Paper Citation Record · LEDGER

Insight-HXMT discovery of the highest energy CRSF from the first Galactic ultra-luminous X-ray pulsar Swift J0243.6+6124

As of 13 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:2206.04283.

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

pith.paper-citation-record.v1
2206.04283 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 4 of 4 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-13T06:32:02.005865+00:00

measured 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-12T18:32:10.461343Z

measured 0 of 1 external citation measurements

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

Source: cited_works

Reference resolution

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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 37ffee25-2705-434d-bebb-1407c2af046e · inbound

X-Ray Views of Galactic Accreting Pulsars in High-Mass X-Ray Binaries cites this paper.

X-Ray Views of Galactic Accreting Pulsars in High-Mass X-Ray Binaries Insight-HXMT discovery of the highest energy CRSF from the first Galactic ultra-luminous X-ray pulsar Swift J0243.6+6124

Reference 256

Resolution: unresolved; no resolver link, observed 2026-08-11T05:41:09.652182Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a6291c45-d531-4039-92e3-ecc470b5d32a · inbound

Physics of Strong Magnetism with eXTP cites this paper.

Physics of Strong Magnetism with eXTP Insight-HXMT discovery of the highest energy CRSF from the first Galactic ultra-luminous X-ray pulsar Swift J0243.6+6124

Reference 221

Resolution: unresolved; no resolver link, observed 2026-08-07T05:19:03.538765Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation b4489299-22b1-4101-8f5f-74ed9f413419 · 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 Insight-HXMT discovery of the highest energy CRSF from the first Galactic ultra-luminous X-ray pulsar Swift J0243.6+6124

Reference 254

Resolution: unresolved; no resolver link, observed 2026-08-07T20:40:57.779713Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f21bffb8-bbb0-43f4-bc99-3d167b9a9f4f · inbound

Real-time observations of the transition to the quiescent state in an accreting magnetised neutron star: No propeller required? cites this paper.

Real-time observations of the transition to the quiescent state in an accreting magnetised neutron star: No propeller required? Insight-HXMT discovery of the highest energy CRSF from the first Galactic ultra-luminous X-ray pulsar Swift J0243.6+6124

Reference 6

Resolution: unresolved; no resolver link, observed 2026-08-12T18:32:10.461343Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.