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Paper Citation Record · LEDGER

The fraction of dark matter within galaxies from the IllustrisTNG simulations

As of 12 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:1801.10170.

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

pith.paper-citation-record.v1
1801.10170 v3

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 5 of 5 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-12T06:34:41.77262+00:00

measured 5 of 5 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-10T17:17:46.140853Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-06-27T01:00:20.771460Z

Reference resolution

0 of 0 outbound references displayed

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  • verified fuzzy0
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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 c45ec831-58dc-4f80-bf67-7cc9e52add19 · inbound

Introducing the AIDA-TNG project: galaxy formation in alternative dark matter models cites this paper.

Introducing the AIDA-TNG project: galaxy formation in alternative dark matter models The fraction of dark matter within galaxies from the IllustrisTNG simulations

Reference 54

Resolution
unresolved
no resolver link, observed 2026-08-10T17:17:46.140853Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T17:17:46.140853Z digest=sha256:02d48c6f6c770731ebcb3381fbabe86e7849dc51698e2cf4967eefd720363f50

Observation 64bd99ef-dff2-4992-957f-0be5ede247c7 · inbound

Secondary Dependence of Baryonic Effects on the Density Profile of Dark Matter Halos cites this paper.

Secondary Dependence of Baryonic Effects on the Density Profile of Dark Matter Halos The fraction of dark matter within galaxies from the IllustrisTNG simulations

Reference 70

Resolution
verified exact
arxiv_id, observed 2026-05-12T00:41:14.644003Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

source=pdf_text observed=2026-05-07T14:53:02.246257Z digest=sha256:1cf4508c4d6f60d89225eecb20ff6e03d3f63c94c6c43395c8414c514f2ec00d

Observation d93a775d-000a-48d5-bf66-9273519f39f6 · inbound

Probing the Fundamental Nature of Particle Dark Matter cites this paper.

Probing the Fundamental Nature of Particle Dark Matter The fraction of dark matter within galaxies from the IllustrisTNG simulations

Reference 182

Resolution
verified exact
local_arxiv, observed 2026-06-25T21:38:29.538188Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:6fe3868410380566d4bf27d5a0194b5980df87965f4b460f4081bb07131d4612

Observation 91c1462e-2626-4b57-bbce-b986c806a726 · inbound

Columba: isolated dwarf galaxy populations in diverse cosmological environments simulated with a cold interstellar medium cites this paper.

Columba: isolated dwarf galaxy populations in diverse cosmological environments simulated with a cold interstellar medium The fraction of dark matter within galaxies from the IllustrisTNG simulations

Reference 163

Resolution
verified exact
local_arxiv, observed 2026-06-27T01:00:20.772846Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:3bae35d0623d82c81de0e49a7bfef1feec593c888517e671c5121e17b6caab1e

Observation bb32dd7d-9908-4a74-96d4-9e89dde33cc5 · inbound

Primordial Physics in the Nonlinear Universe: Revealing the oscillating halo bias from cosmological collider models cites this paper.

Primordial Physics in the Nonlinear Universe: Revealing the oscillating halo bias from cosmological collider models The fraction of dark matter within galaxies from the IllustrisTNG simulations

Reference 65

Resolution
unresolved
no resolver link, observed 2026-07-31T05:29:29.877850Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-31T05:29:29.877850Z digest=sha256:6ba6b46014ce6830127d3c8be4408f5ac947c3cc1b67f678fbae90cc22f0971b