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Paper Citation Record · LEDGER

The Bolometric Quasar Luminosity Function at z = 0-7

As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 8 inbound Pith citation observations for arXiv:2001.02696.

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

pith.paper-citation-record.v1
2001.02696 v2

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 2026-08-07T06:34:17.273281+00:00

measured 8 of 8 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-05T11:14:26.179835Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-02T11:06:53.186813Z

Reference resolution

0 of 0 outbound references displayed

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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 883cbb9d-01a6-4f1d-b572-b64918710df4 · inbound

Influence of supermassive primordial black holes on ultraviolet luminosity of high-redshift galaxies cites this paper.

Influence of supermassive primordial black holes on ultraviolet luminosity of high-redshift galaxies The Bolometric Quasar Luminosity Function at z = 0-7

Reference 81

Resolution
unresolved
no resolver link, observed 2026-08-05T11:14:26.179835Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 52324c1a-6e7b-4669-a343-d5e889d92198 · inbound

Uncertainties in the supermassive black hole abundance and implications for the GW background cites this paper.

Uncertainties in the supermassive black hole abundance and implications for the GW background The Bolometric Quasar Luminosity Function at z = 0-7

Reference 67

Resolution
unresolved
no resolver link, observed 2026-08-04T21:30:31.576654Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-04T21:30:31.576654Z digest=sha256:712d8036377dacc2cac73392dbb66fba59dd279eea390f56b9536be114eab5bc

Observation 1a1dc49d-3286-4fdd-a7d7-f76f1cf592de · inbound

Primordial black holes and the velocity acoustic oscillations features in 21 cm signals from the cosmic Dark Ages cites this paper.

Primordial black holes and the velocity acoustic oscillations features in 21 cm signals from the cosmic Dark Ages The Bolometric Quasar Luminosity Function at z = 0-7

Reference 68

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verified exact
arxiv_id, observed 2026-05-15T08:35:18.657276Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

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Observation 8fa56010-b69f-414f-aaf1-88e3ed4e2bf3 · inbound

Light, heavy, primordial: exploring the diversity of black hole seeding and growth mechanisms in the JWST era cites this paper.

Light, heavy, primordial: exploring the diversity of black hole seeding and growth mechanisms in the JWST era The Bolometric Quasar Luminosity Function at z = 0-7

Reference 13

Resolution
verified exact
arxiv_id, observed 2026-05-09T23:24:43.010419Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

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Observation fea26c85-876a-4576-a554-14d4f1eae325 · inbound

AGN Line-Intensity Mapping: A Probe of Faint Black Holes at Cosmic Noon cites this paper.

AGN Line-Intensity Mapping: A Probe of Faint Black Holes at Cosmic Noon The Bolometric Quasar Luminosity Function at z = 0-7

Reference 15

Resolution
verified exact
arxiv_id, observed 2026-07-02T11:06:53.188927Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

source=pdf_text observed=2026-06-28T04:41:14.082299Z digest=sha256:35afc4be14206103d527e44c489d4dfe534cbf553f758d81d5b28a87483eb916

Observation e67a51ab-7ff7-44e1-a745-8e23f721b4dd · inbound

A hierarchical Bayesian framework for cosmology using Type 1 AGN variability cites this paper.

A hierarchical Bayesian framework for cosmology using Type 1 AGN variability The Bolometric Quasar Luminosity Function at z = 0-7

Reference 69

Resolution
verified exact
arxiv_id, observed 2026-07-01T15:35:47.789179Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

source=pdf_text observed=2026-06-30T01:21:18.798989Z digest=sha256:f4cc37b39e3c1011d61a54cbf29b17f1ce8135cf13c42df7eeb17e780ef78cdd

Observation 68244f95-266d-4f8a-9154-5b699c29ae73 · 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 Bolometric Quasar Luminosity Function at z = 0-7

Reference 246

Resolution
unresolved
no resolver link, observed 2026-08-01T06:58:57.601792Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 52c053d9-d8e6-4bd8-a92f-551512a48375 · inbound

How greedy is the Universe? An entropy ledger and a causal envelope for early black hole growth cites this paper.

How greedy is the Universe? An entropy ledger and a causal envelope for early black hole growth The Bolometric Quasar Luminosity Function at z = 0-7

Reference 21

Resolution
unresolved
no resolver link, observed 2026-08-04T00:52:06.979476Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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