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Paper Citation Record · LEDGER

A model for core formation in dark matter haloes and ultra diffuse galaxies by outflow episodes

As of 21 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1907.11726.

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

pith.paper-citation-record.v1
1907.11726 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 2026-08-21T06:32:19.484+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-14T11:36:26.544225Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-08-04T22:14:32.667952Z

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 76b11311-57de-4bbe-aad7-a8fd35c172c8 · inbound

The effect of fluctuating fuzzy axion haloes on stellar dynamics: a stochastic model cites this paper.

The effect of fluctuating fuzzy axion haloes on stellar dynamics: a stochastic model A model for core formation in dark matter haloes and ultra diffuse galaxies by outflow episodes

Reference 35

Resolution
unresolved
no resolver link, observed 2026-08-14T11:36:26.544225Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T11:36:26.544225Z digest=sha256:4edeea48c7aa41235993d64229cb39eab85ba715b68b23981b0e96bb97978346

Observation f2e56460-4cf3-4b43-bb7a-a5369916bb31 · inbound

Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps cites this paper.

Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps A model for core formation in dark matter haloes and ultra diffuse galaxies by outflow episodes

Reference 92

Resolution
verified exact
local_arxiv, observed 2026-08-04T22:14:32.765825Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

source=pdf_text observed=2026-08-04T22:14:29.546955Z digest=sha256:c3452a485e161e31937bd552c4083db8357240a834235fb45df45888573aa2e5