Pith. sign in

Paper Citation Record · LEDGER

Minimalist model of the W50/SS433 "Extended X-ray Jet": anisotropic wind with recollimation shocks

As of 16 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2401.14770.

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

pith.paper-citation-record.v1
2401.14770 v3

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 2026-08-16T06:30:59.297886+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-04T18:36:22.939966Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-11T00:05:50.455235Z

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 0b4fb9cd-ffcb-4ae2-a64e-032dcd6f4127 · inbound

PeV particle acceleration and non-thermal emission in the `minimalist' model of the extended jets in W50/SS433 cites this paper.

PeV particle acceleration and non-thermal emission in the `minimalist' model of the extended jets in W50/SS433 Minimalist model of the W50/SS433 "Extended X-ray Jet": anisotropic wind with recollimation shocks

Reference 46

Resolution
unresolved
no resolver link, observed 2026-08-04T18:36:22.939966Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-04T18:36:22.939966Z digest=sha256:31d643bef8f1fa7b30dde1dd2e954b73b3a78315bdf8afb231cf40feaf433af9

Observation d52ec3c9-f907-49fc-99de-daece29bb27c · inbound

How many VHE gamma-ray binaries with young pulsars can be observed? cites this paper.

How many VHE gamma-ray binaries with young pulsars can be observed? Minimalist model of the W50/SS433 "Extended X-ray Jet": anisotropic wind with recollimation shocks

Reference 88

Resolution
malformed identifier
arxiv_id, observed 2026-05-11T00:05:50.456957Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

source=pdf_text observed=2026-05-10T18:42:16.317215Z digest=sha256:e75a81671dd5fd01ca6a058f44ea421811ebe88e0b08c3fccaa0a4b96ce961db