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Paper Citation Record · LEDGER

The pre-launch Planck Sky Model: a model of sky emission at submillimetre to centimetre wavelengths

As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:1207.3675.

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

pith.paper-citation-record.v1
1207.3675 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 2026-08-10T06:31:04.303077+00:00

measured 5 of 5 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-04T00:27:31.739810Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-05-25T03:56:35.822069Z

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 3faf0e8a-80ce-4935-b65b-c087907b913a · inbound

Reconstructing the Thermal Sunyaev Zeldovich Power Spectrum from Planck using the ABS Method cites this paper.

Reconstructing the Thermal Sunyaev Zeldovich Power Spectrum from Planck using the ABS Method The pre-launch Planck Sky Model: a model of sky emission at submillimetre to centimetre wavelengths

Reference 52

Resolution
verified exact
local_arxiv, observed 2026-05-23T07:42:43.899616Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

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Observation 09674a61-281f-41fa-b93b-ae3ac05f5bbf · inbound

Fast End-to-End Framework for Cosmological Parameter Inference from CMB Data Using Machine Learning cites this paper.

Fast End-to-End Framework for Cosmological Parameter Inference from CMB Data Using Machine Learning The pre-launch Planck Sky Model: a model of sky emission at submillimetre to centimetre wavelengths

Reference 17

Resolution
unresolved
no resolver link, observed 2026-08-04T00:27:31.739810Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 09659df0-2172-4ea8-8d20-6cfdfb8569e2 · inbound

Deep learning with hybrid frequency differencing and principal component analysis for 21-cm foreground and beam mitigation cites this paper.

Deep learning with hybrid frequency differencing and principal component analysis for 21-cm foreground and beam mitigation The pre-launch Planck Sky Model: a model of sky emission at submillimetre to centimetre wavelengths

Reference 64

Resolution
unresolved
no resolver link, observed 2026-08-03T21:30:54.485560Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-03T21:30:54.485560Z digest=sha256:a81c5b34342d61c87c8af830ef5648811fd551e7967c80744bb67101111c91d0

Observation c865e216-6364-442d-a44c-9a6880939c2e · inbound

Enhanced foreground mitigation in thermal SZ Compton-$y$ maps via polarization and deprojection cites this paper.

Enhanced foreground mitigation in thermal SZ Compton-$y$ maps via polarization and deprojection The pre-launch Planck Sky Model: a model of sky emission at submillimetre to centimetre wavelengths

Reference 61

Resolution
unresolved
no resolver link, observed 2026-08-02T18:02:44.272755Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-02T18:02:44.272755Z digest=sha256:72f0d531000a1f00880513002c5c630692f1c2f5fb825d0972db5acc37bd2952

Observation af4de5e6-36fd-4698-b034-db0304645a37 · 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 The pre-launch Planck Sky Model: a model of sky emission at submillimetre to centimetre wavelengths

Reference 105

Resolution
metadata mismatch
local_arxiv, observed 2026-05-25T03:56:35.824191Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:a7a5c2f20a18f8c2840f181c333bb1e926fd76519598ba8802a8da19f3c41143