Paper Citation Record · LEDGER

Collimation of astrophysical jets - the role of the accretion disk magnetic field distribution

As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:astro-ph/0511611.

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

pith.paper-citation-record.v1
astro-ph/0511611 v2

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 2026-08-11T06:34:44.6726+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-07-11T11:50:26.030339Z

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

verified exact0
verified fuzzy0
unresolved0
parse uncertain0
malformed identifier0
metadata mismatch0

External citation measurements

83
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation dc71f10b-12ad-452f-a121-efa0f1d8462c · inbound

A robust super-time-stepping scheme for Ohmic and ambipolar diffusion cites this paper.

A robust super-time-stepping scheme for Ohmic and ambipolar diffusion Collimation of astrophysical jets - the role of the accretion disk magnetic field distribution

Reference 23

Resolution: verified exact; local_arxiv, observed 2026-06-28T16:32:22.895100Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation db300816-5c4e-4132-96d6-f854cb015a91 · inbound

Polarization Architecture of Steady GRMHD Jets from the Horizon to Infinity cites this paper.

Polarization Architecture of Steady GRMHD Jets from the Horizon to Infinity Collimation of astrophysical jets - the role of the accretion disk magnetic field distribution

Reference 62

Resolution: verified exact; local_arxiv, observed 2026-07-03T08:07:44.430809Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.