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Paper Citation Record · LEDGER

H-AMR: A New GPU-accelerated GRMHD Code for Exascale Computing With 3D Adaptive Mesh Refinement and Local Adaptive Time-stepping

As of 19 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:1912.10192.

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

pith.paper-citation-record.v1
1912.10192 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 2026-08-19T06:32:44.657259+00:00

measured 5 of 5 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-11T04:39:37.569479Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-15T03:08:59.266219Z

Reference resolution

0 of 0 outbound references displayed

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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 43eb70ac-cf9b-451d-bc6e-c365c170e880 · inbound

Gamma-ray bursts: what do we know today that we did not know 10 years ago? cites this paper.

Gamma-ray bursts: what do we know today that we did not know 10 years ago? H-AMR: A New GPU-accelerated GRMHD Code for Exascale Computing With 3D Adaptive Mesh Refinement and Local Adaptive Time-stepping

Reference 176

Resolution
unresolved
no resolver link, observed 2026-08-11T04:39:37.569479Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation ce593b56-d19e-4a83-8413-90280efc84cb · inbound

Polarization Signatures from GRMHD Simulations of Black Hole Accretion cites this paper.

Polarization Signatures from GRMHD Simulations of Black Hole Accretion H-AMR: A New GPU-accelerated GRMHD Code for Exascale Computing With 3D Adaptive Mesh Refinement and Local Adaptive Time-stepping

Reference 107

Resolution
verified exact
arxiv_id, observed 2026-05-15T03:08:59.269790Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

source=pdf_text observed=2026-05-15T03:06:24.087052Z digest=sha256:bc40f28916eed766da3174bbef9c816b991ddf07b7a1a853d92ee80657fa8c7d

Observation 2f7e250d-6573-4b07-a085-6bb9017e51ff · inbound

GRACE: An Open-Source Framework for GPU-Accelerated Numerical Relativity cites this paper.

GRACE: An Open-Source Framework for GPU-Accelerated Numerical Relativity H-AMR: A New GPU-accelerated GRMHD Code for Exascale Computing With 3D Adaptive Mesh Refinement and Local Adaptive Time-stepping

Reference 36

Resolution
unresolved
no resolver link, observed 2026-07-14T15:02:35.854356Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-07-14T15:02:35.854356Z digest=sha256:d7b9e18c2567604296f03dc335689cee8c90e785f21961d28d3b6a5327f10a22

Observation a76d32a9-b0bf-4395-a86f-11de6638646c · inbound

The COLIBRE-SKIRT pipeline: Calibration-free dust radiative transfer postprocessing for cosmological simulations cites this paper.

The COLIBRE-SKIRT pipeline: Calibration-free dust radiative transfer postprocessing for cosmological simulations H-AMR: A New GPU-accelerated GRMHD Code for Exascale Computing With 3D Adaptive Mesh Refinement and Local Adaptive Time-stepping

Reference 199

Resolution
unresolved
no resolver link, observed 2026-08-02T00:50:15.611314Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T00:50:15.611314Z digest=sha256:b70bdeb0f36990644bde10b0a87b5bf068e05a1febbbe88d76cfb6da8b774139

Observation 722f8049-1a86-4046-a175-0e3ebac4bf73 · 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 $z \gtrsim 6$ H-AMR: A New GPU-accelerated GRMHD Code for Exascale Computing With 3D Adaptive Mesh Refinement and Local Adaptive Time-stepping

Reference 210

Resolution
unresolved
no resolver link, observed 2026-08-01T06:58:53.195899Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T06:58:53.195899Z digest=sha256:7672d7a25e75b4c1a5db2c226deea2038bc67554b5e2781ac898d15a10cb996c