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Paper Citation Record · LEDGER

The Origin of Supermassive Black Holes from Pop III.1 Seeds

As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 8 inbound Pith citation observations for arXiv:2412.01828.

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

pith.paper-citation-record.v1
2412.01828 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 8 of 8 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 8 of 8 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T05:00:00.362069Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-04T02:39:24.313483Z

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External citation measurements

No source-named external measurement is stored.

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation a35b60bf-9ee6-4159-a5db-e91ab799a631 · inbound

Dynamics of low-mass black hole seeds in the BRAHMA simulations using subgrid-dynamical friction: Impact on merger-driven black hole growth in the high redshift Universe cites this paper.

Dynamics of low-mass black hole seeds in the BRAHMA simulations using subgrid-dynamical friction: Impact on merger-driven black hole growth in the high redshift Universe The Origin of Supermassive Black Holes from Pop III.1 Seeds

Reference 92

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unresolved
no resolver link, observed 2026-08-07T05:00:00.362069Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 92b18dc3-7c7f-4b9e-af4d-bdaa6dda54b6 · 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 The Origin of Supermassive Black Holes from Pop III.1 Seeds

Reference 48

Resolution
unresolved
no resolver link, observed 2026-08-06T23:21:44.086241Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T23:21:44.086241Z digest=sha256:0680fb208275f1a447a627d8e0e7813f5d079c36ca2661064bcad0e4f6ad5bc9

Observation 44f8dab7-8760-44ca-a91f-d88c54735e4e · 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 The Origin of Supermassive Black Holes from Pop III.1 Seeds

Reference 38

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unresolved
no resolver link, observed 2026-08-06T21:15:08.661445Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T21:15:08.661445Z digest=sha256:eb78ea207f1ae0bfa5f7e4ebd702ecb3c91cd267f6c39af5abd46b1017632c94

Observation f9204fe0-5760-4cdf-80e0-f7731efc071c · inbound

On the rapid growth of SMBHs in high-z galaxies: the aftermath of Population III.1 stars cites this paper.

On the rapid growth of SMBHs in high-z galaxies: the aftermath of Population III.1 stars The Origin of Supermassive Black Holes from Pop III.1 Seeds

Reference 189

Resolution
unresolved
no resolver link, observed 2026-08-06T20:45:12.360048Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation d0bc8bed-a4c5-45b2-913d-cc294c43e013 · inbound

Reconstructing PTA measurements via early seeding of supermassive black holes cites this paper.

Reconstructing PTA measurements via early seeding of supermassive black holes The Origin of Supermassive Black Holes from Pop III.1 Seeds

Reference 77

Resolution
unresolved
no resolver link, observed 2026-08-06T19:15:32.042501Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-06T19:15:32.042501Z digest=sha256:2732eb587fb9a4e644dc4b2f8b99df242dd34f6d20a527d27a51f25c29edd221

Observation f2d0568c-f2b4-4ac2-8b11-e4271cb6184b · 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 The Origin of Supermassive Black Holes from Pop III.1 Seeds

Reference 79

Resolution
unresolved
no resolver link, observed 2026-08-06T11:17:50.457781Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-06T11:17:50.457781Z digest=sha256:832c615f8a2f05f65a0e697226899f5867c2b3f20611026b1d014c3da1ace7ba

Observation a291babc-094f-49d0-a5e9-40ed2af54bd1 · inbound

The Impact of Population III.1 Flash Reionization for CMB Polarization and Thomson Scattering Optical Depth cites this paper.

The Impact of Population III.1 Flash Reionization for CMB Polarization and Thomson Scattering Optical Depth The Origin of Supermassive Black Holes from Pop III.1 Seeds

Reference 5

Resolution
unresolved
no resolver link, observed 2026-08-04T08:41:19.235986Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-04T08:41:19.235986Z digest=sha256:82e2b883344de49fb1016177d9b312a5499767bd787388c8adfc65ee57e665e7

Observation 09c4dc24-6765-4814-925a-be36aafeda30 · inbound

Fireworks at Cosmic Dawn: relieving BAO-CMB tensions with the Pop III.1 Flash cites this paper.

Fireworks at Cosmic Dawn: relieving BAO-CMB tensions with the Pop III.1 Flash The Origin of Supermassive Black Holes from Pop III.1 Seeds

Reference 68

Resolution
verified exact
arxiv_id, observed 2026-07-04T02:39:24.314899Z

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.

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