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Paper Citation Record · LEDGER

No evidence (yet) for increased star-formation efficiency at early times

As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 6 inbound Pith citation observations for arXiv:2501.03217.

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

pith.paper-citation-record.v1
2501.03217 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 6 of 6 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-10T06:31:04.303077+00:00

measured 6 of 6 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T18:45:27.254495Z

measured 1 of 1 external citation measurements

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

Source: pith, observed 2026-08-05T02:28:24.338817Z

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
  • unresolved0
  • parse uncertain0
  • malformed identifier0
  • metadata mismatch0

External citation measurements

1
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation acd8d3c8-3e6c-46e0-9e07-bb0a6a5dba70 · inbound

The impact of medium-width bands on the selection, and subsequent luminosity function measurements, of high-z galaxies cites this paper.

The impact of medium-width bands on the selection, and subsequent luminosity function measurements, of high-z galaxies No evidence (yet) for increased star-formation efficiency at early times

Reference 35

Resolution
unresolved
no resolver link, observed 2026-08-07T18:45:27.254495Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-07T18:45:27.254495Z digest=sha256:c347ff14d776bdf465aef3bed90278fe330b4b592977b82f8ce316229091417f

Observation a86bd545-e52e-487c-9193-d8f93b44ce0f · inbound

Exploring Cosmic Dawn with PANORAMIC I: The Bright End of the UVLF at $z\sim9 -17$ cites this paper.

Exploring Cosmic Dawn with PANORAMIC I: The Bright End of the UVLF at $z\sim9 -17$ No evidence (yet) for increased star-formation efficiency at early times

Reference 49

Resolution
unresolved
no resolver link, observed 2026-08-06T19:14:38.159767Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T19:14:38.159767Z digest=sha256:24a7cbe84bb6994ce898590573ac3d5bc7968e0d262e12e81d474d6b40c4eea6

Observation 20a7a166-e314-45eb-8187-7c09bd43345a · inbound

Physical properties of galaxies and the UV Luminosity Function from $z\sim6$ to $z\sim14$ in COSMOS-Web cites this paper.

Physical properties of galaxies and the UV Luminosity Function from $z\sim6$ to $z\sim14$ in COSMOS-Web No evidence (yet) for increased star-formation efficiency at early times

Reference 68

Resolution
unresolved
no resolver link, observed 2026-08-05T23:52:39.394879Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-05T23:52:39.394879Z digest=sha256:a8228e02c226633df2e2fe767a05241faf438c14cc313c17ff2d59f8dc5ee8d1

Observation f06d41a9-dc48-4c99-a868-754bfc8ca3e9 · inbound

Exploring Cosmic Dawn with PANORAMIC II: Cosmic Variance and Galaxy Clustering at $z\sim10$ cites this paper.

Exploring Cosmic Dawn with PANORAMIC II: Cosmic Variance and Galaxy Clustering at $z\sim10$ No evidence (yet) for increased star-formation efficiency at early times

Reference 30

Resolution
unresolved
no resolver link, observed 2026-08-03T16:19:30.887267Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-03T16:19:30.887267Z digest=sha256:7f7045ca0fa0fe6dffb736d81aafd9a6dc6d6738058fea6a0078d779b837ca8c

Observation bcb689f8-933f-4cf3-8a72-c24cb616ce6f · inbound

Grain-size evolution and rapid dust growth in high-redshift galaxies cites this paper.

Grain-size evolution and rapid dust growth in high-redshift galaxies No evidence (yet) for increased star-formation efficiency at early times

Reference 188

Resolution
metadata mismatch
arxiv_id, observed 2026-06-28T00:51:27.057892Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=arxiv_source observed=2026-06-28T00:44:40.243679Z digest=sha256:87f8995aad4cbad5d01753b1b2b0c233ac839df9f517822c9b8110127b2a2ec9

Observation e1c8de1f-f7d0-4cd3-a36f-60bc899fdff8 · inbound

Gamma-ray bursts reveal the history and faint contributors of cosmic reionization cites this paper.

Gamma-ray bursts reveal the history and faint contributors of cosmic reionization No evidence (yet) for increased star-formation efficiency at early times

Reference 247

Resolution
metadata mismatch
local_arxiv, observed 2026-07-09T05:26:01.856097Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=arxiv_source observed=2026-07-09T05:25:12.742172Z digest=sha256:6be0a2fa6e736421c3d8b1f786f6cccfb41a95be309efd2d6348300671b916b9