Paper Citation Record · LEDGER

A p<0.0001 detection of CMB cooling in galactic halos and its possible relation to dark matter

As of 13 August 2026, this Paper Citation Record lists 33 of 33 outbound references and 3 inbound Pith citation observations for arXiv:2411.15307.

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

pith.paper-citation-record.v1
2411.15307 v2

Coverage vector

measured 33 of 33 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links, observed 2026-08-12T14:34:19.928908Z

measured 36 of 36 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-12T06:34:41.77262+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-06-27T15:25:40.842345Z

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

33 of 33 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 7851c2fb-b654-466d-9831-cf8c1abd4215 · outbound

This paper cites E 2024, ApJ, 969, 66.

A p<0.0001 detection of CMB cooling in galactic halos and its possible relation to dark matter E 2024, ApJ, 969, 66

Reference 1

Resolution: verified fuzzy; raw_fallback, observed 2026-08-12T14:34:20.500936Z

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Observation ab4750a2-754d-4c70-8e4b-198bedd04fc7 · outbound

This paper cites 2003, ApJS, 148, 97.

A p<0.0001 detection of CMB cooling in galactic halos and its possible relation to dark matter 2003, ApJS, 148, 97

Reference 2

Resolution: verified fuzzy; raw_fallback, observed 2026-08-12T14:34:20.485789Z

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Observation 02fa668f-9ead-460a-9bc7-07f26a51145e · outbound

This paper cites 2013, ApJ, 208, 20.

A p<0.0001 detection of CMB cooling in galactic halos and its possible relation to dark matter 2013, ApJ, 208, 20

Reference 3

Resolution: verified fuzzy; raw_fallback, observed 2026-08-12T14:34:20.470175Z

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Observation b44ad5bf-56c7-4fd8-924a-bebf3da2d889 · outbound

This paper cites & Shaw, D.J.

A p<0.0001 detection of CMB cooling in galactic halos and its possible relation to dark matter & Shaw, D.J

Reference 4

Resolution: verified fuzzy; raw_fallback, observed 2026-08-12T14:34:20.454918Z

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Observation 9e331d85-3972-4950-a5b6-53c3390ee7b1 · outbound

This paper cites 2023, MNRAS, 526, 5682.

A p<0.0001 detection of CMB cooling in galactic halos and its possible relation to dark matter 2023, MNRAS, 526, 5682

Reference 5

Resolution: verified fuzzy; raw_fallback, observed 2026-08-12T14:34:20.438643Z

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Observation 726c8c3c-95b4-4700-8ddb-a29414652e24 · outbound

This paper cites Unexplained correlation between the Cosmic Microwave Background temperature and the local matter density distribution.

A p<0.0001 detection of CMB cooling in galactic halos and its possible relation to dark matter Unexplained correlation between the Cosmic Microwave Background temperature and the local matter density distribution

Reference 6

Resolution: unresolved; no resolver link, observed 2026-08-12T14:34:19.789821Z

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Observation 0154b515-d116-4072-aea9-7571cc274df9 · outbound

This paper cites & Shaw, D.J.

A p<0.0001 detection of CMB cooling in galactic halos and its possible relation to dark matter & Shaw, D.J

Reference 7

Resolution: verified fuzzy; raw_fallback, observed 2026-08-12T14:34:20.421802Z

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Observation c616c837-bd15-4600-8c9d-a54fec8f3b26 · outbound

This paper cites and Kraljic , K.

A p<0.0001 detection of CMB cooling in galactic halos and its possible relation to dark matter and Kraljic , K

Reference 8

Resolution: verified fuzzy; raw_fallback, observed 2026-08-12T14:34:20.406305Z

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Observation 86a5f711-5a5d-45cc-95c0-e686134ed474 · outbound

This paper cites et al 2020, MNRAS, 495, 4542.

A p<0.0001 detection of CMB cooling in galactic halos and its possible relation to dark matter et al 2020, MNRAS, 495, 4542

Reference 9

Resolution: verified fuzzy; raw_fallback, observed 2026-08-12T14:34:20.389572Z

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Observation 9d2f33e8-2d5e-4054-bb4f-24f20235824c · outbound

This paper cites an unresolved cited work.

A p<0.0001 detection of CMB cooling in galactic halos and its possible relation to dark matter Unresolved cited work

Reference 10

Resolution: unresolved; raw_fallback, observed 2026-08-12T14:34:20.371450Z

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Observation 63b3ed29-502f-497b-9bdb-c21f9e68a9cc · outbound

This paper cites & Gazta \ n aga , E.

A p<0.0001 detection of CMB cooling in galactic halos and its possible relation to dark matter & Gazta \ n aga , E

Reference 11

Resolution: verified fuzzy; raw_fallback, observed 2026-08-12T14:34:20.354270Z

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Observation af7e8d21-039c-46d8-8eaa-a538a1ad8adc · outbound

This paper cites Langer , M.

A p<0.0001 detection of CMB cooling in galactic halos and its possible relation to dark matter Langer , M

Reference 12

Resolution: verified fuzzy; raw_fallback, observed 2026-08-12T14:34:20.338042Z

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Observation b844907e-dbf5-4585-9b18-d0c84b264ea7 · outbound

This paper cites K., Toscano, F., Luparello, H.

A p<0.0001 detection of CMB cooling in galactic halos and its possible relation to dark matter K., Toscano, F., Luparello, H

Reference 13

Resolution: verified fuzzy; raw_fallback, observed 2026-08-12T14:34:20.321811Z

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Observation cd65c759-4572-4f0e-98c6-91f0ea797c38 · outbound

This paper cites an unresolved cited work.

A p<0.0001 detection of CMB cooling in galactic halos and its possible relation to dark matter Unresolved cited work

Reference 14

Resolution: unresolved; raw_fallback, observed 2026-08-12T14:34:20.306415Z

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Observation 245befc9-961e-4b8b-8f55-7ec9718cf824 · outbound

This paper cites K., Boero, E.

A p<0.0001 detection of CMB cooling in galactic halos and its possible relation to dark matter K., Boero, E

Reference 15

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Observation 28f02a86-0595-4c7b-a123-4b83dd3becb1 · outbound

This paper cites 2012, ApJS, 199, 2.

A p<0.0001 detection of CMB cooling in galactic halos and its possible relation to dark matter 2012, ApJS, 199, 2

Reference 16

Resolution: verified fuzzy; raw_fallback, observed 2026-08-12T14:34:20.278227Z

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Observation 38b15989-4aae-42e8-ae0c-8466c1ec28f8 · outbound

This paper cites & Macri, L.M 2020, MNRAS, 497, 2954.

A p<0.0001 detection of CMB cooling in galactic halos and its possible relation to dark matter & Macri, L.M 2020, MNRAS, 497, 2954

Reference 17

Resolution: verified fuzzy; raw_fallback, observed 2026-08-12T14:34:20.261687Z

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Observation fff3935f-f336-46e4-abec-b0e9da8ec6b3 · outbound

This paper cites E, Boero, E.

A p<0.0001 detection of CMB cooling in galactic halos and its possible relation to dark matter E, Boero, E

Reference 18

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Observation 782ba92b-6ca6-415d-9ccd-6996cf4eb229 · outbound

This paper cites and Douspis , M.

A p<0.0001 detection of CMB cooling in galactic halos and its possible relation to dark matter and Douspis , M

Reference 19

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Observation d3988d53-80bc-41b0-9b3a-9b795c7b35ad · outbound

This paper cites and Bonjean , V.

A p<0.0001 detection of CMB cooling in galactic halos and its possible relation to dark matter and Bonjean , V

Reference 20

Resolution: verified fuzzy; raw_fallback, observed 2026-08-12T14:34:20.218745Z

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Observation 98e77870-4bda-49db-9b27-42aba0d88db8 · outbound

This paper cites & Mukherjee, S.

A p<0.0001 detection of CMB cooling in galactic halos and its possible relation to dark matter & Mukherjee, S

Reference 21

Resolution: verified fuzzy; raw_fallback, observed 2026-08-12T14:34:20.202917Z

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Observation 0f44a0f4-75d0-4659-a15c-b8dae19a8949 · outbound

This paper cites & Johnson, M.

A p<0.0001 detection of CMB cooling in galactic halos and its possible relation to dark matter & Johnson, M

Reference 22

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A p<0.0001 detection of CMB cooling in galactic halos and its possible relation to dark matter Unresolved cited work

Reference 23

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A p<0.0001 detection of CMB cooling in galactic halos and its possible relation to dark matter Unresolved cited work

Reference 24

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Observation 91b9e95c-0d5a-4642-b381-790cc7d24e94 · outbound

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A p<0.0001 detection of CMB cooling in galactic halos and its possible relation to dark matter Unresolved cited work

Reference 25

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A p<0.0001 detection of CMB cooling in galactic halos and its possible relation to dark matter Unresolved cited work

Reference 26

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Observation 85ef7aca-b792-4e53-a392-72daa22b199d · outbound

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A p<0.0001 detection of CMB cooling in galactic halos and its possible relation to dark matter Unresolved cited work

Reference 27

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Observation 3fd22e22-1a38-47c6-9bb5-7894ad7bab63 · outbound

This paper cites & Sigl, G.

A p<0.0001 detection of CMB cooling in galactic halos and its possible relation to dark matter & Sigl, G

Reference 28

Resolution: verified fuzzy; raw_fallback, observed 2026-08-12T14:34:20.080410Z

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Observation 418f7081-7b42-421d-b23f-053efebe9253 · outbound

This paper cites 2011, MNRAS, 414, 350.

A p<0.0001 detection of CMB cooling in galactic halos and its possible relation to dark matter 2011, MNRAS, 414, 350

Reference 29

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Observation 460d162c-8361-49f4-8e24-831b1b1ff38e · outbound

This paper cites and Kawahara , H.

A p<0.0001 detection of CMB cooling in galactic halos and its possible relation to dark matter and Kawahara , H

Reference 30

Resolution: verified fuzzy; raw_fallback, observed 2026-08-12T14:34:20.051407Z

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Observation e4339c86-7f25-45f1-b10f-39cae0b29358 · outbound

This paper cites Are CMB derived cosmological parameters affected by foregrounds associated to nearby galaxies?.

A p<0.0001 detection of CMB cooling in galactic halos and its possible relation to dark matter Are CMB derived cosmological parameters affected by foregrounds associated to nearby galaxies?

Reference 31

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Observation 721a7fde-e5b8-48b6-a2c1-a41c7d70da8c · outbound

This paper cites B., Sanz, J.

A p<0.0001 detection of CMB cooling in galactic halos and its possible relation to dark matter B., Sanz, J

Reference 32

Resolution: unresolved; no resolver link, observed 2026-08-12T14:34:19.923189Z

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Observation fe2913d5-82eb-41b5-861b-69d8a3e5357d · outbound

This paper cites & Lai, D.

A p<0.0001 detection of CMB cooling in galactic halos and its possible relation to dark matter & Lai, D

Reference 33

Resolution: verified fuzzy; raw_fallback, observed 2026-08-12T14:34:20.022321Z

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Pith citing papers

Observation df359049-3c0c-4f0b-b71d-5ad087478bdc · inbound

Cosmic filaments confirm unexplained CMB temperature decrements in two independent redshift ranges cites this paper.

Cosmic filaments confirm unexplained CMB temperature decrements in two independent redshift ranges A p<0.0001 detection of CMB cooling in galactic halos and its possible relation to dark matter

Reference 14

Resolution: verified exact; arxiv_id, observed 2026-05-19T10:22:14.445174Z

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Observation 5b5bdb68-34bb-422b-9de6-237ce2a88600 · inbound

Forecasts of CMB $E$-mode anomalies for AliCPT-1 cites this paper.

Forecasts of CMB $E$-mode anomalies for AliCPT-1 A p<0.0001 detection of CMB cooling in galactic halos and its possible relation to dark matter

Reference 32

Resolution: verified exact; arxiv_id, observed 2026-05-11T14:06:04.753800Z

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Observation 3aae36fc-bbb1-4f0b-97fc-6f8868477388 · inbound

The Manticore Project II: Bayesian digital twins of cosmic structure across the SDSS and BOSS volumes cites this paper.

The Manticore Project II: Bayesian digital twins of cosmic structure across the SDSS and BOSS volumes A p<0.0001 detection of CMB cooling in galactic halos and its possible relation to dark matter

Reference 12

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