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Paper Citation Record · LEDGER

Galaxy spin alignment in filaments and sheets: observational evidence

As of 5 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1308.2816.

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

pith.paper-citation-record.v1
1308.2816 v2

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 2026-08-05T06:32:48.257954+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-07-11T11:50:26.030339Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-06-26T20:39:57.006068Z

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
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  • 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 d8fcf8c6-78cb-4c2c-9236-8fe9f0ac12b3 · inbound

IllustrisTNG50 angular momentum maps: tracing the morpho-kinematic evolution of galaxies cites this paper.

IllustrisTNG50 angular momentum maps: tracing the morpho-kinematic evolution of galaxies Galaxy spin alignment in filaments and sheets: observational evidence

Reference 31

Resolution
verified exact
local_arxiv, observed 2026-06-26T20:39:57.007341Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:9ee6613a428319107eb9bec33dec7136f5b37985a52e9f41fcaca4d7c0249d73

Observation a5b94c76-c691-48bc-bbb2-1add5f408d34 · 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 Galaxy spin alignment in filaments and sheets: observational evidence

Reference 139

Resolution
unresolved
no resolver link, observed 2026-07-11T06:35:48.157333Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-11T06:35:48.157333Z digest=sha256:e80707c819104d1f08d6fb511894e757a2ad0b1b573b251a67704d9ac663706c