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Paper Citation Record · LEDGER
As of 9 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 20 inbound Pith citation observations for arXiv:2001.09213.
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
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 2026-08-08T17:56:52.007016Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-07-04T05:19:35.674180Z
0 of 0 outbound references displayed
External citation measurements
No source-named external measurement is stored.
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Dark Energy Survey Year 3 Results: Cosmological Constraints from Galaxy Clustering and Weak Lensing The Megamaser Cosmology Project. XIII. Combined Hubble constant constraints
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The Hubble Tension and Early Dark Energy The Megamaser Cosmology Project. XIII. Combined Hubble constant constraints
Reference 28
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$\Lambda_{\rm s}$CDM cosmology from a type-II minimally modified gravity The Megamaser Cosmology Project. XIII. Combined Hubble constant constraints
Reference 31
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DESI 2024 VI: Cosmological Constraints from the Measurements of Baryon Acoustic Oscillations The Megamaser Cosmology Project. XIII. Combined Hubble constant constraints
Reference 235
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Little ado about everything II: an `emergent' dark energy from structure formation to rule cosmic tensions The Megamaser Cosmology Project. XIII. Combined Hubble constant constraints
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Interacting Early Dark Energy The Megamaser Cosmology Project. XIII. Combined Hubble constant constraints
Reference 4
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Constraints on Dark Energy Models Using Late Universe Probes The Megamaser Cosmology Project. XIII. Combined Hubble constant constraints
Reference 156
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Interacting $k$-essence field with non-pressureless Dark Matter: Cosmological Dynamics and Observational Constraints The Megamaser Cosmology Project. XIII. Combined Hubble constant constraints
Reference 29
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Crosschecking Cosmic Distances from DESI BAO and DES SNe The Megamaser Cosmology Project. XIII. Combined Hubble constant constraints
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Crosschecking Cosmic Distances from DESI BAO and DES SNe The Megamaser Cosmology Project. XIII. Combined Hubble constant constraints
Reference 7
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Nonlinear Matter Power Spectrum from relativistic $N$-body Simulations: $\Lambda_{\rm s}$CDM versus $\Lambda$CDM The Megamaser Cosmology Project. XIII. Combined Hubble constant constraints
Reference 30
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Dissipative Cosmology and the Nature of Dark Energy: Insights from Bulk Viscosity with DESI DR2 observations The Megamaser Cosmology Project. XIII. Combined Hubble constant constraints
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Cosmological Constraints on Minimal Cubic Galileon Models in Teleparallel Gravity The Megamaser Cosmology Project. XIII. Combined Hubble constant constraints
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The Hubble tension: A decade review The Megamaser Cosmology Project. XIII. Combined Hubble constant constraints
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The Hubble tension: A decade review The Megamaser Cosmology Project. XIII. Combined Hubble constant constraints
Reference 172
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Intertwined Constraints in Extended Cosmologies: Dark Energy, Curvature, Neutrinos, and Inflation The Megamaser Cosmology Project. XIII. Combined Hubble constant constraints
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Late-time cosmological constraints on three holographic dark energy models with DESI DR2 BAO and Type Ia supernovae The Megamaser Cosmology Project. XIII. Combined Hubble constant constraints
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Observation 9d33ec9e-916e-4985-ac79-9799de36e196 · inbound
Hubble tension: a short review of theoretical explanations The Megamaser Cosmology Project. XIII. Combined Hubble constant constraints
Reference 23
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Updated 1.1% Precision Values of the Hubble Constant with Corrected Pantheon+ and Dark Energy Survey (DES)-DOVEKIE Type Ia Supernovae The Megamaser Cosmology Project. XIII. Combined Hubble constant constraints
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Reanalyzing Megamasers: a low value of $H_0$ from a local probe changes our view of the Hubble Tension The Megamaser Cosmology Project. XIII. Combined Hubble constant constraints
Reference 2
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