Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links, observed 2026-08-09T18:37:36.164362Z
Paper Citation Record · LEDGER
Predicting the number density of heavy seed massive black holes due to an intense Lyman-Werner field
As of 22 August 2026, this Paper Citation Record lists 75 of 75 outbound references and 5 inbound Pith citation observations for arXiv:2502.00574.
A citation records a reference. It does not transfer a finding from one paper to another.
Coverage vector
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-22T06:32:14.747728+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-15T19:14:52.922592Z
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
- verified fuzzy34
- unresolved39
- parse uncertain0
- malformed identifier0
- metadata mismatch2
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
No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.
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
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.
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
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.
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
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.
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
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.
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
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.
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
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.
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
No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.
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
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.
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
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.
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
No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.
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
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.
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
No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.
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
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.
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
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.
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
Unavailable: canonical work link unavailable.
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
No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.
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
Unavailable: canonical work link unavailable.
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
No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.
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
No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.
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
Unavailable: canonical work link unavailable.
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
No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.
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
No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.
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
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.
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 2026-08-22T06:32:14.747728+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 2026-08-22T06:32:14.747728+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 2026-08-22T06:32:14.747728+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 2026-08-22T06:32:14.747728+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 2026-08-22T06:32:14.747728+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 2026-08-22T06:32:14.747728+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 2026-08-22T06:32:14.747728+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 2026-08-22T06:32:14.747728+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 2026-08-22T06:32:14.747728+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 2026-08-22T06:32:14.747728+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 2026-08-22T06:32:14.747728+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 2026-08-22T06:32:14.747728+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 2026-08-22T06:32:14.747728+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 2026-08-22T06:32:14.747728+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 2026-08-22T06:32:14.747728+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 2026-08-22T06:32:14.747728+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 2026-08-22T06:32:14.747728+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 2026-08-22T06:32:14.747728+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 2026-08-22T06:32:14.747728+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 2026-08-22T06:32:14.747728+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 2026-08-22T06:32:14.747728+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 2026-08-22T06:32:14.747728+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 2026-08-22T06:32:14.747728+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 2026-08-22T06:32:14.747728+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 2026-08-22T06:32:14.747728+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 2026-08-22T06:32:14.747728+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 2026-08-22T06:32:14.747728+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 2026-08-22T06:32:14.747728+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 2026-08-22T06:32:14.747728+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 2026-08-22T06:32:14.747728+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 2026-08-22T06:32:14.747728+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 2026-08-22T06:32:14.747728+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 2026-08-22T06:32:14.747728+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 2026-08-22T06:32:14.747728+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 2026-08-22T06:32:14.747728+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 2026-08-22T06:32:14.747728+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 2026-08-22T06:32:14.747728+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 2026-08-22T06:32:14.747728+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 2026-08-22T06:32:14.747728+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 2026-08-22T06:32:14.747728+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 2026-08-22T06:32:14.747728+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 2026-08-22T06:32:14.747728+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 2026-08-22T06:32:14.747728+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 6e0b7d84-cf37-4910-bff3-dcde7f725d5e · inbound
Signatures of BH seeding on the $\mathrm{M_{\displaystyle \bullet}}-\sigma$ relation: Predictions from the BRAHMA simulations cites this paper.
Signatures of BH seeding on the $\mathrm{M_{\displaystyle \bullet}}-\sigma$ relation: Predictions from the BRAHMA simulations Predicting the number density of heavy seed massive black holes due to an intense Lyman-Werner field
Reference 57
- Resolution
- unresolved
- no resolver link, observed 2026-08-15T19:14:52.922592Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
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 2026-08-22T06:32:14.747728+00:00.