Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
$\texttt{StreamSculptor}$: Hamiltonian Perturbation Theory for Stellar Streams in Flexible Potentials with Differentiable Simulations
As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2410.21174.
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 2026-08-10T06:31:04.303077+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-09T00:16:28.639991Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-07-03T02:17:35.328443Z
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 556a68b2-a0c2-4c6d-9fb7-c7de17bb4f47 · inbound
Gaps in stellar streams as a result of globular cluster fly-bys cites this paper.
Gaps in stellar streams as a result of globular cluster fly-bys $\texttt{StreamSculptor}$: Hamiltonian Perturbation Theory for Stellar Streams in Flexible Potentials with Differentiable Simulations
Reference 84
- Resolution
- unresolved
- no resolver link, observed 2026-08-09T00:16:28.639991Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation a9b250df-7821-498f-b58d-69af0a4caabc · inbound
A differentiable forward model for weakly perturbed stellar streams: substructure forecasts from density and kinematics spectra cites this paper.
A differentiable forward model for weakly perturbed stellar streams: substructure forecasts from density and kinematics spectra $\texttt{StreamSculptor}$: Hamiltonian Perturbation Theory for Stellar Streams in Flexible Potentials with Differentiable Simulations
Reference 33
- Resolution
- verified exact
- arxiv_id, observed 2026-07-03T02:17:35.329908Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.