Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
As of 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:1309.0755.
A citation records a reference. It does not transfer a finding from one paper to another.
Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-08T06:32:00.761636+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-07T20:40:57.671882Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-07-08T00:54:20.848078Z
0 of 0 outbound references displayed
External citation measurements
No source-named external measurement is stored.
No outbound reference observations are available for this paper version.
Observation 2508a2b1-be6f-436b-82f7-777422b5979f · inbound
Effectiveness of Stacks in the Stacked Hilbert-Huang Transform The Swift/BAT Hard X-ray Transient Monitor
Reference 34
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 1d89d57f-8797-4246-af6a-ce8ba032dd1e · inbound
EP260321a/SN 2026gzf: The Faintest Shock Breakout Associated with a Broad-Lined Supernova The Swift/BAT Hard X-ray Transient Monitor
Reference 257
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.
Observation 60a3ef2e-7d7d-4540-a98c-6c6aac8ad230 · inbound
Spectropolarimetric detection of baryonic mass loading in a transient relativistic jet: application to the black hole X-ray binary Swift J1727.8$-$1613 The Swift/BAT Hard X-ray Transient Monitor
Reference 286
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.
Observation 60bf9298-c425-4d61-bc96-811b85442053 · inbound
Why do massive stars form bow shocks? Bulk ISM motion as the main driver of bow shock formation and geometry The Swift/BAT Hard X-ray Transient Monitor
Reference 226
Source-reported events for the cited work
Unavailable: canonical work link unavailable.