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Paper Citation Record · LEDGER

The role of mergers and halo spin in shaping galaxy morphology

As of 17 July 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1609.09498.

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

pith.paper-citation-record.v1
1609.09498 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 2026-07-17T06:31:00.352745+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 2026-06-27T16:11:01.863003Z

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 e3e264fd-30db-4ea5-a1b2-e893383c1f9a · inbound

Bulgeless Evolution And the Rise of Discs (BEARD) I. Physical drivers of the mass-size relation for Milky Way-like galaxies cites this paper.

Bulgeless Evolution And the Rise of Discs (BEARD) I. Physical drivers of the mass-size relation for Milky Way-like galaxies The role of mergers and halo spin in shaping galaxy morphology

Reference 8

Resolution
verified exact
local_arxiv, observed 2026-05-20T08:58:09.932089Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-07-17T06:31:00.352745+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:2c9d2d3208269c1e24531d7d5b986bc7359e7253faeeec99dd832fc507aa6824

Observation 2f15955b-77a3-45dc-9a01-2d5c511f96e0 · inbound

Satellite compaction pathways: environmental drivers shaping dwarf galaxy corpulence in the TNG50 simulation cites this paper.

Satellite compaction pathways: environmental drivers shaping dwarf galaxy corpulence in the TNG50 simulation The role of mergers and halo spin in shaping galaxy morphology

Reference 184

Resolution
verified exact
local_arxiv, observed 2026-06-27T16:11:01.864554Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-07-17T06:31:00.352745+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:9bbd6e82346cf9477c1e439fbe8921148ac276b3495bd813bbc4988ced080df8