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Paper Citation Record · LEDGER

An efficient shock-capturing central-type scheme for multidimensional relativistic flows. I. Hydrodynamics

As of 15 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:astro-ph/0205290.

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

pith.paper-citation-record.v1
astro-ph/0205290 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 2026-08-14T06:32:32.682623+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T11:45:03.749879Z

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

0 of 0 outbound references displayed

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  • verified fuzzy0
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  • malformed identifier0
  • metadata mismatch0

External citation measurements

198
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation da0e37b1-0c57-4e9f-925b-1600df39f5d4 · inbound

A general relativistic hydrodynamic simulation code for studying advective, sub-Keplerian accretion flow onto black holes cites this paper.

A general relativistic hydrodynamic simulation code for studying advective, sub-Keplerian accretion flow onto black holes An efficient shock-capturing central-type scheme for multidimensional relativistic flows. I. Hydrodynamics

Reference 25

Resolution
unresolved
no resolver link, observed 2026-08-07T11:45:03.749879Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T11:45:03.749879Z digest=sha256:34716f4a2960956e8256f4446b053de4bda62873de19078f6fe8361998943eb1

Observation 8e05a941-7a50-47b8-a135-a7bbbf8e5c0b · inbound

Exact Mass Conservation in Binary Neutron Star Merger Simulations cites this paper.

Exact Mass Conservation in Binary Neutron Star Merger Simulations An efficient shock-capturing central-type scheme for multidimensional relativistic flows. I. Hydrodynamics

Reference 28

Resolution
verified exact
local_arxiv, observed 2026-06-29T05:53:09.133991Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

source=pdf_text observed=2026-06-29T05:45:55.511016Z digest=sha256:e1a102751a654254de36b7c40f1ee3e281a8ae5068fbe0aa2c4c845dc3eb9579

Observation 83654cc4-f502-4ded-a858-99f4d8fa36b3 · inbound

Simulation based parameter space for shock in transonic, sub-Keplerian accretion flow onto non-rotating black holes cites this paper.

Simulation based parameter space for shock in transonic, sub-Keplerian accretion flow onto non-rotating black holes An efficient shock-capturing central-type scheme for multidimensional relativistic flows. I. Hydrodynamics

Reference 72

Resolution
verified exact
local_arxiv, observed 2026-06-28T09:21:48.771676Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:a865e56c7351a616bc26fe173449fdb6c5fb7795f71444bb4c549c18f5cdd509