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Paper Citation Record · LEDGER

The Engineering Development Array: A low frequency radio telescope utilising SKA precursor technology

As of 6 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1707.03499.

A citation records a reference. It does not transfer a finding from one paper to another.

pith.paper-citation-record.v1
1707.03499 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 2 of 2 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-06T06:34:29.942622+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-07-11T11:50:26.030339Z

measured 1 of 1 external citation measurements

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

Source: pith, observed 2026-08-05T02:28:24.338817Z

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
  • unresolved0
  • parse uncertain0
  • malformed identifier0
  • metadata mismatch0

External citation measurements

21
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 02090d97-bfb9-4edb-bb5b-e77867303965 · inbound

The Information Content of Quasar Variability Light Curves: How Well Can we Infer Stochastic Model Parameters? cites this paper.

The Information Content of Quasar Variability Light Curves: How Well Can we Infer Stochastic Model Parameters? The Engineering Development Array: A low frequency radio telescope utilising SKA precursor technology

Reference 21

Resolution
verified exact
local_arxiv, observed 2026-06-28T16:32:22.539281Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:37b4fdef6f2b1186d4aa6628f69d0bee0d339613bb5b8c1810c5ed7fd70d860a

Observation a0f29b42-3143-4b78-9d5e-000e8810abbe · inbound

The Murchison Widefield Array Phase III upgrade: Sensitivity Doubled, Number of Baselines Quadrupled, Flexibility Enhanced, and EoR Observations Optimised cites this paper.

The Murchison Widefield Array Phase III upgrade: Sensitivity Doubled, Number of Baselines Quadrupled, Flexibility Enhanced, and EoR Observations Optimised The Engineering Development Array: A low frequency radio telescope utilising SKA precursor technology

Reference 46

Resolution
verified exact
local_arxiv, observed 2026-06-28T13:12:13.516407Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:4b483a150c002a60dafbba99a468f98bbfd8e4593fbcf833c5c67210d04f00e5