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Paper Citation Record · LEDGER

The origin of ultra-fast outflows in AGN: Monte-Carlo simulations of the wind in PDS 456

As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1410.1640.

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

pith.paper-citation-record.v1
1410.1640 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 2026-08-11T06:34:44.6726+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-02T06:14:11.122821Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-12T03:38:27.307221Z

Reference resolution

0 of 0 outbound references displayed

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  • verified fuzzy0
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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 0f72a96f-aa5a-4f0a-86fc-00383f316394 · inbound

Physically motivated AGN emissivity profiles and their effects on quasar microlensing signatures. 1. Multi-epoch accretion disc size inference cites this paper.

Physically motivated AGN emissivity profiles and their effects on quasar microlensing signatures. 1. Multi-epoch accretion disc size inference The origin of ultra-fast outflows in AGN: Monte-Carlo simulations of the wind in PDS 456

Reference 202

Resolution
verified exact
local_arxiv, observed 2026-07-12T03:38:27.309516Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

source=arxiv_source observed=2026-07-12T03:29:42.101488Z digest=sha256:e516598bcd0372ddd01146592cfe8f7c52bb57de9a9c4e54d0e10a9f055ed908

Observation ef2cfcd3-72c8-4d52-87f1-78df59ce66f7 · inbound

Fe K$\alpha$ line from the Broad Line Region of PDS456 with XRISM/Resolve cites this paper.

Fe K$\alpha$ line from the Broad Line Region of PDS456 with XRISM/Resolve The origin of ultra-fast outflows in AGN: Monte-Carlo simulations of the wind in PDS 456

Reference 78

Resolution
unresolved
no resolver link, observed 2026-08-02T06:14:11.122821Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T06:14:11.122821Z digest=sha256:eefd3d57594f4a7e8cc0f1d811c923c21e9baddc60d81f3808f3af158b9581c2