Paper Citation Record · LEDGER

Is the lack of power anomaly in the CMB correlated with the orientation of the Galactic plane?

As of 14 August 2026, this Paper Citation Record lists 25 of 25 outbound references and 0 inbound Pith citation observations for arXiv:1908.10637.

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

pith.paper-citation-record.v1
1908.10637 v2

Coverage vector

measured 25 of 25 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links, observed 2026-08-14T10:44:58.115589Z

measured 25 of 25 standing notices

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Source: scholarly_work_events, retraction_status_cache, observed 2026-08-14T06:32:32.682623+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

25 of 25 outbound references displayed

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External citation measurements

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Outbound references

Observation e85664de-1b54-410d-bf2c-f724832020e4 · outbound

This paper cites Monteserin, R.

Is the lack of power anomaly in the CMB correlated with the orientation of the Galactic plane? Monteserin, R

Reference 1

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Observation 1e86a3a5-e9f8-4d0a-916e-9d3dd1267917 · outbound

This paper cites Low Variance at large scales of WMAP 9 year data.

Is the lack of power anomaly in the CMB correlated with the orientation of the Galactic plane? Low Variance at large scales of WMAP 9 year data

Reference 3

Resolution: unresolved; no resolver link, observed 2026-08-14T10:44:58.017518Z

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Observation 87ff7dcf-f9da-4cde-a034-2c79affeba5e · outbound

This paper cites Planck 2013 results. XXIII. Isotropy and statistics of the CMB.

Is the lack of power anomaly in the CMB correlated with the orientation of the Galactic plane? Planck 2013 results. XXIII. Isotropy and statistics of the CMB

Reference 4

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Observation 487cd017-f761-47fb-82da-d9615efd9155 · outbound

This paper cites Planck 2015 results. XVI. Isotropy and statistics of the CMB.

Is the lack of power anomaly in the CMB correlated with the orientation of the Galactic plane? Planck 2015 results. XVI. Isotropy and statistics of the CMB

Reference 5

Resolution: unresolved; no resolver link, observed 2026-08-14T10:44:58.026729Z

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Observation 6460a8c5-3891-40e2-8aae-5a6b64a94a18 · outbound

This paper cites Planck 2018 results. VII. Isotropy and Statistics of the CMB.

Is the lack of power anomaly in the CMB correlated with the orientation of the Galactic plane? Planck 2018 results. VII. Isotropy and Statistics of the CMB

Reference 6

Resolution: unresolved; no resolver link, observed 2026-08-14T10:44:58.031083Z

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Observation 1e9f1d92-5e4e-45a5-a783-e9f5f5059f4f · outbound

This paper cites The Uncorrelated Universe: Statistical Anisotropy and the Vanishing Angular Correlation Function in WMAP Years 1-3.

Is the lack of power anomaly in the CMB correlated with the orientation of the Galactic plane? The Uncorrelated Universe: Statistical Anisotropy and the Vanishing Angular Correlation Function in WMAP Years 1-3

Reference 7

Resolution: verified exact; local_arxiv, observed 2026-08-14T10:44:58.410935Z

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No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation d324484c-5f3a-432e-8184-df37847019b9 · outbound

This paper cites Large-angle anomalies in the CMB.

Is the lack of power anomaly in the CMB correlated with the orientation of the Galactic plane? Large-angle anomalies in the CMB

Reference 9

Resolution: unresolved; no resolver link, observed 2026-08-14T10:44:58.044042Z

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Observation c340e463-cb17-45c2-9610-dbac609f366a · outbound

This paper cites CMB Anomalies after Planck.

Is the lack of power anomaly in the CMB correlated with the orientation of the Galactic plane? CMB Anomalies after Planck

Reference 10

Resolution: unresolved; no resolver link, observed 2026-08-14T10:44:58.048427Z

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Observation 918429a1-a1aa-4054-8538-8b9dd08e554c · outbound

This paper cites Covariance of CMB anomalies.

Is the lack of power anomaly in the CMB correlated with the orientation of the Galactic plane? Covariance of CMB anomalies

Reference 11

Resolution: unresolved; no resolver link, observed 2026-08-14T10:44:58.052453Z

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Observation 0f108f92-0b18-4f61-9a47-8c1f1b1fccc8 · outbound

This paper cites Observational Hints of a Pre--Inflationary Scale?.

Is the lack of power anomaly in the CMB correlated with the orientation of the Galactic plane? Observational Hints of a Pre--Inflationary Scale?

Reference 12

Resolution: verified exact; local_arxiv, observed 2026-08-14T10:44:58.306721Z

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Observation 6958c8fe-4895-4f6c-bd9f-a5fb92aa9bad · outbound

This paper cites A Complete Statistical Analysis for the Quadrupole Amplitude in an Ellipsoidal Universe.

Is the lack of power anomaly in the CMB correlated with the orientation of the Galactic plane? A Complete Statistical Analysis for the Quadrupole Amplitude in an Ellipsoidal Universe

Reference 13

Resolution: verified exact; local_arxiv, observed 2026-08-14T10:44:58.291782Z

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No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation 882e638c-ad44-492f-96fd-57d34687175c · outbound

This paper cites Contamination cannot explain the lack of large-scale power in the cosmic microwave background radiation.

Is the lack of power anomaly in the CMB correlated with the orientation of the Galactic plane? Contamination cannot explain the lack of large-scale power in the cosmic microwave background radiation

Reference 14

Resolution: verified exact; local_arxiv, observed 2026-08-14T10:44:58.276110Z

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Observation 674b2fbd-48ea-45a0-839e-5c60260598d5 · outbound

This paper cites Pre-Inflationary Relics in the CMB?.

Is the lack of power anomaly in the CMB correlated with the orientation of the Galactic plane? Pre-Inflationary Relics in the CMB?

Reference 15

Resolution: unresolved; no resolver link, observed 2026-08-14T10:44:58.068441Z

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Observation 8365efb8-ba54-46c2-8269-5262a7d01e50 · outbound

This paper cites The Evens and Odds of CMB Anomalies.

Is the lack of power anomaly in the CMB correlated with the orientation of the Galactic plane? The Evens and Odds of CMB Anomalies

Reference 16

Resolution: verified exact; local_arxiv, observed 2026-08-14T10:44:58.249690Z

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No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation 2369e268-0824-402b-a356-a7e59bac2afd · outbound

This paper cites Anomalous parity asymmetry of the Wilkinson Microwave Anisotropy Probe power spectrum data at low multipoles.

Is the lack of power anomaly in the CMB correlated with the orientation of the Galactic plane? Anomalous parity asymmetry of the Wilkinson Microwave Anisotropy Probe power spectrum data at low multipoles

Reference 17

Resolution: unresolved; no resolver link, observed 2026-08-14T10:44:58.076224Z

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Observation 8a000b0d-afd7-408b-9fb7-9feef9922182 · outbound

This paper cites Anomalous parity asymmetry of WMAP power spectrum data at low multpoles: is it cosmological or systematics?.

Is the lack of power anomaly in the CMB correlated with the orientation of the Galactic plane? Anomalous parity asymmetry of WMAP power spectrum data at low multpoles: is it cosmological or systematics?

Reference 18

Resolution: verified exact; local_arxiv, observed 2026-08-14T10:44:58.221096Z

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No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation 0665afaa-51d6-4ea9-a904-5b6046fcd81a · outbound

This paper cites Gruppuso, F.

Is the lack of power anomaly in the CMB correlated with the orientation of the Galactic plane? Gruppuso, F

Reference 19

Resolution: unresolved; no resolver link, observed 2026-08-14T10:44:58.083791Z

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Observation 031e4c7b-36c0-47f8-a0dc-ccf97a397da2 · outbound

This paper cites Planck 2015 results. XI. CMB power spectra, likelihoods, and robustness of parameters.

Is the lack of power anomaly in the CMB correlated with the orientation of the Galactic plane? Planck 2015 results. XI. CMB power spectra, likelihoods, and robustness of parameters

Reference 20

Resolution: unresolved; no resolver link, observed 2026-08-14T10:44:58.087657Z

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Observation 96cc7806-d1c3-42d0-abe6-f1018a6f40b7 · outbound

This paper cites Planck 2018 results. IV. Diffuse component separation.

Is the lack of power anomaly in the CMB correlated with the orientation of the Galactic plane? Planck 2018 results. IV. Diffuse component separation

Reference 21

Resolution: unresolved; no resolver link, observed 2026-08-14T10:44:58.091658Z

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Observation 455f79d0-928f-4ae9-8e7b-f30ee361ccd8 · outbound

This paper cites Planck 2018 results. V. CMB power spectra and likelihoods.

Is the lack of power anomaly in the CMB correlated with the orientation of the Galactic plane? Planck 2018 results. V. CMB power spectra and likelihoods

Reference 22

Resolution: unresolved; no resolver link, observed 2026-08-14T10:44:58.095641Z

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Observation b88773e7-7d86-4403-b4d8-3066cbb26cf6 · outbound

This paper cites HEALPix -- a Framework for High Resolution Discretization, and Fast Analysis of Data Distributed on the Sphere.

Is the lack of power anomaly in the CMB correlated with the orientation of the Galactic plane? HEALPix -- a Framework for High Resolution Discretization, and Fast Analysis of Data Distributed on the Sphere

Reference 23

Resolution: unresolved; no resolver link, observed 2026-08-14T10:44:58.099764Z

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Observation 0f421a92-3261-47dd-8167-6dc2815bdbd2 · outbound

This paper cites Gruppuso, A.

Is the lack of power anomaly in the CMB correlated with the orientation of the Galactic plane? Gruppuso, A

Reference 24

Resolution: unresolved; no resolver link, observed 2026-08-14T10:44:58.104166Z

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Observation c4dd626b-772f-418b-9e42-1f26dca737e9 · outbound

This paper cites an unresolved cited work.

Is the lack of power anomaly in the CMB correlated with the orientation of the Galactic plane? Unresolved cited work

Reference 25

Resolution: unresolved; no resolver link, observed 2026-08-14T10:44:58.107885Z

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Observation 02be69b0-fdf4-4cde-9a3b-55c75d204b04 · outbound

This paper cites and de Oliveira-Costa, A., Phys.

Is the lack of power anomaly in the CMB correlated with the orientation of the Galactic plane? and de Oliveira-Costa, A., Phys

Reference 26

Resolution: unresolved; no resolver link, observed 2026-08-14T10:44:58.111800Z

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Observation 8aec7434-e290-4e2f-90b2-55e8dba51f80 · outbound

This paper cites A comparison of CMB Angular Power Spectrum Estimators at Large Scales: the TT case.

Is the lack of power anomaly in the CMB correlated with the orientation of the Galactic plane? A comparison of CMB Angular Power Spectrum Estimators at Large Scales: the TT case

Reference 27

Resolution: verified exact; local_arxiv, observed 2026-08-14T10:44:58.165116Z

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No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Pith citing papers

No inbound Pith citation observations are available.