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Paper Citation Record · LEDGER

The Phase II Murchison Widefield Array: Design Overview

As of 5 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 8 inbound Pith citation observations for arXiv:1809.06466.

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

pith.paper-citation-record.v1
1809.06466 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 8 of 8 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-04T06:34:03.388597+00:00

measured 8 of 8 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-02T02:24:39.743487Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-10T13:07:05.087524Z

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
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  • malformed identifier0
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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 f4789d2d-4c31-47f6-84b9-66334a54a2af · inbound

Mapping Cosmological Signal Scales to Beam Calibration Requirements in 21cm Experiments and Implications for Near-Field Measurement cites this paper.

Mapping Cosmological Signal Scales to Beam Calibration Requirements in 21cm Experiments and Implications for Near-Field Measurement The Phase II Murchison Widefield Array: Design Overview

Reference 57

Resolution
verified exact
local_arxiv, observed 2026-05-21T06:49:44.715214Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:0e9d966e78d399e1927f985cb395e255c2f812b0b525bc8b6664209b3cfc3f0b

Observation 630971cf-d2d9-4e33-a7a7-3f9b0e172cc4 · 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 Phase II Murchison Widefield Array: Design Overview

Reference 58

Resolution
verified exact
local_arxiv, observed 2026-06-28T16:32:22.507261Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:0bb25bc82e245737ec6b5c5ee88f94f489d1166acb270134b8f0481f21f9cb3a

Observation 0765e772-9e83-4079-9ad0-26e518cf8074 · 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 Phase II Murchison Widefield Array: Design Overview

Reference 10

Resolution
verified exact
local_arxiv, observed 2026-06-28T13:12:13.445397Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:470acdb0d682bd1c240e87539c6d4575f6e7310dd08915509e595884c78249ee

Observation 6220c986-b9a3-440c-a23d-382cce2ead5a · inbound

Observations of the Cosmic Dawn and Epoch of Reionization with the SKAO: Observational Lessons Learned from Precursors and Pathfinder Instruments cites this paper.

Observations of the Cosmic Dawn and Epoch of Reionization with the SKAO: Observational Lessons Learned from Precursors and Pathfinder Instruments The Phase II Murchison Widefield Array: Design Overview

Reference 122

Resolution
metadata mismatch
local_arxiv, observed 2026-06-25T19:08:13.883291Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:aed2a1567bfa165b25fca6d0973382dc2c77cc156722e52115ef8b91239f81c4

Observation 7ea14fcf-43fb-4209-9863-d616e55ce97a · inbound

The Southern-sky MWA Rapid Two-metre (SMART) pulsar survey--IV. Survey update and an atlas of 205 non-recycled southern pulsars cites this paper.

The Southern-sky MWA Rapid Two-metre (SMART) pulsar survey--IV. Survey update and an atlas of 205 non-recycled southern pulsars The Phase II Murchison Widefield Array: Design Overview

Reference 136

Resolution
verified exact
local_arxiv, observed 2026-07-10T13:07:05.089066Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-04T06:34:03.388597+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:e243544b77af08cd8381efa9def6c6accf92450ccdb2b5e2345a227a8becc65b

Observation 2b721918-7fd3-47f6-9cfd-08ed69ceab6a · inbound

The plethora of diffuse emission in Abell 2034 as revealed by MeerKAT polarization observations cites this paper.

The plethora of diffuse emission in Abell 2034 as revealed by MeerKAT polarization observations The Phase II Murchison Widefield Array: Design Overview

Reference 147

Resolution
unresolved
no resolver link, observed 2026-08-02T02:24:39.743487Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T02:24:39.743487Z digest=sha256:38e304c9a9af2089dc4285abcaa78659ff35221adbf5bfa04575bf2bd20f277c

Observation 4fcbcc81-8f05-4a6a-bb5a-b19b36974ad4 · inbound

Forest without Trees is still Fruitful: Constraints on the thermal state of the neutral IGM at $z\approx5.6$ with the 21-cm forest power spectrum cites this paper.

Forest without Trees is still Fruitful: Constraints on the thermal state of the neutral IGM at $z\approx5.6$ with the 21-cm forest power spectrum The Phase II Murchison Widefield Array: Design Overview

Reference 142

Resolution
unresolved
no resolver link, observed 2026-08-01T23:44:19.866904Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T23:44:19.866904Z digest=sha256:7b0ea31a2e88e983028ee317c4e84dc2c1532b40c61a37463d1ca5ebbbb497c2

Observation e6785e11-fb74-4d2e-bf51-401311c4f148 · inbound

The Study of Quasi-Periodic Pulsations in Solar and Stellar Flares with SKA cites this paper.

The Study of Quasi-Periodic Pulsations in Solar and Stellar Flares with SKA The Phase II Murchison Widefield Array: Design Overview

Reference 112

Resolution
unresolved
no resolver link, observed 2026-07-31T22:27:31.712000Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-31T22:27:31.712000Z digest=sha256:71af8d532aeee8141ecd7663b0618581600a7fdee11c901bd6aef4cd0e822a44