Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links, observed 2026-08-11T10:29:11.776667Z
Paper Citation Record · LEDGER
Why do galaxies have extended flat rotation curves?
As of 11 August 2026, this Paper Citation Record lists 12 of 12 outbound references and 1 inbound Pith citation observation for arXiv:2412.17869.
A citation records a reference. It does not transfer a finding from one paper to another.
Coverage vector
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-11T06:34:44.6726+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-04T16:47:01.189547Z
A source-named dated measurement, never combined with another source.
Source: cited_works
Reference resolution
12 of 12 outbound references displayed
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- verified fuzzy9
- unresolved3
- parse uncertain0
- malformed identifier0
- metadata mismatch0
External citation measurements
No source-named external measurement is stored.
Outbound references
Observation aeef0044-4461-4fd4-80bd-9ac14ea81910 · outbound
This paper cites Indefinitely Flat Circular Velocities and the Baryonic Tully-Fisher Relation from Weak Lensing.
Why do galaxies have extended flat rotation curves? Indefinitely Flat Circular Velocities and the Baryonic Tully-Fisher Relation from Weak Lensing
Reference 1
- Resolution
- unresolved
- no resolver link, observed 2026-08-11T10:29:11.736451Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 3f02200f-7b77-4f23-ab30-c2d5567ae069 · outbound
This paper cites Dark matter halos of massive elliptical galaxies at $z \sim 0.2$ are well described by the Navarro-Frenk-White profile.
Why do galaxies have extended flat rotation curves? Dark matter halos of massive elliptical galaxies at $z \sim 0.2$ are well described by the Navarro-Frenk-White profile
Reference 2
- Resolution
- unresolved
- no resolver link, observed 2026-08-11T10:29:11.741252Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 661027c0-7e67-4961-850c-259fd33702cc · outbound
This paper cites (2023) Understanding the Formation of Galaxies w ith Warm Dark Matter.
Why do galaxies have extended flat rotation curves? (2023) Understanding the Formation of Galaxies w ith Warm Dark Matter
Reference 3
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-11T10:29:11.941664Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation 6b63b475-90bb-46a6-856c-c22e6e410a8f · outbound
This paper cites (2024) Understanding Elliptical Galaxies with Warm D ark Matter, Physics of the Dark Universe , 46 (2024) 101643.
Why do galaxies have extended flat rotation curves? (2024) Understanding Elliptical Galaxies with Warm D ark Matter, Physics of the Dark Universe , 46 (2024) 101643
Reference 4
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-11T10:29:11.931043Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation 14b03884-639b-41c2-a13a-69fed1e0ee49 · outbound
This paper cites (2019) The Adiabatic Invariant of Dark Matter in S piral Galaxies.
Why do galaxies have extended flat rotation curves? (2019) The Adiabatic Invariant of Dark Matter in S piral Galaxies
Reference 5
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-11T10:29:11.919241Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation 25a909e6-a199-40a5-b448-326354940af9 · outbound
This paper cites (2022) Measurement of the Dark Matter Velocity Disper- sion with Dwarf Galaxy Rotation Curves.
Why do galaxies have extended flat rotation curves? (2022) Measurement of the Dark Matter Velocity Disper- sion with Dwarf Galaxy Rotation Curves
Reference 6
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-11T10:29:11.907987Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation b62680ab-92c9-4094-9fe9-c0d01938c902 · outbound
This paper cites (2024) Measurements of the Dark Matter Mass, Tempera- ture and Spin.
Why do galaxies have extended flat rotation curves? (2024) Measurements of the Dark Matter Mass, Tempera- ture and Spin
Reference 7
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-11T10:29:11.895972Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation e98a8e00-7729-49bf-9d11-043af84377e3 · outbound
This paper cites and Schechter, P.
Why do galaxies have extended flat rotation curves? and Schechter, P
Reference 8
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-11T10:29:11.883891Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation c8086386-401b-44a0-8696-9bb6a35195c3 · outbound
This paper cites (2024) Are James Webb Space Telescope Observa tions Consistent with Warm Dark Matter? International Journal of Astron- omy and Astrophysics , 14, 45-60.
Why do galaxies have extended flat rotation curves? (2024) Are James Webb Space Telescope Observa tions Consistent with Warm Dark Matter? International Journal of Astron- omy and Astrophysics , 14, 45-60
Reference 9
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-11T10:29:11.872022Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation 4bd1040b-b0d0-4431-abf9-8094f7069e46 · outbound
This paper cites (2022) Measurement of the Dark Matter Velocit y Dis- persion with Galaxy Stellar Masses, UV Luminosities, and Reionization.
Why do galaxies have extended flat rotation curves? (2022) Measurement of the Dark Matter Velocit y Dis- persion with Galaxy Stellar Masses, UV Luminosities, and Reionization
Reference 10
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-11T10:29:11.859513Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation a0b4e099-6cf3-45ab-be2f-0c28da3845e9 · outbound
This paper cites an unresolved cited work.
Why do galaxies have extended flat rotation curves? Unresolved cited work
Reference 11
- Resolution
- unresolved
- raw_fallback, observed 2026-08-11T10:29:11.847614Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation 85ea2211-049e-4c37-b08c-245a540a4ca9 · outbound
This paper cites (2001) Ellipsoidal collapse and an improved model for the number and spatial distribution of dark mat ter haloes, Mon.
Why do galaxies have extended flat rotation curves? (2001) Ellipsoidal collapse and an improved model for the number and spatial distribution of dark mat ter haloes, Mon
Reference 12
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-11T10:29:11.835412Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Pith citing papers
Observation 39209d64-a73b-4574-b187-d1a79069b1e5 · inbound
Testing CCC+TL Cosmology with Galaxy Rotation Curves cites this paper.
Testing CCC+TL Cosmology with Galaxy Rotation Curves Why do galaxies have extended flat rotation curves?
Reference 51
- Resolution
- unresolved
- no resolver link, observed 2026-08-04T16:47:01.189547Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.