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Paper Citation Record · LEDGER

Observations of high-order multiplicity in a high-mass stellar protocluster

As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:2401.06545.

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

pith.paper-citation-record.v1
2401.06545 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 2026-08-07T06:34:17.273281+00:00

measured 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-04T23:13:56.730837Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-14T01:00:11.238396Z

Reference resolution

0 of 0 outbound references displayed

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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 11b5a056-7f6a-43b0-ab51-18d6bd938255 · 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 Observations of high-order multiplicity in a high-mass stellar protocluster

Reference 61

Resolution
unresolved
no resolver link, observed 2026-08-04T23:13:56.730837Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-04T23:13:56.730837Z digest=sha256:352fce9b1461d547bf039b396372a0ce0dae9070d74cfb651e2dfa7f12a73880

Observation 7865313f-f26a-44d6-a394-affd1cb13cc2 · 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 Observations of high-order multiplicity in a high-mass stellar protocluster

Reference 58

Resolution
unresolved
no resolver link, observed 2026-07-14T15:02:03.459139Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-14T15:02:03.459139Z digest=sha256:c6ea80ed475be8923b4db85329777c0e0f90f9af01ccb7bbc66c548cfdff3cd2

Observation facb96a3-2073-47ea-a0e7-66c1cc8a4093 · 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 Observations of high-order multiplicity in a high-mass stellar protocluster

Reference 58

Resolution
unresolved
no resolver link, observed 2026-08-02T07:32:03.704292Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T07:32:03.704292Z digest=sha256:5c1d3c1742b804f4e9d01578f54c8d982df372e88bb6bb0a8d1475a69c1717b9

Observation 5d8eff91-61ec-4e8c-b941-9f50ded1d76e · 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 Observations of high-order multiplicity in a high-mass stellar protocluster

Reference 136

Resolution
metadata mismatch
local_arxiv, observed 2026-07-14T01:00:11.240199Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

source=arxiv_source observed=2026-07-14T00:54:38.663915Z digest=sha256:149a699a567aae16b29bd594899483d0459a4a197dd8e18bb817642a2094663c