Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Full-sky, arcminute-scale, 3D models of Galactic microwave foreground dust emission based on filaments
As of 18 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2107.08317.
A citation records a reference. It does not transfer a finding from one paper to another.
Coverage vector
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-18T06:34:40.430872+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-15T23:51:27.643446Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-07-04T09:39:46.288729Z
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 6965677c-ad29-41b6-9334-4c6969c13137 · inbound
Impact of Galactic non-Gaussian foregrounds on CMB lensing measurements cites this paper.
Impact of Galactic non-Gaussian foregrounds on CMB lensing measurements Full-sky, arcminute-scale, 3D models of Galactic microwave foreground dust emission based on filaments
Reference 69
- Resolution
- unresolved
- no resolver link, observed 2026-08-15T23:51:27.643446Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation b4db2a6d-794b-4736-b518-4b02b38efc10 · inbound
Understanding the non-Gaussian nature of Galactic foreground emissions towards small scales cites this paper.
Understanding the non-Gaussian nature of Galactic foreground emissions towards small scales Full-sky, arcminute-scale, 3D models of Galactic microwave foreground dust emission based on filaments
Reference 7
- Resolution
- verified exact
- arxiv_id, observed 2026-07-04T09:39:46.290108Z
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.
Observation a126f71e-2910-434d-9b51-a5636232b344 · inbound
Single Frequency CMB Foreground Removal with Inter-scale Machine Learning cites this paper.
Single Frequency CMB Foreground Removal with Inter-scale Machine Learning Full-sky, arcminute-scale, 3D models of Galactic microwave foreground dust emission based on filaments
Reference 71
- Resolution
- unresolved
- no resolver link, observed 2026-08-03T00:45:31.782545Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.