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Paper Citation Record · LEDGER

Emission Line Diagnostics for IMBHs in Dwarf Galaxies: Accounting for BH Seeding and ULX Excitation

As of 4 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:2505.07749.

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

pith.paper-citation-record.v1
2505.07749 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 5 of 5 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-03T06:30:56.289259+00:00

measured 5 of 5 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-02T12:55:20.618180Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-10T12:15:01.137692Z

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 cb7d5d7b-0c81-4aa8-9f98-408b610dfc28 · inbound

RUBIES: The Evolution of the Ionization Parameter from 0 < z < 9 cites this paper.

RUBIES: The Evolution of the Ionization Parameter from 0 < z < 9 Emission Line Diagnostics for IMBHs in Dwarf Galaxies: Accounting for BH Seeding and ULX Excitation

Reference 82

Resolution
verified exact
arxiv_id, observed 2026-06-29T06:43:09.788258Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-03T06:30:56.289259+00:00.

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Observation d5e123e1-af1f-474a-8d6e-5673d4320665 · inbound

RUBIES: The Evolution of the Ionization Parameter from 0 < z < 9 cites this paper.

RUBIES: The Evolution of the Ionization Parameter from 0 < z < 9 Emission Line Diagnostics for IMBHs in Dwarf Galaxies: Accounting for BH Seeding and ULX Excitation

Reference 82

Resolution
unresolved
no resolver link, observed 2026-08-02T12:55:20.618180Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 7b564f04-867c-4bda-9015-d361b7901e2d · inbound

LEGGOS I: The JWST LEGGOS Survey -- LEnsing and Galaxy Growth: Observing Substructures -- Unpacks the Nature of Clumpy Star Formation and Quenching in Gravitationally Lensed Galaxies beyond Cosmic Noon cites this paper.

LEGGOS I: The JWST LEGGOS Survey -- LEnsing and Galaxy Growth: Observing Substructures -- Unpacks the Nature of Clumpy Star Formation and Quenching in Gravitationally Lensed Galaxies beyond Cosmic Noon Emission Line Diagnostics for IMBHs in Dwarf Galaxies: Accounting for BH Seeding and ULX Excitation

Reference 87

Resolution
metadata mismatch
arxiv_id, observed 2026-06-26T16:19:35.458821Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-03T06:30:56.289259+00:00.

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Observation 9fdc3cc6-1aec-4d98-88ff-9ae296b0430f · inbound

LEGGOS I: The JWST LEGGOS Survey -- LEnsing and Galaxy Growth: Observing Substructures -- Unpacks the Nature of Clumpy Star Formation and Quenching in Gravitationally Lensed Galaxies beyond Cosmic Noon cites this paper.

LEGGOS I: The JWST LEGGOS Survey -- LEnsing and Galaxy Growth: Observing Substructures -- Unpacks the Nature of Clumpy Star Formation and Quenching in Gravitationally Lensed Galaxies beyond Cosmic Noon Emission Line Diagnostics for IMBHs in Dwarf Galaxies: Accounting for BH Seeding and ULX Excitation

Reference 153

Resolution
unresolved
no resolver link, observed 2026-08-02T10:49:40.845862Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T10:49:40.845862Z digest=sha256:134dad2c307891cc19ee0188e98ca665f5f6bfe95069c5339ce0117e47e63363

Observation 479b9b16-3514-4b38-9ee2-73fc27f80034 · inbound

The Goldilocks Molecule: H$_{2}$ Emission Lines Can Identify Elusive Dwarf AGN cites this paper.

The Goldilocks Molecule: H$_{2}$ Emission Lines Can Identify Elusive Dwarf AGN Emission Line Diagnostics for IMBHs in Dwarf Galaxies: Accounting for BH Seeding and ULX Excitation

Reference 12

Resolution
unresolved
no resolver link, observed 2026-08-02T00:38:33.159559Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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