Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
The Chandra COSMOS Legacy survey: overview and point source catalog
As of 25 July 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:1601.00941.
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 2026-07-24T06:31:00.690269+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-07-11T11:50:26.030339Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-07-10T10:27:02.114067Z
Reference resolution
0 of 0 outbound references displayed
- verified exact0
- verified fuzzy0
- unresolved0
- parse uncertain0
- malformed identifier0
- metadata mismatch0
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 d1d48312-c0bf-4c65-9d34-fa06e0850b05 · inbound
PEARLS: JWST Counterparts of Micro-Jy Radio Sources in the NEP Time Domain Field. II. All Four Spokes cites this paper.
PEARLS: JWST Counterparts of Micro-Jy Radio Sources in the NEP Time Domain Field. II. All Four Spokes The Chandra COSMOS Legacy survey: overview and point source catalog
Reference 148
- Resolution
- verified exact
- local_arxiv, observed 2026-05-20T15:38:26.195077Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-07-24T06:31:00.690269+00:00.
Observation bd3987c1-c34c-4ced-82d4-2f95eb2b033d · inbound
Multiphase images of a powerful supernova-driven wind in the early Universe cites this paper.
Multiphase images of a powerful supernova-driven wind in the early Universe The Chandra COSMOS Legacy survey: overview and point source catalog
Reference 273
- Resolution
- verified exact
- local_arxiv, observed 2026-06-27T13:00:56.737144Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-07-24T06:31:00.690269+00:00.
Observation 6757bc58-bbe9-4703-a482-610b81bc44a6 · inbound
X-ray luminosity function of Compton-thick AGN in the early Universe (z > 3). Robustness and biases of the CTK population cites this paper.
X-ray luminosity function of Compton-thick AGN in the early Universe (z > 3). Robustness and biases of the CTK population The Chandra COSMOS Legacy survey: overview and point source catalog
Reference 28
- Resolution
- metadata mismatch
- local_arxiv, observed 2026-07-03T11:28:04.831244Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-07-24T06:31:00.690269+00:00.
Observation e536366f-9569-4475-9e3e-05f7ad4ee93a · inbound
Unveil the nature of JWST-AGN and Little Red Dots with SKAO continuum surveys cites this paper.
Unveil the nature of JWST-AGN and Little Red Dots with SKAO continuum surveys The Chandra COSMOS Legacy survey: overview and point source catalog
Reference 213
- Resolution
- verified exact
- local_arxiv, observed 2026-07-01T06:25:27.875582Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-07-24T06:31:00.690269+00:00.
Observation 56546e75-4dec-49a5-9db5-d44bbbe8f8b7 · inbound
Subaru meets JWST: A Direct Measurement of Ly$\boldsymbol{\alpha}$ Escape Fraction at $\boldsymbol{z\simeq6.2}$ with Dual Narrow-Band Imaging cites this paper.
Subaru meets JWST: A Direct Measurement of Ly$\boldsymbol{\alpha}$ Escape Fraction at $\boldsymbol{z\simeq6.2}$ with Dual Narrow-Band Imaging The Chandra COSMOS Legacy survey: overview and point source catalog
Reference 35
- Resolution
- verified exact
- local_arxiv, observed 2026-07-10T10:27:02.115624Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-07-24T06:31:00.690269+00:00.