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Paper Citation Record · LEDGER

Absorption lines from magnetically-driven winds in X-ray binaries

As of 22 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 1 inbound Pith citation observation for arXiv:1512.09149.

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

pith.paper-citation-record.v1
1512.09149 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 1 of 1 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-21T06:32:19.484+00:00

measured 1 of 1 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-07-31T03:00:27.898774Z

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

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  • malformed identifier0
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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 04c77a5f-823c-445b-b106-5a0867b8e7af · inbound

How massive and clumpy must a quasar wind be to create emission line blueshifts? cites this paper.

How massive and clumpy must a quasar wind be to create emission line blueshifts? Absorption lines from magnetically-driven winds in X-ray binaries

Reference 105

Resolution
unresolved
no resolver link, observed 2026-07-31T03:00:27.898774Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-31T03:00:27.898774Z digest=sha256:4484ea0a424ebc890ccc1530eaacda9580ee175bd747e91e0b688b1e86488d8a