Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
ALMA-IMF XVIII: The assembly of a star cluster: Dense N$_2$H$^+$ (1-0) kinematics in the massive G351.77 protocluster
As of 5 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:2410.09843.
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 2026-08-05T06:32:48.257954+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-04T23:14:02.322768Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-07-14T01:00:11.422653Z
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 708ad667-4156-42da-a51a-db213e11df8a · inbound
ALMA-IMF XX: Core fragmentation in the W51 high-mass star-forming region cites this paper.
ALMA-IMF XX: Core fragmentation in the W51 high-mass star-forming region ALMA-IMF XVIII: The assembly of a star cluster: Dense N$_2$H$^+$ (1-0) kinematics in the massive G351.77 protocluster
Reference 102
- Resolution
- unresolved
- no resolver link, observed 2026-08-04T23:14:02.322768Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 0e1a63a3-fae4-471e-b749-71d7beaa70d4 · inbound
How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching cites this paper.
How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching ALMA-IMF XVIII: The assembly of a star cluster: Dense N$_2$H$^+$ (1-0) kinematics in the massive G351.77 protocluster
Reference 48
- Resolution
- unresolved
- no resolver link, observed 2026-07-14T15:02:03.459139Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 14d18c73-b51b-486e-a947-a67dc1a1181d · inbound
How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching cites this paper.
How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching ALMA-IMF XVIII: The assembly of a star cluster: Dense N$_2$H$^+$ (1-0) kinematics in the massive G351.77 protocluster
Reference 48
- Resolution
- unresolved
- no resolver link, observed 2026-08-02T07:32:02.574352Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 944a6049-dc50-4da1-962f-1534c83920c9 · 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 ALMA-IMF XVIII: The assembly of a star cluster: Dense N$_2$H$^+$ (1-0) kinematics in the massive G351.77 protocluster
Reference 182
- Resolution
- verified exact
- local_arxiv, observed 2026-07-14T01:00:11.424874Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.