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Paper Citation Record · LEDGER

Large-scale Array for Radio Astronomy on the Farside

As of 19 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 8 inbound Pith citation observations for arXiv:2403.16409.

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

pith.paper-citation-record.v1
2403.16409 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 2026-08-19T06:32:44.657259+00:00

measured 8 of 8 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-16T11:41:41.467042Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-04T11:59:50.117051Z

Reference resolution

0 of 0 outbound references displayed

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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 7cedcfcc-181d-4052-a455-7f03b1bf233e · inbound

Nonlinear reconstruction of 21cm global signal from 21cm power spectrum with artificial neural networks cites this paper.

Nonlinear reconstruction of 21cm global signal from 21cm power spectrum with artificial neural networks Large-scale Array for Radio Astronomy on the Farside

Reference 11

Resolution
unresolved
no resolver link, observed 2026-08-10T23:13:22.833946Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T23:13:22.833946Z digest=sha256:12c0afbb978bd16ee3654cc81445a103ea7982dd39b3a609dfed1745cbebc609

Observation c92031c6-1a3c-492b-8175-f3a3beb67bfd · inbound

Loop I/NPS morphology predictions in the ultralong-wavelength band cites this paper.

Loop I/NPS morphology predictions in the ultralong-wavelength band Large-scale Array for Radio Astronomy on the Farside

Reference 13

Resolution
unresolved
no resolver link, observed 2026-08-10T22:57:23.263689Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T22:57:23.263689Z digest=sha256:783c0b5df290e4ac764ace026404a0bbb82b791fd1f9fea8386801c59309e6e3

Observation 2f938d66-a863-40a8-b1e0-125a5562a680 · inbound

Sub-MHz Radio Background from Ultralight Dark Photon Dark Matter cites this paper.

Sub-MHz Radio Background from Ultralight Dark Photon Dark Matter Large-scale Array for Radio Astronomy on the Farside

Reference 63

Resolution
unresolved
no resolver link, observed 2026-08-10T22:40:43.510341Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T22:40:43.510341Z digest=sha256:1eed0b2a9df5d61e3ea96e757bd29a7b7d7a86b13a45584fca8dfe4f0c95343b

Observation 5f76a506-3ee7-478d-a6d4-c4ee60ba188f · inbound

Configuration Requirements for 21-cm Forest Background Quasar Searches with the Moon-based Interferometer cites this paper.

Configuration Requirements for 21-cm Forest Background Quasar Searches with the Moon-based Interferometer Large-scale Array for Radio Astronomy on the Farside

Reference 30

Resolution
unresolved
no resolver link, observed 2026-08-16T11:41:41.467042Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-16T11:41:41.467042Z digest=sha256:5aedfd4573bf1bc87c3d6da22632fcbdacccb9e936055b25b01934cfa14462c0

Observation 781c9fba-8f8f-4709-a5d7-e38b36b14d07 · inbound

Joint 21-cm and CMB Forecasts for Constraining Self-Interacting Massive Neutrinos cites this paper.

Joint 21-cm and CMB Forecasts for Constraining Self-Interacting Massive Neutrinos Large-scale Array for Radio Astronomy on the Farside

Reference 66

Resolution
unresolved
no resolver link, observed 2026-08-16T11:34:40.924416Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-16T11:34:40.924416Z digest=sha256:e2ff1d2e729f26460d840ea2c66b4b54556325446310ef04754997bfada48364

Observation cfae8147-0c83-4388-ac6d-25f8e95dfb46 · inbound

A Designer's Guide to Lunar Far-Side Interferometer Array: Power Spectrum Measurement and Cosmological Constraints from the Dark Ages cites this paper.

A Designer's Guide to Lunar Far-Side Interferometer Array: Power Spectrum Measurement and Cosmological Constraints from the Dark Ages Large-scale Array for Radio Astronomy on the Farside

Reference 32

Resolution
verified exact
arxiv_id, observed 2026-06-29T06:23:09.284806Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

source=pdf_text observed=2026-06-29T06:18:58.883095Z digest=sha256:458a525e055cb6757e90c17f572ec62bc5b4fb4865f9ac58996d82176de9c7ba

Observation f53876e0-5d9c-434e-b96f-f052a3b738f8 · inbound

Wedge-avoidance Fisher Forecasts for Primordial Non-Gaussianity from Dark-Ages 21-cm Power Spectrum and Bispectrum cites this paper.

Wedge-avoidance Fisher Forecasts for Primordial Non-Gaussianity from Dark-Ages 21-cm Power Spectrum and Bispectrum Large-scale Array for Radio Astronomy on the Farside

Reference 21

Resolution
verified exact
arxiv_id, observed 2026-07-04T11:59:50.119163Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

source=pdf_text observed=2026-06-26T07:29:58.947735Z digest=sha256:b6973033c2be1272f9a7182472a5b590249e43c745a49ba042ccc06405141a87

Observation f7325679-3bee-4dea-a18e-050508abad7f · inbound

Synthesis imaging with a lunar orbit array: III. Augmented lagrangian Multiplier Imaging using Gradient descent Optimization (AMIGO) cites this paper.

Synthesis imaging with a lunar orbit array: III. Augmented lagrangian Multiplier Imaging using Gradient descent Optimization (AMIGO) Large-scale Array for Radio Astronomy on the Farside

Reference 16

Resolution
unresolved
no resolver link, observed 2026-07-14T07:42:21.237160Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-07-14T07:42:21.237160Z digest=sha256:5bd2023f9f5b550d9de8b44a06b3769d1b2218f5843433f1a1c2f26039846989