Paper Citation Record · LEDGER

Cosmological Hydrodynamics with Adaptive Mesh Refinement: a new high resolution code called RAMSES

As of 17 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 24 inbound Pith citation observations for arXiv:astro-ph/0111367.

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

pith.paper-citation-record.v1
astro-ph/0111367 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 24 of 24 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 24 of 24 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-15T14:38:14.433794Z

measured 1 of 1 external citation measurements

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

Source: pith, observed 2026-08-05T02:28:24.338817Z

Reference resolution

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External citation measurements

1094
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 078b5811-124c-4f5b-be10-505114fbfe22 · inbound

Theoretical Predictions for the Inner Dark Matter Distribution in the Milky Way Informed by Simulations cites this paper.

Theoretical Predictions for the Inner Dark Matter Distribution in the Milky Way Informed by Simulations Cosmological Hydrodynamics with Adaptive Mesh Refinement: a new high resolution code called RAMSES

Reference 98

Resolution: unresolved; no resolver link, observed 2026-08-10T14:57:14.356922Z

Source-reported events for the cited work

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Observation 905fb0c1-5c02-436b-9b57-176421d55ac9 · inbound

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

Perturbative Likelihoods for Large-Scale Structure of the Universe Cosmological Hydrodynamics with Adaptive Mesh Refinement: a new high resolution code called RAMSES

Reference 11

Resolution: unresolved; no resolver link, observed 2026-08-07T12:48:14.631790Z

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Observation 297c5f8e-6705-4a78-b0b8-24c7540cd832 · inbound

Cosmological Simulations of Galaxies cites this paper.

Cosmological Simulations of Galaxies Cosmological Hydrodynamics with Adaptive Mesh Refinement: a new high resolution code called RAMSES

Reference 296

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Observation c61627ae-b7ee-4a1d-945e-9882ae53e971 · 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 Cosmological Hydrodynamics with Adaptive Mesh Refinement: a new high resolution code called RAMSES

Reference 54

Resolution: unresolved; no resolver link, observed 2026-08-04T22:14:26.376812Z

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Observation 6e40a207-a976-42a5-b7c7-78e8255a2559 · 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 Cosmological Hydrodynamics with Adaptive Mesh Refinement: a new high resolution code called RAMSES

Reference 12

Resolution: verified exact; arxiv_id, observed 2026-05-12T00:36:17.772517Z

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.

Observation c349bccf-6963-4d57-ace1-1e9dd07f5b2b · inbound

One Merge to Rule Them All: From Galaxy Interactions to Black Hole Mergers Using Horizon-AGN cites this paper.

One Merge to Rule Them All: From Galaxy Interactions to Black Hole Mergers Using Horizon-AGN Cosmological Hydrodynamics with Adaptive Mesh Refinement: a new high resolution code called RAMSES

Reference 52

Resolution: metadata mismatch; local_arxiv, observed 2026-05-14T20:47:57.323971Z

Source-reported events for the cited work

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Observation 31dfeff7-62f9-4757-96de-ffc9ea0d09d2 · inbound

NOEMA$^\rm{3D}$: A deep view of cold gas flows in a barred spiral galaxy at $z\sim1$ cites this paper.

NOEMA$^\rm{3D}$: A deep view of cold gas flows in a barred spiral galaxy at $z\sim1$ Cosmological Hydrodynamics with Adaptive Mesh Refinement: a new high resolution code called RAMSES

Reference 230

Resolution: metadata mismatch; local_arxiv, observed 2026-06-28T13:42:15.535404Z

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.

Observation f76207e4-74d6-4dda-a710-a1a723f57219 · inbound

Biased tracers, Hybrid Effective Field Theory and Modified Gravity cites this paper.

Biased tracers, Hybrid Effective Field Theory and Modified Gravity Cosmological Hydrodynamics with Adaptive Mesh Refinement: a new high resolution code called RAMSES

Reference 70

Resolution: verified exact; local_arxiv, observed 2026-07-02T05:16:39.043294Z

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.

Observation 725948bb-c39e-40c8-939a-19963e7e6ef7 · inbound

Virial-based extraction of structures in numerical simulations: The vibes tool cites this paper.

Virial-based extraction of structures in numerical simulations: The vibes tool Cosmological Hydrodynamics with Adaptive Mesh Refinement: a new high resolution code called RAMSES

Reference 48

Resolution: metadata mismatch; local_arxiv, observed 2026-06-27T18:11:07.635263Z

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.

Observation 2b714267-d0ad-4b6f-91d6-f56f713365f8 · inbound

Virial-based extraction of structures in numerical simulations: The vibes tool cites this paper.

Virial-based extraction of structures in numerical simulations: The vibes tool Cosmological Hydrodynamics with Adaptive Mesh Refinement: a new high resolution code called RAMSES

Reference 48

Resolution: metadata mismatch; local_arxiv, observed 2026-07-04T00:09:13.765266Z

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.

Observation b36a7d4f-07f0-4f99-a5b8-0b640d9c59e7 · inbound

Non-linear Structure Formation in Planck+DESI Favoured Interacting Dark Energy Cosmologies cites this paper.

Non-linear Structure Formation in Planck+DESI Favoured Interacting Dark Energy Cosmologies Cosmological Hydrodynamics with Adaptive Mesh Refinement: a new high resolution code called RAMSES

Reference 97

Resolution: verified exact; local_arxiv, observed 2026-07-03T07:47:45.304042Z

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.

Observation 9356a440-31b1-465a-8f17-6e7a6e50c9e2 · inbound

Galaxy formation in modified gravity -- II. galaxy halo connection and assembly bias cites this paper.

Galaxy formation in modified gravity -- II. galaxy halo connection and assembly bias Cosmological Hydrodynamics with Adaptive Mesh Refinement: a new high resolution code called RAMSES

Reference 43

Resolution: metadata mismatch; local_arxiv, observed 2026-07-03T13:18:12.393547Z

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.

Observation 20927f3d-8e80-4bb0-bc3f-e81d5db96390 · inbound

Variability in Cosmological Hydrodynamical Simulations: how Stochastic Processes, Numerical Effects, and Reproducibility Limits impact Predictability cites this paper.

Variability in Cosmological Hydrodynamical Simulations: how Stochastic Processes, Numerical Effects, and Reproducibility Limits impact Predictability Cosmological Hydrodynamics with Adaptive Mesh Refinement: a new high resolution code called RAMSES

Reference 41

Resolution: verified exact; local_arxiv, observed 2026-06-27T00:30:16.681508Z

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.

Observation a3e42328-813c-4c12-b6fe-44b6f2d556bb · inbound

Early phases of star formation with SKAO: synchrotron emission from dense starless cores in molecular clouds cites this paper.

Early phases of star formation with SKAO: synchrotron emission from dense starless cores in molecular clouds Cosmological Hydrodynamics with Adaptive Mesh Refinement: a new high resolution code called RAMSES

Reference 296

Resolution: metadata mismatch; local_arxiv, observed 2026-06-27T01:20:20.904507Z

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.

Observation 9b09c36e-1064-4e04-ab6b-fd3350ed21e3 · inbound

The dynamical origin of the magnetic field distributions in compressible turbulence cites this paper.

The dynamical origin of the magnetic field distributions in compressible turbulence Cosmological Hydrodynamics with Adaptive Mesh Refinement: a new high resolution code called RAMSES

Reference 49

Resolution: metadata mismatch; local_arxiv, observed 2026-07-09T22:06:35.083086Z

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.

Observation 465a06e2-9555-4c2e-aadf-eb18b21bdd07 · inbound

mitigating the overcooling problem with sink-based bursty star formation in a high-z dwarf galaxy cites this paper.

mitigating the overcooling problem with sink-based bursty star formation in a high-z dwarf galaxy Cosmological Hydrodynamics with Adaptive Mesh Refinement: a new high resolution code called RAMSES

Reference 9

Resolution: unresolved; no resolver link, observed 2026-07-13T06:20:04.707661Z

Source-reported events for the cited work

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Observation 6c78e1d6-7143-45a3-883d-421c0f1c66d8 · inbound

Performance of morphological classifiers for galaxy mergers compared to current machine learning methods cites this paper.

Performance of morphological classifiers for galaxy mergers compared to current machine learning methods Cosmological Hydrodynamics with Adaptive Mesh Refinement: a new high resolution code called RAMSES

Reference 57

Resolution: unresolved; no resolver link, observed 2026-07-13T04:41:12.165957Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f86cd5ca-de40-4f95-acda-4ec6fd42cda9 · inbound

Cold Stream Penetration of Virial Shocks: Fragmentation, Coagulation, and Disruption in the Hot Circumgalactic Medium cites this paper.

Cold Stream Penetration of Virial Shocks: Fragmentation, Coagulation, and Disruption in the Hot Circumgalactic Medium Cosmological Hydrodynamics with Adaptive Mesh Refinement: a new high resolution code called RAMSES

Reference 7

Resolution: unresolved; no resolver link, observed 2026-08-02T02:50:41.707549Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 03833245-d553-496d-9ad0-e5fa6234e3ae · inbound

A Scalable Fast Multipole Method Poisson Solver for the RAMSES code: II. Adaptive Mesh Refinement and Adaptive Time Stepping cites this paper.

A Scalable Fast Multipole Method Poisson Solver for the RAMSES code: II. Adaptive Mesh Refinement and Adaptive Time Stepping Cosmological Hydrodynamics with Adaptive Mesh Refinement: a new high resolution code called RAMSES

Reference 8

Resolution: unresolved; no resolver link, observed 2026-08-01T12:41:17.197900Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 2ced6025-2cd6-4b30-a7ff-747ed7295c64 · inbound

Outflows in super-Eddington quasars drive clumpy circumgalactic medium and extended H$\alpha$ nebulae at $z \gtrsim 6$ cites this paper.

Outflows in super-Eddington quasars drive clumpy circumgalactic medium and extended H$\alpha$ nebulae at $z \gtrsim 6$ Cosmological Hydrodynamics with Adaptive Mesh Refinement: a new high resolution code called RAMSES

Reference 226

Resolution: unresolved; no resolver link, observed 2026-08-01T06:58:55.542235Z

Source-reported events for the cited work

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Observation 43c59055-5781-45f9-86d3-f10e07e2025c · inbound

End-to-end differentiable retrieval of molecular spectra using hydrodynamics, chemistry, and radiative transfer cites this paper.

End-to-end differentiable retrieval of molecular spectra using hydrodynamics, chemistry, and radiative transfer Cosmological Hydrodynamics with Adaptive Mesh Refinement: a new high resolution code called RAMSES

Reference 9

Resolution: unresolved; no resolver link, observed 2026-08-03T00:38:57.804039Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 57e22544-13c3-4fb5-b5f1-f49a5979f188 · inbound

Accretion across scales: streamers, surface-layer transport, and rapid replenishment in young protoplanetary discs cites this paper.

Accretion across scales: streamers, surface-layer transport, and rapid replenishment in young protoplanetary discs Cosmological Hydrodynamics with Adaptive Mesh Refinement: a new high resolution code called RAMSES

Reference 296

Resolution: unresolved; no resolver link, observed 2026-08-04T11:34:25.672731Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e5f88d2d-518c-448a-9df1-5bcf6a82c593 · inbound

N-body Simulations of Large-Scale Structure in the Generalized Cubic Covariant Galileon Model cites this paper.

N-body Simulations of Large-Scale Structure in the Generalized Cubic Covariant Galileon Model Cosmological Hydrodynamics with Adaptive Mesh Refinement: a new high resolution code called RAMSES

Reference 55

Resolution: unresolved; no resolver link, observed 2026-08-15T14:38:14.433794Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7ed662c9-dce3-40fc-aee8-0b00d66c41b1 · inbound

Smoothed particle magnetohydrodynamics for simulations of galaxy and cosmic structure formation cites this paper.

Smoothed particle magnetohydrodynamics for simulations of galaxy and cosmic structure formation Cosmological Hydrodynamics with Adaptive Mesh Refinement: a new high resolution code called RAMSES

Reference 40

Resolution: unresolved; no resolver link, observed 2026-08-10T17:19:39.664327Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.