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Paper Citation Record · LEDGER

Multiwavelength monitoring and X-ray brightening of Be X-ray binary PSR J2032+4127/MT91 213 on its approach to periastron

As of 16 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1609.06328.

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

pith.paper-citation-record.v1
1609.06328 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 2026-08-16T06:30:59.297886+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-14T13:23:57.141488Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-11T00:05:50.373187Z

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
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  • 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 575434ce-4d64-4060-a8e5-b9b5149e744e · inbound

Highlights of Galactic Physics with VERITAS cites this paper.

Highlights of Galactic Physics with VERITAS Multiwavelength monitoring and X-ray brightening of Be X-ray binary PSR J2032+4127/MT91 213 on its approach to periastron

Reference 5

Resolution
unresolved
no resolver link, observed 2026-08-14T13:23:57.141488Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T13:23:57.141488Z digest=sha256:67b84ba62e7e105bac07b22d4ab970ce6d46e3807be567913a8f05c3a9f41596

Observation 8b74d881-e905-4ca4-97bc-0adc129829eb · 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? Multiwavelength monitoring and X-ray brightening of Be X-ray binary PSR J2032+4127/MT91 213 on its approach to periastron

Reference 53

Resolution
verified exact
arxiv_id, observed 2026-07-04T21:29:43.791435Z

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:bd5f5abeea8438ef4851bc88e31b47bc39149c9c0f4f788c776f5398513a376e