Pith. sign in

Paper Citation Record · LEDGER

A Hierarchy of Normalizing Flows for Modelling the Galaxy-Halo Relationship

As of 19 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2307.06967.

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

pith.paper-citation-record.v1
2307.06967 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 3 of 3 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-19T06:32:44.657259+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-05T14:37:46.412717Z

measured 1 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-08-05T02:28:24.338817Z

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
  • unresolved0
  • parse uncertain0
  • malformed identifier0
  • metadata mismatch0

External citation measurements

6
arxiv_reference, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation a638b0fc-a995-4058-80b9-4a97b21308e3 · inbound

How does feedback affect the star formation histories of galaxies? cites this paper.

How does feedback affect the star formation histories of galaxies? A Hierarchy of Normalizing Flows for Modelling the Galaxy-Halo Relationship

Reference 100

Resolution
unresolved
no resolver link, observed 2026-08-05T14:37:46.412717Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-05T14:37:46.412717Z digest=sha256:d03d6cbf82dbb903821259907115cbb8a81fb485585c73fd216223e35b161a3f

Observation 9363cf63-2e57-45e3-97ae-4e86a0a46e94 · inbound

Efficiently emulating distribution functions in gigaparsec volumes for varying cosmological parameters cites this paper.

Efficiently emulating distribution functions in gigaparsec volumes for varying cosmological parameters A Hierarchy of Normalizing Flows for Modelling the Galaxy-Halo Relationship

Reference 37

Resolution
verified exact
arxiv_id, observed 2026-05-10T04:25:06.336941Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

source=arxiv_source observed=2026-05-10T04:20:49.944504Z digest=sha256:2907751b0bbb9a4ca6ae07dfaa79736cc910cc5eda387b8c6c84511924213c8f

Observation d6e7f003-13fc-42eb-9c93-f4bb3dd65737 · inbound

From Dark Matter to Galaxies: Halo-Free Mock Generation via Conditional Point-Cloud Diffusion cites this paper.

From Dark Matter to Galaxies: Halo-Free Mock Generation via Conditional Point-Cloud Diffusion A Hierarchy of Normalizing Flows for Modelling the Galaxy-Halo Relationship

Reference 20

Resolution
unresolved
no resolver link, observed 2026-08-01T11:43:20.785434Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T11:43:20.785434Z digest=sha256:a0609ef47800c4cc732c27d10371bb295e588bc86d97455af982e6605c1fc2a6