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Paper Citation Record · LEDGER

Are we surprised to find SMBHs with JWST at z > 9?

As of 21 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:2305.12504.

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

pith.paper-citation-record.v1
2305.12504 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 5 of 5 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-21T06:32:19.484+00:00

measured 5 of 5 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-11T21:08:51.925035Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-11T06:27:50.617753Z

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
  • unresolved0
  • parse uncertain0
  • malformed identifier0
  • metadata mismatch0

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 6d58a0da-91bf-4acf-b02a-9e5aa47dffaa · inbound

Red, hot, and very metal poor: extreme properties of a massive accreting black hole in the first 500 Myr cites this paper.

Red, hot, and very metal poor: extreme properties of a massive accreting black hole in the first 500 Myr Are we surprised to find SMBHs with JWST at z > 9?

Reference 46

Resolution
malformed identifier
no resolver link, observed 2026-08-11T21:08:51.925035Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-11T21:08:51.925035Z digest=sha256:8f0075805e7d256214cf05eed7ed043f6ac9476b9746d19f2025a389653bf766

Observation 658e3e57-1646-4770-8302-46612d9def1a · inbound

What drives the growth of black holes: a decade of progress cites this paper.

What drives the growth of black holes: a decade of progress Are we surprised to find SMBHs with JWST at z > 9?

Reference 88

Resolution
unresolved
no resolver link, observed 2026-08-06T23:10:49.229451Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T23:10:49.229451Z digest=sha256:e132f8f59e4c1ee13ed9dc5987147cea7beba25e1d2f4d0188d201b6894f9f79

Observation 4556c4b0-d34b-4f80-b3c2-f400f703eb57 · inbound

Evolution of Size, Mass, and Density of Galaxies Since Cosmic Dawn cites this paper.

Evolution of Size, Mass, and Density of Galaxies Since Cosmic Dawn Are we surprised to find SMBHs with JWST at z > 9?

Reference 56

Resolution
unresolved
no resolver link, observed 2026-08-04T10:26:49.170861Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-04T10:26:49.170861Z digest=sha256:e7b03ffca506d45835b980852b69de7551f71af1d866831a6009cd616c5f41c1

Observation 0bff42b1-ead4-47b3-a754-8f631c4ddfcf · inbound

BlackTHUNDER Reveals a Massive Filament around a Compact AGN at $z\simeq5.23$ cites this paper.

BlackTHUNDER Reveals a Massive Filament around a Compact AGN at $z\simeq5.23$ Are we surprised to find SMBHs with JWST at z > 9?

Reference 5

Resolution
verified exact
local_arxiv, observed 2026-07-11T06:27:50.619853Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

source=arxiv_source observed=2026-07-11T06:23:06.110361Z digest=sha256:ceb1ff8854039278d5243de1241bc01f0844b5ecfa39a7f88c1e19b06e6a68a7

Observation 447e8e8d-ea27-491e-8f26-df650a12161e · inbound

An (in)complete NIRSpec census of Balmer absorption in Type 1 AGN -- radiation-driven outflows in little red dots, quasars and variable stars cites this paper.

An (in)complete NIRSpec census of Balmer absorption in Type 1 AGN -- radiation-driven outflows in little red dots, quasars and variable stars Are we surprised to find SMBHs with JWST at z > 9?

Reference 70

Resolution
unresolved
no resolver link, observed 2026-08-01T13:38:27.657908Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T13:38:27.657908Z digest=sha256:b04a90e7ebd079154341a14abd112fc1110cd6b424b9fc824cdcb8a6f736034e