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Paper Citation Record · LEDGER

A Post-Starburst Pathway for the Formation of Massive Galaxies and Black Holes at z>6

As of 5 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2409.07113.

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

pith.paper-citation-record.v1
2409.07113 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 2 of 2 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-05T06:32:48.257954+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-06-29T06:28:28.831162Z

measured 1 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-08-05T02:28:24.338817Z

Reference resolution

0 of 0 outbound references displayed

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

External citation measurements

2
arxiv_reference, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 1f750a7f-1d04-4784-acb6-5f76557e4bdb · inbound

Winding Back the Clock: Recent Star Formation Histories of Massive Quiescent Galaxies Are Consistent With Their Rapid Number Density Evolution Since $\mathbf{z\sim7}$ cites this paper.

Winding Back the Clock: Recent Star Formation Histories of Massive Quiescent Galaxies Are Consistent With Their Rapid Number Density Evolution Since $\mathbf{z\sim7}$ A Post-Starburst Pathway for the Formation of Massive Galaxies and Black Holes at z>6

Reference 81

Resolution
verified exact
arxiv_id, observed 2026-05-10T19:05:44.766753Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-05-10T19:04:02.059130Z digest=sha256:a747cc2d78883a2fa35a4c9d2b2c0181a9f9218ad6ef152d0009f927926d1e53

Observation e991e5ed-81f3-47eb-b320-307298721463 · inbound

High-ionization coronal lines trace quasar-like activity in recently quenched galaxies at high redshift cites this paper.

High-ionization coronal lines trace quasar-like activity in recently quenched galaxies at high redshift A Post-Starburst Pathway for the Formation of Massive Galaxies and Black Holes at z>6

Reference 71

Resolution
verified exact
arxiv_id, observed 2026-06-29T06:33:12.167904Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=pdf_text observed=2026-06-29T06:28:28.831162Z digest=sha256:6a4662d9f92365ea3350bfefe43f9bfabddb3390035290b98ac9f3e65cf53cf7