Paper Citation Record · LEDGER

A jet model for the broadband spectrum of XTE J1118+480: Synchrotron emission from radio to X-rays in the Low/Hard spectral state

As of 14 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:astro-ph/0010560.

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

pith.paper-citation-record.v1
astro-ph/0010560 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 2026-08-14T06:32:32.682623+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T20:40:57.728957Z

measured 0 of 1 external citation measurements

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

Source: cited_works

Reference resolution

0 of 0 outbound references displayed

verified exact0
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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 99129e99-9f5e-46bd-9aa6-c91591ae223d · inbound

Energy-dependent Optical/Near-infrared and X-ray Correlations in Swift J1727.8-1613 cites this paper.

Energy-dependent Optical/Near-infrared and X-ray Correlations in Swift J1727.8-1613 A jet model for the broadband spectrum of XTE J1118+480: Synchrotron emission from radio to X-rays in the Low/Hard spectral state

Reference 118

Resolution: unresolved; no resolver link, observed 2026-08-03T01:34:17.008967Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation b35f606a-f8b9-442b-8c9c-88e0fd6fd5bb · inbound

Why do massive stars form bow shocks? Bulk ISM motion as the main driver of bow shock formation and geometry cites this paper.

Why do massive stars form bow shocks? Bulk ISM motion as the main driver of bow shock formation and geometry A jet model for the broadband spectrum of XTE J1118+480: Synchrotron emission from radio to X-rays in the Low/Hard spectral state

Reference 241

Resolution: unresolved; no resolver link, observed 2026-08-07T20:40:57.728957Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.