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Paper Citation Record · LEDGER

Broadband Intensity Tomography: Spectral Tagging of the Cosmic UV Background

As of 12 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1810.00885.

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

pith.paper-citation-record.v1
1810.00885 v2

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 2026-08-12T06:34:41.77262+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-01T21:31:40.279405Z

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

42
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 20d3d69f-9162-4685-a826-15b87c110d0b · inbound

Measuring cosmic bulk flow with kinetic Sunyaev-Zel'dovich velocity reconstruction cites this paper.

Measuring cosmic bulk flow with kinetic Sunyaev-Zel'dovich velocity reconstruction Broadband Intensity Tomography: Spectral Tagging of the Cosmic UV Background

Reference 85

Resolution
verified exact
arxiv_id, observed 2026-05-13T02:52:09.016615Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

source=pdf_text observed=2026-05-13T02:47:50.523877Z digest=sha256:d3b96102897cb7388517672e818c7f60e58feadac7ffbf7d3a6ce609a6568b9e

Observation cbf298f3-467b-4023-a14a-72f4ad386aa7 · inbound

Using SKAO to Understand the Clustering of Gravitational Wave Sources cites this paper.

Using SKAO to Understand the Clustering of Gravitational Wave Sources Broadband Intensity Tomography: Spectral Tagging of the Cosmic UV Background

Reference 58

Resolution
metadata mismatch
local_arxiv, observed 2026-06-25T23:08:41.209613Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:352d65a2d0cb0c95131d3e3b677efb1a04475933656a2946e6a0593c4354c6de

Observation a8cb7647-24a2-43ef-ab0a-ea8ba6532004 · inbound

Constraints on the remote quadrupole field from the polarized Sunyaev Zel'dovich effect cites this paper.

Constraints on the remote quadrupole field from the polarized Sunyaev Zel'dovich effect Broadband Intensity Tomography: Spectral Tagging of the Cosmic UV Background

Reference 61

Resolution
unresolved
no resolver link, observed 2026-08-01T21:31:40.279405Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T21:31:40.279405Z digest=sha256:acfd17280233ab8e336a876d7156aa74e66a738ae24405068dec07907c617127