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Paper Citation Record · LEDGER

Does IRS13 require an intermediate-mass black hole?

As of 15 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 2026-08-15T06:32:42.880941+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

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  • 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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Unavailable: canonical work link unavailable.

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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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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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Source-reported events for the cited work

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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Unavailable: canonical work link unavailable.

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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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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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Unavailable: canonical work link unavailable.

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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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Unavailable: canonical work link unavailable.

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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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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+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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No event found in the named queried sources as of 2026-08-15T06:32:42.880941+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 2026-08-15T06:32:42.880941+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 2026-08-15T06:32:42.880941+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 2026-08-15T06:32:42.880941+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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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
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Source-reported events for the cited work

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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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unresolved
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Unavailable: canonical work link unavailable.

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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

Unavailable: canonical work link unavailable.

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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

Unavailable: canonical work link unavailable.

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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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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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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=sha256:33bedfeb865252c00698df5a4ffddec9a3b4f6182c71b769663f51ba32a2d687

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:c9ee136c306347f9cc4ddaf34a90eb23971a7d07e3b9c600cc0434ed0844a5ad

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=sha256:9b47f80e3edb375fbbd7a7b54d4fd2581c92b22d3681fd82ff11d209b206a64f

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=sha256:6f04b2619ee2cf5f8d357c5980b45b205f7f27eb86f9d8476b7e06bf264a9e4d

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=sha256:88d3340af1551e35d6eb47bd873d06ef311fe411bb44490d9cd1dd755f278c72

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:a6e936d1925b10fed3e0c2ea01b6e07d6265fdeed1ca9f3d1ba1c8d97f5d68e6

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:d1c01f999edd45ef63f01b3cb59a1bda32839c2c5db7a9a0e0772bb826e0073b

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=sha256:1e71bad9aca77f9bcbb93318c1a7bfe875077c9237ee122135a54e41cb5c1113

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=sha256:6bb988a71b020653dec63db0b7ddb8d8cb113576325b02bb4c05ceb9bba61376

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=sha256:2c98e4c7c108c6101167bcf2d9f6a2e53ff77f9af7042c62893a4aa912aa0ea3

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=sha256:926a60cbe96839bb3f0d660a083df09bc767473f8eb4ef672a29e1a0e48644ef

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=sha256:5a98e0827dd6995df3d21b9abba105cbc6046c5caa248770801b1f109de1ecbd

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=sha256:83ec066ce4e3801f03bd030528d252de4406f7c6889d0fd08b0554fabcb5b3ee

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=sha256:1c4d1193f76291bcf51b21ae6119f5d86dcebc2eabe543081d3378e4d4c322a3

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 2026-08-15T06:32:42.880941+00:00.

source=arxiv_source observed=2026-08-14T04:17:25.916692Z digest=sha256:c8a90cedde06231c22e225415fec91d6d0f79d5b7f8ed06da1eb5e696a4b1c05

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=sha256:88af0ca0a0b5596d5632c0a083f291466d4171c2b10b80ac558220bb466c393d

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=sha256:865362315958f2b4b8abadac19d7d46fcb651e9939fb7f02c81b746c025f92d6

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=sha256:80a628b6e9eac8c707d71df3a67fb59f4a8c198d37d51ec4b3c6927f8bf30f19

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 2026-08-15T06:32:42.880941+00:00.

source=arxiv_source observed=2026-08-14T04:17:25.938629Z digest=sha256:0fe85c6e9669f2a950c0a7afe74127fc8bd1ace251e5eb705c5ef4a954f3df90

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:b299bfe93bef4cc1c3fc167252b97998a33cb6a1d318efe981bd5ce95d8fa117

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:db2c4b11642a55de93b9b7ff4ec82f247c4fbb520599c6db85a2c26944e314a4

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=sha256:98f9ae3484f1760845e15ccc668a1482a93f46df85c3f8141f9bdabc8484bf17

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:dea5900e6041dc0dcb14525e6282f309c04ec0c63d6a11afeda521bd47874376

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=sha256:767e63eb29848308091c38cfed949d2c0155d95b0552d4a00d45710947577ce3

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=sha256:2bb2a3a0efcb53643696cc3eb4eab003c03a05b120dc7e64252a2a45b9a36357

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=sha256:9de3ec9e32671550a8f5ccd3fbb20e12d79e47d040d53c5dbdbbbaab7731aa5a

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:befa0d32cf8775603833129275edf4080f9fe69bb9fbc86d46a637acd7581234

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=sha256:6dc12b5af6ffb6e06e0d8173ffbb5d738722fc67533bfbd462a0289424d473d4

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:b07605be57a11906402b9061e3cf2fc4e162097a608d717f70c12fc35a451985

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=sha256:6e63f711d4789e12f6641dbf06ca09617309211d2e412b19c8738aaca02b3dec

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:a2a03f1c2ff3ffaa6c23964249bca4c361f3e77da7e42bbcd98ce767d5d24e89

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=sha256:1266ff1507a24fcab51a19e79da4ee00bfc6bcbc4c514ea71e89380f1eda0602

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=sha256:4f3b2636fe455df30b022d5f539a382ee7fa4009afc95987bc0001392ea597f8

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 2026-08-15T06:32:42.880941+00:00.

source=arxiv_source observed=2026-08-14T04:17:26.022111Z digest=sha256:c7ed54fe9ba49b4e84dc7ca5a1a5f6527157ec9fb5dee6ce7acd8f2084c0cb05

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=sha256:8518cb33bb029e6286d32b57718f7380b0519f9db812c43c619a444ce9c17d5b

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:f8d793ea18ed4c4e854a81e88df69499a1f942aede7b794d29866489d30b790e

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:d8b3d42952a6be88b922adb1e4997e00461a71429095694a3def98ed967e8ad2

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=sha256:5fab211a25721a04a4e27a7f99e3c6a9a88d48351c5f05f55231dba8109ca10e

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 2026-08-15T06:32:42.880941+00:00.

source=arxiv_source observed=2026-08-14T04:17:26.048711Z digest=sha256:4c59159c135fe68f8b7b4172cf26f32507aaa74e1518c523a8cedb76958aef9e

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 2026-08-15T06:32:42.880941+00:00.

source=arxiv_source observed=2026-08-14T04:17:26.071137Z digest=sha256:1d137f2e0dbb16c5ff2f841cbe020f6529561d4f3c7e68b04dc2b7b9ec503f7b

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=sha256:49ffa04856441329a3df8f9f85dee7f8aa3eb110fcd5b869e9e6b0afb9563c5a

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=sha256:05b0d1af7feab304363db4d382798822c54300eda8d96513d0d44af89449b022

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:c2e004c384a894ed0900eb9fbb3028228240b661ec7041d15ee5f053e4c3fe16

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 2026-08-15T06:32:42.880941+00:00.

source=arxiv_source observed=2026-08-14T04:17:26.092695Z digest=sha256:a2ee9467460ff8d1984aa0371773dae2047ae4d29aa14c3cb491f603f2a0402b

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=sha256:037d807b72e58a4c4fc41822e4159b34abff7d28c645084f2b2b1fe131f15090

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=sha256:586e5ee8f57ca9258109a481b20c5325929736b2eba7c94200e416128b804a61

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=sha256:222829f04c44ca7c193f8775d977b1e8619cabdb2f3ae9f35489e220bb1e6239

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=sha256:8e14e46a74d21ccf78b99a564f60b158ab0235d7899ebf8a67651674bb5f5811

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:a8ce60f7545997e4a3d62e239fb8667ac0694f98cfdebdd46e64d7968c33a0c0

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=sha256:8590c3a753582be500215d60994354356beb47bd45208bd67c238a5cdb036de3

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=sha256:41bf225563375df0ca26dc4b7761d64f66b465d51f0358281719313707c737fa

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=sha256:110b041efc1d0be31ffa3554c019d611a788b800e42027eeb974457443ca8ea1

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=sha256:53d6df98982fadbb70d7c68c6d4c86bd47a7b1245628e56cb05e2d91a6ead83f

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:c2153047a592b30556ed0b8bcc74be43c7bf7c6d0b7b537b88f544c03deb939a

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=sha256:79bf88a757ea94fb8b6ef47e50ecbc9d7a38ddf386ecf650faec866a82e8e709

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:a48fd8409870a258c78fd25e252f01d4c3f44647a4dd2be7f357d19cf505ff6d

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=sha256:32cb733dc19da5a6790f12f6336efb19ab7acf7eb5c25579b887ed598d0b9496

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:f6decbabed6862534462c2bda9eb29b1cf238b7cf994553f3957e23276df17ef

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=sha256:1158678fd359fb43091dcb0fdfccfac3f929b48a4160a51628e09c6e47a416f6

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 2026-08-15T06:32:42.880941+00:00.

source=arxiv_source observed=2026-08-14T04:17:26.179472Z digest=sha256:9ff940d10c8e609bdebcc364cebf46da9b9a06dd6624ab827e89b78b40ac024d

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:cd3eafa2473cddccbdea86303f05ae988f817121bf970278fd8745420ad988a9

Pith citing papers

No inbound Pith citation observations are available.