Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers | Paper Citation Record

Observation 30390b5a-71cd-4b81-b4e8-759577033ddc · outbound

This paper cites If formed in pairs, such stars may form BH binaries with both components masses above∼ 150M⊙, as suggested by population synthesis codes [90, 91].

Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers If formed in pairs, such stars may form BH binaries with both components masses above∼ 150M⊙, as suggested by population synthesis codes [90, 91]

Reference 1

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Observation ca70eab9-15cf-453f-9ad9-5b80d2a1a892 · outbound

This paper cites an unresolved cited work.

Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers Unresolved cited work

Reference 2

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Observation 4f431020-4a17-4fc4-aec7-0299d4c8ae71 · outbound

This paper cites an unresolved cited work.

Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers Unresolved cited work

Reference 3

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Observation 926e70e0-83b9-41a6-97b9-ad69bd18a242 · outbound

This paper cites IID, star clusters with a sufficiently high escape velocity undergo runaway BH mergers (see also [42, 71, 102]).

Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers IID, star clusters with a sufficiently high escape velocity undergo runaway BH mergers (see also [42, 71, 102])

Reference 4

Resolution: unresolved; no resolver link, observed 2026-08-10T13:27:09.980521Z

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Observation 364ef543-e05b-4f40-bba0-c942e2093639 · outbound

This paper cites worst case scenario.

Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers worst case scenario

Reference 5

Resolution: unresolved; no resolver link, observed 2026-08-10T13:27:09.986545Z

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Observation 5edd53ac-f57a-43c9-a3df-51dafb2aedc7 · outbound

This paper cites GWTC-1: A Gravitational-Wave Transient Catalog of Compact Binary Mergers Observed by LIGO and Virgo during the First and Second Observing Runs.

Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers GWTC-1: A Gravitational-Wave Transient Catalog of Compact Binary Mergers Observed by LIGO and Virgo during the First and Second Observing Runs

Reference 6

Resolution: unresolved; no resolver link, observed 2026-08-10T13:27:10.001269Z

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Observation 55b18d97-ba7e-4774-8d16-7abd9bec72e9 · outbound

This paper cites GWTC-2: Compact Binary Coalescences Observed by LIGO and Virgo During the First Half of the Third Observing Run.

Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers GWTC-2: Compact Binary Coalescences Observed by LIGO and Virgo During the First Half of the Third Observing Run

Reference 7

Resolution: unresolved; no resolver link, observed 2026-08-10T13:27:10.007580Z

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Observation 532a002d-ae7f-4dbe-81c0-c6790fb7c614 · outbound

This paper cites GWTC-3: Compact Binary Coalescences Observed by LIGO and Virgo During the Second Part of the Third Observing Run.

Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers GWTC-3: Compact Binary Coalescences Observed by LIGO and Virgo During the Second Part of the Third Observing Run

Reference 8

Resolution: unresolved; no resolver link, observed 2026-08-10T13:27:10.014278Z

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Observation 9c7459a9-be44-4d2a-ac8e-638eabe564b5 · outbound

This paper cites The Einstein Telescope: A third- generationgravitationalwaveobservatory,.

Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers The Einstein Telescope: A third- generationgravitationalwaveobservatory,

Reference 9

Resolution: unresolved; no resolver link, observed 2026-08-10T13:27:10.020565Z

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Observation 5bcf9e23-1928-461c-a960-c1c42b28c5c1 · outbound

This paper cites A Horizon Study for Cosmic Explorer: Science, Observatories, and Community.

Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers A Horizon Study for Cosmic Explorer: Science, Observatories, and Community

Reference 10

Resolution: unresolved; no resolver link, observed 2026-08-10T13:27:10.026391Z

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Observation ecbef6fc-5a93-4936-93ce-ebce24338d83 · outbound

This paper cites Science with the Einstein Telescope: a comparison of different designs.

Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers Science with the Einstein Telescope: a comparison of different designs

Reference 11

Resolution: unresolved; no resolver link, observed 2026-08-10T13:27:10.034250Z

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Observation 9ab25c55-98b4-4fa7-ad47-7ddfdd7fa0f8 · outbound

This paper cites Characterizing Gravitational Wave Detector Networks: From A$^\sharp$ to Cosmic Explorer.

Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers Characterizing Gravitational Wave Detector Networks: From A$^\sharp$ to Cosmic Explorer

Reference 12

Resolution: unresolved; no resolver link, observed 2026-08-10T13:27:10.040933Z

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Observation b8ae1af9-fd53-4fd3-9e90-80ff2e49d901 · outbound

This paper cites Identifying heavy stellar black holes at cosmological distances with next generation gravitational-wave observatories.

Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers Identifying heavy stellar black holes at cosmological distances with next generation gravitational-wave observatories

Reference 13

Resolution: unresolved; no resolver link, observed 2026-08-10T13:27:10.047047Z

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Observation 1ea257f2-a9b9-432f-b557-633e9434a14c · outbound

This paper cites Intermediate-mass black hole binary parameter estimation with next-generation ground-based detector networks.

Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers Intermediate-mass black hole binary parameter estimation with next-generation ground-based detector networks

Reference 14

Resolution: unresolved; no resolver link, observed 2026-08-10T13:27:10.055158Z

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Observation f8a497c8-6287-42b4-b86b-66aadecbaa71 · outbound

This paper cites The Formation and Evolution of Massive Black Holes.

Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers The Formation and Evolution of Massive Black Holes

Reference 15

Resolution: unresolved; no resolver link, observed 2026-08-10T13:27:10.061066Z

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Observation 2965fc08-1905-455b-9f19-0147be22f2cc · outbound

This paper cites Intermediate-Mass Black Holes.

Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers Intermediate-Mass Black Holes

Reference 16

Resolution: unresolved; no resolver link, observed 2026-08-10T13:27:10.067765Z

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Observation 78247640-4a52-4a99-a7c4-43cd04fa9a38 · outbound

This paper cites Dwarf Galaxies with Optical Signatures of Active Massive Black Holes.

Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers Dwarf Galaxies with Optical Signatures of Active Massive Black Holes

Reference 17

Resolution: unresolved; no resolver link, observed 2026-08-10T13:27:10.076076Z

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Observation 50c2c35c-d6f7-4c77-a73e-4fc2f2b38e0a · outbound

This paper cites A 10,000-solar-mass black hole in the nucleus of a bulgeless dwarf galaxy.

Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers A 10,000-solar-mass black hole in the nucleus of a bulgeless dwarf galaxy

Reference 18

Resolution: unresolved; no resolver link, observed 2026-08-10T13:27:10.084365Z

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Observation 7728070a-dea5-4715-87a8-915d02468d33 · outbound

This paper cites Observational evidence for intermediate-mass black holes.

Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers Observational evidence for intermediate-mass black holes

Reference 19

Resolution: unresolved; no resolver link, observed 2026-08-10T13:27:10.091644Z

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Observation 4ddca758-188e-43f3-a420-5fa7fdf8671c · outbound

This paper cites A 400 solar mass black hole in the Ultraluminous X-ray source M82 X-1 accreting close to its Eddington limit.

Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers A 400 solar mass black hole in the Ultraluminous X-ray source M82 X-1 accreting close to its Eddington limit

Reference 20

Resolution: unresolved; no resolver link, observed 2026-08-10T13:27:10.103171Z

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Observation 77d8a8c9-2dbe-4115-87c4-8423466bc442 · outbound

This paper cites A broadband X-ray spectral study of the intermediate-mass black hole candidate M82 X-1 with NuSTAR, Chandra and Swift.

Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers A broadband X-ray spectral study of the intermediate-mass black hole candidate M82 X-1 with NuSTAR, Chandra and Swift

Reference 21

Resolution: unresolved; no resolver link, observed 2026-08-10T13:27:10.110148Z

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Observation 00ed8f26-b640-4d90-9637-49b374421ec4 · outbound

This paper cites An Intermediate-mass Black Hole of Over 500 Solar Masses in the Galaxy ESO 243-49.

Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers An Intermediate-mass Black Hole of Over 500 Solar Masses in the Galaxy ESO 243-49

Reference 22

Resolution: unresolved; no resolver link, observed 2026-08-10T13:27:10.117550Z

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Observation a607bd1e-b78e-44a9-b5f6-52b004bc26ef · outbound

This paper cites A Young Massive Stellar Population Around the Intermediate Mass Black Hole ESO 243-49 HLX-1.

Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers A Young Massive Stellar Population Around the Intermediate Mass Black Hole ESO 243-49 HLX-1

Reference 23

Resolution: unresolved; no resolver link, observed 2026-08-10T13:27:10.125240Z

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Observation 778a00a0-4540-488f-8629-e1e36ecf5017 · outbound

This paper cites The MAVERIC Survey: Still No Evidence for Accreting Intermediate-mass Black Holes in Globular Clusters.

Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers The MAVERIC Survey: Still No Evidence for Accreting Intermediate-mass Black Holes in Globular Clusters

Reference 24

Resolution: unresolved; no resolver link, observed 2026-08-10T13:27:10.131233Z

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Observation efff66ed-1cc2-4800-8b99-c65abbcc6e1f · outbound

This paper cites An Intermediate-Mass Black Hole in the Globular Cluster G1: Improved Significance from New Keck and Hubble Space Telescope Observations.

Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers An Intermediate-Mass Black Hole in the Globular Cluster G1: Improved Significance from New Keck and Hubble Space Telescope Observations

Reference 25

Resolution: unresolved; no resolver link, observed 2026-08-10T13:27:10.137845Z

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Observation 44eb9ab8-68cc-4220-b64c-656bf6c8a4c2 · outbound

This paper cites Fast-moving stars around an intermediate-mass black hole in Omega Centauri.

Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers Fast-moving stars around an intermediate-mass black hole in Omega Centauri

Reference 26

Resolution: unresolved; no resolver link, observed 2026-08-10T13:27:10.143915Z

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Observation 43fa9173-7b65-4a13-9c06-0380ce6d8bc0 · outbound

This paper cites A high-velocity star recently ejected by an intermediate-mass black hole in M15.

Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers A high-velocity star recently ejected by an intermediate-mass black hole in M15

Reference 27

Resolution: unresolved; no resolver link, observed 2026-08-10T13:27:10.149869Z

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Observation dac15622-9c5a-489c-8d63-aa0c4d4d38e3 · outbound

This paper cites Black hole growth through hierarchical black hole mergers in dense star clusters: implications for gravitational wave detections.

Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers Black hole growth through hierarchical black hole mergers in dense star clusters: implications for gravitational wave detections

Reference 28

Resolution: unresolved; no resolver link, observed 2026-08-10T13:27:10.156152Z

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Observation f1478cea-d67a-46ae-8dc5-fbf12471b22a · outbound

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

Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers The formation of massive black holes through collision runaway in dense young star clusters

Reference 29

Resolution: unresolved; no resolver link, observed 2026-08-10T13:27:10.162238Z

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Observation 2e2f10f0-c360-409d-886c-1567b1e01420 · outbound

This paper cites The growth of intermediate mass black holes through tidal captures and tidal disruption events.

Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers The growth of intermediate mass black holes through tidal captures and tidal disruption events

Reference 30

Resolution: unresolved; no resolver link, observed 2026-08-10T13:27:10.168664Z

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Observation 0a440672-0457-4131-8a98-cec0ff5cee18 · outbound

This paper cites Missing Link Found? --- The ``runaway'' path to supermassive black holes.

Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers Missing Link Found? --- The ``runaway'' path to supermassive black holes

Reference 31

Resolution: unresolved; no resolver link, observed 2026-08-10T13:27:10.174537Z

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Observation 1a8c231b-83c1-4273-891b-02b90d001861 · outbound

This paper cites Mergers of globular clusters in the Galactic disc: intermediate mass black hole coalescence and implications for gravitational waves detection.

Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers Mergers of globular clusters in the Galactic disc: intermediate mass black hole coalescence and implications for gravitational waves detection

Reference 32

Resolution: unresolved; no resolver link, observed 2026-08-10T13:27:10.180349Z

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Observation a8b91989-2826-4b1e-9c7d-6fe613d32ac1 · outbound

This paper cites Formation of super-massive black holes in galactic nuclei I: delivering seed intermediate-mass black holes in massive stellar clusters.

Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers Formation of super-massive black holes in galactic nuclei I: delivering seed intermediate-mass black holes in massive stellar clusters

Reference 33

Resolution: unresolved; no resolver link, observed 2026-08-10T13:27:10.192975Z

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Observation cc3c1fea-b9c4-4dfd-8878-d6453a1e40d5 · outbound

This paper cites Origin and growth of nuclear star clusters around massive black holes.

Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers Origin and growth of nuclear star clusters around massive black holes

Reference 34

Resolution: unresolved; no resolver link, observed 2026-08-10T13:27:10.200241Z

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Observation 8b25586a-1f3a-4660-a113-d4b66e570ae1 · outbound

This paper cites Co-Evolution of Galactic Nuclei and Globular Cluster Systems.

Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers Co-Evolution of Galactic Nuclei and Globular Cluster Systems

Reference 36

Resolution: unresolved; no resolver link, observed 2026-08-10T13:27:10.212765Z

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Observation 2f9d85ec-4a84-4a7f-bccb-eac941a582d3 · outbound

This paper cites Gravitational wave sources from inspiralling globular clusters in the Galactic Centre and similar environments.

Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers Gravitational wave sources from inspiralling globular clusters in the Galactic Centre and similar environments

Reference 37

Resolution: unresolved; no resolver link, observed 2026-08-10T13:27:10.217909Z

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Observation b7c54939-d234-41bf-bfe7-b59746afdfa8 · outbound

This paper cites A Black Hole in the Galactic Center Complex IRS 13E?.

Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers A Black Hole in the Galactic Center Complex IRS 13E?

Reference 38

Resolution: unresolved; no resolver link, observed 2026-08-10T13:27:10.223046Z

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Observation ec63229e-e430-4bf5-8739-e5bb08c1e963 · outbound

This paper cites A new type of compact stellar population: dark star clusters.

Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers A new type of compact stellar population: dark star clusters

Reference 39

Resolution: unresolved; no resolver link, observed 2026-08-10T13:27:10.228368Z

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Observation 27179fc5-c13e-4191-9039-bbc087b0cc05 · outbound

This paper cites GW190521 from the Merger of Ultra-Dwarf Galaxies.

Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers GW190521 from the Merger of Ultra-Dwarf Galaxies

Reference 40

Resolution: unresolved; no resolver link, observed 2026-08-10T13:27:10.234682Z

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Observation 44b06809-0c89-40a2-a8d0-3117a7033e0c · outbound

This paper cites FROST-CLUSTERS -- I. Hierarchical star cluster assembly boosts intermediate-mass black hole formation.

Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers FROST-CLUSTERS -- I. Hierarchical star cluster assembly boosts intermediate-mass black hole formation

Reference 41

Resolution: unresolved; no resolver link, observed 2026-08-10T13:27:10.240656Z

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Observation 485de2e4-89d6-4bc8-81a7-dc2a4ba161c8 · outbound

This paper cites Feedback-regulated Seed Black Hole Growth in Star-Forming Molecular Clouds and Galactic Nuclei.

Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers Feedback-regulated Seed Black Hole Growth in Star-Forming Molecular Clouds and Galactic Nuclei

Reference 42

Resolution: unresolved; no resolver link, observed 2026-08-10T13:27:10.247808Z

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Observation 3d007f58-9f53-42a3-aada-5dd36169563c · outbound

This paper cites Extremely efficient mergers of intermediate mass black hole binaries in nucleated dwarf galaxies.

Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers Extremely efficient mergers of intermediate mass black hole binaries in nucleated dwarf galaxies

Reference 43

Resolution: unresolved; no resolver link, observed 2026-08-10T13:27:10.253740Z

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Observation 60ca8bf9-adfc-4b35-b361-e270d8ba0eaa · outbound

This paper cites MOCCA Code for Star Cluster Simulations - IV. A new Scenario for Intermediate Mass Black Hole Formation in Globular Clusters.

Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers MOCCA Code for Star Cluster Simulations - IV. A new Scenario for Intermediate Mass Black Hole Formation in Globular Clusters

Reference 44

Resolution: unresolved; no resolver link, observed 2026-08-10T13:27:10.259799Z

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Observation dbda3f81-38ff-42d5-bd89-c37366ef19e6 · outbound

This paper cites Massive Black Hole Binaries from Collisional Runaways.

Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers Massive Black Hole Binaries from Collisional Runaways

Reference 45

Resolution: unresolved; no resolver link, observed 2026-08-10T13:27:10.265471Z

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Observation 8fecaf74-fb18-49a4-9558-1a94a6543956 · outbound

This paper cites Concurrent formation of supermassive stars and globular clusters: implications for early self-enrichment.

Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers Concurrent formation of supermassive stars and globular clusters: implications for early self-enrichment

Reference 46

Resolution: unresolved; no resolver link, observed 2026-08-10T13:27:10.271181Z

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Observation 610333fb-b485-4b72-9e0d-46e5d61d0ebd · outbound

This paper cites Massive black hole assembly in nuclear star clusters.

Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers Massive black hole assembly in nuclear star clusters

Reference 47

Resolution: unresolved; no resolver link, observed 2026-08-10T13:27:10.277074Z

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Observation 8659d2d2-ecf4-4781-b914-31830e073586 · outbound

This paper cites Massive black hole binaries from runaway collisions: the impact of metallicity.

Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers Massive black hole binaries from runaway collisions: the impact of metallicity

Reference 48

Resolution: unresolved; no resolver link, observed 2026-08-10T13:27:10.284417Z

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Observation b1e08926-1de9-457c-9ba0-4e554989844f · outbound

This paper cites The evolution of runaway stellar collision products.

Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers The evolution of runaway stellar collision products

Reference 49

Resolution: unresolved; no resolver link, observed 2026-08-10T13:27:10.290141Z

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Observation d896d109-2c76-4d9f-82a6-4b6cdc591b0e · outbound

This paper cites Gravitational Wave Recoil and the Retention of Intermediate Mass Black Holes.

Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers Gravitational Wave Recoil and the Retention of Intermediate Mass Black Holes

Reference 50

Resolution: unresolved; no resolver link, observed 2026-08-10T13:27:10.295787Z

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Observation 4004ab9c-552a-443f-8c00-01f542895e53 · outbound

This paper cites Formation of Massive Black Holes in Galactic Nuclei: Runaway Tidal Encounters.

Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers Formation of Massive Black Holes in Galactic Nuclei: Runaway Tidal Encounters

Reference 51

Resolution: unresolved; no resolver link, observed 2026-08-10T13:27:10.302178Z

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Observation b7aa032a-5cd1-483c-9b66-f1edce30ed25 · outbound

This paper cites Gravitational Waves as a Probe of Globular Cluster Formation and Evolution.

Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers Gravitational Waves as a Probe of Globular Cluster Formation and Evolution

Reference 52

Resolution: unresolved; no resolver link, observed 2026-08-10T13:27:10.310991Z

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Observation 13a61feb-c250-4d97-aa40-33c522e2c56c · outbound

This paper cites Single-event likelihood of star cluster properties with LIGO-Virgo-Kagra binary black hole observations.

Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers Single-event likelihood of star cluster properties with LIGO-Virgo-Kagra binary black hole observations

Reference 53

Resolution: verified exact; local_arxiv, observed 2026-08-10T13:27:37.906059Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation d4a5910b-49f7-42d8-a72f-7b2ddac37b98 · outbound

This paper cites Globular cluster formation histories, masses and radii inferred from gravitational waves.

Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers Globular cluster formation histories, masses and radii inferred from gravitational waves

Reference 54

Resolution: unresolved; no resolver link, observed 2026-08-10T13:27:10.324530Z

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Observation 1b8a977c-ef93-473f-80ba-1268b19cfd94 · outbound

This paper cites The Initial Mass Function of Stars: Evidence for Uniformity in Variable Systems.

Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers The Initial Mass Function of Stars: Evidence for Uniformity in Variable Systems

Reference 55

Resolution: unresolved; no resolver link, observed 2026-08-10T13:27:10.331453Z

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Observation 02ff240c-3102-405f-ab6c-47d17c60bb33 · outbound

This paper cites Evaluating the Merger Rate of Binary Black Holes from Direct Captures and Third-Body Soft Interactions Using the Milky Way Globular Clusters.

Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers Evaluating the Merger Rate of Binary Black Holes from Direct Captures and Third-Body Soft Interactions Using the Milky Way Globular Clusters

Reference 56

Resolution: verified exact; local_arxiv, observed 2026-08-10T13:27:37.848455Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation 2ef3a6b0-73aa-4977-9183-b59267796816 · outbound

This paper cites Random Grav- itational Encounters and the Evolution of Spherical Sys- tems. I. Method,.

Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers Random Grav- itational Encounters and the Evolution of Spherical Sys- tems. I. Method,

Reference 57

Resolution: unresolved; no resolver link, observed 2026-08-10T13:27:10.344557Z

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Observation 6219ec6e-05dd-4450-b2ec-3be698f6f83d · outbound

This paper cites Merritt,Dynamics and Evolution of Galactic Nuclei (Princeton University Press, 41 William Street, Prince- ton, New Jersey 08540, 2013).

Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers Merritt,Dynamics and Evolution of Galactic Nuclei (Princeton University Press, 41 William Street, Prince- ton, New Jersey 08540, 2013)

Reference 58

Resolution: unresolved; no resolver link, observed 2026-08-10T13:27:10.350623Z

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Observation 7c78cd59-562a-4992-895d-fcac57ba7ba0 · outbound

This paper cites Tidal capture formation of binary systems and X-ray sources in globular clusters.

Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers Tidal capture formation of binary systems and X-ray sources in globular clusters

Reference 59

Resolution: unresolved; no resolver link, observed 2026-08-10T13:27:10.356524Z

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Observation c3cd155b-521d-4451-97f2-e24392b264a7 · outbound

This paper cites On formation of close 27 binaries by two-body tidal capture.

Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers On formation of close 27 binaries by two-body tidal capture

Reference 60

Resolution: unresolved; no resolver link, observed 2026-08-10T13:27:10.362055Z

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Observation 1bb70cf2-3f5c-4499-8553-94781b911605 · outbound

This paper cites Effects of massive black holes on dense stellar systems.

Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers Effects of massive black holes on dense stellar systems

Reference 61

Resolution: unresolved; no resolver link, observed 2026-08-10T13:27:10.367126Z

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Observation 3df59cfe-221f-4da4-9c2a-2569db385f35 · outbound

This paper cites The distribution and consumption rate of stars around a massive, collapsed object.

Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers The distribution and consumption rate of stars around a massive, collapsed object

Reference 62

Resolution: unresolved; no resolver link, observed 2026-08-10T13:27:10.372475Z

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Observation fa0a33e9-a2f0-4ff0-b76e-85ae1cda5dff · outbound

This paper cites The dissolution of globular clusters con- taining massive black holes.

Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers The dissolution of globular clusters con- taining massive black holes

Reference 63

Resolution: unresolved; no resolver link, observed 2026-08-10T13:27:10.379571Z

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Observation fe017a2d-acc0-4ad5-a190-2dfeb80b3d42 · outbound

This paper cites Star distribution around a massive black hole in a globular cluster.

Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers Star distribution around a massive black hole in a globular cluster

Reference 64

Resolution: unresolved; no resolver link, observed 2026-08-10T13:27:10.384947Z

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Observation ae7fcf66-60bf-4ddf-bc4d-acab31d5dcc0 · outbound

This paper cites N- body growth of a Bahcall-Wolf cusp around a black hole,.

Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers N- body growth of a Bahcall-Wolf cusp around a black hole,

Reference 65

Resolution: verified exact; raw_fallback, observed 2026-08-10T13:27:37.822317Z

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No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation d7bcfdcd-3872-4cfc-92c9-433ea6c273fb · outbound

This paper cites Population synthesis of black hole binary mergers from star clusters.

Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers Population synthesis of black hole binary mergers from star clusters

Reference 66

Resolution: unresolved; no resolver link, observed 2026-08-10T13:27:10.396537Z

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Observation 2e6600ba-f871-47c3-8ce4-d56a36102a8b · outbound

This paper cites The life cycle of star cluster in a tidal field.

Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers The life cycle of star cluster in a tidal field

Reference 67

Resolution: verified exact; local_arxiv, observed 2026-08-10T13:27:37.624480Z

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No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation 9d5db9e3-6dae-4d7c-9e7b-2e556a53f74b · outbound

This paper cites A prescription and fast code for the long-term evolution of star clusters - III. Unequal masses and stellar evolution.

Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers A prescription and fast code for the long-term evolution of star clusters - III. Unequal masses and stellar evolution

Reference 68

Resolution: unresolved; no resolver link, observed 2026-08-10T13:27:10.407605Z

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Observation 7147b98c-6c60-4a1f-b8f8-c471ae62b95f · outbound

This paper cites On the dynamics of open clus- ters,.

Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers On the dynamics of open clus- ters,

Reference 69

Resolution: unresolved; no resolver link, observed 2026-08-10T13:27:10.413863Z

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Observation 1cb1977a-689d-4c1f-8ffa-8e0ceeb75b91 · outbound

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Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers Lifetimes of tidally limited star clusters with different radii

Reference 70

Resolution: unresolved; no resolver link, observed 2026-08-10T13:27:10.419929Z

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Observation 12fceca8-3d67-48fd-b618-8349d6d51da9 · outbound

This paper cites The runaway growth of intermediate-mass black holes in dense star clusters.

Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers The runaway growth of intermediate-mass black holes in dense star clusters

Reference 71

Resolution: unresolved; no resolver link, observed 2026-08-10T13:27:10.426106Z

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Observation aff58fcf-74e8-4776-985a-c5cd7d98d5a5 · outbound

This paper cites Dynamical evolution of black hole sub-systems in idealised star clusters.

Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers Dynamical evolution of black hole sub-systems in idealised star clusters

Reference 72

Resolution: unresolved; no resolver link, observed 2026-08-10T13:27:10.435938Z

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Observation c3fbf42c-11bb-483b-a0eb-76f7384e44d5 · outbound

This paper cites Tidal disruption of stars by black holes of 106-108 solar masses in nearby galaxies,.

Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers Tidal disruption of stars by black holes of 106-108 solar masses in nearby galaxies,

Reference 73

Resolution: unresolved; no resolver link, observed 2026-08-10T13:27:10.445319Z

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Observation bc037991-a0f9-4c32-ade4-60c853b7f82d · outbound

This paper cites A Bright Year for Tidal Disruptions?.

Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers A Bright Year for Tidal Disruptions?

Reference 74

Resolution: unresolved; no resolver link, observed 2026-08-10T13:27:10.451806Z

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Observation 8ccbef80-6f89-4431-9c7d-2582ae18abe6 · outbound

This paper cites Escape speed of stellar clusters from multiple-generation black-hole mergers in the upper mass gap.

Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers Escape speed of stellar clusters from multiple-generation black-hole mergers in the upper mass gap

Reference 75

Resolution: verified exact; local_arxiv, observed 2026-08-10T13:27:37.502691Z

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No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation 1ed53171-6e3d-403d-b92a-7344bf40aa54 · outbound

This paper cites Avoiding a Cluster Catastrophe: Retention Efficiency and the Binary Black Hole Mass Spectrum.

Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers Avoiding a Cluster Catastrophe: Retention Efficiency and the Binary Black Hole Mass Spectrum

Reference 76

Resolution: unresolved; no resolver link, observed 2026-08-10T13:27:10.464015Z

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Observation e9653991-0141-4798-a7c4-a85800ba5092 · outbound

This paper cites Dynamical formation of black hole binaries in dense star clusters: Rapid cluster evolution code.

Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers Dynamical formation of black hole binaries in dense star clusters: Rapid cluster evolution code

Reference 77

Resolution: unresolved; no resolver link, observed 2026-08-10T13:27:10.478511Z

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Observation 670b5a0b-d863-4899-90d8-a39acb764ecd · outbound

This paper cites Nonlinear quasinormal mode detectability with next-generation gravitational wave detectors.

Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers Nonlinear quasinormal mode detectability with next-generation gravitational wave detectors

Reference 78

Resolution: unresolved; no resolver link, observed 2026-08-10T13:27:10.489491Z

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Observation 2a30312f-5364-4964-a6f9-d06d70658f28 · outbound

This paper cites Constraining the high redshift formation of black hole seeds in nuclear star clusters with gas inflows.

Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers Constraining the high redshift formation of black hole seeds in nuclear star clusters with gas inflows

Reference 79

Resolution: unresolved; no resolver link, observed 2026-08-10T13:27:10.501957Z

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Observation 62a0a55f-0278-4ec5-9f80-c235893a1f38 · outbound

This paper cites an unresolved cited work.

Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers Unresolved cited work

Reference 80

Resolution: unresolved; no resolver link, observed 2026-08-10T13:27:10.522056Z

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Observation bb88abff-bdbf-4b35-9bd4-59c28880ecdc · outbound

This paper cites The dynamical evolution of mas- sive black hole binaries - I. hardening in a fixed stellar background,.

Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers The dynamical evolution of mas- sive black hole binaries - I. hardening in a fixed stellar background,

Reference 81

Resolution: verified exact; raw_fallback, observed 2026-08-10T13:27:37.387791Z

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No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation af9f2c18-1c1f-438b-a488-bab4cc4b6a2d · outbound

This paper cites Chaotic Loss Cones, Black Hole Fueling and the M-Sigma Relation.

Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers Chaotic Loss Cones, Black Hole Fueling and the M-Sigma Relation

Reference 82

Resolution: unresolved; no resolver link, observed 2026-08-10T13:27:10.541145Z

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Observation ed9601bf-f5d4-4167-bf5e-36ed1dbe0c88 · outbound

This paper cites Lecture notes on black hole binary astrophysics.

Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers Lecture notes on black hole binary astrophysics

Reference 83

Resolution: unresolved; no resolver link, observed 2026-08-10T13:27:10.549830Z

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Observation 289a83a0-13cd-4f15-8c9c-9f85960f7562 · outbound

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Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers Scattering experiments meet N-body I: a practical recipe for the evolution of massive black hole binaries in stellar environments

Reference 84

Resolution: unresolved; no resolver link, observed 2026-08-10T13:27:10.563525Z

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Observation aaf788b7-d6e1-4c61-9ffe-d3fa90a5f9ad · outbound

This paper cites An accurate analytical fit to the gravitational-wave inspiral duration for eccentric binaries.

Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers An accurate analytical fit to the gravitational-wave inspiral duration for eccentric binaries

Reference 85

Resolution: unresolved; no resolver link, observed 2026-08-10T13:27:10.573765Z

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Observation 7adbdee7-dd3b-4819-95df-9f4573fbad27 · outbound

This paper cites Planck 2018 results. VI. Cosmological parameters.

Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers Planck 2018 results. VI. Cosmological parameters

Reference 86

Resolution: unresolved; no resolver link, observed 2026-08-10T13:27:10.581379Z

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Observation 39a67f96-9497-40ee-ac45-aafa4f78bdfb · outbound

This paper cites The Structure and Environment of Young Stellar Clusters in Spiral Galaxies.

Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers The Structure and Environment of Young Stellar Clusters in Spiral Galaxies

Reference 87

Resolution: verified exact; local_arxiv, observed 2026-08-10T13:27:37.043811Z

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No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation 954c05d1-17fe-4f75-89a9-1f1d73f405f4 · outbound

This paper cites Star Clusters Across Cosmic Time.

Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers Star Clusters Across Cosmic Time

Reference 88

Resolution: unresolved; no resolver link, observed 2026-08-10T13:27:10.597881Z

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Observation 2e0dac25-8cf9-4adf-9c96-0cf14a08a104 · outbound

This paper cites Globular cluster formation in the context of galaxy formation and evolution.

Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers Globular cluster formation in the context of galaxy formation and evolution

Reference 89

Resolution: unresolved; no resolver link, observed 2026-08-10T13:27:10.603811Z

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Observation 6fdfd27a-2a71-4230-8821-10b3345f1071 · outbound

This paper cites The formation and hierarchical assembly of globular cluster populations.

Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers The formation and hierarchical assembly of globular cluster populations

Reference 90

Resolution: unresolved; no resolver link, observed 2026-08-10T13:27:10.613574Z

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Observation ad9627be-4c8a-4c31-96b0-3e3714a43288 · outbound

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Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers Introducing EMP-Pathfinder: modelling the simultaneous formation and evolution of stellar clusters in their host galaxies

Reference 91

Resolution: unresolved; no resolver link, observed 2026-08-10T13:27:10.623823Z

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Observation 51939966-a68a-44e6-899a-463691ce8165 · outbound

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Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers The Cosmic Evolution of Binary Black Holes in Young, Globular and Nuclear Star Clusters: Rates, Masses, Spins and Mixing Fractions

Reference 92

Resolution: unresolved; no resolver link, observed 2026-08-10T13:27:10.634105Z

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Observation ce9f81f6-96e0-44bf-9b6c-36680295027b · outbound

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Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers Kinematic Masses of Super Star Clusters in M82 from High-Resolution Near-Infrared Spectroscopy

Reference 93

Resolution: verified exact; local_arxiv, observed 2026-08-10T13:27:36.930913Z

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No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation 4d776e13-b1ba-4422-ae6d-32b52e7e5161 · outbound

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Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers Massive Black Holes as Population III Remnants

Reference 94

Resolution: unresolved; no resolver link, observed 2026-08-10T13:27:10.657365Z

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Observation b875b55f-635d-450b-bc23-4d277207d2be · outbound

This paper cites Merger rate of stellar black hole binaries above the pair instability mass gap.

Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers Merger rate of stellar black hole binaries above the pair instability mass gap

Reference 95

Resolution: verified exact; local_arxiv, observed 2026-08-10T13:27:36.886893Z

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No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation e0bc0133-1cb7-49b2-b8a0-d00fcd9586ed · outbound

This paper cites On the population III binary black hole mergers beyond the pair-instability mass gap.

Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers On the population III binary black hole mergers beyond the pair-instability mass gap

Reference 96

Resolution: unresolved; no resolver link, observed 2026-08-10T13:27:10.675033Z

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Observation aa1577bb-e86d-4f69-8867-d8f80185a217 · outbound

This paper cites Probing multiple populations of compact binaries with third-generation gravitational-wave detectors.

Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers Probing multiple populations of compact binaries with third-generation gravitational-wave detectors

Reference 97

Resolution: unresolved; no resolver link, observed 2026-08-10T13:27:10.680990Z

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Observation b0f3201e-a3da-4fa6-b3b6-5f20bd082a80 · outbound

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Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers "Super-Kilonovae" from Massive Collapsars as Signatures of Black-Hole Birth in the Pair-instability Mass Gap

Reference 98

Resolution: verified exact; local_arxiv, observed 2026-08-10T13:27:36.822615Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation 5d0a8c83-1f71-4e93-a134-5aca368bb044 · outbound

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Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers Star cluster ecol- ogy. 3. Runaway collisions in young compact star clus- ters,

Reference 99

Resolution: verified exact; raw_fallback, observed 2026-08-10T13:27:36.799839Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation 2bfcf7eb-72e2-422b-a85a-a39e65289af7 · outbound

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Gravitational wave inference of star cluster properties from intermediate-mass black hole mergers IMBH Progenitors from Stellar Collisions in Dense Star Clusters

Reference 100

Resolution: unresolved; no resolver link, observed 2026-08-10T13:27:10.704248Z

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