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Paper Citation Record · LEDGER

Evidence for GeV emission of the superluminous supernova SN 2017egm

As of 13 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2407.05968.

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

pith.paper-citation-record.v1
2407.05968 v2

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 2026-08-12T06:34:41.77262+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-10T22:01:52.701847Z

measured 1 of 1 external citation measurements

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

Source: arxiv_reference, 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

0
arxiv_reference, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 7ca65d9e-4652-48a6-913a-4979f7abf65e · inbound

Stellar Tidal Disruptions by Newborn Neutron Stars or Black Holes: A Mechanism for Hydrogen-poor (Super)luminous Supernovae and Fast Blue Optical Transients cites this paper.

Stellar Tidal Disruptions by Newborn Neutron Stars or Black Holes: A Mechanism for Hydrogen-poor (Super)luminous Supernovae and Fast Blue Optical Transients Evidence for GeV emission of the superluminous supernova SN 2017egm

Reference 62

Resolution
unresolved
no resolver link, observed 2026-08-10T22:01:52.701847Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T22:01:52.701847Z digest=sha256:8f0457306534d593885876e6dbe07469933dc82f8af7f82951a344856b72375b

Observation 7748ca1a-3b9d-470e-ac8f-029b6aa4a807 · inbound

On the Gamma-ray Efficiency of Superluminous Supernovae: Potential Detections and Population-Level Constraints cites this paper.

On the Gamma-ray Efficiency of Superluminous Supernovae: Potential Detections and Population-Level Constraints Evidence for GeV emission of the superluminous supernova SN 2017egm

Reference 25

Resolution
verified exact
arxiv_id, observed 2026-07-16T02:22:24.270310Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

source=pdf_text observed=2026-05-10T07:28:20.494507Z digest=sha256:02d5f56de83c769c7d7bf7189052c0acdef8add32cba41bb80e4dc1e56076f4e

Observation 6ee40e46-75c9-473b-8aed-d1c3939705e0 · inbound

A Magnetar Engine and Circumstellar Medium Interaction: Synergistic Effects in Producing Superluminous Supernovae cites this paper.

A Magnetar Engine and Circumstellar Medium Interaction: Synergistic Effects in Producing Superluminous Supernovae Evidence for GeV emission of the superluminous supernova SN 2017egm

Reference 62

Resolution
metadata mismatch
arxiv_id, observed 2026-07-16T02:22:24.270310Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

source=pdf_text observed=2026-07-10T11:12:04.532736Z digest=sha256:00c6a63152bafe6f5737059222189d64670e38262468309a8f935f5368f28111