Paper Citation Record · LEDGER

Physical properties of 15 quasars at $z\gtrsim 6.5$

As of 16 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 6 inbound Pith citation observations for arXiv:1710.01251.

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

pith.paper-citation-record.v1
1710.01251 v1

Coverage vector

measured 0 of 0 reference resolution

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Source: paper_references, paper_reference_links

measured 6 of 6 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-16T06:30:59.297886+00:00

measured 6 of 6 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-16T00:12:18.766466Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-04T20:10:08.676625Z

Reference resolution

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Outbound references

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Pith citing papers

Observation 1cb88b2d-cb33-4908-a477-13a2f015fca6 · inbound

Estimating the spins of supermassive black holes in distant ultraluminous quasars cites this paper.

Estimating the spins of supermassive black holes in distant ultraluminous quasars Physical properties of 15 quasars at $z\gtrsim 6.5$

Reference 3

Resolution: unresolved; no resolver link, observed 2026-08-15T22:06:52.967425Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e5aebfda-727d-4752-affc-63c44e4ff205 · inbound

JWST Absorption-Line Analysis of UV-Bright Galaxies at $z=7.2-10.6$: Early Chemical Enrichment Traced by C, O, Mg, Al, Si, and Fe cites this paper.

JWST Absorption-Line Analysis of UV-Bright Galaxies at $z=7.2-10.6$: Early Chemical Enrichment Traced by C, O, Mg, Al, Si, and Fe Physical properties of 15 quasars at $z\gtrsim 6.5$

Reference 114

Resolution: verified exact; local_arxiv, observed 2026-06-27T18:01:08.020614Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

Observation 84949433-c5ad-477b-8d53-33aed69a9542 · inbound

Constraining supermassive primordial black hole clustering with the angular auto-correlation of $z\simeq 6$ quasars cites this paper.

Constraining supermassive primordial black hole clustering with the angular auto-correlation of $z\simeq 6$ quasars Physical properties of 15 quasars at $z\gtrsim 6.5$

Reference 77

Resolution: verified exact; local_arxiv, observed 2026-07-04T20:10:08.677974Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

Observation 177442ba-89d7-4064-ab76-a87c668b1e52 · 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 $z \gtrsim 6$ Physical properties of 15 quasars at $z\gtrsim 6.5$

Reference 197

Resolution: unresolved; no resolver link, observed 2026-08-01T06:58:52.107621Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation af1a61b0-cd21-402b-8751-89edb6beb9a9 · inbound

The most extreme high-z radio quasars in the eRASS:1 X-ray survey cites this paper.

The most extreme high-z radio quasars in the eRASS:1 X-ray survey Physical properties of 15 quasars at $z\gtrsim 6.5$

Reference 294

Resolution: unresolved; no resolver link, observed 2026-08-15T14:49:10.775248Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f5210de5-b5f9-4ba2-8f3a-ba4cb466afb1 · inbound

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics cites this paper.

Why is GN-z11 Bright, Compact, and Nitrogen Enhanced? Insights from UV Absorption and Emission Diagnostics Physical properties of 15 quasars at $z\gtrsim 6.5$

Reference 260

Resolution: unresolved; no resolver link, observed 2026-08-16T00:12:18.766466Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.