Pith. sign in

Paper Citation Record · LEDGER

The origin of the red sequence galaxy population in the EAGLE simulation

As of 17 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1810.07189.

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

pith.paper-citation-record.v1
1810.07189 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 2026-08-17T06:30:58.91139+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-16T04:13:34.284882Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-06-26T20:09:57.402945Z

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 60aa0e9f-1ff5-4ffb-a0e7-7fa96da8cd6a · inbound

Mapping Nearby Galaxies with Apache Point Observatory: Group and field galaxies' morphologies in the colour-magnitude plane cites this paper.

Mapping Nearby Galaxies with Apache Point Observatory: Group and field galaxies' morphologies in the colour-magnitude plane The origin of the red sequence galaxy population in the EAGLE simulation

Reference 10

Resolution
unresolved
no resolver link, observed 2026-08-16T04:13:34.284882Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-16T04:13:34.284882Z digest=sha256:a7cda399ea816c656daa92bdc7bc75db9d4f7ef34e2f0c20fb84630a232c64ad

Observation 15632660-87eb-4edd-847a-7d6968931f51 · inbound

On the later evolution of observationally selected protocluster candidates at $z\,{\gtrsim}\,5$ cites this paper.

On the later evolution of observationally selected protocluster candidates at $z\,{\gtrsim}\,5$ The origin of the red sequence galaxy population in the EAGLE simulation

Reference 249

Resolution
verified exact
local_arxiv, observed 2026-06-26T20:09:57.404149Z

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=2026-07-11T11:50:26.030339Z digest=sha256:52d0662d56141cfa7289b08331491e35c269086223a493502486087206923e1b

Observation ea920e3b-4f1c-4c9c-b3d0-797a2e3f3f42 · inbound

The chemodynamical signature of coherent metal-poor inflow and enriched recycled accretion in the cool circumgalactic medium cites this paper.

The chemodynamical signature of coherent metal-poor inflow and enriched recycled accretion in the cool circumgalactic medium The origin of the red sequence galaxy population in the EAGLE simulation

Reference 100

Resolution
unresolved
no resolver link, observed 2026-08-02T02:22:48.000934Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T02:22:48.000934Z digest=sha256:b6b25b329fc33b8495ae72882bdce957cd84d91c4869111149d196af790a2e64