Pith. sign in

Paper Citation Record · LEDGER

Accretion of low angular momentum material onto black holes: 2D magnetohydrodynamical case

As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:astro-ph/0303093.

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

pith.paper-citation-record.v1
astro-ph/0303093 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 2 of 2 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-07T06:34:17.273281+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T11:45:37.721345Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-06-28T09:21:48.856078Z

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 5fd0b446-2e07-4855-bd70-795cdde1b862 · 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 Accretion of low angular momentum material onto black holes: 2D magnetohydrodynamical case

Reference 57

Resolution
unresolved
no resolver link, observed 2026-08-07T11:45:37.721345Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T11:45:37.721345Z digest=sha256:547987f5cee6c2459e8a8d9705b3ca2389b872152eb4690a4ffd054c9c4e4cc7

Observation 14c3544a-1cb7-4bff-b132-d2660faffbf2 · 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 Accretion of low angular momentum material onto black holes: 2D magnetohydrodynamical case

Reference 93

Resolution
verified exact
local_arxiv, observed 2026-06-28T09:21:48.857767Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:747e82f66931c347a3cbb4434680160157198b48026d04af1fe831106675d76d