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Paper Citation Record · LEDGER

Dark Matter Cores and Cusps in Spiral Galaxies and their Explanations

As of 18 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:1911.00544.

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

pith.paper-citation-record.v1
1911.00544 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 2026-08-18T06:34:40.430872+00:00

measured 5 of 5 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-08T23:34:35.127190Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-03T06:57:42.756883Z

Reference resolution

0 of 0 outbound references displayed

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

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 6c51ed7e-3b35-424b-b09e-d8e6ba6bf199 · inbound

Can a secluded self-interacting dark sector generate detectable gravitational waves? cites this paper.

Can a secluded self-interacting dark sector generate detectable gravitational waves? Dark Matter Cores and Cusps in Spiral Galaxies and their Explanations

Reference 125

Resolution
unresolved
no resolver link, observed 2026-08-08T23:34:35.127190Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-08T23:34:35.127190Z digest=sha256:53324eab75a69a712c5f6ccec5048ba445bbd053a81d98c3071a487e3b0613f8

Observation d788ade0-b671-4939-8c77-cebd7d0e221b · inbound

Non-Equilibrium Relativistic Core Collapse of Self-Interacting Dark Matter Halos -- Limits On Seed Black Hole Mass cites this paper.

Non-Equilibrium Relativistic Core Collapse of Self-Interacting Dark Matter Halos -- Limits On Seed Black Hole Mass Dark Matter Cores and Cusps in Spiral Galaxies and their Explanations

Reference 133

Resolution
verified exact
arxiv_id, observed 2026-05-16T11:37:48.998711Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=pdf_text observed=2026-05-16T11:34:12.521105Z digest=sha256:7b751a215f6e1484365c66cb4741583c32c19af3e5a00ba147d4da5d77a1828f

Observation 2cd2bf91-cbce-40f7-9a65-7420d6c457cd · inbound

MARVELously Dark: the density profile evolution of dwarf halos in velocity-dependent SIDM cites this paper.

MARVELously Dark: the density profile evolution of dwarf halos in velocity-dependent SIDM Dark Matter Cores and Cusps in Spiral Galaxies and their Explanations

Reference 87

Resolution
unresolved
no resolver link, observed 2026-08-03T06:13:38.365063Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-03T06:13:38.365063Z digest=sha256:d38c82b3b592f68fd1b3a6185311e7870d8e32e0a6468fa4b8824b213cbdf3cc

Observation 503c364e-acae-408b-82b6-15611f77ce99 · inbound

Gravothermal Collapse: Robust Against Baryonic Feedback cites this paper.

Gravothermal Collapse: Robust Against Baryonic Feedback Dark Matter Cores and Cusps in Spiral Galaxies and their Explanations

Reference 22

Resolution
verified exact
arxiv_id, observed 2026-07-01T20:36:11.572098Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=pdf_text observed=2026-06-28T20:58:05.796638Z digest=sha256:b9de35e4666c6ea4a7fc13259ccec228b357ffc0d87e7e75e128062c59698654

Observation 69e18f6e-587a-41bb-bc0e-19c785644ddc · inbound

Spherically Symmetric Fluid Simulations of Black Hole Accretion in Self-Interacting Dark Matter Halos cites this paper.

Spherically Symmetric Fluid Simulations of Black Hole Accretion in Self-Interacting Dark Matter Halos Dark Matter Cores and Cusps in Spiral Galaxies and their Explanations

Reference 23

Resolution
verified exact
arxiv_id, observed 2026-07-03T06:57:42.758449Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=pdf_text observed=2026-07-03T06:49:14.051341Z digest=sha256:28e19dd8b2fe3bf9240b39dfd707ad24a5762ea064570fd99da7e04c602ec433