Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Swift monitoring of NGC 4151: Evidence for a Second X-ray/UV Reprocessing
As of 4 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1703.06901.
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 2026-08-04T06:34:03.388597+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-07-12T03:29:42.101488Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-06-27T17:41:07.787738Z
Reference resolution
0 of 0 outbound references displayed
- verified exact0
- verified fuzzy0
- unresolved0
- 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 c18fd433-9a5e-4b00-b7c3-0f022d3f713d · inbound
Disk reflection as the origin of the X-ray polarization of NGC 4151 with IXPE cites this paper.
Disk reflection as the origin of the X-ray polarization of NGC 4151 with IXPE Swift monitoring of NGC 4151: Evidence for a Second X-ray/UV Reprocessing
Reference 14
- Resolution
- verified exact
- local_arxiv, observed 2026-06-27T17:41:07.789136Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.
Observation 9835ec0c-02c8-4037-8550-106f77aab681 · inbound
HALO II: Constraining Hubble constant $H_{0}$ through continuum delay fitting of Fairall 9 cites this paper.
HALO II: Constraining Hubble constant $H_{0}$ through continuum delay fitting of Fairall 9 Swift monitoring of NGC 4151: Evidence for a Second X-ray/UV Reprocessing
Reference 201
- Resolution
- verified exact
- local_arxiv, observed 2026-06-26T03:58:58.257503Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.
Observation 0421ecf0-3815-4577-b476-be280ee6255c · 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 Swift monitoring of NGC 4151: Evidence for a Second X-ray/UV Reprocessing
Reference 148
- Resolution
- unresolved
- no resolver link, observed 2026-07-12T03:29:42.101488Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.