Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
HMcode-2020: Improved modelling of non-linear cosmological power spectra with baryonic feedback
As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 22 inbound Pith citation observations for arXiv:2009.01858.
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 2026-08-10T06:31:04.303077+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-10T20:26:54.956593Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-07-03T12:58:08.248342Z
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External citation measurements
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Outbound references
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Pith citing papers
Observation 1ff2dd83-c497-48d1-8a01-7809323c7e54 · inbound
Pixelization effects in cosmic shear angular power spectra cites this paper.
Pixelization effects in cosmic shear angular power spectra HMcode-2020: Improved modelling of non-linear cosmological power spectra with baryonic feedback
Reference 40
- Resolution
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Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 79e82145-9b2e-406d-943d-3583bb2f8d86 · inbound
Tuning the cosmic instrument: robust cosmology through combined probes cites this paper.
Tuning the cosmic instrument: robust cosmology through combined probes HMcode-2020: Improved modelling of non-linear cosmological power spectra with baryonic feedback
Reference 105
- Resolution
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Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation ac3ab785-1a4d-438b-b5f0-d88933990cc8 · inbound
Reconstructing the shape of the non-linear matter power spectrum using CMB lensing and cosmic shear cites this paper.
Reconstructing the shape of the non-linear matter power spectrum using CMB lensing and cosmic shear HMcode-2020: Improved modelling of non-linear cosmological power spectra with baryonic feedback
Reference 41
- Resolution
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Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 0e6061d8-b114-424b-8753-6d3f31f86a93 · inbound
A frequentist view on the two-body decaying dark matter model cites this paper.
A frequentist view on the two-body decaying dark matter model HMcode-2020: Improved modelling of non-linear cosmological power spectra with baryonic feedback
Reference 67
- Resolution
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Source-reported events for the cited work
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Observation e7420bfa-3fea-4655-a839-f8120ace0473 · inbound
Measurement of the Dispersion$\unicode{x2013}$Galaxy Cross-Power Spectrum with the Second CHIME/FRB Catalog cites this paper.
Measurement of the Dispersion$\unicode{x2013}$Galaxy Cross-Power Spectrum with the Second CHIME/FRB Catalog HMcode-2020: Improved modelling of non-linear cosmological power spectra with baryonic feedback
Reference 49
- Resolution
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Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 89fbfd75-1dae-41f5-ba0e-ff8f9c1c41e5 · inbound
Bayesian and frequentist perspectives agree on dynamical dark energy cites this paper.
Bayesian and frequentist perspectives agree on dynamical dark energy HMcode-2020: Improved modelling of non-linear cosmological power spectra with baryonic feedback
Reference 43
- Resolution
- unresolved
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Source-reported events for the cited work
Unavailable: canonical work link unavailable.
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 cites this paper.
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
- Resolution
- unresolved
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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 cites this paper.
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
- Resolution
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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 cites this paper.
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
- Resolution
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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 cites this paper.
Cosmological tensions in Proca-Nuevo theory HMcode-2020: Improved modelling of non-linear cosmological power spectra with baryonic feedback
Reference 95
- Resolution
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Unavailable: canonical work link unavailable.
Observation dbe17caa-0538-41f1-b0c2-061815c5c0c3 · inbound
Floquet Dissipative Phase Transitions cites this paper.
Floquet Dissipative Phase Transitions HMcode-2020: Improved modelling of non-linear cosmological power spectra with baryonic feedback
Reference 17
- Resolution
- unresolved
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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 cites this paper.
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
- Resolution
- verified exact
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Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.
Observation c79aa056-d7c2-4f46-bbf4-b7fd73c646d1 · inbound
(The) Wiggles going non-linear cites this paper.
(The) Wiggles going non-linear HMcode-2020: Improved modelling of non-linear cosmological power spectra with baryonic feedback
Reference 32
- Resolution
- verified exact
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Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.
Observation 179bba5e-7e90-4346-8225-a4d4d1238bbc · inbound
(The) Wiggles going non-linear cites this paper.
(The) Wiggles going non-linear HMcode-2020: Improved modelling of non-linear cosmological power spectra with baryonic feedback
Reference 32
- Resolution
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Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.
Observation cb03bfa6-353b-4a72-a584-e85e5b22fbe5 · inbound
The sound of dynamical dark energy and modified gravity cites this paper.
The sound of dynamical dark energy and modified gravity HMcode-2020: Improved modelling of non-linear cosmological power spectra with baryonic feedback
Reference 99
- Resolution
- verified exact
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Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.
Observation 625fbe46-47ab-4ba1-893e-3d611ea90b77 · inbound
CMB Constraints on Pre-Inflationary Axion Dark Matter Isocurvature cites this paper.
CMB Constraints on Pre-Inflationary Axion Dark Matter Isocurvature HMcode-2020: Improved modelling of non-linear cosmological power spectra with baryonic feedback
Reference 43
- Resolution
- verified exact
- arxiv_id, observed 2026-07-03T07:37:45.612917Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.
Observation 996569f4-f746-4471-9f55-25df63c10f88 · inbound
Dark Matter with a Drag at Low Redshift cites this paper.
Dark Matter with a Drag at Low Redshift HMcode-2020: Improved modelling of non-linear cosmological power spectra with baryonic feedback
Reference 74
- Resolution
- verified exact
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Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.
Observation 64963412-633c-4a69-8fae-b0dd1b8f0104 · inbound
The $H_0$ world cup. II. A comprehensive competition between proposed Hubble tension solutions cites this paper.
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
- Resolution
- unresolved
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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 cites this paper.
CAMB v2: cosmological power spectra for high-precision surveys HMcode-2020: Improved modelling of non-linear cosmological power spectra with baryonic feedback
Reference 74
- Resolution
- unresolved
- no resolver link, observed 2026-08-02T00:56:20.239945Z
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 cites this paper.
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
- Resolution
- unresolved
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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 cites this paper.
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
- Resolution
- unresolved
- no resolver link, observed 2026-07-30T11:19:10.422670Z
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 cites this paper.
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
- Resolution
- unresolved
- no resolver link, observed 2026-08-03T13:53:45.308454Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.