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Paper Citation Record · LEDGER

A Non-thermal Study of the Brightest Cluster Galaxy NGC 1275 - The Gamma-Radio Connection Over Four Decades

As of 15 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1405.3647.

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

pith.paper-citation-record.v1
1405.3647 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 3 of 3 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-14T06:32:32.682623+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-14T14:48:15.207275Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-01T17:25:51.899888Z

Reference resolution

0 of 0 outbound references displayed

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  • verified fuzzy0
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  • 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 d8cf4bc1-93a9-4d92-9b70-ecbd04cb4af6 · inbound

A Model for Magnetic Reconnection as the Origin of TeV Outbursts from NGC 1275 cites this paper.

A Model for Magnetic Reconnection as the Origin of TeV Outbursts from NGC 1275 A Non-thermal Study of the Brightest Cluster Galaxy NGC 1275 - The Gamma-Radio Connection Over Four Decades

Reference 23

Resolution
verified exact
local_arxiv, observed 2026-07-01T17:25:51.901097Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

source=pdf_text observed=2026-06-29T03:43:28.647231Z digest=sha256:ce12fb1094f9b8cb2f00f51b7248a3d3a8cc2edda8c2771bc7ca47d25f85d8dd

Observation 105e82b0-b4aa-4467-9ef1-d8da8851e68d · inbound

Decoding the jet of BL Lacertae using relativistic magneto-hydrodynamics cites this paper.

Decoding the jet of BL Lacertae using relativistic magneto-hydrodynamics A Non-thermal Study of the Brightest Cluster Galaxy NGC 1275 - The Gamma-Radio Connection Over Four Decades

Reference 84

Resolution
unresolved
no resolver link, observed 2026-08-14T04:20:28.425904Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T04:20:28.425904Z digest=sha256:095a18d7e95b651064e8dbed155f73f0c3bce77b91ad31fb8c4e4769f200496f

Observation 591ea202-1bb1-4c2d-91a9-252b33e3dd53 · inbound

X-ray Flaring and Variability in NGC 1275, the Heart of the Perseus Cluster cites this paper.

X-ray Flaring and Variability in NGC 1275, the Heart of the Perseus Cluster A Non-thermal Study of the Brightest Cluster Galaxy NGC 1275 - The Gamma-Radio Connection Over Four Decades

Reference 58

Resolution
unresolved
no resolver link, observed 2026-08-14T14:48:15.207275Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-14T14:48:15.207275Z digest=sha256:5404562a87c147f3ecd0d0e4973fdf794af589a3774115f74cd932a19595a850