Pith. sign in

Paper Citation Record · LEDGER

Large-scale dark matter simulations

As of 9 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 18 inbound Pith citation observations for arXiv:2112.05165.

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

pith.paper-citation-record.v1
2112.05165 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 18 of 18 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-09T06:31:02.800959+00:00

measured 18 of 18 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-09T11:48:21.571730Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-01T20:16:11.531407Z

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 d13538e9-aab0-4966-9e7f-b08ee7a20dee · inbound

Primordial Sharp Features through the Nonlinear Regime of Structure Formation cites this paper.

Primordial Sharp Features through the Nonlinear Regime of Structure Formation Large-scale dark matter simulations

Reference 158

Resolution
malformed identifier
no resolver link, observed 2026-08-09T11:48:21.571730Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-09T11:48:21.571730Z digest=sha256:00c085830433f450c5ce055736dd273e7be0c0ebd36fe4f22b3f5031ccc560c2

Observation 126e7b89-b379-49d0-9086-1856394266f5 · inbound

Perturbative Likelihoods for Large-Scale Structure of the Universe cites this paper.

Perturbative Likelihoods for Large-Scale Structure of the Universe Large-scale dark matter simulations

Reference 7

Resolution
unresolved
no resolver link, observed 2026-08-07T12:48:14.242733Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T12:48:14.242733Z digest=sha256:8d96926e84f6c90953bd55edbe68129f813a4d491faaa2a1771bd5651829c87d

Observation 099f8cd3-c993-4cd9-8a6c-9bd70097ea26 · inbound

Exploring the halo occupation distribution for moderate X-ray luminosity active galactic nuclei in the EAGLE cosmological simulation cites this paper.

Exploring the halo occupation distribution for moderate X-ray luminosity active galactic nuclei in the EAGLE cosmological simulation Large-scale dark matter simulations

Reference 34

Resolution
unresolved
no resolver link, observed 2026-08-07T10:26:30.740142Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T10:26:30.740142Z digest=sha256:6192fd5ba4e0dc51fd191b675ce691c57a31b3cb90eb2163fea6b54ee338f969

Observation ce7bde4b-3f85-401e-8482-910d6f77fcd8 · inbound

CSST Cosmological Emulator II: Generalized Accurate Halo Mass Function Emulation cites this paper.

CSST Cosmological Emulator II: Generalized Accurate Halo Mass Function Emulation Large-scale dark matter simulations

Reference 53

Resolution
unresolved
no resolver link, observed 2026-08-07T04:48:07.648048Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T04:48:07.648048Z digest=sha256:cd6a4e96ed8bf1c18a6998dd8a86d77044fd3955eaff63ab0b94879f4451ca68

Observation a1eb5721-4524-496e-a943-88aab0989d8a · inbound

Generating Moving Field Initial Conditions with Spatially Varying Boost cites this paper.

Generating Moving Field Initial Conditions with Spatially Varying Boost Large-scale dark matter simulations

Reference 22

Resolution
unresolved
no resolver link, observed 2026-08-06T22:01:31.960107Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T22:01:31.960107Z digest=sha256:145d09879a126ecb7f69e5494f022bb26ff0e4dc058ad28cccefe561dfc30f00

Observation a743124b-c5fb-4e05-a584-884771676991 · inbound

Cosmological Simulations of Galaxies cites this paper.

Cosmological Simulations of Galaxies Large-scale dark matter simulations

Reference 15

Resolution
unresolved
no resolver link, observed 2026-08-06T18:15:55.343499Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-06T18:15:55.343499Z digest=sha256:ff81b1bb6265747d47cec530f9b382e6ea4797544b90ca9f69fd863c12cd1507

Observation d87dc8c5-8dab-4a59-82eb-ad9797393f64 · inbound

Artifacts in Halo Shapes: Imprints of the Initial Condition cites this paper.

Artifacts in Halo Shapes: Imprints of the Initial Condition Large-scale dark matter simulations

Reference 7

Resolution
unresolved
no resolver link, observed 2026-08-06T15:06:52.627718Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T15:06:52.627718Z digest=sha256:bdeee0ac4d3728897dc58ad1839bd026906ed16314b40b86952b77c49c07b7be

Observation 9eccccbd-7c18-454b-b2f2-38ecb8695464 · inbound

DISCO-DJ II: a differentiable particle-mesh code for cosmology cites this paper.

DISCO-DJ II: a differentiable particle-mesh code for cosmology Large-scale dark matter simulations

Reference 56

Resolution
unresolved
no resolver link, observed 2026-08-04T11:25:29.846185Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-04T11:25:29.846185Z digest=sha256:2d1e4ba96112034c481007954b643b2742e1e332036d39644f92f7130b1e64d7

Observation 9aec3528-2616-4c95-b8cf-77ffdea8b412 · inbound

Extending CSST Emulator to post-DESI era cites this paper.

Extending CSST Emulator to post-DESI era Large-scale dark matter simulations

Reference 28

Resolution
unresolved
no resolver link, observed 2026-08-04T10:39:31.669164Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-04T10:39:31.669164Z digest=sha256:5b2556e2f6daab1073f46d71025f8fe1828bb19972ab9214ca64140344263441

Observation 2375ea8a-2b9f-4344-9039-554e976fd3a8 · inbound

Field-level multi-tracers simulation-based inference of cosmological parameters from 3D maps cites this paper.

Field-level multi-tracers simulation-based inference of cosmological parameters from 3D maps Large-scale dark matter simulations

Reference 18

Resolution
verified exact
arxiv_id, observed 2026-07-01T16:45:51.803982Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

source=pdf_text observed=2026-06-29T20:14:12.879470Z digest=sha256:0313a26f961a55ce7de763de9563cf931d6d1127cdc47bffc4ee4cb10eae226c

Observation 9a97d9d3-c489-402d-97f1-6b7b271d2e43 · inbound

(The) Wiggles going non-linear cites this paper.

(The) Wiggles going non-linear Large-scale dark matter simulations

Reference 29

Resolution
verified exact
arxiv_id, observed 2026-07-01T20:16:11.533567Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

source=pdf_text observed=2026-06-28T21:29:32.587896Z digest=sha256:da832ae8992c17f39ef264c016e972bef19499968d2420e26bb4f90b8eb36408

Observation c0e4358b-20d2-41f1-b759-2fba9907cc63 · inbound

(The) Wiggles going non-linear cites this paper.

(The) Wiggles going non-linear Large-scale dark matter simulations

Reference 29

Resolution
verified exact
arxiv_id, observed 2026-07-01T07:55:31.870786Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

source=pdf_text observed=2026-07-01T07:43:18.262396Z digest=sha256:a4c041a1e3bf741f30174bb9b8cee86c3148ec1ed450365ad7505d0918d7e495

Observation ce6521fa-e5d6-483e-8d51-0ea77f07b10f · inbound

Disentangling modified gravity and galaxy bias with field-level inference cites this paper.

Disentangling modified gravity and galaxy bias with field-level inference Large-scale dark matter simulations

Reference 128

Resolution
unresolved
no resolver link, observed 2026-07-12T01:57:41.636527Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-12T01:57:41.636527Z digest=sha256:d8052325e8dcc164d4aeb3dc8d5e44a64cf6b8b7001d65ccf37dbb427910eaae

Observation 090ea000-de53-4b9a-971a-bf78d0e1c17d · inbound

Assessing the large-scale angular clustering of UNIONS Lyman Break Galaxies via cross-correlations cites this paper.

Assessing the large-scale angular clustering of UNIONS Lyman Break Galaxies via cross-correlations Large-scale dark matter simulations

Reference 52

Resolution
unresolved
no resolver link, observed 2026-07-14T14:25:37.540627Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-14T14:25:37.540627Z digest=sha256:4e6a914718c71254ab5b9776e415f9370661098e6f7b74be1cfc9699fa06983a

Observation 5ef76f85-ee3c-4df6-bf3e-3ba332955d50 · inbound

Assessing the large-scale angular clustering of UNIONS Lyman Break Galaxies via cross-correlations cites this paper.

Assessing the large-scale angular clustering of UNIONS Lyman Break Galaxies via cross-correlations Large-scale dark matter simulations

Reference 52

Resolution
unresolved
no resolver link, observed 2026-08-02T07:32:44.273807Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T07:32:44.273807Z digest=sha256:18f578e63f6cc80f68e4b1bf146eeee34b1722188f39d5f7d7427b995933604f

Observation 75c7111e-9e98-4f31-ae9b-592e9ffe52f6 · inbound

Evaluating the flexibility of the MillenniumTNG galaxy formation model with multi-zoom re-simulations cites this paper.

Evaluating the flexibility of the MillenniumTNG galaxy formation model with multi-zoom re-simulations Large-scale dark matter simulations

Reference 92

Resolution
unresolved
no resolver link, observed 2026-08-02T06:10:49.058874Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T06:10:49.058874Z digest=sha256:d0e170b72c6839f2109ce936dd89550430abb0ae75f67d923d4cb0895b0ee6ea

Observation 2de83f88-b93c-401b-9f33-8d04b04fafad · 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 Large-scale dark matter simulations

Reference 182

Resolution
unresolved
no resolver link, observed 2026-07-31T05:29:30.240378Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-31T05:29:30.240378Z digest=sha256:b8d8190a19798ee48b5423785eb889e36ea7890dbe8e888de13a3389a09f697d

Observation ac586021-3cdb-4448-a629-08921a6f99ef · inbound

Cosmic Velocity Flows: from Theory to Observations cites this paper.

Cosmic Velocity Flows: from Theory to Observations Large-scale dark matter simulations

Reference 188

Resolution
unresolved
no resolver link, observed 2026-08-05T17:19:49.348821Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-05T17:19:49.348821Z digest=sha256:56afa7e63c4fe410ad560fbe21e20e21d8a2e5d99440bf364695ea91cddf232d