Paper Citation Record · LEDGER

Cross-frequency SGWB anisotropy from compact topology: CMB B-mode covariance as a transfer probe

As of 13 August 2026, this Paper Citation Record lists 33 of 33 outbound references and 0 inbound Pith citation observations for arXiv:2608.09697.

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

pith.paper-citation-record.v1
2608.09697 v1

Coverage vector

measured 33 of 33 reference resolution

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Source: paper_references, paper_reference_links, observed 2026-08-11T12:38:58.844603Z

measured 33 of 33 standing notices

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Source: scholarly_work_events, retraction_status_cache, observed 2026-08-13T06:32:02.005865+00:00

measured 0 of 0 inbound itemization

Pith citing papers itemized under the disclosed page cap.

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measured 0 of 1 external citation measurements

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

Source: cited_works

Reference resolution

33 of 33 outbound references displayed

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External citation measurements

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Outbound references

Observation 9c7ef8f4-6482-4cd0-b69d-8af3a793b682 · outbound

This paper cites Lachi` eze-Rey and J.-P.

Cross-frequency SGWB anisotropy from compact topology: CMB B-mode covariance as a transfer probe Lachi` eze-Rey and J.-P

Reference 1

Resolution: verified fuzzy; raw_fallback, observed 2026-08-11T12:38:59.786911Z

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Observation aaf32623-5c7e-4b0e-9408-9230b3796166 · outbound

This paper cites Levin, Phys.

Cross-frequency SGWB anisotropy from compact topology: CMB B-mode covariance as a transfer probe Levin, Phys

Reference 2

Resolution: verified exact; raw_fallback, observed 2026-08-11T12:38:59.675450Z

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Observation e44c6da6-0a3f-466e-a154-81125bf12f95 · outbound

This paper cites an unresolved cited work.

Cross-frequency SGWB anisotropy from compact topology: CMB B-mode covariance as a transfer probe Unresolved cited work

Reference 3

Resolution: verified exact; raw_fallback, observed 2026-08-11T12:38:59.582460Z

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Observation d62a1495-10ef-4ad6-8ac6-e0a10ce63c4b · outbound

This paper cites Planck 2015 results. XVIII. Background geometry & topology.

Cross-frequency SGWB anisotropy from compact topology: CMB B-mode covariance as a transfer probe Planck 2015 results. XVIII. Background geometry & topology

Reference 4

Resolution: unresolved; no resolver link, observed 2026-08-11T12:38:58.692749Z

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Observation 27cd060f-5abe-4693-963a-982b87c96abe · outbound

This paper cites Cosmic topology. Part I. Limits on orientable Euclidean manifolds from circle searches.

Cross-frequency SGWB anisotropy from compact topology: CMB B-mode covariance as a transfer probe Cosmic topology. Part I. Limits on orientable Euclidean manifolds from circle searches

Reference 5

Resolution: unresolved; no resolver link, observed 2026-08-11T12:38:58.698452Z

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Observation 09ae4488-43e3-4229-b472-9d4306e10da9 · outbound

This paper cites Promise of Future Searches for Cosmic Topology.

Cross-frequency SGWB anisotropy from compact topology: CMB B-mode covariance as a transfer probe Promise of Future Searches for Cosmic Topology

Reference 6

Resolution: unresolved; no resolver link, observed 2026-08-11T12:38:58.704575Z

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Observation cfb7074d-5cb9-4544-ae91-4c1bc61a301e · outbound

This paper cites Cosmic topology. Part IIa. Eigenmodes, correlation matrices, and detectability of orientable Euclidean manifolds.

Cross-frequency SGWB anisotropy from compact topology: CMB B-mode covariance as a transfer probe Cosmic topology. Part IIa. Eigenmodes, correlation matrices, and detectability of orientable Euclidean manifolds

Reference 7

Resolution: unresolved; no resolver link, observed 2026-08-11T12:38:58.711023Z

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Observation 0caf982b-9667-4703-92d1-623eaca31138 · outbound

This paper cites Cosmic topology. Part IIIb. Eigenmodes and correlation matrices of spin-2 perturbations in orientable Euclidean manifolds.

Cross-frequency SGWB anisotropy from compact topology: CMB B-mode covariance as a transfer probe Cosmic topology. Part IIIb. Eigenmodes and correlation matrices of spin-2 perturbations in orientable Euclidean manifolds

Reference 8

Resolution: unresolved; no resolver link, observed 2026-08-11T12:38:58.716863Z

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Observation f3e71ed3-f59f-4e17-b9e3-f03a6dfff06b · outbound

This paper cites CMB statistical anisotropy from noncommutative gravitational waves.

Cross-frequency SGWB anisotropy from compact topology: CMB B-mode covariance as a transfer probe CMB statistical anisotropy from noncommutative gravitational waves

Reference 9

Resolution: verified exact; local_arxiv, observed 2026-08-11T12:38:59.361385Z

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Observation 6c9a6880-14d3-42e1-a15d-861e6ec1cf8f · outbound

This paper cites Hunting for Statistical Anisotropy in Tensor Modes with B-mode Observations.

Cross-frequency SGWB anisotropy from compact topology: CMB B-mode covariance as a transfer probe Hunting for Statistical Anisotropy in Tensor Modes with B-mode Observations

Reference 10

Resolution: verified exact; local_arxiv, observed 2026-08-11T12:38:59.331223Z

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Observation e3f06a31-3817-4c06-b54b-7cfd7cd63149 · outbound

This paper cites Cosmic topology. Part IIIa. Microwave background parity violation without parity-violating microphysics.

Cross-frequency SGWB anisotropy from compact topology: CMB B-mode covariance as a transfer probe Cosmic topology. Part IIIa. Microwave background parity violation without parity-violating microphysics

Reference 11

Resolution: unresolved; no resolver link, observed 2026-08-11T12:38:58.732173Z

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Observation 54193848-f1a7-40ee-808f-0921bebbf6c2 · outbound

This paper cites an unresolved cited work.

Cross-frequency SGWB anisotropy from compact topology: CMB B-mode covariance as a transfer probe Unresolved cited work

Reference 12

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Observation cf5d826c-0990-4aa2-8f3c-9a2b3cc7980b · outbound

This paper cites An All-Sky Analysis of Polarization in the Microwave Background.

Cross-frequency SGWB anisotropy from compact topology: CMB B-mode covariance as a transfer probe An All-Sky Analysis of Polarization in the Microwave Background

Reference 13

Resolution: unresolved; no resolver link, observed 2026-08-11T12:38:58.737233Z

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Observation 674880b1-2a1f-4f6a-ac95-3adaf49117fe · outbound

This paper cites Statistics of Cosmic Microwave Background Polarization.

Cross-frequency SGWB anisotropy from compact topology: CMB B-mode covariance as a transfer probe Statistics of Cosmic Microwave Background Polarization

Reference 14

Resolution: unresolved; no resolver link, observed 2026-08-11T12:38:58.742164Z

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Observation ca0777fa-14ac-4ee1-8e9b-599c971d00fe · outbound

This paper cites Cosmic Microwave Background Fluctuations from Gravitational Waves: An Analytic Approach.

Cross-frequency SGWB anisotropy from compact topology: CMB B-mode covariance as a transfer probe Cosmic Microwave Background Fluctuations from Gravitational Waves: An Analytic Approach

Reference 15

Resolution: unresolved; no resolver link, observed 2026-08-11T12:38:58.747936Z

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Observation d8342f22-b7f2-4717-9b65-09db84aedb34 · outbound

This paper cites Detection methods for stochastic gravitational-wave backgrounds: a unified treatment.

Cross-frequency SGWB anisotropy from compact topology: CMB B-mode covariance as a transfer probe Detection methods for stochastic gravitational-wave backgrounds: a unified treatment

Reference 16

Resolution: unresolved; no resolver link, observed 2026-08-11T12:38:58.754080Z

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Observation 7daef16c-4741-42f2-91cb-21cae0c6401e · outbound

This paper cites Characterising gravitational wave stochastic background anisotropy with Pulsar Timing Arrays.

Cross-frequency SGWB anisotropy from compact topology: CMB B-mode covariance as a transfer probe Characterising gravitational wave stochastic background anisotropy with Pulsar Timing Arrays

Reference 17

Resolution: unresolved; no resolver link, observed 2026-08-11T12:38:58.759991Z

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Observation 82655223-18a2-4c96-b75c-6bb385fa0f8d · outbound

This paper cites Searching For Anisotropic Gravitational-wave Backgrounds Using Pulsar Timing Arrays.

Cross-frequency SGWB anisotropy from compact topology: CMB B-mode covariance as a transfer probe Searching For Anisotropic Gravitational-wave Backgrounds Using Pulsar Timing Arrays

Reference 18

Resolution: unresolved; no resolver link, observed 2026-08-11T12:38:58.765494Z

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Observation c0b20e1e-13a9-4774-b76b-fdbe1658fd34 · outbound

This paper cites The NANOGrav 15-year Data Set: Search for Anisotropy in the Gravitational-Wave Background.

Cross-frequency SGWB anisotropy from compact topology: CMB B-mode covariance as a transfer probe The NANOGrav 15-year Data Set: Search for Anisotropy in the Gravitational-Wave Background

Reference 19

Resolution: unresolved; no resolver link, observed 2026-08-11T12:38:58.770784Z

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Observation 2adf2ac3-c89c-4776-97cd-3744fa50a39e · outbound

This paper cites Probing Anisotropies of the Stochastic Gravitational Wave Background with LISA.

Cross-frequency SGWB anisotropy from compact topology: CMB B-mode covariance as a transfer probe Probing Anisotropies of the Stochastic Gravitational Wave Background with LISA

Reference 20

Resolution: unresolved; no resolver link, observed 2026-08-11T12:38:58.776579Z

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Observation 358a7124-741b-45b0-8479-10ecf3dff019 · outbound

This paper cites Measuring the anisotropies in astrophysical and cosmological gravitational-wave backgrounds with Taiji and LISA networks.

Cross-frequency SGWB anisotropy from compact topology: CMB B-mode covariance as a transfer probe Measuring the anisotropies in astrophysical and cosmological gravitational-wave backgrounds with Taiji and LISA networks

Reference 21

Resolution: unresolved; no resolver link, observed 2026-08-11T12:38:58.783002Z

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Observation 7bcd4999-265b-4755-bbea-cbb20593ffdc · outbound

This paper cites an unresolved cited work.

Cross-frequency SGWB anisotropy from compact topology: CMB B-mode covariance as a transfer probe Unresolved cited work

Reference 22

Resolution: unresolved; no resolver link, observed 2026-08-11T12:38:58.788565Z

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Observation f7ba8763-1385-4dd1-be41-0fea2d580568 · outbound

This paper cites Hamermesh,Group Theory and Its Application to Physical Problems(Addison-Wesley, Reading, MA, 1962) Dover reprint, New York, 1989.

Cross-frequency SGWB anisotropy from compact topology: CMB B-mode covariance as a transfer probe Hamermesh,Group Theory and Its Application to Physical Problems(Addison-Wesley, Reading, MA, 1962) Dover reprint, New York, 1989

Reference 23

Resolution: verified fuzzy; raw_fallback, observed 2026-08-11T12:38:59.755966Z

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Observation b5cb7ea5-e6b2-4110-a98c-261103e6742c · outbound

This paper cites Simulating Cosmic Microwave Background maps in multi-connected spaces.

Cross-frequency SGWB anisotropy from compact topology: CMB B-mode covariance as a transfer probe Simulating Cosmic Microwave Background maps in multi-connected spaces

Reference 24

Resolution: verified exact; local_arxiv, observed 2026-08-11T12:38:59.101497Z

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Observation c220556f-857e-4c61-b93a-8c1e80d8a091 · outbound

This paper cites Laser Interferometer Space Antenna.

Cross-frequency SGWB anisotropy from compact topology: CMB B-mode covariance as a transfer probe Laser Interferometer Space Antenna

Reference 25

Resolution: unresolved; no resolver link, observed 2026-08-11T12:38:58.804167Z

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Observation 9a5ccd24-b440-44ae-9767-e55f06b4e878 · outbound

This paper cites an unresolved cited work.

Cross-frequency SGWB anisotropy from compact topology: CMB B-mode covariance as a transfer probe Unresolved cited work

Reference 26

Resolution: unresolved; raw_fallback, observed 2026-08-11T12:38:59.735341Z

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No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.

Observation bbed1689-0ac4-425b-bde7-a456f01fdde7 · outbound

This paper cites TianQin: a space-borne gravitational wave detector.

Cross-frequency SGWB anisotropy from compact topology: CMB B-mode covariance as a transfer probe TianQin: a space-borne gravitational wave detector

Reference 27

Resolution: unresolved; no resolver link, observed 2026-08-11T12:38:58.813966Z

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Observation f0ba8980-4fae-46a5-bc5f-49ad508ddf78 · outbound

This paper cites an unresolved cited work.

Cross-frequency SGWB anisotropy from compact topology: CMB B-mode covariance as a transfer probe Unresolved cited work

Reference 28

Resolution: unresolved; raw_fallback, observed 2026-08-11T12:38:59.716844Z

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No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.

Observation 2bf46fc6-f1ea-48ab-a5e0-8ca8755d6b69 · outbound

This paper cites Tomita, Prog.

Cross-frequency SGWB anisotropy from compact topology: CMB B-mode covariance as a transfer probe Tomita, Prog

Reference 29

Resolution: verified fuzzy; raw_fallback, observed 2026-08-11T12:38:59.698110Z

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Observation e7135167-2a4b-403b-b8a7-4a24dc15d41d · outbound

This paper cites Karhunen-Loeve eigenvalue problems in cosmology: how should we tackle large data sets?.

Cross-frequency SGWB anisotropy from compact topology: CMB B-mode covariance as a transfer probe Karhunen-Loeve eigenvalue problems in cosmology: how should we tackle large data sets?

Reference 30

Resolution: unresolved; no resolver link, observed 2026-08-11T12:38:58.829482Z

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Observation 7b054344-1cb7-4372-bb9d-cb7fffe987d8 · outbound

This paper cites Efficient Computation of CMB anisotropies in closed FRW models.

Cross-frequency SGWB anisotropy from compact topology: CMB B-mode covariance as a transfer probe Efficient Computation of CMB anisotropies in closed FRW models

Reference 31

Resolution: unresolved; no resolver link, observed 2026-08-11T12:38:58.834783Z

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Observation 34fec55a-bc57-434e-a646-d96b99de0975 · outbound

This paper cites Planck 2018 results. VI. Cosmological parameters.

Cross-frequency SGWB anisotropy from compact topology: CMB B-mode covariance as a transfer probe Planck 2018 results. VI. Cosmological parameters

Reference 32

Resolution: unresolved; no resolver link, observed 2026-08-11T12:38:58.840031Z

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Unavailable: canonical work link unavailable.

Observation a74a0ebc-c30a-41ca-9ade-8e6557e162f0 · outbound

This paper cites an unresolved cited work.

Cross-frequency SGWB anisotropy from compact topology: CMB B-mode covariance as a transfer probe Unresolved cited work

Reference 33

Resolution: unresolved; no resolver link, observed 2026-08-11T12:38:58.844603Z

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