Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
The Star Formation Rate of the Milky Way as seen by Herschel
As of 22 July 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2211.05573.
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 2026-07-22T06:31:00.163083+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-07-14T00:54:38.663915Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-07-01T20:06:11.988754Z
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 bb9f5c14-2756-4a6f-95df-b7c2c38b83f1 · inbound
Collective Winds of Massive Star Clusters as the Dominant PeVatrons for Galactic Cosmic Rays cites this paper.
Collective Winds of Massive Star Clusters as the Dominant PeVatrons for Galactic Cosmic Rays The Star Formation Rate of the Milky Way as seen by Herschel
Reference 38
- Resolution
- verified exact
- arxiv_id, observed 2026-07-01T20:06:11.989940Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-07-22T06:31:00.163083+00:00.
Observation 048590ee-5567-42ce-9726-ccecbd42da27 · inbound
Challenges in probing turbulent and magnetic support in cores: the W43-MM1 protocluster case study cites this paper.
Challenges in probing turbulent and magnetic support in cores: the W43-MM1 protocluster case study The Star Formation Rate of the Milky Way as seen by Herschel
Reference 58
- Resolution
- unresolved
- no resolver link, observed 2026-07-14T00:54:38.663915Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.