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 5 inbound Pith citation observations for arXiv:2311.01827.
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 2026-08-08T13:33:06.380063Z
A source-named dated measurement, never combined with another source.
Source: cited_works
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 15f229f3-3432-4c14-9e60-18ca20c151f9 · inbound
Runaway OB stars within 1 kpc of the Sun Galactic runaway O and Be stars found using Gaia DR3
Reference 5
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation b3c059b7-6465-4975-9366-e22a0f24caa3 · inbound
Large-scale emission from gamma-ray binaries: the case of LS 5039 Galactic runaway O and Be stars found using Gaia DR3
Reference 75
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 8b7b1966-10ce-43f8-98c9-bc3240291580 · inbound
An Halpha survey of infrared bow-shocks around OB-type stars Galactic runaway O and Be stars found using Gaia DR3
Reference 73
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation c1488e50-8b8c-4ef8-a509-664d90ae62c9 · inbound
The IACOB project XVIII. Prevalence of short-period binaries among Galactic helium rich O-type stars Galactic runaway O and Be stars found using Gaia DR3
Reference 44
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 7318eb3e-7552-41b6-bc9a-2b63c378eb87 · inbound
Why do massive stars form bow shocks? Bulk ISM motion as the main driver of bow shock formation and geometry Galactic runaway O and Be stars found using Gaia DR3
Reference 58
Source-reported events for the cited work
Unavailable: canonical work link unavailable.