Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
As of 6 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 16 inbound Pith citation observations for arXiv:2009.01858.
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.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-06T06:34:29.942622+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-05T18:54:25.401389Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-07-03T12:58:08.248342Z
0 of 0 outbound references displayed
External citation measurements
No source-named external measurement is stored.
No outbound reference observations are available for this paper version.
Observation 169e54b7-8fbd-46f6-a22f-35bad5fb3c51 · inbound
Cosmology from a joint analysis of second and third order shear statistics with Subaru Hyper Suprime-Cam Year 3 data HMcode-2020: Improved modelling of non-linear cosmological power spectra with baryonic feedback
Reference 63
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 01ec59a3-f3f1-43b0-8a50-677cabb6431b · inbound
The simple way to measure evolving dark energy without prior-volume effects HMcode-2020: Improved modelling of non-linear cosmological power spectra with baryonic feedback
Reference 60
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 2c9542a9-a41c-4bf1-8806-760bb1dc8bbe · inbound
Unbiased analysis of primordial non-Gaussianity: the multipoles of the full relativistic power spectrum HMcode-2020: Improved modelling of non-linear cosmological power spectra with baryonic feedback
Reference 82
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 4f04fa9d-210b-4597-a0c9-5d395e8feb2b · inbound
Cosmological tensions in Proca-Nuevo theory HMcode-2020: Improved modelling of non-linear cosmological power spectra with baryonic feedback
Reference 95
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation dbe17caa-0538-41f1-b0c2-061815c5c0c3 · inbound
Floquet Dissipative Phase Transitions HMcode-2020: Improved modelling of non-linear cosmological power spectra with baryonic feedback
Reference 17
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation ed0a00aa-154c-4b54-b001-99b46ef70045 · inbound
Ultra-light axion constraints from Planck and ACT: the role of nonlinear modelling HMcode-2020: Improved modelling of non-linear cosmological power spectra with baryonic feedback
Reference 19
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.
Observation c79aa056-d7c2-4f46-bbf4-b7fd73c646d1 · inbound
(The) Wiggles going non-linear HMcode-2020: Improved modelling of non-linear cosmological power spectra with baryonic feedback
Reference 32
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.
Observation 179bba5e-7e90-4346-8225-a4d4d1238bbc · inbound
(The) Wiggles going non-linear HMcode-2020: Improved modelling of non-linear cosmological power spectra with baryonic feedback
Reference 32
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.
Observation cb03bfa6-353b-4a72-a584-e85e5b22fbe5 · inbound
The sound of dynamical dark energy and modified gravity HMcode-2020: Improved modelling of non-linear cosmological power spectra with baryonic feedback
Reference 99
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.
Observation 625fbe46-47ab-4ba1-893e-3d611ea90b77 · inbound
CMB Constraints on Pre-Inflationary Axion Dark Matter Isocurvature HMcode-2020: Improved modelling of non-linear cosmological power spectra with baryonic feedback
Reference 43
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.
Observation 996569f4-f746-4471-9f55-25df63c10f88 · inbound
Dark Matter with a Drag at Low Redshift HMcode-2020: Improved modelling of non-linear cosmological power spectra with baryonic feedback
Reference 74
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.
Observation 64963412-633c-4a69-8fae-b0dd1b8f0104 · inbound
The $H_0$ world cup. II. A comprehensive competition between proposed Hubble tension solutions HMcode-2020: Improved modelling of non-linear cosmological power spectra with baryonic feedback
Reference 248
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation d3bba61c-b2cb-4908-9ed0-c2d5323ff539 · inbound
CAMB v2: cosmological power spectra for high-precision surveys HMcode-2020: Improved modelling of non-linear cosmological power spectra with baryonic feedback
Reference 74
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 6ee78f2c-f08d-4a88-bf02-1c1a2ba85b2a · inbound
Early- and late-time constraints on Wald-Gauss-Bonnet topological dark energy and implications for the $H_0$ and $S_8$ tensions HMcode-2020: Improved modelling of non-linear cosmological power spectra with baryonic feedback
Reference 104
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 8b9bc5e7-6760-4d58-bf9a-44f896b87dbe · inbound
Shear-kSZ: A New Estimator for the Matter-Electron Power Spectrum from kSZ Tomography and Weak Lensing HMcode-2020: Improved modelling of non-linear cosmological power spectra with baryonic feedback
Reference 64
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 0eca1098-cfbf-4391-b4e0-59032a6bfed1 · inbound
Direct shear $\times$ kSZ correlation: controlling baryons without modeling galaxies HMcode-2020: Improved modelling of non-linear cosmological power spectra with baryonic feedback
Reference 5
Source-reported events for the cited work
Unavailable: canonical work link unavailable.