Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
The Causes of Halo Shape Changes Induced by Cooling Baryons: Disks Versus Substructures
As of 18 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:0707.0737.
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 2026-08-18T06:34:40.430872+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-11T04:27:08.459192Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-07-01T11:05:42.053052Z
Reference resolution
0 of 0 outbound references displayed
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- 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 d98edaf0-d8dc-4a65-b4a4-0022bad59ae5 · inbound
Variable gravitational potential of Milky Way analogues in HESTIA suite cites this paper.
Variable gravitational potential of Milky Way analogues in HESTIA suite The Causes of Halo Shape Changes Induced by Cooling Baryons: Disks Versus Substructures
Reference 1088
- Resolution
- unresolved
- no resolver link, observed 2026-08-11T04:27:08.459192Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation d0a66191-ddaf-4043-8b4a-699513f01c22 · inbound
Unveiling the properties of galaxy cores excavated by supermassive black hole binaries with SHARP cites this paper.
Unveiling the properties of galaxy cores excavated by supermassive black hole binaries with SHARP The Causes of Halo Shape Changes Induced by Cooling Baryons: Disks Versus Substructures
Reference 99
- Resolution
- metadata mismatch
- local_arxiv, observed 2026-07-01T11:05:42.054465Z
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.
Observation c4d07668-ef99-4ae9-96f8-6b0c9ea22c60 · inbound
Constraints on the population level distribution of nearby Dark Matter halo shapes with extragalactic streams cites this paper.
Constraints on the population level distribution of nearby Dark Matter halo shapes with extragalactic streams The Causes of Halo Shape Changes Induced by Cooling Baryons: Disks Versus Substructures
Reference 161
- Resolution
- unresolved
- no resolver link, observed 2026-07-11T06:35:48.157333Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.