Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links, observed 2026-07-11T11:50:26.030339Z
Paper Citation Record · LEDGER
The Murchison Widefield Array Phase III upgrade: Sensitivity Doubled, Number of Baselines Quadrupled, Flexibility Enhanced, and EoR Observations Optimised
As of 11 August 2026, this Paper Citation Record lists 68 of 68 outbound references and 0 inbound Pith citation observations for arXiv:2606.01644.
A citation records a reference. It does not transfer a finding from one paper to another.
Coverage vector
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-11T06:34:44.6726+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links
A source-named dated measurement, never combined with another source.
Source: cited_works
Reference resolution
68 of 68 outbound references displayed
- verified exact51
- verified fuzzy0
- unresolved5
- parse uncertain0
- malformed identifier0
- metadata mismatch12
External citation measurements
No source-named external measurement is stored.
Outbound references
Observation ad3e8d02-d2d0-4629-9420-2e77c8cf126c · outbound
This paper cites The Murchison Widefield Array: the Square Kilometre Array Precursor at low radio frequencies.
The Murchison Widefield Array Phase III upgrade: Sensitivity Doubled, Number of Baselines Quadrupled, Flexibility Enhanced, and EoR Observations Optimised The Murchison Widefield Array: the Square Kilometre Array Precursor at low radio frequencies
Reference 1
- Resolution
- verified exact
- local_arxiv, observed 2026-06-28T13:12:13.530896Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation 43f02511-9994-451b-9d6b-8db691ecf2b6 · outbound
This paper cites LOFAR: The LOw-Frequency ARray.
The Murchison Widefield Array Phase III upgrade: Sensitivity Doubled, Number of Baselines Quadrupled, Flexibility Enhanced, and EoR Observations Optimised LOFAR: The LOw-Frequency ARray
Reference 2
- Resolution
- metadata mismatch
- local_arxiv, observed 2026-06-28T13:12:13.546232Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation ff2b94de-eae5-4be6-b760-016d1d96ac4a · outbound
This paper cites and Hall, Peter J.
The Murchison Widefield Array Phase III upgrade: Sensitivity Doubled, Number of Baselines Quadrupled, Flexibility Enhanced, and EoR Observations Optimised and Hall, Peter J
Reference 3
- Resolution
- unresolved
- no resolver link, observed 2026-06-28T13:07:48.528000Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 8df5f3e0-470c-4ab4-9447-9a855a020b64 · outbound
This paper cites Science with ASKAP - the Australian Square Kilometre Array Pathfinder.
The Murchison Widefield Array Phase III upgrade: Sensitivity Doubled, Number of Baselines Quadrupled, Flexibility Enhanced, and EoR Observations Optimised Science with ASKAP - the Australian Square Kilometre Array Pathfinder
Reference 4
- Resolution
- verified exact
- local_arxiv, observed 2026-06-28T13:12:13.449589Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation 57b12dd2-7c92-451d-8186-112f97bb731e · outbound
This paper cites System overview and performance characteristics.
The Murchison Widefield Array Phase III upgrade: Sensitivity Doubled, Number of Baselines Quadrupled, Flexibility Enhanced, and EoR Observations Optimised System overview and performance characteristics
Reference 5
- Resolution
- verified exact
- doi, observed 2026-06-28T13:12:13.440433Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation 44888787-70e8-4ee5-a925-929f45ec1f13 · outbound
This paper cites Cosmology at Low Frequencies: The 21 cm Transition and the High-Redshift Universe.
The Murchison Widefield Array Phase III upgrade: Sensitivity Doubled, Number of Baselines Quadrupled, Flexibility Enhanced, and EoR Observations Optimised Cosmology at Low Frequencies: The 21 cm Transition and the High-Redshift Universe
Reference 6
- Resolution
- metadata mismatch
- local_arxiv, observed 2026-06-28T13:12:13.534661Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation 323767e8-da5b-47bb-b5b9-9f2870f17893 · outbound
This paper cites Science with the Murchison Widefield Array.
The Murchison Widefield Array Phase III upgrade: Sensitivity Doubled, Number of Baselines Quadrupled, Flexibility Enhanced, and EoR Observations Optimised Science with the Murchison Widefield Array
Reference 7
- Resolution
- verified exact
- local_arxiv, observed 2026-06-28T13:12:13.537021Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation c9febdf3-a990-446c-aefe-7c1de1cc6632 · outbound
This paper cites PASA , keywords =.
The Murchison Widefield Array Phase III upgrade: Sensitivity Doubled, Number of Baselines Quadrupled, Flexibility Enhanced, and EoR Observations Optimised PASA , keywords =
Reference 8
- Resolution
- verified exact
- doi, observed 2026-06-28T13:12:13.552654Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation 5b759ae5-bbfa-4960-9ced-a3303a54ba4d · outbound
This paper cites doi:10.1109/JPROC.2009.2017564 , eprint =.
The Murchison Widefield Array Phase III upgrade: Sensitivity Doubled, Number of Baselines Quadrupled, Flexibility Enhanced, and EoR Observations Optimised doi:10.1109/JPROC.2009.2017564 , eprint =
Reference 9
- Resolution
- verified exact
- arxiv_id, observed 2026-06-28T13:12:13.436969Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation 0765e772-9e83-4079-9ad0-26e518cf8074 · outbound
This paper cites The Phase II Murchison Widefield Array: Design Overview.
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 2026-08-11T06:34:44.6726+00:00.
Observation 4183228e-0b5f-4eca-9f23-dfd2e8f5e998 · outbound
This paper cites and Ekers, Ronald D.
The Murchison Widefield Array Phase III upgrade: Sensitivity Doubled, Number of Baselines Quadrupled, Flexibility Enhanced, and EoR Observations Optimised and Ekers, Ronald D
Reference 11
- Resolution
- verified exact
- doi, observed 2026-06-28T13:12:13.432922Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation b1de8889-86a5-464d-85c9-8a9d14fc26e9 · outbound
This paper cites Characterisation of the ionosphere above the Murchison Radio Observatory using the Murchison Widefield Array.
The Murchison Widefield Array Phase III upgrade: Sensitivity Doubled, Number of Baselines Quadrupled, Flexibility Enhanced, and EoR Observations Optimised Characterisation of the ionosphere above the Murchison Radio Observatory using the Murchison Widefield Array
Reference 12
- Resolution
- verified exact
- local_arxiv, observed 2026-06-28T13:12:13.431201Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation 98cc1ec6-ca08-477c-b28c-563f1a0c1820 · outbound
This paper cites DiFX: A software correlator for very long baseline interferometry using multi-processor computing environments.
The Murchison Widefield Array Phase III upgrade: Sensitivity Doubled, Number of Baselines Quadrupled, Flexibility Enhanced, and EoR Observations Optimised DiFX: A software correlator for very long baseline interferometry using multi-processor computing environments
Reference 13
- Resolution
- verified exact
- local_arxiv, observed 2026-06-28T13:12:13.443046Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation c7d7e193-7ea4-4658-9642-dd34f4050829 · outbound
This paper cites Experimental Astronomy , keywords =.
The Murchison Widefield Array Phase III upgrade: Sensitivity Doubled, Number of Baselines Quadrupled, Flexibility Enhanced, and EoR Observations Optimised Experimental Astronomy , keywords =
Reference 14
- Resolution
- verified exact
- doi, observed 2026-06-28T13:12:13.452777Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation c9ec84c6-1bb0-42bc-a88e-3546ab60b0e3 · outbound
This paper cites The Murchison Widefield Array Correlator.
The Murchison Widefield Array Phase III upgrade: Sensitivity Doubled, Number of Baselines Quadrupled, Flexibility Enhanced, and EoR Observations Optimised The Murchison Widefield Array Correlator
Reference 15
- Resolution
- verified exact
- local_arxiv, observed 2026-06-28T13:12:13.490060Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation 9c8aa9ce-34c7-4e79-8df8-1005aa8978b9 · outbound
This paper cites A Digital-Receiver for the Murchison Widefield Array.
The Murchison Widefield Array Phase III upgrade: Sensitivity Doubled, Number of Baselines Quadrupled, Flexibility Enhanced, and EoR Observations Optimised A Digital-Receiver for the Murchison Widefield Array
Reference 16
- Resolution
- metadata mismatch
- local_arxiv, observed 2026-06-28T13:12:13.573754Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation 87f2ad43-a94c-4785-9164-55292f8ae48c · outbound
This paper cites A GPU based real-time software correlation system for the Murchison Widefield Array prototype.
The Murchison Widefield Array Phase III upgrade: Sensitivity Doubled, Number of Baselines Quadrupled, Flexibility Enhanced, and EoR Observations Optimised A GPU based real-time software correlation system for the Murchison Widefield Array prototype
Reference 17
- Resolution
- verified exact
- local_arxiv, observed 2026-06-28T13:12:13.571475Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation e25de76a-4bde-495e-8aa9-47902a1d88d2 · outbound
This paper cites The High Time and Frequency Resolution Capabilities of the Murchison Widefield Array.
The Murchison Widefield Array Phase III upgrade: Sensitivity Doubled, Number of Baselines Quadrupled, Flexibility Enhanced, and EoR Observations Optimised The High Time and Frequency Resolution Capabilities of the Murchison Widefield Array
Reference 18
- Resolution
- verified exact
- local_arxiv, observed 2026-06-28T13:12:13.564433Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation 478c703e-dde0-4684-889a-19bec2adcaf2 · outbound
This paper cites S., Crosse, B., Sleap, G., et al.
The Murchison Widefield Array Phase III upgrade: Sensitivity Doubled, Number of Baselines Quadrupled, Flexibility Enhanced, and EoR Observations Optimised S., Crosse, B., Sleap, G., et al
Reference 19
- Resolution
- verified exact
- doi, observed 2026-06-28T13:12:13.557088Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation 34a81415-5476-4525-bed8-d9546fbf1dde · outbound
This paper cites Monthly Notices of the Royal Astronomical Society , volume =.
The Murchison Widefield Array Phase III upgrade: Sensitivity Doubled, Number of Baselines Quadrupled, Flexibility Enhanced, and EoR Observations Optimised Monthly Notices of the Royal Astronomical Society , volume =
Reference 20
- Resolution
- verified exact
- doi, observed 2026-06-28T13:12:13.566151Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation 95d2c9b2-f52a-4fd8-b906-06f755c6fc12 · outbound
This paper cites R., Galvin, T.
Reference 21
- Resolution
- metadata mismatch
- doi, observed 2026-06-28T13:12:13.555150Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation e3ada85a-1ae5-47be-ba97-6e10af34b718 · outbound
This paper cites and Shibahashi , H.
The Murchison Widefield Array Phase III upgrade: Sensitivity Doubled, Number of Baselines Quadrupled, Flexibility Enhanced, and EoR Observations Optimised and Shibahashi , H
Reference 22
- Resolution
- metadata mismatch
- arxiv_id, observed 2026-06-28T13:12:13.568669Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation 86bdb201-0131-4525-afa2-3153a1bdf2aa · outbound
This paper cites A 189 MHz, 2400 square degree polarization survey with the Murchison Widefield Array 32-element prototype.
The Murchison Widefield Array Phase III upgrade: Sensitivity Doubled, Number of Baselines Quadrupled, Flexibility Enhanced, and EoR Observations Optimised A 189 MHz, 2400 square degree polarization survey with the Murchison Widefield Array 32-element prototype
Reference 23
- Resolution
- verified exact
- local_arxiv, observed 2026-06-28T13:12:13.548672Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation 94b99a0d-c78c-4445-9547-adf721e2b01a · outbound
This paper cites A survey for transients and variables with the Murchison Widefield Array 32-tile prototype at 154 MHz.
The Murchison Widefield Array Phase III upgrade: Sensitivity Doubled, Number of Baselines Quadrupled, Flexibility Enhanced, and EoR Observations Optimised A survey for transients and variables with the Murchison Widefield Array 32-tile prototype at 154 MHz
Reference 24
- Resolution
- verified exact
- local_arxiv, observed 2026-06-28T13:12:13.541638Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation 70fea82b-3ffc-4a6d-a495-69cccdf3afcb · outbound
This paper cites Interferometric imaging with the 32 element Murchison Wide-field Array.
The Murchison Widefield Array Phase III upgrade: Sensitivity Doubled, Number of Baselines Quadrupled, Flexibility Enhanced, and EoR Observations Optimised Interferometric imaging with the 32 element Murchison Wide-field Array
Reference 25
- Resolution
- verified exact
- local_arxiv, observed 2026-06-28T13:12:13.551026Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation 5a88a644-2e0d-45a6-96e5-dd820132b26a · outbound
This paper cites Low Frequency Imaging of Fields at High Galactic Latitude with the Murchison Widefield Array 32-Element Prototype.
The Murchison Widefield Array Phase III upgrade: Sensitivity Doubled, Number of Baselines Quadrupled, Flexibility Enhanced, and EoR Observations Optimised Low Frequency Imaging of Fields at High Galactic Latitude with the Murchison Widefield Array 32-Element Prototype
Reference 26
- Resolution
- verified exact
- local_arxiv, observed 2026-06-28T13:12:13.521651Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation 58de3723-0f8e-4aa1-b0b2-7b3a1c72d741 · outbound
This paper cites First Spectroscopic Imaging Observations of the Sun at Low Radio Frequencies with the Murchison Widefield Array Prototype.
The Murchison Widefield Array Phase III upgrade: Sensitivity Doubled, Number of Baselines Quadrupled, Flexibility Enhanced, and EoR Observations Optimised First Spectroscopic Imaging Observations of the Sun at Low Radio Frequencies with the Murchison Widefield Array Prototype
Reference 27
- Resolution
- metadata mismatch
- local_arxiv, observed 2026-06-28T13:12:13.526038Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation ce337140-a32c-4867-8eed-a387fe8ec76d · outbound
This paper cites The Murchison Widefield Array Commissioning Survey: A Low-Frequency Catalogue of 14,110 Compact Radio Sources over 6,100 Square Degrees.
The Murchison Widefield Array Phase III upgrade: Sensitivity Doubled, Number of Baselines Quadrupled, Flexibility Enhanced, and EoR Observations Optimised The Murchison Widefield Array Commissioning Survey: A Low-Frequency Catalogue of 14,110 Compact Radio Sources over 6,100 Square Degrees
Reference 28
- Resolution
- verified exact
- local_arxiv, observed 2026-06-28T13:12:13.528647Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation c46a6a74-e2a9-4bff-970c-d70087b3de4f · outbound
This paper cites FAIR standards for astronomical data.
The Murchison Widefield Array Phase III upgrade: Sensitivity Doubled, Number of Baselines Quadrupled, Flexibility Enhanced, and EoR Observations Optimised FAIR standards for astronomical data
Reference 29
- Resolution
- verified exact
- arxiv_id, observed 2026-06-28T13:12:13.544011Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation f645541c-64ba-4d44-8d2c-6ec3cae57531 · outbound
This paper cites Optimising NGAS for the MWA Archive.
The Murchison Widefield Array Phase III upgrade: Sensitivity Doubled, Number of Baselines Quadrupled, Flexibility Enhanced, and EoR Observations Optimised Optimising NGAS for the MWA Archive
Reference 30
- Resolution
- metadata mismatch
- local_arxiv, observed 2026-06-28T13:12:13.559207Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation 5e02d333-1dcc-4e12-b613-3f28617e0abd · outbound
This paper cites GaLactic and Extragalactic All-sky Murchison Widefield Array (GLEAM) survey I: A low-frequency extragalactic catalogue.
The Murchison Widefield Array Phase III upgrade: Sensitivity Doubled, Number of Baselines Quadrupled, Flexibility Enhanced, and EoR Observations Optimised GaLactic and Extragalactic All-sky Murchison Widefield Array (GLEAM) survey I: A low-frequency extragalactic catalogue
Reference 31
- Resolution
- verified exact
- local_arxiv, observed 2026-06-28T13:12:13.579732Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation ebc73d81-5c26-41fd-a7f4-9f8bfb458020 · outbound
This paper cites GLEAM: The GaLactic and Extragalactic All-sky MWA survey.
The Murchison Widefield Array Phase III upgrade: Sensitivity Doubled, Number of Baselines Quadrupled, Flexibility Enhanced, and EoR Observations Optimised GLEAM: The GaLactic and Extragalactic All-sky MWA survey
Reference 32
- Resolution
- verified exact
- local_arxiv, observed 2026-06-28T13:12:13.576382Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation 5e97ff49-44ca-457a-b596-0ac87eb55b2d · outbound
This paper cites PASA , keywords =.
The Murchison Widefield Array Phase III upgrade: Sensitivity Doubled, Number of Baselines Quadrupled, Flexibility Enhanced, and EoR Observations Optimised PASA , keywords =
Reference 33
- Resolution
- verified exact
- doi, observed 2026-06-28T13:12:13.438682Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation d888bdd7-b846-4dec-aee8-af23b1d9e562 · outbound
This paper cites keywords =.
Reference 34
- Resolution
- verified exact
- doi, observed 2026-06-28T13:12:13.434519Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation feb7c6bd-827a-4492-8f0b-d24e451fad5e · outbound
This paper cites 2022, Nature, 601, 526, doi: 10.1038/s41586-021-04272-x.
The Murchison Widefield Array Phase III upgrade: Sensitivity Doubled, Number of Baselines Quadrupled, Flexibility Enhanced, and EoR Observations Optimised 2022, Nature, 601, 526, doi: 10.1038/s41586-021-04272-x
Reference 35
- Resolution
- verified exact
- doi, observed 2026-06-28T13:12:13.487506Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation ce7d7c7e-7f6a-4ffa-8541-96e4cc0698b3 · outbound
This paper cites J., et al.
Reference 36
- Resolution
- verified exact
- doi, observed 2026-06-28T13:12:13.509841Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation 98cb27cb-6ec9-4651-9628-4f40bab9b0d3 · outbound
This paper cites J., Franzen, T.
Reference 37
- Resolution
- verified exact
- doi, observed 2026-06-28T13:12:13.511493Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation 4ae43bae-0688-4b23-9421-127346532a7c · outbound
This paper cites Scientific Reports , year = 2018, month =.
The Murchison Widefield Array Phase III upgrade: Sensitivity Doubled, Number of Baselines Quadrupled, Flexibility Enhanced, and EoR Observations Optimised Scientific Reports , year = 2018, month =
Reference 38
- Resolution
- verified exact
- doi, observed 2026-06-28T13:12:13.513146Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation 2defcb72-cbc7-46e7-8637-7751e6a49d50 · outbound
This paper cites , keywords =.
Reference 39
- Resolution
- verified exact
- doi, observed 2026-06-28T13:12:13.503004Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation 66845c9e-5c4e-485b-8ae7-1f30f41ab62e · outbound
This paper cites First Season MWA EoR Power Spectrum Results at Redshift 7.
The Murchison Widefield Array Phase III upgrade: Sensitivity Doubled, Number of Baselines Quadrupled, Flexibility Enhanced, and EoR Observations Optimised First Season MWA EoR Power Spectrum Results at Redshift 7
Reference 40
- Resolution
- verified exact
- local_arxiv, observed 2026-06-28T13:12:13.508114Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation a6569d87-03a4-49a8-85fe-53b389f694b5 · outbound
This paper cites Overcoming real-world obstacles in 21 cm power spectrum estimation: A method demonstration and results from early Murchison Widefield Array data.
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 2026-08-11T06:34:44.6726+00:00.
Observation 113076fa-cc53-4638-9482-cf9e0c502f14 · outbound
This paper cites Spectral Flattening at Low Frequencies in Crab Giant Pulses.
The Murchison Widefield Array Phase III upgrade: Sensitivity Doubled, Number of Baselines Quadrupled, Flexibility Enhanced, and EoR Observations Optimised Spectral Flattening at Low Frequencies in Crab Giant Pulses
Reference 42
- Resolution
- verified exact
- local_arxiv, observed 2026-06-28T13:12:13.492459Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation 1c2167f4-86eb-4996-857f-b637f97bc658 · outbound
This paper cites Real-time imaging of density ducts between the plasmasphere and ionosphere.
The Murchison Widefield Array Phase III upgrade: Sensitivity Doubled, Number of Baselines Quadrupled, Flexibility Enhanced, and EoR Observations Optimised Real-time imaging of density ducts between the plasmasphere and ionosphere
Reference 43
- Resolution
- metadata mismatch
- local_arxiv, observed 2026-06-28T13:12:13.500720Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation 7f942504-6e6d-4a6f-bbf7-a923ba36f4ce · outbound
This paper cites 2013 International Conference on Electromagnetics in Advanced Applications (ICEAA , year = 2013, month =.
The Murchison Widefield Array Phase III upgrade: Sensitivity Doubled, Number of Baselines Quadrupled, Flexibility Enhanced, and EoR Observations Optimised 2013 International Conference on Electromagnetics in Advanced Applications (ICEAA , year = 2013, month =
Reference 44
- Resolution
- verified exact
- arxiv_id, observed 2026-06-28T13:12:13.505578Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation d7ddeaab-a507-44a3-b314-c38c13777018 · outbound
This paper cites IEEE Transactions on Antennas and Propagation , keywords =.
The Murchison Widefield Array Phase III upgrade: Sensitivity Doubled, Number of Baselines Quadrupled, Flexibility Enhanced, and EoR Observations Optimised IEEE Transactions on Antennas and Propagation , keywords =
Reference 45
- Resolution
- verified exact
- arxiv_id, observed 2026-06-28T13:12:13.518754Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation a0f29b42-3143-4b78-9d5e-000e8810abbe · outbound
This paper cites The Engineering Development Array: A low frequency radio telescope utilising SKA precursor technology.
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 2026-08-11T06:34:44.6726+00:00.
Observation 18e3f3c7-3986-4e3f-8c01-13d382f23254 · outbound
This paper cites A&A , keywords =.
Reference 47
- Resolution
- verified exact
- doi, observed 2026-06-28T13:12:13.581986Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation 025b4ffa-ea68-470a-9890-8ed7d03b89e9 · outbound
This paper cites 2022, NewA, 8, 011010, doi: 10.1117/1.JATIS.8.1.011010.
The Murchison Widefield Array Phase III upgrade: Sensitivity Doubled, Number of Baselines Quadrupled, Flexibility Enhanced, and EoR Observations Optimised 2022, NewA, 8, 011010, doi: 10.1117/1.JATIS.8.1.011010
Reference 48
- Resolution
- metadata mismatch
- doi, observed 2026-06-28T13:12:13.454430Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation b9fcb9f7-7607-44c7-8046-c6b2591a7845 · outbound
This paper cites Journal of Astronomical Telescopes, Instruments, and Systems , keywords =.
The Murchison Widefield Array Phase III upgrade: Sensitivity Doubled, Number of Baselines Quadrupled, Flexibility Enhanced, and EoR Observations Optimised Journal of Astronomical Telescopes, Instruments, and Systems , keywords =
Reference 49
- Resolution
- verified exact
- doi, observed 2026-06-28T13:12:13.470911Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation bd79f42d-1e3e-4f93-a390-858ece077e06 · outbound
This paper cites Cobalt: A GPU-based correlator and beamformer for LOFAR.
The Murchison Widefield Array Phase III upgrade: Sensitivity Doubled, Number of Baselines Quadrupled, Flexibility Enhanced, and EoR Observations Optimised Cobalt: A GPU-based correlator and beamformer for LOFAR
Reference 50
- Resolution
- metadata mismatch
- local_arxiv, observed 2026-06-28T13:12:13.478540Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation 18244442-148d-416e-8079-4eb75c538216 · outbound
This paper cites Galaxies , keywords =.
The Murchison Widefield Array Phase III upgrade: Sensitivity Doubled, Number of Baselines Quadrupled, Flexibility Enhanced, and EoR Observations Optimised Galaxies , keywords =
Reference 51
- Resolution
- verified exact
- doi, observed 2026-06-28T13:12:13.480311Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation 35630e89-562f-4ed7-90d5-4059e04de46a · outbound
This paper cites doi:10.1017/pasa.2020.17 , keywords =.
The Murchison Widefield Array Phase III upgrade: Sensitivity Doubled, Number of Baselines Quadrupled, Flexibility Enhanced, and EoR Observations Optimised doi:10.1017/pasa.2020.17 , keywords =
Reference 52
- Resolution
- verified exact
- doi, observed 2026-06-28T13:12:13.467088Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation 58e19983-6b3c-4d2a-9fc1-231583a22a4f · outbound
This paper cites an unresolved cited work.
The Murchison Widefield Array Phase III upgrade: Sensitivity Doubled, Number of Baselines Quadrupled, Flexibility Enhanced, and EoR Observations Optimised Unresolved cited work
Reference 53
- Resolution
- unresolved
- no resolver link, observed 2026-06-28T13:07:48.528000Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 207a89bb-0ed8-4f95-b3e4-70022111f9b3 · outbound
This paper cites PASP , keywords =.
The Murchison Widefield Array Phase III upgrade: Sensitivity Doubled, Number of Baselines Quadrupled, Flexibility Enhanced, and EoR Observations Optimised PASP , keywords =
Reference 54
- Resolution
- verified exact
- doi, observed 2026-06-28T13:12:13.481914Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation 13beac92-d717-438c-b30e-92a37fe6e4e6 · outbound
This paper cites 2016, in MeerKAT Science: On the Pathway to the SKA, 1, doi: 10.22323/1.277.0001.
The Murchison Widefield Array Phase III upgrade: Sensitivity Doubled, Number of Baselines Quadrupled, Flexibility Enhanced, and EoR Observations Optimised 2016, in MeerKAT Science: On the Pathway to the SKA, 1, doi: 10.22323/1.277.0001
Reference 55
- Resolution
- verified exact
- doi, observed 2026-06-28T13:12:13.447234Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation 72f5a7b9-d53d-41ea-9cbd-a75c9ba305f4 · outbound
This paper cites Current Science , year = 2017, month = aug, volume =.
The Murchison Widefield Array Phase III upgrade: Sensitivity Doubled, Number of Baselines Quadrupled, Flexibility Enhanced, and EoR Observations Optimised Current Science , year = 2017, month = aug, volume =
Reference 56
- Resolution
- verified exact
- doi, observed 2026-06-28T13:12:13.462913Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation 1fb1c434-b573-4bab-8d3b-d35204f4f998 · outbound
This paper cites 2015 International Conference on Antenna Theory and Techniques (ICATT , year = 2015, month = jun, eid =.
The Murchison Widefield Array Phase III upgrade: Sensitivity Doubled, Number of Baselines Quadrupled, Flexibility Enhanced, and EoR Observations Optimised 2015 International Conference on Antenna Theory and Techniques (ICATT , year = 2015, month = jun, eid =
Reference 57
- Resolution
- verified exact
- arxiv_id, observed 2026-06-28T13:12:13.465388Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation 3e6b417f-a383-49e6-8438-cfb77da5975a · outbound
This paper cites Advanced Maui Optical and Space Surveillance Technologies Conference , year = 2010, editor =.
The Murchison Widefield Array Phase III upgrade: Sensitivity Doubled, Number of Baselines Quadrupled, Flexibility Enhanced, and EoR Observations Optimised Advanced Maui Optical and Space Surveillance Technologies Conference , year = 2010, editor =
Reference 58
- Resolution
- unresolved
- no resolver link, observed 2026-06-28T13:07:48.528000Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 4937b89c-dd85-4269-a31d-9e5b71d97566 · outbound
This paper cites PASA , keywords =.
The Murchison Widefield Array Phase III upgrade: Sensitivity Doubled, Number of Baselines Quadrupled, Flexibility Enhanced, and EoR Observations Optimised PASA , keywords =
Reference 59
- Resolution
- verified exact
- doi, observed 2026-06-28T13:12:13.469103Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation dbde5249-cd70-4da6-b5ea-f3dd4a786293 · outbound
This paper cites PASA , keywords =.
The Murchison Widefield Array Phase III upgrade: Sensitivity Doubled, Number of Baselines Quadrupled, Flexibility Enhanced, and EoR Observations Optimised PASA , keywords =
Reference 60
- Resolution
- verified exact
- arxiv_id, observed 2026-06-28T13:12:13.473224Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation 0ce36937-efc7-469a-a731-5fce35f5a3af · outbound
This paper cites and Null, Dev and Trott, Cathryn M.
The Murchison Widefield Array Phase III upgrade: Sensitivity Doubled, Number of Baselines Quadrupled, Flexibility Enhanced, and EoR Observations Optimised and Null, Dev and Trott, Cathryn M
Reference 61
- Resolution
- unresolved
- no resolver link, observed 2026-06-28T13:07:48.528000Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 8b18905d-18a4-4b1c-a26c-4d44e33b6c93 · outbound
This paper cites CHIPS: The Cosmological HI Power Spectrum Estimator.
The Murchison Widefield Array Phase III upgrade: Sensitivity Doubled, Number of Baselines Quadrupled, Flexibility Enhanced, and EoR Observations Optimised CHIPS: The Cosmological HI Power Spectrum Estimator
Reference 62
- Resolution
- verified exact
- local_arxiv, observed 2026-06-28T13:12:13.485854Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation 409046d4-f573-432a-be5b-89b7eff08fdb · outbound
This paper cites D., Null, D., Trott, C.
The Murchison Widefield Array Phase III upgrade: Sensitivity Doubled, Number of Baselines Quadrupled, Flexibility Enhanced, and EoR Observations Optimised D., Null, D., Trott, C
Reference 63
- Resolution
- verified exact
- doi, observed 2026-06-28T13:12:13.456173Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation 30e2bcef-09b6-4530-8926-32ac9a08827a · outbound
This paper cites Canadian Hydrogen Intensity Mapping Experiment (CHIME) Pathfinder.
The Murchison Widefield Array Phase III upgrade: Sensitivity Doubled, Number of Baselines Quadrupled, Flexibility Enhanced, and EoR Observations Optimised Canadian Hydrogen Intensity Mapping Experiment (CHIME) Pathfinder
Reference 64
- Resolution
- metadata mismatch
- local_arxiv, observed 2026-06-28T13:12:13.461115Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation 80893824-43ba-46e3-ad62-145e240e8b4c · outbound
This paper cites Radio Sources in the NCP Region Observed with the 21 Centimeter Array.
The Murchison Widefield Array Phase III upgrade: Sensitivity Doubled, Number of Baselines Quadrupled, Flexibility Enhanced, and EoR Observations Optimised Radio Sources in the NCP Region Observed with the 21 Centimeter Array
Reference 65
- Resolution
- verified exact
- local_arxiv, observed 2026-06-28T13:12:13.458708Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation 4987ba63-5453-49ad-9a7c-1e86736b0d09 · outbound
This paper cites In Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series.
The Murchison Widefield Array Phase III upgrade: Sensitivity Doubled, Number of Baselines Quadrupled, Flexibility Enhanced, and EoR Observations Optimised In Society of Photo-Optical Instrumentation Engineers (SPIE) Conference Series
Reference 66
- Resolution
- metadata mismatch
- doi, observed 2026-06-28T13:12:13.483551Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation c1f28192-a06f-437e-9d67-b1beb6f2cf91 · outbound
This paper cites keywords =.
Reference 67
- Resolution
- verified exact
- doi, observed 2026-06-28T13:12:13.451211Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.
Observation 63442b27-bd13-47c4-91ba-91aa583c7fdf · outbound
This paper cites and Sarma, V.V.
Reference 68
- Resolution
- unresolved
- no resolver link, observed 2026-06-28T13:07:48.528000Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Pith citing papers
No inbound Pith citation observations are available.