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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 18 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 12 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 12 of 12 standing notices

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

measured 12 of 12 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-11T21:08:51.846095Z

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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 f177cf69-3081-4fa2-b9a3-3ea4c26a7dec · inbound

Red, hot, and very metal poor: extreme properties of a massive accreting black hole in the first 500 Myr cites this paper.

Red, hot, and very metal poor: extreme properties of a massive accreting black hole in the first 500 Myr RUBIES: Evolved Stellar Populations with Extended Formation Histories at $z \sim 7-8$ in Candidate Massive Galaxies Identified with JWST/NIRSpec

Reference 11

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Observation fa3a1ab4-49cf-4a1c-aae6-622ed91a5792 · inbound

Evaluating the Predictive Capacity of FLARES Simulations for High Redshift "Little Red Dots" cites this paper.

Evaluating the Predictive Capacity of FLARES Simulations for High Redshift "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 52

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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

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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

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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

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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

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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

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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

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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

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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

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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

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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

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