Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Resolved observations at 31 GHz of spinning dust emissivity variations in $\rho$ Oph
As of 22 July 2026, this Paper Citation Record lists 0 of 0 outbound references and 1 inbound Pith citation observation for arXiv:1910.06359.
A citation records a reference. It does not transfer a finding from one paper to another.
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One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-07-21T06:31:05.380196+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-05-25T03:56:11.714959Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-05-25T03:56:36.413709Z
Reference resolution
0 of 0 outbound references displayed
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External citation measurements
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Pith citing papers
Observation af2ec6b7-5775-4c66-b317-b546bc92f3eb · 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 Resolved observations at 31 GHz of spinning dust emissivity variations in $\rho$ Oph
Reference 19
- Resolution
- verified exact
- arxiv_id, observed 2026-05-25T03:56:36.416097Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-07-21T06:31:05.380196+00:00.