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Paper Citation Record · LEDGER

Overcoming real-world obstacles in 21 cm power spectrum estimation: A method demonstration and results from early Murchison Widefield Array data

As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:1304.4229.

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

pith.paper-citation-record.v1
1304.4229 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 2026-08-10T06:31:04.303077+00:00

measured 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T22:22:30.384797Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-10T17:37:25.723030Z

Reference resolution

0 of 0 outbound references displayed

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  • verified fuzzy0
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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 a6569d87-03a4-49a8-85fe-53b389f694b5 · 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 Overcoming real-world obstacles in 21 cm power spectrum estimation: A method demonstration and results from early Murchison Widefield Array data

Reference 41

Resolution
verified exact
local_arxiv, observed 2026-06-28T13:12:13.495661Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:e28a51d6f47fa69e35f0ef792aca92a15fcb30bebeeb77052dd205bd53c56499

Observation 2a328730-4efe-4a32-b63c-c1e84318fcf3 · 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 Overcoming real-world obstacles in 21 cm power spectrum estimation: A method demonstration and results from early Murchison Widefield Array data

Reference 169

Resolution
verified exact
local_arxiv, observed 2026-06-25T19:08:13.942419Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:2ab42c8b84385e03d0e525bd88ebfd7d4379c7df4190f9491e0946ed4745e7af

Observation b4ae4b8e-3427-4849-9cc3-0d4fa63e55b3 · inbound

Intensity fluctuations of radio halo in galaxy cluster: Insights from power spectrum estimation cites this paper.

Intensity fluctuations of radio halo in galaxy cluster: Insights from power spectrum estimation Overcoming real-world obstacles in 21 cm power spectrum estimation: A method demonstration and results from early Murchison Widefield Array data

Reference 124

Resolution
verified exact
local_arxiv, observed 2026-07-10T17:37:25.724343Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:d86b7d970921f47a2860ce434fd4a1667633adb0573f84d842e21ef47fafa9ca

Observation 931bb6c2-0819-4e25-9730-b4cf98461b5e · inbound

Investigating radio source population $\&$ spatial characteristics of diffuse Galactic synchrotron emission in the GAMA-23 field with uGMRT Band-3 cites this paper.

Investigating radio source population $\&$ spatial characteristics of diffuse Galactic synchrotron emission in the GAMA-23 field with uGMRT Band-3 Overcoming real-world obstacles in 21 cm power spectrum estimation: A method demonstration and results from early Murchison Widefield Array data

Reference 157

Resolution
unresolved
no resolver link, observed 2026-08-07T22:22:30.384797Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T22:22:30.384797Z digest=sha256:ac7175dc7b7aa97500b5708daa7310062b9b45773be0f56bac3df3b20878ae51