Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Constraints on the early Universe star formation efficiency from galaxy clustering and halo modeling of H$\alpha$ and [O III] emitters
As of 9 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 7 inbound Pith citation observations for arXiv:2503.14280.
A citation records a reference. It does not transfer a finding from one paper to another.
Coverage vector
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-09T06:31:02.800959+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-06T19:14:43.649280Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, 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
arxiv_reference, observed 2026-08-05T02:28:24.338817Z
Outbound references
No outbound reference observations are available for this paper version.
Pith citing papers
Observation 68cbec28-fb0f-4d96-9f04-7fc9dd184538 · 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 $z\sim9 -17$ Constraints on the early Universe star formation efficiency from galaxy clustering and halo modeling of H$\alpha$ and [O III] emitters
Reference 126
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T19:14:43.649280Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 218d8892-a15f-481f-ad7a-499cddbadcaf · 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 Constraints on the early Universe star formation efficiency from galaxy clustering and halo modeling of H$\alpha$ and [O III] emitters
Reference 180
- Resolution
- unresolved
- no resolver link, observed 2026-08-05T23:52:53.057569Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 921a0302-d96d-4317-9d0d-84e1d0c2b179 · 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 $z\sim10$ Constraints on the early Universe star formation efficiency from galaxy clustering and halo modeling of H$\alpha$ and [O III] emitters
Reference 89
- Resolution
- unresolved
- no resolver link, observed 2026-08-03T16:19:36.514238Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 9c2b5c7e-4750-493b-a71a-5638045d337b · inbound
An Improved Fit for Linear Halo Bias at High Redshift cites this paper.
An Improved Fit for Linear Halo Bias at High Redshift Constraints on the early Universe star formation efficiency from galaxy clustering and halo modeling of H$\alpha$ and [O III] emitters
Reference 23
- Resolution
- verified exact
- arxiv_id, observed 2026-05-10T12:00:21.847407Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.
Observation 0a70e7b1-45cd-43af-bba7-dedd6a290def · inbound
The Impact of Cosmic Variance and Satellites on JWST Clustering Measurements at Redshift around 6 cites this paper.
The Impact of Cosmic Variance and Satellites on JWST Clustering Measurements at Redshift around 6 Constraints on the early Universe star formation efficiency from galaxy clustering and halo modeling of H$\alpha$ and [O III] emitters
Reference 51
- Resolution
- verified exact
- arxiv_id, observed 2026-05-13T00:51:58.714236Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.
Observation ab360e4a-98d9-4754-ba62-e5abd2d8bc06 · inbound
Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution cites this paper.
Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution Constraints on the early Universe star formation efficiency from galaxy clustering and halo modeling of H$\alpha$ and [O III] emitters
Reference 61
- Resolution
- malformed identifier
- arxiv_id, observed 2026-07-02T00:36:24.469418Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.
Observation 219be0de-b6fc-4c46-a62c-024532389076 · inbound
Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution cites this paper.
Reduced Incidence of Little Red Dots at z < 3 from Number Density and Halo Mass Evolution Constraints on the early Universe star formation efficiency from galaxy clustering and halo modeling of H$\alpha$ and [O III] emitters
Reference 61
- Resolution
- malformed identifier
- no resolver link, observed 2026-08-02T12:34:30.232268Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.