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Paper Citation Record · LEDGER

Expected neutrino fluence from short Gamma-Ray Burst 170817A and off-axis angle constraints

As of 16 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1712.00449.

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

pith.paper-citation-record.v1
1712.00449 v2

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 2026-08-16T06:30:59.297886+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-15T19:10:39.489523Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-08-15T19:10:40.957891Z

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 ec3d43b1-4925-40bd-aa8c-053b6a87c4ec · inbound

Neutrinos from explosive transients at the dawn of multi-messenger astronomy cites this paper.

Neutrinos from explosive transients at the dawn of multi-messenger astronomy Expected neutrino fluence from short Gamma-Ray Burst 170817A and off-axis angle constraints

Reference 64

Resolution
unresolved
no resolver link, observed 2026-08-11T16:53:00.628632Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-11T16:53:00.628632Z digest=sha256:7c051cde2efdf73044bbab9c6d40403369e73b7593720a9832b2f4f9f898a330

Observation 8d171c7a-03b7-4ea9-a9ff-7e7c4cccf145 · inbound

Binary Neutron Star Mergers as Potential Sources for Ultra-High-Energy Cosmic Rays and High-Energy Neutrinos cites this paper.

Binary Neutron Star Mergers as Potential Sources for Ultra-High-Energy Cosmic Rays and High-Energy Neutrinos Expected neutrino fluence from short Gamma-Ray Burst 170817A and off-axis angle constraints

Reference 56

Resolution
verified exact
local_arxiv, observed 2026-08-15T19:10:40.962760Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

source=pdf_text observed=2026-08-15T19:10:39.489523Z digest=sha256:ef8262e438d070ca7f4ceb669e3f5c92eab83a4b110b0f9fe245cbaef9166505