Paper Citation Record · LEDGER

Predicting the number density of heavy seed massive black holes due to an intense Lyman-Werner field

As of 10 August 2026, this Paper Citation Record lists 75 of 75 outbound references and 4 inbound Pith citation observations for arXiv:2502.00574.

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

pith.paper-citation-record.v1
2502.00574 v2

Coverage vector

measured 75 of 75 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links, observed 2026-08-09T18:37:36.164362Z

measured 79 of 79 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-10T06:31:04.303077+00:00

measured 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-06T23:21:42.547743Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-18T12:11:22.576878Z

Reference resolution

75 of 75 outbound references displayed

verified exact0
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External citation measurements

No source-named external measurement is stored.

Outbound references

Observation aee1aaff-b1d0-4e2c-91d0-8fd9ebb4a31a · outbound

This paper cites an unresolved cited work.

Predicting the number density of heavy seed massive black holes due to an intense Lyman-Werner field Unresolved cited work

Reference 1

Resolution: unresolved; raw_fallback, observed 2026-08-09T18:37:37.255148Z

Source-reported events for the cited work

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Observation 1f4b85dd-9877-4fc9-827e-465c7320bb64 · outbound

This paper cites an unresolved cited work.

Predicting the number density of heavy seed massive black holes due to an intense Lyman-Werner field Unresolved cited work

Reference 2

Resolution: unresolved; raw_fallback, observed 2026-08-09T18:37:37.242061Z

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Observation 4bf0705a-48b7-47c2-839b-94b1fadfe8cf · outbound

This paper cites A., Wise J.

Predicting the number density of heavy seed massive black holes due to an intense Lyman-Werner field A., Wise J

Reference 3

Resolution: verified fuzzy; raw_fallback, observed 2026-08-09T18:37:37.228525Z

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Observation 8128ebe5-4743-493b-9ec6-03380f979eed · outbound

This paper cites an unresolved cited work.

Predicting the number density of heavy seed massive black holes due to an intense Lyman-Werner field Unresolved cited work

Reference 4

Resolution: unresolved; raw_fallback, observed 2026-08-09T18:37:37.215090Z

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Observation 792be602-43f4-4051-a3c1-bda9a360cea7 · outbound

This paper cites an unresolved cited work.

Predicting the number density of heavy seed massive black holes due to an intense Lyman-Werner field Unresolved cited work

Reference 5

Resolution: unresolved; raw_fallback, observed 2026-08-09T18:37:37.201582Z

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Observation 0d9801ac-e239-44f3-bf16-d35f078c3921 · outbound

This paper cites an unresolved cited work.

Predicting the number density of heavy seed massive black holes due to an intense Lyman-Werner field Unresolved cited work

Reference 6

Resolution: unresolved; raw_fallback, observed 2026-08-09T18:37:37.187448Z

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Observation 283bc3fc-a50c-4939-bbcf-40890643592c · outbound

This paper cites L., Norman M.

Predicting the number density of heavy seed massive black holes due to an intense Lyman-Werner field L., Norman M

Reference 7

Resolution: verified fuzzy; raw_fallback, observed 2026-08-09T18:37:37.173526Z

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Observation 49cd56e7-57e8-4161-8ac0-bb2c8b40f50b · outbound

This paper cites H., Norman M.

Predicting the number density of heavy seed massive black holes due to an intense Lyman-Werner field H., Norman M

Reference 8

Resolution: verified fuzzy; raw_fallback, observed 2026-08-09T18:37:37.159402Z

Source-reported events for the cited work

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Observation 25857fba-32cc-4a74-8c12-b7c213617cc4 · outbound

This paper cites an unresolved cited work.

Predicting the number density of heavy seed massive black holes due to an intense Lyman-Werner field Unresolved cited work

Reference 9

Resolution: unresolved; raw_fallback, observed 2026-08-09T18:37:37.145767Z

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Observation de19069e-7223-4ad2-be33-da9e1678457b · outbound

This paper cites an unresolved cited work.

Predicting the number density of heavy seed massive black holes due to an intense Lyman-Werner field Unresolved cited work

Reference 10

Resolution: unresolved; raw_fallback, observed 2026-08-09T18:37:37.131108Z

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Observation b1aee3c6-643a-46e9-8743-6662488fb821 · outbound

This paper cites L., Haiman Z., Li M., 2014, , 439, 3798.

Predicting the number density of heavy seed massive black holes due to an intense Lyman-Werner field L., Haiman Z., Li M., 2014, , 439, 3798

Reference 11

Resolution: verified fuzzy; raw_fallback, observed 2026-08-09T18:37:37.115437Z

Source-reported events for the cited work

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Observation 9f14fc16-478a-4189-8f9c-6d1697926709 · outbound

This paper cites an unresolved cited work.

Predicting the number density of heavy seed massive black holes due to an intense Lyman-Werner field Unresolved cited work

Reference 12

Resolution: unresolved; raw_fallback, observed 2026-08-09T18:37:37.101631Z

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Observation f25f9f6e-2de1-4c33-bee4-9b519739886c · outbound

This paper cites an unresolved cited work.

Predicting the number density of heavy seed massive black holes due to an intense Lyman-Werner field Unresolved cited work

Reference 13

Resolution: unresolved; raw_fallback, observed 2026-08-09T18:37:37.087486Z

Source-reported events for the cited work

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Observation cbdd29df-fd36-4cc7-9174-36d4c29ae82e · outbound

This paper cites E., Strader J., Ho L.

Predicting the number density of heavy seed massive black holes due to an intense Lyman-Werner field E., Strader J., Ho L

Reference 14

Resolution: verified fuzzy; raw_fallback, observed 2026-08-09T18:37:37.073456Z

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Observation 8453d2ab-31b4-4973-a5d5-9c16271799b1 · outbound

This paper cites an unresolved cited work.

Predicting the number density of heavy seed massive black holes due to an intense Lyman-Werner field Unresolved cited work

Reference 15

Resolution: unresolved; raw_fallback, observed 2026-08-09T18:37:37.060038Z

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Observation 3118d514-8bfc-4776-a5e8-2ae1dd6ccc16 · outbound

This paper cites L., Woosley S.

Predicting the number density of heavy seed massive black holes due to an intense Lyman-Werner field L., Woosley S

Reference 16

Resolution: unresolved; no resolver link, observed 2026-08-09T18:37:35.902239Z

Source-reported events for the cited work

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Observation fc401e5f-7d33-4989-a9dd-42df5c044996 · outbound

This paper cites an unresolved cited work.

Predicting the number density of heavy seed massive black holes due to an intense Lyman-Werner field Unresolved cited work

Reference 17

Resolution: unresolved; raw_fallback, observed 2026-08-09T18:37:37.035857Z

Source-reported events for the cited work

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Observation 67fd78d9-33f3-4f96-8db4-ac87a75346cb · outbound

This paper cites The Assembly of the First Massive Black Holes.

Predicting the number density of heavy seed massive black holes due to an intense Lyman-Werner field The Assembly of the First Massive Black Holes

Reference 18

Resolution: unresolved; no resolver link, observed 2026-08-09T18:37:35.910376Z

Source-reported events for the cited work

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Observation a0ab5112-b190-4f67-b58c-371f131ab903 · outbound

This paper cites L., 2012, in The First Galaxies, Springer Berlin Heidelberg, pp.

Predicting the number density of heavy seed massive black holes due to an intense Lyman-Werner field L., 2012, in The First Galaxies, Springer Berlin Heidelberg, pp

Reference 19

Resolution: verified fuzzy; raw_fallback, observed 2026-08-09T18:37:37.021214Z

Source-reported events for the cited work

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Observation 2d8b6292-ffcd-441f-a9ed-85c5d82f9252 · outbound

This paper cites L., 2021, , 917, 40.

Predicting the number density of heavy seed massive black holes due to an intense Lyman-Werner field L., 2021, , 917, 40

Reference 20

Resolution: verified fuzzy; raw_fallback, observed 2026-08-09T18:37:37.006630Z

Source-reported events for the cited work

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Observation e053caf6-e283-403c-a4fe-ea4769e57453 · outbound

This paper cites The case for super-Eddington accretion in JWST broad-line AGN during the first billion years.

Predicting the number density of heavy seed massive black holes due to an intense Lyman-Werner field The case for super-Eddington accretion in JWST broad-line AGN during the first billion years

Reference 21

Resolution: unresolved; no resolver link, observed 2026-08-09T18:37:35.923378Z

Source-reported events for the cited work

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Observation fb257c27-545b-4fdd-ad27-59a0a4d898c7 · outbound

This paper cites A., Bovino S., Van Borm C., Grassi T., Schleicher D.

Predicting the number density of heavy seed massive black holes due to an intense Lyman-Werner field A., Bovino S., Van Borm C., Grassi T., Schleicher D

Reference 22

Resolution: verified fuzzy; raw_fallback, observed 2026-08-09T18:37:36.992515Z

Source-reported events for the cited work

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Observation f4191fce-c932-43a4-8a77-4c02a434715e · outbound

This paper cites A., Niemeyer J.

Predicting the number density of heavy seed massive black holes due to an intense Lyman-Werner field A., Niemeyer J

Reference 23

Resolution: verified fuzzy; raw_fallback, observed 2026-08-09T18:37:36.978458Z

Source-reported events for the cited work

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Observation 54e11727-6ce6-4bed-9191-09122202d92c · outbound

This paper cites A., Whalen D.

Predicting the number density of heavy seed massive black holes due to an intense Lyman-Werner field A., Whalen D

Reference 24

Resolution: verified fuzzy; raw_fallback, observed 2026-08-09T18:37:36.964722Z

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Observation 88f7d389-be6f-4416-be69-f2d843158ab1 · outbound

This paper cites an unresolved cited work.

Predicting the number density of heavy seed massive black holes due to an intense Lyman-Werner field Unresolved cited work

Reference 25

Resolution: unresolved; raw_fallback, observed 2026-08-09T18:37:36.951343Z

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 9a182ab3-4120-4e43-a0c5-83513b54fcec · outbound

This paper cites Tip of the iceberg: overmassive black holes at 4<z<7 found by JWST are not inconsistent with the local $\mathcal{M}_{\rm BH}$-$\mathcal{M}_\star$ relation.

Predicting the number density of heavy seed massive black holes due to an intense Lyman-Werner field Tip of the iceberg: overmassive black holes at 4<z<7 found by JWST are not inconsistent with the local $\mathcal{M}_{\rm BH}$-$\mathcal{M}_\star$ relation

Reference 26

Resolution: unresolved; no resolver link, observed 2026-08-09T18:37:35.945909Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 6c527b1e-56a2-4c36-9de5-cd8ac37b6949 · outbound

This paper cites M., 2007, , 671, 1160.

Predicting the number density of heavy seed massive black holes due to an intense Lyman-Werner field M., 2007, , 671, 1160

Reference 27

Resolution: verified fuzzy; raw_fallback, observed 2026-08-09T18:37:36.937557Z

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 8c08b8fd-48c8-4923-9815-3a7233321cc2 · outbound

This paper cites an unresolved cited work.

Predicting the number density of heavy seed massive black holes due to an intense Lyman-Werner field Unresolved cited work

Reference 28

Resolution: unresolved; raw_fallback, observed 2026-08-09T18:37:36.922024Z

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 1694a23d-ee1a-4b17-8a1c-b8fb2730f0d1 · outbound

This paper cites an unresolved cited work.

Predicting the number density of heavy seed massive black holes due to an intense Lyman-Werner field Unresolved cited work

Reference 29

Resolution: unresolved; raw_fallback, observed 2026-08-09T18:37:36.907935Z

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 de752501-fe05-4234-8578-66470468cc4a · outbound

This paper cites UNCOVER: 404 Error -- Models Not Found for the Triply Imaged Little Red Dot A2744-QSO1.

Predicting the number density of heavy seed massive black holes due to an intense Lyman-Werner field UNCOVER: 404 Error -- Models Not Found for the Triply Imaged Little Red Dot A2744-QSO1

Reference 30

Resolution: unresolved; no resolver link, observed 2026-08-09T18:37:35.963991Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 12a44c91-fffb-4e7f-8ca6-9e7b7864f918 · outbound

This paper cites an unresolved cited work.

Predicting the number density of heavy seed massive black holes due to an intense Lyman-Werner field Unresolved cited work

Reference 31

Resolution: unresolved; raw_fallback, observed 2026-08-09T18:37:36.893753Z

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 cffe0544-4e1d-4e78-ac5f-c513287b9d52 · outbound

This paper cites J., 2001, , 551, L27.

Predicting the number density of heavy seed massive black holes due to an intense Lyman-Werner field J., 2001, , 551, L27

Reference 32

Resolution: verified fuzzy; raw_fallback, observed 2026-08-09T18:37:36.879817Z

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 4dc7eff3-08d7-474e-a009-5c7b79ff4008 · outbound

This paper cites Direct formation of massive black holes via dynamical collapse in metal-enriched merging galaxies at $z \sim 10$: fully cosmological simulations.

Predicting the number density of heavy seed massive black holes due to an intense Lyman-Werner field Direct formation of massive black holes via dynamical collapse in metal-enriched merging galaxies at $z \sim 10$: fully cosmological simulations

Reference 33

Resolution: unresolved; no resolver link, observed 2026-08-09T18:37:35.977610Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 059c6485-234d-4e9b-a998-051fc2b03ccc · outbound

This paper cites an unresolved cited work.

Predicting the number density of heavy seed massive black holes due to an intense Lyman-Werner field Unresolved cited work

Reference 34

Resolution: unresolved; raw_fallback, observed 2026-08-09T18:37:36.865474Z

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 7ba3dce1-484a-40ab-95ac-85275776b35d · outbound

This paper cites an unresolved cited work.

Predicting the number density of heavy seed massive black holes due to an intense Lyman-Werner field Unresolved cited work

Reference 35

Resolution: unresolved; raw_fallback, observed 2026-08-09T18:37:36.850697Z

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 6887a5cc-908d-4201-a89f-7c597fbbca2d · outbound

This paper cites In-situ formation of star clusters at z > 7 via galactic disk fragmentation; shedding light on ultra-compact clusters and overmassive black holes seen by JWST.

Predicting the number density of heavy seed massive black holes due to an intense Lyman-Werner field In-situ formation of star clusters at z > 7 via galactic disk fragmentation; shedding light on ultra-compact clusters and overmassive black holes seen by JWST

Reference 36

Resolution: metadata mismatch; local_arxiv, observed 2026-08-09T18:37:36.279283Z

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 414ffe55-d270-4fa0-b0b1-157d563c048e · outbound

This paper cites A Heavy Seed Black Hole Mass Function at High Redshift -- Prospects for LISA.

Predicting the number density of heavy seed massive black holes due to an intense Lyman-Werner field A Heavy Seed Black Hole Mass Function at High Redshift -- Prospects for LISA

Reference 37

Resolution: unresolved; no resolver link, observed 2026-08-09T18:37:35.996380Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f98a6d08-ec81-4085-9e2e-901c2275b89e · outbound

This paper cites Growth of Light-Seed Black Holes in Gas-Rich Galaxies at High Redshift.

Predicting the number density of heavy seed massive black holes due to an intense Lyman-Werner field Growth of Light-Seed Black Holes in Gas-Rich Galaxies at High Redshift

Reference 38

Resolution: metadata mismatch; local_arxiv, observed 2026-08-09T18:37:36.241216Z

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 47fc17ef-ab8a-4141-b3d8-26b99eecd6a9 · outbound

This paper cites an unresolved cited work.

Predicting the number density of heavy seed massive black holes due to an intense Lyman-Werner field Unresolved cited work

Reference 39

Resolution: unresolved; raw_fallback, observed 2026-08-09T18:37:36.836506Z

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 cc934b50-0a5f-44d8-b299-773ebdc984ea · outbound

This paper cites G., Power C., Robotham A.

Predicting the number density of heavy seed massive black holes due to an intense Lyman-Werner field G., Power C., Robotham A

Reference 40

Resolution: verified fuzzy; raw_fallback, observed 2026-08-09T18:37:36.822952Z

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 f889e9c6-3d7a-4d0c-9eb9-b0777e039949 · outbound

This paper cites Y., 2012, , 747, 128.

Predicting the number density of heavy seed massive black holes due to an intense Lyman-Werner field Y., 2012, , 747, 128

Reference 41

Resolution: verified fuzzy; raw_fallback, observed 2026-08-09T18:37:36.809487Z

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 5d45314e-e692-4b7d-8b11-cdf7e9996716 · outbound

This paper cites Y., 2013, , 763, 27.

Predicting the number density of heavy seed massive black holes due to an intense Lyman-Werner field Y., 2013, , 763, 27

Reference 42

Resolution: verified fuzzy; raw_fallback, observed 2026-08-09T18:37:36.796031Z

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 0cbb148a-a9fa-420f-9fe2-72a238917c0e · outbound

This paper cites M., McQuinn M., 2012, The Astrophysical Journal, 760, 4.

Predicting the number density of heavy seed massive black holes due to an intense Lyman-Werner field M., McQuinn M., 2012, The Astrophysical Journal, 760, 4

Reference 43

Resolution: verified fuzzy; raw_fallback, observed 2026-08-09T18:37:36.782247Z

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 01d8e414-6de5-4a94-b95c-c3c8b82c0f26 · outbound

This paper cites W., Wise J.

Predicting the number density of heavy seed massive black holes due to an intense Lyman-Werner field W., Wise J

Reference 44

Resolution: verified fuzzy; raw_fallback, observed 2026-08-09T18:37:36.768352Z

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 aa6e7da7-4ae5-4c7d-9459-c994fa827924 · outbound

This paper cites A., Power C., Ward S., Brennan J., McCaffrey J., 2024, The Open Journal of Astrophysics, 7.

Predicting the number density of heavy seed massive black holes due to an intense Lyman-Werner field A., Power C., Ward S., Brennan J., McCaffrey J., 2024, The Open Journal of Astrophysics, 7

Reference 45

Resolution: verified fuzzy; raw_fallback, observed 2026-08-09T18:37:36.754008Z

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 738945b6-886e-4fbf-8377-8a1cba28cbfc · outbound

This paper cites an unresolved cited work.

Predicting the number density of heavy seed massive black holes due to an intense Lyman-Werner field Unresolved cited work

Reference 46

Resolution: unresolved; raw_fallback, observed 2026-08-09T18:37:36.739416Z

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 f97280a2-2244-4f56-af9a-05fe0b9fdc07 · outbound

This paper cites H., Schechter P., 1974, , 187, 425.

Predicting the number density of heavy seed massive black holes due to an intense Lyman-Werner field H., Schechter P., 1974, , 187, 425

Reference 47

Resolution: verified fuzzy; raw_fallback, observed 2026-08-09T18:37:36.725241Z

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 8e133c85-08f2-4773-9472-868f10412064 · outbound

This paper cites Massive Star Formation in Overdense Regions of the Early Universe.

Predicting the number density of heavy seed massive black holes due to an intense Lyman-Werner field Massive Star Formation in Overdense Regions of the Early Universe

Reference 48

Resolution: unresolved; no resolver link, observed 2026-08-09T18:37:36.045469Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 5ab83bb2-05f6-446b-9def-eb76c6cd9f7f · outbound

This paper cites an unresolved cited work.

Predicting the number density of heavy seed massive black holes due to an intense Lyman-Werner field Unresolved cited work

Reference 49

Resolution: unresolved; raw_fallback, observed 2026-08-09T18:37:36.710863Z

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 06415072-2de2-4fc9-8756-a14b53d724e3 · outbound

This paper cites A., Visbal E., Wise J.

Predicting the number density of heavy seed massive black holes due to an intense Lyman-Werner field A., Visbal E., Wise J

Reference 50

Resolution: verified fuzzy; raw_fallback, observed 2026-08-09T18:37:36.697111Z

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 6a5e19b0-9700-4158-917f-304f08f4668f · outbound

This paper cites A., Wise J.

Predicting the number density of heavy seed massive black holes due to an intense Lyman-Werner field A., Wise J

Reference 51

Resolution: verified fuzzy; raw_fallback, observed 2026-08-09T18:37:36.683778Z

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 1815ebfc-cc44-4807-8389-02f2e6f5b92f · outbound

This paper cites an unresolved cited work.

Predicting the number density of heavy seed massive black holes due to an intense Lyman-Werner field Unresolved cited work

Reference 52

Resolution: unresolved; raw_fallback, observed 2026-08-09T18:37:36.669548Z

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 661ae2dd-05c2-4932-94c8-d0fcffb6114f · outbound

This paper cites an unresolved cited work.

Predicting the number density of heavy seed massive black holes due to an intense Lyman-Werner field Unresolved cited work

Reference 53

Resolution: unresolved; raw_fallback, observed 2026-08-09T18:37:36.655726Z

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 7d30fd31-6bb7-4a48-9075-4274d90db77b · outbound

This paper cites L., Haiman Z., 2010, Monthly Notices of the Royal Astronomical Society, 402, 1249.

Predicting the number density of heavy seed massive black holes due to an intense Lyman-Werner field L., Haiman Z., 2010, Monthly Notices of the Royal Astronomical Society, 402, 1249

Reference 54

Resolution: verified fuzzy; raw_fallback, observed 2026-08-09T18:37:36.642344Z

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 62609cc5-4216-40b8-8391-a4491d5fea8b · outbound

This paper cites K., Mo H.

Predicting the number density of heavy seed massive black holes due to an intense Lyman-Werner field K., Mo H

Reference 55

Resolution: verified fuzzy; raw_fallback, observed 2026-08-09T18:37:36.628746Z

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 504a75c8-8f21-452c-b429-d8bd282b06cd · outbound

This paper cites F., 2024, , 691, A24.

Predicting the number density of heavy seed massive black holes due to an intense Lyman-Werner field F., 2024, , 691, A24

Reference 56

Resolution: verified fuzzy; raw_fallback, observed 2026-08-09T18:37:36.616094Z

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 58f19b3d-f05a-43df-a3f8-600df328a2ee · outbound

This paper cites D., Regan J.

Predicting the number density of heavy seed massive black holes due to an intense Lyman-Werner field D., Regan J

Reference 57

Resolution: verified fuzzy; raw_fallback, observed 2026-08-09T18:37:36.602186Z

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 a86bccef-0bbe-4ba3-ae16-fc2097304e5c · outbound

This paper cites L., Li M., 2014, , 439, 1092.

Predicting the number density of heavy seed massive black holes due to an intense Lyman-Werner field L., Li M., 2014, , 439, 1092

Reference 58

Resolution: verified fuzzy; raw_fallback, observed 2026-08-09T18:37:36.588630Z

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 51dde2da-aac6-4541-a6e7-72433e5c553b · outbound

This paper cites an unresolved cited work.

Predicting the number density of heavy seed massive black holes due to an intense Lyman-Werner field Unresolved cited work

Reference 59

Resolution: unresolved; raw_fallback, observed 2026-08-09T18:37:36.574765Z

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 f6096fad-b3c4-48e4-a0c1-1b735bbf21fb · outbound

This paper cites an unresolved cited work.

Predicting the number density of heavy seed massive black holes due to an intense Lyman-Werner field Unresolved cited work

Reference 60

Resolution: unresolved; raw_fallback, observed 2026-08-09T18:37:36.560210Z

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 c1866a47-7993-433c-b124-52a5938e17f4 · outbound

This paper cites an unresolved cited work.

Predicting the number density of heavy seed massive black holes due to an intense Lyman-Werner field Unresolved cited work

Reference 61

Resolution: unresolved; raw_fallback, observed 2026-08-09T18:37:36.546292Z

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 ef5df949-845b-466c-9c1d-428135b1acb6 · outbound

This paper cites an unresolved cited work.

Predicting the number density of heavy seed massive black holes due to an intense Lyman-Werner field Unresolved cited work

Reference 62

Resolution: unresolved; raw_fallback, observed 2026-08-09T18:37:36.532326Z

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 a0e3b376-d8fe-49f1-b28d-31d14abe51dd · outbound

This paper cites M., 2011, , 418, 906.

Predicting the number density of heavy seed massive black holes due to an intense Lyman-Werner field M., 2011, , 418, 906

Reference 63

Resolution: verified fuzzy; raw_fallback, observed 2026-08-09T18:37:36.517784Z

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 13576618-7da3-4d7e-b215-36330056e4f0 · outbound

This paper cites an unresolved cited work.

Predicting the number density of heavy seed massive black holes due to an intense Lyman-Werner field Unresolved cited work

Reference 64

Resolution: unresolved; raw_fallback, observed 2026-08-09T18:37:36.503685Z

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 0e01a60e-7677-40fe-95f2-e94268c02318 · outbound

This paper cites C., More S., Cacciato M., Mo H., Yang X., 2013, , 430, 725.

Predicting the number density of heavy seed massive black holes due to an intense Lyman-Werner field C., More S., Cacciato M., Mo H., Yang X., 2013, , 430, 725

Reference 65

Resolution: verified fuzzy; raw_fallback, observed 2026-08-09T18:37:36.489578Z

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 b6da2644-e344-42a1-a59f-57b18aaf3a80 · outbound

This paper cites H., Regan J.

Predicting the number density of heavy seed massive black holes due to an intense Lyman-Werner field H., Regan J

Reference 66

Resolution: verified fuzzy; raw_fallback, observed 2026-08-09T18:37:36.476117Z

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 edc0e7c8-a805-4170-be33-d3ab7928200d · outbound

This paper cites L., 2011, , 418, 838.

Predicting the number density of heavy seed massive black holes due to an intense Lyman-Werner field L., 2011, , 418, 838

Reference 67

Resolution: verified fuzzy; raw_fallback, observed 2026-08-09T18:37:36.462218Z

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 b389e61b-cd6a-42e7-8bd3-d1d8ca8a4fa8 · outbound

This paper cites H., Norman M.

Predicting the number density of heavy seed massive black holes due to an intense Lyman-Werner field H., Norman M

Reference 68

Resolution: verified fuzzy; raw_fallback, observed 2026-08-09T18:37:36.447199Z

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 0b7013f3-595a-4f13-9dd8-81dc22cbb983 · outbound

This paper cites L., O'Shea B.

Predicting the number density of heavy seed massive black holes due to an intense Lyman-Werner field L., O'Shea B

Reference 69

Resolution: verified fuzzy; raw_fallback, observed 2026-08-09T18:37:36.433880Z

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 d650bc3a-3d9a-419d-8acc-34e0e24e400d · outbound

This paper cites H., Norman M.

Predicting the number density of heavy seed massive black holes due to an intense Lyman-Werner field H., Norman M

Reference 70

Resolution: verified fuzzy; raw_fallback, observed 2026-08-09T18:37:36.419568Z

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 8286e788-7f71-4701-a07e-dc92093e342b · outbound

This paper cites an unresolved cited work.

Predicting the number density of heavy seed massive black holes due to an intense Lyman-Werner field Unresolved cited work

Reference 71

Resolution: unresolved; raw_fallback, observed 2026-08-09T18:37:36.404910Z

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 134065a3-39ae-4b45-b563-949af0f6c3e0 · outbound

This paper cites Are the ultra-high-redshift galaxies at z > 10 surprising in the context of standard galaxy formation models?.

Predicting the number density of heavy seed massive black holes due to an intense Lyman-Werner field Are the ultra-high-redshift galaxies at z > 10 surprising in the context of standard galaxy formation models?

Reference 72

Resolution: unresolved; no resolver link, observed 2026-08-09T18:37:36.151035Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 67145c7d-69ea-4406-9ab3-eb3b7d373283 · outbound

This paper cites S., 2023, , 518, 2076.

Predicting the number density of heavy seed massive black holes due to an intense Lyman-Werner field S., 2023, , 518, 2076

Reference 73

Resolution: verified fuzzy; raw_fallback, observed 2026-08-09T18:37:36.390702Z

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 d82bcf9f-5c3b-41f2-bbb2-ddbf17ecee06 · outbound

This paper cites , " * write output.state after.block = add.period write newline.

Predicting the number density of heavy seed massive black holes due to an intense Lyman-Werner field , " * write output.state after.block = add.period write newline

Reference 74

Resolution: unresolved; no resolver link, observed 2026-08-09T18:37:36.159871Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f8358e39-1016-4b07-8eed-05b18801a784 · outbound

This paper cites write newline.

Predicting the number density of heavy seed massive black holes due to an intense Lyman-Werner field write newline

Reference 75

Resolution: unresolved; no resolver link, observed 2026-08-09T18:37:36.164362Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Pith citing papers

Observation d6f9e175-0266-484d-a1da-bdf27a03b4e4 · inbound

Flash Ionization of the Early Universe by Pop III.1 Supermassive Stars cites this paper.

Flash Ionization of the Early Universe by Pop III.1 Supermassive Stars Predicting the number density of heavy seed massive black holes due to an intense Lyman-Werner field

Reference 37

Resolution: unresolved; no resolver link, observed 2026-08-06T23:21:42.547743Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation eac45310-605e-4b18-8434-86bd4d628e67 · inbound

The Evolution of Pop III.1 Protostars Powered by Dark Matter Annihilation. I. Fiducial model and first results cites this paper.

The Evolution of Pop III.1 Protostars Powered by Dark Matter Annihilation. I. Fiducial model and first results Predicting the number density of heavy seed massive black holes due to an intense Lyman-Werner field

Reference 30

Resolution: unresolved; no resolver link, observed 2026-08-06T21:15:08.410822Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a466134d-6958-4a32-9766-874ba4169a8f · inbound

The Emergence and Ionizing Feedback of Pop III.1 Stars as Progenitors for Supermassive Black Holes cites this paper.

The Emergence and Ionizing Feedback of Pop III.1 Stars as Progenitors for Supermassive Black Holes Predicting the number density of heavy seed massive black holes due to an intense Lyman-Werner field

Reference 59

Resolution: unresolved; no resolver link, observed 2026-08-06T11:17:50.397541Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 6c3919f7-520d-413d-94ad-f5b01d94bdd1 · inbound

Direct Collapse Black Hole Candidates from Decaying Dark Matter cites this paper.

Direct Collapse Black Hole Candidates from Decaying Dark Matter Predicting the number density of heavy seed massive black holes due to an intense Lyman-Werner field

Reference 55

Resolution: verified exact; arxiv_id, observed 2026-05-18T12:11:22.579715Z

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.