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Paper Citation Record · LEDGER

Pulse-amplitude-resolved spectroscopy of bright accreting pulsars: indication of two accretion regimes

As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1107.2202.

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

pith.paper-citation-record.v1
1107.2202 v1

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 2026-08-06T06:34:29.942622+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
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  • malformed identifier0
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External citation measurements

86
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 3996daf0-b0eb-4607-bd5b-e83aee12be14 · inbound

Rapid quasi-periodic reconfiguration of the accretion column in pulsar 1A 0535+262 cites this paper.

Rapid quasi-periodic reconfiguration of the accretion column in pulsar 1A 0535+262 Pulse-amplitude-resolved spectroscopy of bright accreting pulsars: indication of two accretion regimes

Reference 95

Resolution
verified exact
local_arxiv, observed 2026-06-28T13:52:16.823220Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:4e6b8f12a12a4c46210e6151639b422fabde7292f828ae61dd5f9041c1802ff4

Observation 4c9ee03d-f324-41f9-b074-059f6945564d · inbound

A New Relativistic Model for Spectral Formation in Accretion-Powered X-ray Pulsars: Pulse Profiles and Phase-Averaged Spectra cites this paper.

A New Relativistic Model for Spectral Formation in Accretion-Powered X-ray Pulsars: Pulse Profiles and Phase-Averaged Spectra Pulse-amplitude-resolved spectroscopy of bright accreting pulsars: indication of two accretion regimes

Reference 35

Resolution
verified exact
local_arxiv, observed 2026-07-01T01:55:14.909928Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:c4cb98b060c2682ed6189e9f2db0c51dfb20ef4766e9efa15d867c422e089859