Pith. sign in

Paper Citation Record · LEDGER

Galaxy Groups

As of 17 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1411.1511.

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

pith.paper-citation-record.v1
1411.1511 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 2 of 2 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-17T06:30:58.91139+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-01T23:43:54.472285Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-14T04:10:13.611841Z

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 db461068-74e1-4a8e-b76a-4bbad38d07cc · inbound

New optical velocities for local galaxy candidates cites this paper.

New optical velocities for local galaxy candidates Galaxy Groups

Reference 12

Resolution
verified exact
local_arxiv, observed 2026-07-14T04:10:13.613524Z

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.

source=arxiv_source observed=2026-07-14T04:03:16.335097Z digest=sha256:1a3f75c5a3871c9017011d4cf02f90c6ee3e44aa9420cda270db98726e546e02

Observation 31e104a6-9afb-4a29-8e94-67b00172a3a3 · inbound

Tighter Dark Matter Constraints from the Projected Mass Method: A Neural Network Enhanced Method for Galaxy Groups and Clusters cites this paper.

Tighter Dark Matter Constraints from the Projected Mass Method: A Neural Network Enhanced Method for Galaxy Groups and Clusters Galaxy Groups

Reference 4

Resolution
unresolved
no resolver link, observed 2026-08-01T23:43:54.472285Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T23:43:54.472285Z digest=sha256:7df25e48d9df8a819c013bb71ac7837b76d1c92e5e55dba24a983b2e49967df6