Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links, observed 2026-08-14T05:25:36.426456Z
Paper Citation Record · LEDGER
As of 15 August 2026, this Paper Citation Record lists 88 of 88 outbound references and 2 inbound Pith citation observations for arXiv:1909.01400.
A citation records a reference. It does not transfer a finding from one paper to another.
Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links, observed 2026-08-14T05:25:36.426456Z
One-hop event checks from named stored sources.
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Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-05-16T02:22:49.920780Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-05-16T02:27:10.168943Z
88 of 88 outbound references displayed
External citation measurements
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Quasar X-ray and UV flux, baryon acoustic oscillation, and Hubble parameter measurement constraints on cosmological model parameters A new measurement of the Hubble constant and matter content of the Universe using extragalactic background light $\gamma$-ray attenuation
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Quasar X-ray and UV flux, baryon acoustic oscillation, and Hubble parameter measurement constraints on cosmological model parameters Unresolved cited work
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Quasar X-ray and UV flux, baryon acoustic oscillation, and Hubble parameter measurement constraints on cosmological model parameters Unresolved cited work
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Quasar X-ray and UV flux, baryon acoustic oscillation, and Hubble parameter measurement constraints on cosmological model parameters et al., 2018, MNRAS, 477, 122
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Quasar X-ray and UV flux, baryon acoustic oscillation, and Hubble parameter measurement constraints on cosmological model parameters Unresolved cited work
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Observation f001f8a4-6868-471f-bd62-a59f8e3c633f · outbound
Quasar X-ray and UV flux, baryon acoustic oscillation, and Hubble parameter measurement constraints on cosmological model parameters Unresolved cited work
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Quasar X-ray and UV flux, baryon acoustic oscillation, and Hubble parameter measurement constraints on cosmological model parameters et al., 2009, Phys
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Quasar X-ray and UV flux, baryon acoustic oscillation, and Hubble parameter measurement constraints on cosmological model parameters Unresolved cited work
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Quasar X-ray and UV flux, baryon acoustic oscillation, and Hubble parameter measurement constraints on cosmological model parameters Y., 2016, ApJ, 828, 85
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Quasar X-ray and UV flux, baryon acoustic oscillation, and Hubble parameter measurement constraints on cosmological model parameters Consistent Calibration of the Tip of the Red Giant Branch in the Large Magellanic Cloud on the Hubble Space Telescope Photometric System and a Re-determination of the Hubble Constant
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Quasar X-ray and UV flux, baryon acoustic oscillation, and Hubble parameter measurement constraints on cosmological model parameters Unresolved cited work
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Quasar X-ray and UV flux, baryon acoustic oscillation, and Hubble parameter measurement constraints on cosmological model parameters Constraints on $H_0$ from WMAP and baryon acoustic osillation measurements
Reference 87
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Observation 5ae97594-70de-447e-92a9-ec9724c644e7 · outbound
Quasar X-ray and UV flux, baryon acoustic oscillation, and Hubble parameter measurement constraints on cosmological model parameters A Model-Independent Measurement of the Spatial Curvature using Cosmic Chronometers and the HII Hubble Diagram
Reference 88
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Observation fc549316-3024-4d8e-b831-a9abac132088 · inbound
New constraints on cosmic anisotropy from galaxy clusters using an improved dipole fitting method Quasar X-ray and UV flux, baryon acoustic oscillation, and Hubble parameter measurement constraints on cosmological model parameters
Reference 3
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Observation 478e4e06-ecb8-4eb0-b58f-7e0d0894952b · inbound
Is the $w_0w_a$CDM cosmological parameterization evidence for dark energy dynamics partially caused by the excess smoothing of Planck PR4 CMB anisotropy data? Quasar X-ray and UV flux, baryon acoustic oscillation, and Hubble parameter measurement constraints on cosmological model parameters
Reference 14
Source-reported events for the cited work
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