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:2102.11753.
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 2026-08-07T20:40:57.146732Z
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 622e7502-6fe3-4b65-91dc-07363ae2050d · inbound
Can a gamma-ray dim radio blazar produce a 200-PeV neutrino? The case of PMN J0606$-$0724 and KM3-230213A A Quick Look at the $3\,$GHz Radio Sky I. Source Statistics from the Very Large Array Sky Survey
Reference 26
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 55decbdc-f0ef-49c7-9823-2fe89ece1060 · inbound
Satellite quenching by radio jets of central galaxies in galaxy groups A Quick Look at the $3\,$GHz Radio Sky I. Source Statistics from the Very Large Array Sky Survey
Reference 130
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation c18831da-7f8e-4122-a5dd-83e706498fe0 · inbound
Cosmic Pairs: A DESI Census of Dual and Offset AGN as Precursors to Massive Black Hole Binaries A Quick Look at the $3\,$GHz Radio Sky I. Source Statistics from the Very Large Array Sky Survey
Reference 212
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 9bb7c71c-7df3-4a8f-b901-d68b9ad540ff · inbound
Why do massive stars form bow shocks? Bulk ISM motion as the main driver of bow shock formation and geometry A Quick Look at the $3\,$GHz Radio Sky I. Source Statistics from the Very Large Array Sky Survey
Reference 87
Source-reported events for the cited work
Unavailable: canonical work link unavailable.