Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
The non-thermal emission following GW170817 is consistent with a conical radially-stratified outflow with initial Lorentz factor $\lesssim10$
As of 19 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2410.02166.
A citation records a reference. It does not transfer a finding from one paper to another.
Coverage vector
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-19T06:32:44.657259+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-16T12:40:27.616303Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-05-14T17:49:23.236723Z
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 f329ca49-8283-4e84-8da0-c1738b73bc4e · inbound
The Late-time Afterglow of GW170817 and Implications for Jet Dynamics cites this paper.
The Late-time Afterglow of GW170817 and Implications for Jet Dynamics The non-thermal emission following GW170817 is consistent with a conical radially-stratified outflow with initial Lorentz factor $\lesssim10$
Reference 61
- Resolution
- unresolved
- no resolver link, observed 2026-08-16T12:40:27.616303Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 8db1655f-7df2-4881-88ca-d5aeeb769d9d · inbound
X-ray Emission Signatures of Neutron Star Mergers cites this paper.
X-ray Emission Signatures of Neutron Star Mergers The non-thermal emission following GW170817 is consistent with a conical radially-stratified outflow with initial Lorentz factor $\lesssim10$
Reference 116
- Resolution
- unresolved
- no resolver link, observed 2026-08-16T04:26:20.668085Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation c9a9697b-0b9a-406d-b58d-125db64a60b4 · inbound
The Very Late Time Afterglow of GW170817 Favors a Wobbling Jet cites this paper.
The Very Late Time Afterglow of GW170817 Favors a Wobbling Jet The non-thermal emission following GW170817 is consistent with a conical radially-stratified outflow with initial Lorentz factor $\lesssim10$
Reference 51
- Resolution
- verified exact
- arxiv_id, observed 2026-05-14T17:49:23.238647Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.