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Paper Citation Record · LEDGER

All-sky Galactic radiation at 45 MHz and spectral index between 45 and 408 MHz

As of 19 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:1011.4298.

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

pith.paper-citation-record.v1
1011.4298 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 5 of 5 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-18T06:34:40.430872+00:00

measured 5 of 5 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-04T19:14:20.688557Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-06-25T23:08:41.527284Z

Reference resolution

0 of 0 outbound references displayed

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

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 f14ccdbe-08f3-43f9-afd2-b3e082f241e7 · inbound

Axion-Photon Conversion in FLRW with Primordial Magnetic Fields: Explaining the Radio Excess cites this paper.

Axion-Photon Conversion in FLRW with Primordial Magnetic Fields: Explaining the Radio Excess All-sky Galactic radiation at 45 MHz and spectral index between 45 and 408 MHz

Reference 15

Resolution
unresolved
no resolver link, observed 2026-08-04T19:14:20.688557Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-04T19:14:20.688557Z digest=sha256:c6f7661cacf76a51769538c59ee0772387f435fa3947a0a42eb9010414d3674b

Observation 00cdb408-d210-4d75-a9dc-2cdbf89622ae · inbound

Constraints on Primordial Black Holes from Galactic Diffuse Synchrotron Emissions cites this paper.

Constraints on Primordial Black Holes from Galactic Diffuse Synchrotron Emissions All-sky Galactic radiation at 45 MHz and spectral index between 45 and 408 MHz

Reference 160

Resolution
verified exact
local_arxiv, observed 2026-05-16T11:00:52.103820Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=pdf_text observed=2026-05-16T10:58:02.187531Z digest=sha256:de31b68a3f09840fcd2fb7d2f7335d92a33ceb614e39bc1851a0fbcdf701a160

Observation 3bf59680-1eb2-4ad3-bc67-9a27ddd58148 · inbound

Nested Fermi and eROSITA bubbles require very similar $\sim10^{56}$ erg collimated Galactic-center outbursts; their asymmetry indicates an eastern density gradient cites this paper.

Nested Fermi and eROSITA bubbles require very similar $\sim10^{56}$ erg collimated Galactic-center outbursts; their asymmetry indicates an eastern density gradient All-sky Galactic radiation at 45 MHz and spectral index between 45 and 408 MHz

Reference 31

Resolution
verified exact
local_arxiv, observed 2026-05-16T09:10:47.277433Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=pdf_text observed=2026-05-16T09:10:43.109855Z digest=sha256:c650cd540756761902f5673ac21bf78d66a40dd91dba24b1f6b49444127a1494

Observation 6fd3d1d3-bbc5-4527-9ec0-3557f2647518 · inbound

A comparison between Galactic magnetic field models and polarized synchrotron emission with C-BASS at 4.76 GHz and S-PASS at 2.3 GHz cites this paper.

A comparison between Galactic magnetic field models and polarized synchrotron emission with C-BASS at 4.76 GHz and S-PASS at 2.3 GHz All-sky Galactic radiation at 45 MHz and spectral index between 45 and 408 MHz

Reference 194

Resolution
metadata mismatch
local_arxiv, observed 2026-05-25T03:56:35.804357Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:8248cd9b52eeb5f9a52f9d6a65eed5a1980df4b8628d728d78166b099e429d36

Observation a4093dcf-30cc-4a89-a78a-cc92a16eaf67 · inbound

Early phases of star formation with SKAO: synchrotron emission from dense starless cores in molecular clouds cites this paper.

Early phases of star formation with SKAO: synchrotron emission from dense starless cores in molecular clouds All-sky Galactic radiation at 45 MHz and spectral index between 45 and 408 MHz

Reference 180

Resolution
metadata mismatch
local_arxiv, observed 2026-06-25T23:08:41.528643Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:c4f0e99380724f5dc3790b09dc7b6a5fc796031ca63287814f7ed152c57c3278