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Paper Citation Record · LEDGER

The Field Substellar Mass Function Based on the Full-sky 20-pc Census of 525 L, T, and Y Dwarfs

As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2011.11616.

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

pith.paper-citation-record.v1
2011.11616 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 2 of 2 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-11T06:34:44.6726+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-10T04:20:27.472204Z

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

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Pith citing papers

Observation 4fff397e-2ade-4aff-8c6a-3b00f7b07081 · inbound

Statistics on the population of distant substellar companions to nearby stars cites this paper.

Statistics on the population of distant substellar companions to nearby stars The Field Substellar Mass Function Based on the Full-sky 20-pc Census of 525 L, T, and Y Dwarfs

Reference 175

Resolution
unresolved
no resolver link, observed 2026-08-01T09:46:15.332872Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T09:46:15.332872Z digest=sha256:ededf4fd5b1a52e0e8b2220456879dd43cfbaab5e7ebd492c77cf0670cb57af8

Observation 2ade7485-fd49-4cd9-b157-93d2014d2119 · inbound

A clear detection of proper motion confirms that the claimed $\mathbf{z\simeq32}$ galaxy candidate, "Capotauro'', is a Y-type brown dwarf cites this paper.

A clear detection of proper motion confirms that the claimed $\mathbf{z\simeq32}$ galaxy candidate, "Capotauro'', is a Y-type brown dwarf The Field Substellar Mass Function Based on the Full-sky 20-pc Census of 525 L, T, and Y Dwarfs

Reference 63

Resolution
unresolved
no resolver link, observed 2026-08-10T04:20:27.472204Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T04:20:27.472204Z digest=sha256:fcf12e232a47c21de6756af36425907aa7a562cb534f5f1e7e311591fc09b26a