Paper Citation Record · LEDGER

Is the core of M87 the source of its TeV emission? Implications for unified schemes

As of 15 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:astro-ph/0510783.

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

pith.paper-citation-record.v1
astro-ph/0510783 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 2026-08-15T06:32:42.880941+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-11T19:13:04.356354Z

measured 1 of 1 external citation measurements

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

Source: pith, observed 2026-08-05T02:28:24.338817Z

Reference resolution

0 of 0 outbound references displayed

verified exact0
verified fuzzy0
unresolved0
parse uncertain0
malformed identifier0
metadata mismatch0

External citation measurements

72
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation f4715a80-05d5-47d1-a4c4-3f912d6a4cef · inbound

M87: a cosmic laboratory for deciphering black hole accretion and jet formation cites this paper.

M87: a cosmic laboratory for deciphering black hole accretion and jet formation Is the core of M87 the source of its TeV emission? Implications for unified schemes

Reference 102

Resolution: unresolved; no resolver link, observed 2026-08-11T19:13:04.356354Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 908359c3-c008-4c00-8aa8-27d2fb7f1e6a · inbound

Fermi-Large Area Telescope Detection of Very High Energy (>100 GeV) Emission from Compton-Dominated Blazars cites this paper.

Fermi-Large Area Telescope Detection of Very High Energy (>100 GeV) Emission from Compton-Dominated Blazars Is the core of M87 the source of its TeV emission? Implications for unified schemes

Reference 144

Resolution: verified exact; local_arxiv, observed 2026-07-14T12:00:26.265896Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.