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Paper Citation Record · LEDGER

What is the role of stellar radiative feedback in setting the stellar mass spectrum?

As of 15 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2010.03539.

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

pith.paper-citation-record.v1
2010.03539 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 2026-08-15T06:32:42.880941+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-02T07:31:58.368224Z

measured 0 of 1 external citation measurements

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

Source: cited_works

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 bedfe64f-ec47-4bf1-83ec-ba8f7471fcbb · 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 What is the role of stellar radiative feedback in setting the stellar mass spectrum?

Reference 17

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=sha256:8d4381f9e71004a64070f177f9d91cbb9813eae8fd4b40e891dfb15b4856e419

Observation 1f07f07e-8d1d-4fcd-bd2f-621deb471e64 · 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 What is the role of stellar radiative feedback in setting the stellar mass spectrum?

Reference 17

Resolution
unresolved
no resolver link, observed 2026-08-02T07:31:58.368224Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-02T07:31:58.368224Z digest=sha256:7d972769b6f672b70fd3bf540dfb53b031136e78226988f7d3c1cf735c121407

Observation 7149e277-e1ac-43c8-9e21-920a74766f11 · inbound

Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity cites this paper.

Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity What is the role of stellar radiative feedback in setting the stellar mass spectrum?

Reference 46

Resolution
unresolved
no resolver link, observed 2026-08-01T14:10:52.141000Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T14:10:52.141000Z digest=sha256:67cd9aec2b941741de607430b870c9a96f730781f205e5183b43933ec70d1fce