Paper Citation Record · LEDGER

RUBIES: Evolved Stellar Populations with Extended Formation Histories at $z \sim 7-8$ in Candidate Massive Galaxies Identified with JWST/NIRSpec

As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 10 inbound Pith citation observations for arXiv:2405.01473.

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

pith.paper-citation-record.v1
2405.01473 v2

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measured 10 of 10 standing notices

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Source: scholarly_work_events, retraction_status_cache, observed 2026-08-11T06:34:44.6726+00:00

measured 10 of 10 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-08T20:32:19.337359Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-02T09:56:51.914393Z

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Outbound references

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Pith citing papers

Observation 70d00e64-6ee7-421f-80ec-17cb90eac2e7 · inbound

A prevalent population of normal-mass central black holes in high-redshift massive galaxies cites this paper.

A prevalent population of normal-mass central black holes in high-redshift massive galaxies RUBIES: Evolved Stellar Populations with Extended Formation Histories at $z \sim 7-8$ in Candidate Massive Galaxies Identified with JWST/NIRSpec

Reference 81

Resolution: malformed identifier; no resolver link, observed 2026-08-08T20:32:19.337359Z

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Observation b7c50685-7211-4fcc-a491-e93f9daa8a64 · inbound

A "Black Hole Star" Reveals the Remarkable Gas-Enshrouded Hearts of the Little Red Dots cites this paper.

A "Black Hole Star" Reveals the Remarkable Gas-Enshrouded Hearts of the Little Red Dots RUBIES: Evolved Stellar Populations with Extended Formation Histories at $z \sim 7-8$ in Candidate Massive Galaxies Identified with JWST/NIRSpec

Reference 23

Resolution: verified exact; arxiv_id, observed 2026-05-16T08:53:14.719386Z

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Observation ae8576d7-30c9-4ca5-a05b-15794ad48493 · inbound

Discovery of a Pair of Galaxies with Both Hosting X-ray Binary Candidates at $z=2.544$ cites this paper.

Discovery of a Pair of Galaxies with Both Hosting X-ray Binary Candidates at $z=2.544$ RUBIES: Evolved Stellar Populations with Extended Formation Histories at $z \sim 7-8$ in Candidate Massive Galaxies Identified with JWST/NIRSpec

Reference 81

Resolution: unresolved; no resolver link, observed 2026-08-06T11:03:53.703606Z

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Observation 0ba1d609-039a-49d2-9376-352adc01a592 · inbound

Little Red reionization factories cites this paper.

Little Red reionization factories RUBIES: Evolved Stellar Populations with Extended Formation Histories at $z \sim 7-8$ in Candidate Massive Galaxies Identified with JWST/NIRSpec

Reference 3

Resolution: unresolved; no resolver link, observed 2026-08-05T19:03:19.973818Z

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Observation 2333510c-d887-4d19-9952-967e0e07506f · inbound

Discovery of Multiply Ionized Iron Emission Powered by an Active Galactic Nucleus in a z~7 Little Red Dot cites this paper.

Discovery of Multiply Ionized Iron Emission Powered by an Active Galactic Nucleus in a z~7 Little Red Dot RUBIES: Evolved Stellar Populations with Extended Formation Histories at $z \sim 7-8$ in Candidate Massive Galaxies Identified with JWST/NIRSpec

Reference 54

Resolution: malformed identifier; no resolver link, observed 2026-08-04T18:47:40.889133Z

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Observation ba33f0f5-a06b-4e3a-ac31-7c2449fbe23a · inbound

Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution cites this paper.

Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution RUBIES: Evolved Stellar Populations with Extended Formation Histories at $z \sim 7-8$ in Candidate Massive Galaxies Identified with JWST/NIRSpec

Reference 9

Resolution: unresolved; no resolver link, observed 2026-08-02T12:34:25.914675Z

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Observation f5bde585-f1a9-47e1-aeb0-0d2c1523eb46 · inbound

Little red dots as a cosmological probe: constraining $H_0$ with quasi-periodic pulsations cites this paper.

Little red dots as a cosmological probe: constraining $H_0$ with quasi-periodic pulsations RUBIES: Evolved Stellar Populations with Extended Formation Histories at $z \sim 7-8$ in Candidate Massive Galaxies Identified with JWST/NIRSpec

Reference 10

Resolution: verified exact; arxiv_id, observed 2026-07-02T09:56:51.916080Z

Source-reported events for the cited work

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Observation 74427383-9129-43c4-be60-03a2508d097f · 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 RUBIES: Evolved Stellar Populations with Extended Formation Histories at $z \sim 7-8$ in Candidate Massive Galaxies Identified with JWST/NIRSpec

Reference 125

Resolution: unresolved; no resolver link, observed 2026-08-01T13:38:33.321455Z

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Observation 105372ed-d41f-49ef-a56c-662e4c718c39 · inbound

Misaligned or chaotic? A strong break of axial symmetry in the local LRD J1025 revealed with VLT/FORS2 spectropolarimetry cites this paper.

Misaligned or chaotic? A strong break of axial symmetry in the local LRD J1025 revealed with VLT/FORS2 spectropolarimetry RUBIES: Evolved Stellar Populations with Extended Formation Histories at $z \sim 7-8$ in Candidate Massive Galaxies Identified with JWST/NIRSpec

Reference 168

Resolution: unresolved; no resolver link, observed 2026-08-03T00:41:33.065433Z

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Observation b6346810-2b8d-44f1-88d0-bb17415245ee · inbound

Where did all the Little Red Dots go? The abundance of LRD analogues among objects with broad lines at $z < 0.35$ cites this paper.

Where did all the Little Red Dots go? The abundance of LRD analogues among objects with broad lines at $z < 0.35$ RUBIES: Evolved Stellar Populations with Extended Formation Histories at $z \sim 7-8$ in Candidate Massive Galaxies Identified with JWST/NIRSpec

Reference 114

Resolution: unresolved; no resolver link, observed 2026-08-08T16:36:20.738548Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.