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Paper Citation Record · LEDGER

The Atacama Cosmology Telescope: Semi-Analytic Covariance Matrices for the DR6 CMB Power Spectra

As of 17 August 2026, this Paper Citation Record lists 16 of 16 outbound references and 5 inbound Pith citation observations for arXiv:2412.07068.

A citation records a reference. It does not transfer a finding from one paper to another.

pith.paper-citation-record.v1
2412.07068 v1

Coverage vector

measured 16 of 16 reference resolution

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Source: paper_references, paper_reference_links, observed 2026-08-11T19:17:09.334748Z

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measured 5 of 5 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-15T14:36:18.294784Z

measured 1 of 1 external citation measurements

A source-named dated measurement, never combined with another source.

Source: arxiv_reference, observed 2026-08-05T02:28:24.338817Z

Reference resolution

16 of 16 outbound references displayed

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External citation measurements

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arxiv_reference, observed 2026-08-05T02:28:24.338817Z

Outbound references

Observation f4daab10-9dfe-419d-946a-2c9ac30bbf76 · outbound

This paper cites 2020, JCAP, 2020, 47, doi: 10.1088/1475-7516/2020/12/047 Alonso, D., Fabbian, G., Storey-Fisher, K., et al.

The Atacama Cosmology Telescope: Semi-Analytic Covariance Matrices for the DR6 CMB Power Spectra 2020, JCAP, 2020, 47, doi: 10.1088/1475-7516/2020/12/047 Alonso, D., Fabbian, G., Storey-Fisher, K., et al

Reference 1

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Observation bc1deebc-a087-48c5-a10c-87f9a01db472 · outbound

This paper cites −−” couplings are small compared to “++.

The Atacama Cosmology Telescope: Semi-Analytic Covariance Matrices for the DR6 CMB Power Spectra −−” couplings are small compared to “++

Reference 2

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Observation a27c290e-6051-436b-b894-518b466fe23a · outbound

This paper cites an unresolved cited work.

The Atacama Cosmology Telescope: Semi-Analytic Covariance Matrices for the DR6 CMB Power Spectra Unresolved cited work

Reference 3

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Observation 910dc3f5-6328-4ea2-989c-d4a12f4e7512 · outbound

This paper cites an unresolved cited work.

The Atacama Cosmology Telescope: Semi-Analytic Covariance Matrices for the DR6 CMB Power Spectra Unresolved cited work

Reference 5

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Observation 043c551b-a515-4d34-83c9-d18578251bdf · outbound

This paper cites (B10) Because ˜a is Gaussian, we expand the product of four fields using Wick’s theorem.

The Atacama Cosmology Telescope: Semi-Analytic Covariance Matrices for the DR6 CMB Power Spectra (B10) Because ˜a is Gaussian, we expand the product of four fields using Wick’s theorem

Reference 6

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Observation 85eabf74-b377-4f08-85f5-fa3fae2864e8 · outbound

This paper cites pseudospectrum.

The Atacama Cosmology Telescope: Semi-Analytic Covariance Matrices for the DR6 CMB Power Spectra pseudospectrum

Reference 8

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Observation 1002c5b6-4ef2-48b3-bb54-e3c793c08cc2 · outbound

This paper cites 27 When there is a mask in addition to a harmonic-space filter, these expressions become inexact.

The Atacama Cosmology Telescope: Semi-Analytic Covariance Matrices for the DR6 CMB Power Spectra 27 When there is a mask in addition to a harmonic-space filter, these expressions become inexact

Reference 9

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Observation d7937df9-7600-4e29-9944-1bf5a44f3d91 · outbound

This paper cites A field that follows the model of Equation 9 has zero mean and is Gaussian, so its statistics are fully specified by its covariance.

The Atacama Cosmology Telescope: Semi-Analytic Covariance Matrices for the DR6 CMB Power Spectra A field that follows the model of Equation 9 has zero mean and is Gaussian, so its statistics are fully specified by its covariance

Reference 10

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Observation 8a9c4044-1638-4cf1-ac74-750f07fd2f8d · outbound

This paper cites representative.

The Atacama Cosmology Telescope: Semi-Analytic Covariance Matrices for the DR6 CMB Power Spectra representative

Reference 11

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Observation fa5636dd-29dd-4c04-bbdf-dde2856a296d · outbound

This paper cites Left: In the case that the simulation-based correction only smooths the main diagonal of ΣR.

The Atacama Cosmology Telescope: Semi-Analytic Covariance Matrices for the DR6 CMB Power Spectra Left: In the case that the simulation-based correction only smooths the main diagonal of ΣR

Reference 13

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Observation 665adb29-d9ce-4a7c-a08c-c12ddcbec78b · outbound

This paper cites For each polarization combination, the power spectrum variance increases when point-source holes are added to the mask, as expected.

The Atacama Cosmology Telescope: Semi-Analytic Covariance Matrices for the DR6 CMB Power Spectra For each polarization combination, the power spectrum variance increases when point-source holes are added to the mask, as expected

Reference 14

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Observation 7b0415d8-1230-48bd-953f-124934f64604 · outbound

This paper cites Thus, as is evident in Figure 15, both cases share the same statistical fluctuations, further facilitating a direct comparison.

The Atacama Cosmology Telescope: Semi-Analytic Covariance Matrices for the DR6 CMB Power Spectra Thus, as is evident in Figure 15, both cases share the same statistical fluctuations, further facilitating a direct comparison

Reference 15

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Observation 3ad12064-c351-4068-942c-4c4fc3a8050a · outbound

This paper cites an unresolved cited work.

The Atacama Cosmology Telescope: Semi-Analytic Covariance Matrices for the DR6 CMB Power Spectra Unresolved cited work

Reference 193

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Observation 5147db03-dafb-4c17-a415-f7c7b5f1cf4b · outbound

This paper cites (2023) for this model.

The Atacama Cosmology Telescope: Semi-Analytic Covariance Matrices for the DR6 CMB Power Spectra (2023) for this model

Reference 500

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Observation 1045b596-75c0-4783-894e-623c94f7216c · outbound

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The Atacama Cosmology Telescope: Semi-Analytic Covariance Matrices for the DR6 CMB Power Spectra Unresolved cited work

Reference 1763

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Observation 55a26300-7e22-4cda-ac01-b06e79a19c8d · outbound

This paper cites M., Hivon, E., Banday, A.

The Atacama Cosmology Telescope: Semi-Analytic Covariance Matrices for the DR6 CMB Power Spectra M., Hivon, E., Banday, A

Reference 2016

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Pith citing papers

Observation fe127be5-99c6-4480-b1dd-258607b356b5 · inbound

SPT-3G D1: CMB temperature and polarization power spectra and cosmology from 2019 and 2020 observations of the SPT-3G Main field cites this paper.

SPT-3G D1: CMB temperature and polarization power spectra and cosmology from 2019 and 2020 observations of the SPT-3G Main field The Atacama Cosmology Telescope: Semi-Analytic Covariance Matrices for the DR6 CMB Power Spectra

Reference 55

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Observation 41343699-4c1c-4799-bf52-7779979745ed · inbound

Cosmic Birefringence from the Atacama Cosmology Telescope Data Release 6 cites this paper.

Cosmic Birefringence from the Atacama Cosmology Telescope Data Release 6 The Atacama Cosmology Telescope: Semi-Analytic Covariance Matrices for the DR6 CMB Power Spectra

Reference 29

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Observation 2716d834-bbb1-483c-a15c-d3d1495dd9ad · inbound

Constraining Inflationary Particle Production with CMB Polarization cites this paper.

Constraining Inflationary Particle Production with CMB Polarization The Atacama Cosmology Telescope: Semi-Analytic Covariance Matrices for the DR6 CMB Power Spectra

Reference 35

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Observation 0bb93b1f-2447-4242-a143-d42f301175ed · inbound

Analytical covariances for catalogue-based pseudo-$C_\ell$s cites this paper.

Analytical covariances for catalogue-based pseudo-$C_\ell$s The Atacama Cosmology Telescope: Semi-Analytic Covariance Matrices for the DR6 CMB Power Spectra

Reference 42

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Observation 095055fe-1bb9-4a8f-af07-d0706cd0b064 · inbound

Cosmic birefringence from a joint analysis of ACT and Planck cites this paper.

Cosmic birefringence from a joint analysis of ACT and Planck The Atacama Cosmology Telescope: Semi-Analytic Covariance Matrices for the DR6 CMB Power Spectra

Reference 43

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