Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
A Chandra survey of fluorescence Fe lines in X-ray Binaries at high resolution
As of 15 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1004.2345.
A citation records a reference. It does not transfer a finding from one paper to another.
Coverage vector
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-15T06:32:42.880941+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-11T05:41:09.569535Z
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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- 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 cb355238-cf40-4bd4-a7d0-647b4dacf916 · 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 A Chandra survey of fluorescence Fe lines in X-ray Binaries at high resolution
Reference 234
- Resolution
- unresolved
- no resolver link, observed 2026-08-11T05:41:09.569535Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation cc3761ef-c16a-4244-a697-b36dac67975d · inbound
XMM-Newton follow-up of two eROSITA X-ray binary candidates cites this paper.
XMM-Newton follow-up of two eROSITA X-ray binary candidates A Chandra survey of fluorescence Fe lines in X-ray Binaries at high resolution
Reference 54
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T18:24:53.841862Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 6861a66a-b1ff-4dcb-8228-255b9dcc6e8b · 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 Chandra survey of fluorescence Fe lines in X-ray Binaries at high resolution
Reference 82
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T20:40:57.127269Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.