Paper Citation Record · LEDGER

ALMA-IMF XV: The core mass function in the high-mass star-formation regime

As of 5 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:2407.18719.

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

pith.paper-citation-record.v1
2407.18719 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 4 of 4 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-05T06:32:48.257954+00:00

measured 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-04T23:13:57.119868Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-14T01:00:11.606298Z

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 8fa44f93-a616-445e-9514-f284e782c814 · 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 XV: The core mass function in the high-mass star-formation regime

Reference 64

Resolution: unresolved; no resolver link, observed 2026-08-04T23:13:57.119868Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 05ec4afd-4c76-4c0c-ab32-e6745e5fee88 · 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 XV: The core mass function in the high-mass star-formation regime

Reference 25

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 e5184e8f-7187-46f7-83e9-df14b2fc3d5e · 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 XV: The core mass function in the high-mass star-formation regime

Reference 25

Resolution: unresolved; no resolver link, observed 2026-08-02T07:31:59.344893Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 66efc65e-55db-436a-a4cd-aae1ee28e35d · 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 XV: The core mass function in the high-mass star-formation regime

Reference 64

Resolution: verified exact; local_arxiv, observed 2026-07-14T01:00:11.608246Z

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.