757aa78c84bc6b20

Observation 06e6b3c8-7985-4176-b881-16f305b5f9a1 · outbound

This paper cites Identical point-particles.

Does IRS13 require an intermediate-mass black hole? Identical point-particles

Reference 95

Resolution
unresolved
no resolver link, observed 2026-08-14T04:17:26.120789Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T04:17:26.120789Z digest=sha256:04ef82d281ee20e2529d5919fcdf42b903d040c3a2899d95fe260b59e60ad630

Observation 331032a8-e81f-4eee-9c5b-b3cde7bf8948 · outbound

This paper cites , year = 2016, month = aug, volume = 460, pages =.

Does IRS13 require an intermediate-mass black hole? , year = 2016, month = aug, volume = 460, pages =

Reference 96

Resolution
unresolved
no resolver link, observed 2026-08-14T04:17:26.126613Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T04:17:26.126613Z digest=sha256:dc834e5031f6feaa32c9dda31b24fabcd0bc48b3ebb30ff3ab2d808258116232

Observation 8abb429d-93a1-4f74-b348-66dcf1b4645c · outbound

This paper cites Suppl , year = 2014, month = feb, volume = 210, pages =.

Does IRS13 require an intermediate-mass black hole? Suppl , year = 2014, month = feb, volume = 210, pages =

Reference 97

Resolution
unresolved
no resolver link, observed 2026-08-14T04:17:26.131967Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T04:17:26.131967Z digest=sha256:fb32ca2d333e409c54541421a1bb028664a6ef3f0054b6bf8e98064805d6d232

Observation c56bbbc8-adc2-4fd5-a35b-6d5bc2a1b54c · outbound

This paper cites Jour Astron Telescopes, Instruments, and Systems , year = 2015, month = jan, volume = 1, pages =.

Does IRS13 require an intermediate-mass black hole? Jour Astron Telescopes, Instruments, and Systems , year = 2015, month = jan, volume = 1, pages =

Reference 98

Resolution
unresolved
no resolver link, observed 2026-08-14T04:17:26.136819Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T04:17:26.136819Z digest=sha256:f8e28ed0f9959015f973e5d23c0c3b5a108b847e6b86cbd9b7f1d4bca29e2588

Observation 3460c032-cfa5-49ae-8d89-a339336de43c · outbound

This paper cites The role of binary separation.

Does IRS13 require an intermediate-mass black hole? The role of binary separation

Reference 99

Resolution
unresolved
no resolver link, observed 2026-08-14T04:17:26.141675Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T04:17:26.141675Z digest=sha256:cbf7806d22db75016b4d2cc84a7c4a3ac9d1ecd9fd8fd7fead3cb0193b3b3c33

Observation 61ce2ccc-901e-4c28-8d83-0807ab90fb1e · outbound

This paper cites Nature , year = 2016, month = aug, volume = 536, pages =.

Does IRS13 require an intermediate-mass black hole? Nature , year = 2016, month = aug, volume = 536, pages =

Reference 100

Resolution
unresolved
no resolver link, observed 2026-08-14T04:17:26.147461Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T04:17:26.147461Z digest=sha256:6fbb9e127495f7abd7409c39a2355ab0e3f996b99ee6cf4d930bfd09f0c6ac23

Observation a132fc31-5e15-40b9-85d1-597fc2a7db1f · outbound

This paper cites A& A , year = 2017, month = feb, volume = 598, pages =.

Does IRS13 require an intermediate-mass black hole? A& A , year = 2017, month = feb, volume = 598, pages =

Reference 101

Resolution
unresolved
no resolver link, observed 2026-08-14T04:17:26.152945Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T04:17:26.152945Z digest=sha256:0254dd0ebf9e29bb22d30e630e980f8a4b2a8494161eea33bab4c2ae8b1f7934

Observation 5885535c-2bd8-4407-97bf-c8554dec597b · outbound

This paper cites an unresolved cited work.

Does IRS13 require an intermediate-mass black hole? Unresolved cited work

Reference 102

Resolution
unresolved
no resolver link, observed 2026-08-14T04:17:26.157807Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T04:17:26.157807Z digest=sha256:aa2cc80e6226ee5c22d6131e861fbffe771577dc2e8182e1aa32175d68b2339e

Observation a0cc48e0-0a5c-46cd-976a-6fb748dd8462 · outbound

This paper cites an unresolved cited work.

Does IRS13 require an intermediate-mass black hole? Unresolved cited work

Reference 103

Resolution
unresolved
no resolver link, observed 2026-08-14T04:17:26.163135Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T04:17:26.163135Z digest=sha256:e80be76f75b513c62be3f15187c6fe5c3895308f90da080b5362bf826a2b9a57

Observation ecf0894e-2423-4107-be10-c6e09b419b24 · outbound

This paper cites Mass accretion and planetary formation in young multiple stellar systems.

Does IRS13 require an intermediate-mass black hole? Mass accretion and planetary formation in young multiple stellar systems

Reference 104

Resolution
unresolved
no resolver link, observed 2026-08-14T04:17:26.169308Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T04:17:26.169308Z digest=sha256:6b28a14eeb8ffc300e7a3995fbebed80a6afb15b4646d057127ec089e0543045

Observation 9af16184-a5ac-40da-bcfb-329f89628251 · outbound

This paper cites , year = 2013, month = may, volume = 431, pages =.

Does IRS13 require an intermediate-mass black hole? , year = 2013, month = may, volume = 431, pages =

Reference 105

Resolution
unresolved
no resolver link, observed 2026-08-14T04:17:26.174522Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T04:17:26.174522Z digest=sha256:66dcf7931e9c0453590b8a676183a92647e994f0dd622372551cb854ee471ab5

Observation a12c726a-a00a-4a11-8628-6012d7a235f5 · outbound

This paper cites Lett , year = 2005, month = nov, volume = 633, pages =.

Does IRS13 require an intermediate-mass black hole? Lett , year = 2005, month = nov, volume = 633, pages =

Reference 106

Resolution
verified exact
doi, observed 2026-08-14T04:17:28.225645Z

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.

source=arxiv_source observed=2026-08-14T04:17:26.179472Z digest=sha256:9d89d5aeb10fb513af5d3d4653c3a6c1b9fd0bd37c381a8045b9b604e9bc973f

Observation 79709b46-fbc5-484c-b938-1f2f10d91145 · outbound

This paper cites Black hole mergers in the universe.

Does IRS13 require an intermediate-mass black hole? Black hole mergers in the universe

Reference 107

Resolution
unresolved
no resolver link, observed 2026-08-14T04:17:26.184350Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T04:17:26.184350Z digest=sha256:a72db3c35b21213450d5e0fbf2a65e1ac3043c287d63b73da58a70cce5b4203a

Pith citing papers

No inbound Pith citation observations are available.