Pith. sign in

Paper Citation Record · LEDGER

Short Gamma-Ray Bursts with Extended Emission Observed with Swift/BAT and Fermi/GBM

As of 16 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1506.05899.

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

pith.paper-citation-record.v1
1506.05899 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 2026-08-16T04:31:28.654504Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-08-15T19:10:40.762502Z

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 cdf260cf-ce83-438c-97e7-cf081d1a7059 · inbound

Connecting afterglow light curves to the GRB central engine cites this paper.

Connecting afterglow light curves to the GRB central engine Short Gamma-Ray Bursts with Extended Emission Observed with Swift/BAT and Fermi/GBM

Reference 42

Resolution
unresolved
no resolver link, observed 2026-08-16T04:31:28.654504Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-16T04:31:28.654504Z digest=sha256:6347d5687185c17e0331edbda2b12d8156ddfcb68899a40915fd9a91d43df5dc

Observation 2f99f859-e0ab-470f-a1bf-16e97b78c4a7 · 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 Short Gamma-Ray Bursts with Extended Emission Observed with Swift/BAT and Fermi/GBM

Reference 67

Resolution
verified exact
local_arxiv, observed 2026-08-15T19:10:40.767489Z

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=2026-08-15T19:10:39.539064Z digest=sha256:bb9d932b2c3951f8cc58ee67564ec58e7c1bcdde650d51b3d3bb15fa6d0f89c9