Pith. sign in

Paper Citation Record · LEDGER

A Quick Look at the $3\,$GHz Radio Sky I. Source Statistics from the Very Large Array Sky Survey

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.

pith.paper-citation-record.v1
2102.11753 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 4 of 4 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-08T06:32:00.761636+00:00

measured 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T20:40:57.146732Z

measured 0 of 1 external citation measurements

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

Source: cited_works

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 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 cites this paper.

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

Resolution
unresolved
no resolver link, observed 2026-08-04T18:04:12.496600Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-04T18:04:12.496600Z digest=sha256:a24c2dc3bfdf508da16c35133705f5648241034083fc195f17bcfee9de353d65

Observation 55decbdc-f0ef-49c7-9823-2fe89ece1060 · inbound

Satellite quenching by radio jets of central galaxies in galaxy groups cites this paper.

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

Resolution
unresolved
no resolver link, observed 2026-07-12T06:58:22.474180Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-07-12T06:58:22.474180Z digest=sha256:1ffd95cf4ab8815cad4013fabdc3a069d226697c432a646cf0c4026af9287984

Observation c18831da-7f8e-4122-a5dd-83e706498fe0 · inbound

Cosmic Pairs: A DESI Census of Dual and Offset AGN as Precursors to Massive Black Hole Binaries cites this paper.

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

Resolution
unresolved
no resolver link, observed 2026-08-01T08:21:14.736056Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T08:21:14.736056Z digest=sha256:3fb36fd8a35b67d9793b54d945ceaf41779cac2c977b2fcb6a3f27acf903f74a

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 cites this paper.

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

Resolution
unresolved
no resolver link, observed 2026-08-07T20:40:57.146732Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T20:40:57.146732Z digest=sha256:144013872f10c2a37f97377b9c6aaa6ec22e72272fe4a85a50123257c5371406