Paper Citation Record · LEDGER

Constraints on Dark Matter from Dynamical Heating of Stars in Ultrafaint Dwarfs. Part 2: Substructure and the Primordial Power Spectrum

As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 13 inbound Pith citation observations for arXiv:2404.01378.

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

pith.paper-citation-record.v1
2404.01378 v2

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measured 0 of 0 reference resolution

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measured 13 of 13 standing notices

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Source: scholarly_work_events, retraction_status_cache, observed 2026-08-07T06:34:17.273281+00:00

measured 13 of 13 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T14:41:49.717879Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-04T18:10:02.043440Z

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Outbound references

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Pith citing papers

Observation 82e50952-8359-434c-b854-23a097f25771 · inbound

Dynamical Evolutions in Globular Clusters and Dwarf Galaxies: Conduction Fluid Simulations cites this paper.

Dynamical Evolutions in Globular Clusters and Dwarf Galaxies: Conduction Fluid Simulations Constraints on Dark Matter from Dynamical Heating of Stars in Ultrafaint Dwarfs. Part 2: Substructure and the Primordial Power Spectrum

Reference 32

Resolution: unresolved; no resolver link, observed 2026-08-07T14:41:49.717879Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 2e1f2174-9057-40c0-acb6-75d476d4ca3c · inbound

Early Growth of Structure in Warm Wave Dark Matter cites this paper.

Early Growth of Structure in Warm Wave Dark Matter Constraints on Dark Matter from Dynamical Heating of Stars in Ultrafaint Dwarfs. Part 2: Substructure and the Primordial Power Spectrum

Reference 70

Resolution: verified exact; arxiv_id, observed 2026-05-19T09:23:03.201492Z

Source-reported events for the cited work

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Observation 7545a01d-760a-4d7e-8e7f-add099cb1247 · inbound

From Fluctuation to Polarization: Imprints of $O(1-10)\, \mathrm{Mpc}^{-1}$ Curvature Perturbations in CMB B-modes from Scalar-Induced Gravitational Waves cites this paper.

From Fluctuation to Polarization: Imprints of $O(1-10)\, \mathrm{Mpc}^{-1}$ Curvature Perturbations in CMB B-modes from Scalar-Induced Gravitational Waves Constraints on Dark Matter from Dynamical Heating of Stars in Ultrafaint Dwarfs. Part 2: Substructure and the Primordial Power Spectrum

Reference 10

Resolution: unresolved; no resolver link, observed 2026-08-06T20:48:08.427577Z

Source-reported events for the cited work

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Observation 8643e7f0-4ee4-4a13-86cc-668823d06d88 · inbound

Not-quite-primordial black holes seeded by cosmic string loops cites this paper.

Not-quite-primordial black holes seeded by cosmic string loops Constraints on Dark Matter from Dynamical Heating of Stars in Ultrafaint Dwarfs. Part 2: Substructure and the Primordial Power Spectrum

Reference 50

Resolution: unresolved; no resolver link, observed 2026-08-06T14:45:32.884768Z

Source-reported events for the cited work

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Observation 0a4a9c72-e1a9-4e0e-8c8a-c6e79432d736 · inbound

Growth of Structure in Multi-species Wave Dark Matter cites this paper.

Growth of Structure in Multi-species Wave Dark Matter Constraints on Dark Matter from Dynamical Heating of Stars in Ultrafaint Dwarfs. Part 2: Substructure and the Primordial Power Spectrum

Reference 97

Resolution: verified exact; arxiv_id, observed 2026-05-21T21:00:37.851302Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation 2b7cb4d5-f21b-45c3-9cd9-038dc09b800f · inbound

Isocurvature Induced Gravitational Waves at Pulsar Timing Arrays cites this paper.

Isocurvature Induced Gravitational Waves at Pulsar Timing Arrays Constraints on Dark Matter from Dynamical Heating of Stars in Ultrafaint Dwarfs. Part 2: Substructure and the Primordial Power Spectrum

Reference 55

Resolution: verified exact; arxiv_id, observed 2026-05-17T00:38:45.147335Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation c4112e30-71d8-46db-81f2-b58e9e4d119c · inbound

Across the Universe: GW231123 as a magnified and diffracted black hole merger cites this paper.

Across the Universe: GW231123 as a magnified and diffracted black hole merger Constraints on Dark Matter from Dynamical Heating of Stars in Ultrafaint Dwarfs. Part 2: Substructure and the Primordial Power Spectrum

Reference 131

Resolution: unresolved; no resolver link, observed 2026-08-03T15:22:26.575496Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a6165958-7965-4e8a-a929-49428a653ead · inbound

New Isocurvature Constraints from JWST UV Luminosity Function cites this paper.

New Isocurvature Constraints from JWST UV Luminosity Function Constraints on Dark Matter from Dynamical Heating of Stars in Ultrafaint Dwarfs. Part 2: Substructure and the Primordial Power Spectrum

Reference 66

Resolution: verified exact; arxiv_id, observed 2026-05-13T01:22:01.979983Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation 249fceb1-4d2a-4a17-bace-5d3699586b83 · inbound

Majoron Dark Matter, High-Scale Seesaw, and Leptogenesis cites this paper.

Majoron Dark Matter, High-Scale Seesaw, and Leptogenesis Constraints on Dark Matter from Dynamical Heating of Stars in Ultrafaint Dwarfs. Part 2: Substructure and the Primordial Power Spectrum

Reference 161

Resolution: verified exact; arxiv_id, observed 2026-07-02T00:26:24.398495Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation cb6504df-108e-4003-9687-3b0471249184 · inbound

Projecting the ultimate pulsar timing sensitivity to dark matter substructure in a stochastic gravitational wave background cites this paper.

Projecting the ultimate pulsar timing sensitivity to dark matter substructure in a stochastic gravitational wave background Constraints on Dark Matter from Dynamical Heating of Stars in Ultrafaint Dwarfs. Part 2: Substructure and the Primordial Power Spectrum

Reference 27

Resolution: metadata mismatch; arxiv_id, observed 2026-07-03T22:49:03.232440Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation 052f5b6c-74ee-4c8b-8734-c092736c4d20 · inbound

Probing Confining Dark Sectors with Cosmological Perturbations cites this paper.

Probing Confining Dark Sectors with Cosmological Perturbations Constraints on Dark Matter from Dynamical Heating of Stars in Ultrafaint Dwarfs. Part 2: Substructure and the Primordial Power Spectrum

Reference 65

Resolution: verified exact; arxiv_id, observed 2026-07-04T18:10:02.045239Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation 4aeb40a8-3e82-4e25-a174-d7553107b6fe · inbound

Probing Confining Dark Sectors with Cosmological Perturbations cites this paper.

Probing Confining Dark Sectors with Cosmological Perturbations Constraints on Dark Matter from Dynamical Heating of Stars in Ultrafaint Dwarfs. Part 2: Substructure and the Primordial Power Spectrum

Reference 65

Resolution: unresolved; no resolver link, observed 2026-07-12T12:25:43.531687Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 3ee21bb0-e97a-4288-b43f-9cfbdef313ac · inbound

Wide binaries in ultra-faint dwarf galaxies as a probe of extended dark objects cites this paper.

Wide binaries in ultra-faint dwarf galaxies as a probe of extended dark objects Constraints on Dark Matter from Dynamical Heating of Stars in Ultrafaint Dwarfs. Part 2: Substructure and the Primordial Power Spectrum

Reference 24

Resolution: unresolved; no resolver link, observed 2026-08-01T15:56:18.756378Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.