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Paper Citation Record · LEDGER

The Growth Efficiency of High-Redshift Black Holes

As of 18 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1506.04750.

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

pith.paper-citation-record.v1
1506.04750 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 3 of 3 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-18T06:34:40.430872+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-01T06:58:47.317729Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-06-27T21:01:15.973603Z

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 757d41fe-703b-4299-914d-40359b777967 · inbound

The X-ray-to-UV relation does not evolve in homogeneous quasar samples cites this paper.

The X-ray-to-UV relation does not evolve in homogeneous quasar samples The Growth Efficiency of High-Redshift Black Holes

Reference 204

Resolution
verified exact
local_arxiv, observed 2026-06-27T21:01:15.974830Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:563509bb65629d588c2eb799eb5a49289753b217a204e7f7463c488955d7d5e6

Observation 36d9ce17-1f8d-47ea-aa89-b259e155b079 · inbound

The gravitational-wave fingerprint of dynamically assembled primordial black hole cluster seeds in JWST's Little Red Dots cites this paper.

The gravitational-wave fingerprint of dynamically assembled primordial black hole cluster seeds in JWST's Little Red Dots The Growth Efficiency of High-Redshift Black Holes

Reference 11

Resolution
unresolved
no resolver link, observed 2026-07-13T04:45:18.545506Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-07-13T04:45:18.545506Z digest=sha256:d5849b1d7413ca046801d03e78327c180e84883efa03c00ce26e7a72bf212ce4

Observation 64f07104-b2eb-43e5-ae49-9f7aa6a802ab · inbound

Outflows in super-Eddington quasars drive clumpy circumgalactic medium and extended H$\alpha$ nebulae at $z \gtrsim 6$ cites this paper.

Outflows in super-Eddington quasars drive clumpy circumgalactic medium and extended H$\alpha$ nebulae at $z \gtrsim 6$ The Growth Efficiency of High-Redshift Black Holes

Reference 154

Resolution
unresolved
no resolver link, observed 2026-08-01T06:58:47.317729Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T06:58:47.317729Z digest=sha256:b859a12b4a54c22cda143209da3ea59794d882532a153e8e17d63b195f53f08e