Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
As of 17 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2205.03420.
A citation records a reference. It does not transfer a finding from one paper to another.
Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-17T06:30:58.91139+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-06T21:26:00.477686Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-05T02:28:24.338817Z
0 of 0 outbound references displayed
External citation measurements
27
pith, observed 2026-08-05T02:28:24.338817Z
No outbound reference observations are available for this paper version.
Observation d6eabf66-9996-413c-a705-37ee0e043c80 · inbound
The Density Profile of Dynamical Halos A dynamics-based density profile for dark haloes -- II. Fitting function
Reference 16
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 09c16e2d-f98b-450f-ac20-a4672029aa2b · inbound
S-PLUS Clusters And Large-scale Environments (SCALE): I. A catalog of known clusters and groups in DR5 and a pilot study of Abell 4038 A dynamics-based density profile for dark haloes -- II. Fitting function
Reference 70
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.
Observation 668db66e-8662-4122-afaa-75839b6cec50 · inbound
Anisotropic Secondary Bias of Dark Matter Haloes in a $\Lambda$CDM Universe A dynamics-based density profile for dark haloes -- II. Fitting function
Reference 121
Source-reported events for the cited work
Unavailable: canonical work link unavailable.