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Paper Citation Record · LEDGER

INvestigations of massive Filaments ANd sTar formation (INFANT). I. Core Identification and Core Mass Function

As of 18 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2404.03858.

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

pith.paper-citation-record.v1
2404.03858 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 3 of 3 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-18T06:34:40.430872+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-15T22:15:53.578737Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-08-15T22:15:53.964755Z

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 054009af-8c3a-4a14-af39-f7399298f4f0 · inbound

Why is the Star Formation Rate Proportional to Dense Gas Mass? cites this paper.

Why is the Star Formation Rate Proportional to Dense Gas Mass? INvestigations of massive Filaments ANd sTar formation (INFANT). I. Core Identification and Core Mass Function

Reference 8

Resolution
metadata mismatch
local_arxiv, observed 2026-08-15T22:15:53.971837Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

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Observation 6bf3d284-4e26-4a02-8937-86fcd61c79aa · 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 INvestigations of massive Filaments ANd sTar formation (INFANT). I. Core Identification and Core Mass Function

Reference 84

Resolution
unresolved
no resolver link, observed 2026-08-02T07:32:06.685278Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T07:32:06.685278Z digest=sha256:b5f73ab73384651461b55d29c75f0d5def72661533df3ff73881cebe3ef30ed4

Observation bac15aeb-2cd0-4a94-a218-2cc5ef98c691 · inbound

The Zero-Age Massive Stellar Population of W49A from VLA Observations cites this paper.

The Zero-Age Massive Stellar Population of W49A from VLA Observations INvestigations of massive Filaments ANd sTar formation (INFANT). I. Core Identification and Core Mass Function

Reference 15

Resolution
unresolved
no resolver link, observed 2026-08-08T12:54:37.890470Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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