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Paper Citation Record · LEDGER

The Importance of Wide-field Foreground Removal for 21 cm Cosmology: A Demonstration With Early MWA Epoch of Reionization Observations

As of 15 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1601.06177.

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

pith.paper-citation-record.v1
1601.06177 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 3 of 3 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-15T06:32:42.880941+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-01T12:40:13.067558Z

measured 1 of 1 external citation measurements

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

Source: pith, observed 2026-08-05T02:28:24.338817Z

Reference resolution

0 of 0 outbound references displayed

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

External citation measurements

93
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation bf576577-56bb-4333-9842-7e9981e5b171 · 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 Importance of Wide-field Foreground Removal for 21 cm Cosmology: A Demonstration With Early MWA Epoch of Reionization Observations

Reference 73

Resolution
metadata mismatch
local_arxiv, observed 2026-05-21T06:49:44.860073Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:58bb83a293e0a9c1087a25d9e2022df8bebd63f4c6014ffaff38afa26cf1b300

Observation 331fd2bd-16ee-40f0-b8aa-fe2adaa7e1d4 · 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 The Importance of Wide-field Foreground Removal for 21 cm Cosmology: A Demonstration With Early MWA Epoch of Reionization Observations

Reference 179

Resolution
verified exact
local_arxiv, observed 2026-07-10T17:37:25.727036Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:b0d176bf2f59df7fcc400f8bed8235b20ea56de3d3bba69cf2938f5f5558e6ba

Observation 25755673-e17d-4d1a-a0c9-d17a3e11c82b · inbound

Reading Between the Lines: Forward Modeling Dust, Continuum, and Spectral Cleaning for Multi-Line Intensity Mapping cites this paper.

Reading Between the Lines: Forward Modeling Dust, Continuum, and Spectral Cleaning for Multi-Line Intensity Mapping The Importance of Wide-field Foreground Removal for 21 cm Cosmology: A Demonstration With Early MWA Epoch of Reionization Observations

Reference 49

Resolution
unresolved
no resolver link, observed 2026-08-01T12:40:13.067558Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T12:40:13.067558Z digest=sha256:40d42b49c3a5b3f19a8a2eee13dce0d3e79bb924adfac2e660637b1e965a60fb