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Paper Citation Record · LEDGER

Constraining the Hubble parameter with the 21 cm brightness temperature signal in a universe with inhomogeneities

As of 8 August 2026, this Paper Citation Record lists 100 of 127 outbound references and 3 inbound Pith citation observations for arXiv:2505.22219.

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

pith.paper-citation-record.v1
2505.22219 v2

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measured 100 of 127 reference resolution

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Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T13:18:42.676548Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-02T06:36:43.763109Z

Reference resolution

100 of 127 outbound references displayed

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External citation measurements

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Outbound references

Observation ba12e87b-0224-49d4-8e0a-522b61732776 · outbound

This paper cites The CosmoVerse White Paper: Addressing observational tensions in cosmology with systematics and fundamental physics.

Constraining the Hubble parameter with the 21 cm brightness temperature signal in a universe with inhomogeneities The CosmoVerse White Paper: Addressing observational tensions in cosmology with systematics and fundamental physics

Reference 1

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Observation f4e2b6c7-c1ae-4ab1-b597-aba0c7b029fe · outbound

This paper cites ´O Colg´ ain, S.

Constraining the Hubble parameter with the 21 cm brightness temperature signal in a universe with inhomogeneities ´O Colg´ ain, S

Reference 2

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Constraining the Hubble parameter with the 21 cm brightness temperature signal in a universe with inhomogeneities Unresolved cited work

Reference 3

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Constraining the Hubble parameter with the 21 cm brightness temperature signal in a universe with inhomogeneities Unresolved cited work

Reference 4

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Observation 1d92aed3-45bf-4cc6-b09e-fb10e98b8d10 · outbound

This paper cites Aghanim, Y.

Constraining the Hubble parameter with the 21 cm brightness temperature signal in a universe with inhomogeneities Aghanim, Y

Reference 5

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Constraining the Hubble parameter with the 21 cm brightness temperature signal in a universe with inhomogeneities Unresolved cited work

Reference 6

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Constraining the Hubble parameter with the 21 cm brightness temperature signal in a universe with inhomogeneities Unresolved cited work

Reference 7

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Constraining the Hubble parameter with the 21 cm brightness temperature signal in a universe with inhomogeneities Unresolved cited work

Reference 8

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Constraining the Hubble parameter with the 21 cm brightness temperature signal in a universe with inhomogeneities Unresolved cited work

Reference 9

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Observation 654e319d-f428-4f11-b783-d0e508633067 · outbound

This paper cites Dainotti, B.

Constraining the Hubble parameter with the 21 cm brightness temperature signal in a universe with inhomogeneities Dainotti, B

Reference 10

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Observation 5c7442eb-7ed1-4444-b807-73aaf63dada9 · outbound

This paper cites Labb´ e, P.

Constraining the Hubble parameter with the 21 cm brightness temperature signal in a universe with inhomogeneities Labb´ e, P

Reference 11

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Observation 2f85f7b5-7bc2-4441-a93a-ef5dbcf4ac1b · outbound

This paper cites Boylan-Kolchin, Nature Astronomy 7, 731–735 (2023).

Constraining the Hubble parameter with the 21 cm brightness temperature signal in a universe with inhomogeneities Boylan-Kolchin, Nature Astronomy 7, 731–735 (2023)

Reference 12

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Constraining the Hubble parameter with the 21 cm brightness temperature signal in a universe with inhomogeneities Unresolved cited work

Reference 13

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Observation 5047d567-dfaf-4afb-8104-c6fda28f376a · outbound

This paper cites Wiegand, T.

Constraining the Hubble parameter with the 21 cm brightness temperature signal in a universe with inhomogeneities Wiegand, T

Reference 14

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Constraining the Hubble parameter with the 21 cm brightness temperature signal in a universe with inhomogeneities Unresolved cited work

Reference 15

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This paper cites Gigaparsec structures are nowhere to be seen in $\Lambda$CDM: an enhanced analysis of LSS in FLAMINGO-10K simulations.

Constraining the Hubble parameter with the 21 cm brightness temperature signal in a universe with inhomogeneities Gigaparsec structures are nowhere to be seen in $\Lambda$CDM: an enhanced analysis of LSS in FLAMINGO-10K simulations

Reference 16

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Observation 0b20613e-6467-4453-a16e-8c35cab17e7c · outbound

This paper cites The Emperor's New Arc: gigaparsec patterns abound in a $\Lambda$CDM universe.

Constraining the Hubble parameter with the 21 cm brightness temperature signal in a universe with inhomogeneities The Emperor's New Arc: gigaparsec patterns abound in a $\Lambda$CDM universe

Reference 17

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Observation c5d084f5-19bc-42de-9dd2-e2a2d69bfcd4 · outbound

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Constraining the Hubble parameter with the 21 cm brightness temperature signal in a universe with inhomogeneities Sawala and M

Reference 18

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Constraining the Hubble parameter with the 21 cm brightness temperature signal in a universe with inhomogeneities Barkana and A

Reference 19

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Constraining the Hubble parameter with the 21 cm brightness temperature signal in a universe with inhomogeneities Unresolved cited work

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Constraining the Hubble parameter with the 21 cm brightness temperature signal in a universe with inhomogeneities Barkana, Physics Reports 645, 1 (2016)

Reference 22

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This paper cites Constraining the Hubble parameter with the 21 cm brightness temperature signal in a universe with inhomogeneities.

Constraining the Hubble parameter with the 21 cm brightness temperature signal in a universe with inhomogeneities Constraining the Hubble parameter with the 21 cm brightness temperature signal in a universe with inhomogeneities

Reference 23

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Constraining the Hubble parameter with the 21 cm brightness temperature signal in a universe with inhomogeneities Unresolved cited work

Reference 24

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Constraining the Hubble parameter with the 21 cm brightness temperature signal in a universe with inhomogeneities Madau, A

Reference 25

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This paper cites Mesinger, ed., The Cosmic 21-cm Revolution, 2514- 3433 (IOP Publishing, 2019).

Constraining the Hubble parameter with the 21 cm brightness temperature signal in a universe with inhomogeneities Mesinger, ed., The Cosmic 21-cm Revolution, 2514- 3433 (IOP Publishing, 2019)

Reference 27

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Constraining the Hubble parameter with the 21 cm brightness temperature signal in a universe with inhomogeneities Halder, S

Reference 28

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Constraining the Hubble parameter with the 21 cm brightness temperature signal in a universe with inhomogeneities Singh, J

Reference 29

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Constraining the Hubble parameter with the 21 cm brightness temperature signal in a universe with inhomogeneities ambient region,

Reference 30

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Constraining the Hubble parameter with the 21 cm brightness temperature signal in a universe with inhomogeneities Halder, M

Reference 32

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Constraining the Hubble parameter with the 21 cm brightness temperature signal in a universe with inhomogeneities Mukhopadhyay, D

Reference 33

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Constraining the Hubble parameter with the 21 cm brightness temperature signal in a universe with inhomogeneities Halder and M

Reference 34

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Constraining the Hubble parameter with the 21 cm brightness temperature signal in a universe with inhomogeneities Feng and G

Reference 35

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Constraining the Hubble parameter with the 21 cm brightness temperature signal in a universe with inhomogeneities Ewall-Wice, T.-C

Reference 36

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Constraining the Hubble parameter with the 21 cm brightness temperature signal in a universe with inhomogeneities Fialkov and R

Reference 37

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Constraining the Hubble parameter with the 21 cm brightness temperature signal in a universe with inhomogeneities Ewall-Wice, T.-C

Reference 38

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Constraining the Hubble parameter with the 21 cm brightness temperature signal in a universe with inhomogeneities Unresolved cited work

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Constraining the Hubble parameter with the 21 cm brightness temperature signal in a universe with inhomogeneities Yang, Phys

Reference 40

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Constraining the Hubble parameter with the 21 cm brightness temperature signal in a universe with inhomogeneities Mittal, A

Reference 41

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This paper cites Kumar Aluri, P.

Constraining the Hubble parameter with the 21 cm brightness temperature signal in a universe with inhomogeneities Kumar Aluri, P

Reference 42

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Observation e3f350e5-2f21-4302-86fe-0221c46b637b · outbound

This paper cites Issues in the Philosophy of Cosmology.

Constraining the Hubble parameter with the 21 cm brightness temperature signal in a universe with inhomogeneities Issues in the Philosophy of Cosmology

Reference 43

Resolution
unresolved
no resolver link, observed 2026-08-07T13:18:46.581053Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T13:18:46.581053Z digest=sha256:822dd86e9eaa363a63424f2fd9f8cae6e13d261a6c706aed40336f07f7864113

Observation b3ba50b8-56c1-4a1a-95e6-2328632060cd · outbound

This paper cites Clarkson and R.

Constraining the Hubble parameter with the 21 cm brightness temperature signal in a universe with inhomogeneities Clarkson and R

Reference 44

Resolution
unresolved
no resolver link, observed 2026-08-07T13:18:46.698566Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T13:18:46.698566Z digest=sha256:83c36547e3a97441c393465d19ed2711b3e378aa0de7746bd89dc70b26b3f197

Observation 4250670a-64ac-4d0e-9b7f-3f3ee2f2ecd9 · outbound

This paper cites an unresolved cited work.

Constraining the Hubble parameter with the 21 cm brightness temperature signal in a universe with inhomogeneities Unresolved cited work

Reference 45

Resolution
unresolved
no resolver link, observed 2026-08-07T13:18:46.754827Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T13:18:46.754827Z digest=sha256:c31f971ce0693e64a6c1a10d9a8e7cf3ba63d5dff2e7e43298196c0d67aba2d8

Observation 9daf381c-1cc1-44ef-bbb0-16f599204ee2 · outbound

This paper cites Futamase, Phys.

Constraining the Hubble parameter with the 21 cm brightness temperature signal in a universe with inhomogeneities Futamase, Phys

Reference 46

Resolution
unresolved
no resolver link, observed 2026-08-07T13:18:46.934148Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T13:18:46.934148Z digest=sha256:39a5d2ebf19e4ce23b75844db840f777b377a7e338e5ec2799fc28d527accdcc

Observation ef5cf127-54a6-49b0-9446-80e8782adab1 · outbound

This paper cites an unresolved cited work.

Constraining the Hubble parameter with the 21 cm brightness temperature signal in a universe with inhomogeneities Unresolved cited work

Reference 47

Resolution
unresolved
no resolver link, observed 2026-08-07T13:18:47.055634Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T13:18:47.055634Z digest=sha256:79f40f10a18c8b7ecf5d2034a10389d84c75659bbd01d557ab7f568deadf79ae

Observation 49167216-7fff-4a2f-aa8f-54b56a1be6fc · outbound

This paper cites an unresolved cited work.

Constraining the Hubble parameter with the 21 cm brightness temperature signal in a universe with inhomogeneities Unresolved cited work

Reference 48

Resolution
unresolved
no resolver link, observed 2026-08-07T13:18:47.143665Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T13:18:47.143665Z digest=sha256:bc1e85bda5807292c3bc758761a54e187936108bbf17918947608f5237bdd20f

Observation 3e00f0e6-2d98-45a3-b84d-285e7a21af29 · outbound

This paper cites Gasperini, G.

Constraining the Hubble parameter with the 21 cm brightness temperature signal in a universe with inhomogeneities Gasperini, G

Reference 49

Resolution
unresolved
no resolver link, observed 2026-08-07T13:18:47.215643Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T13:18:47.215643Z digest=sha256:a71b65536f956aa5258d2559c62077adc3579f08b88adddae0b31eece7c6ef5d

Observation 408cbf5e-7ec8-446c-9a4f-697edcc430a4 · outbound

This paper cites Buchert, General Relativity and Gravitation 32, 105 (2000).

Constraining the Hubble parameter with the 21 cm brightness temperature signal in a universe with inhomogeneities Buchert, General Relativity and Gravitation 32, 105 (2000)

Reference 50

Resolution
unresolved
no resolver link, observed 2026-08-07T13:18:47.288091Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T13:18:47.288091Z digest=sha256:bfa11886a670ba0b1e55277a3ee1820058b610a46f58355e2d6e0639085c85af

Observation a8459aba-225f-4e5d-b6e2-f87ec98c0746 · outbound

This paper cites Buchert, General Relativity and Gravitation 33, 1381 (2001).

Constraining the Hubble parameter with the 21 cm brightness temperature signal in a universe with inhomogeneities Buchert, General Relativity and Gravitation 33, 1381 (2001)

Reference 51

Resolution
unresolved
no resolver link, observed 2026-08-07T13:18:47.416917Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T13:18:47.416917Z digest=sha256:339f9d07272ce09dd8af2b9fed820181f551f8cc8c004f081e1f63683cd71947

Observation b6fe0c0b-f7b3-4df6-b557-1be5483b1449 · outbound

This paper cites R¨ as¨ anen, Journal of Cosmology and Astroparticle Physics 2009 (02), 011.

Constraining the Hubble parameter with the 21 cm brightness temperature signal in a universe with inhomogeneities R¨ as¨ anen, Journal of Cosmology and Astroparticle Physics 2009 (02), 011

Reference 52

Resolution
unresolved
no resolver link, observed 2026-08-07T13:18:47.517413Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T13:18:47.517413Z digest=sha256:8fe0373795a6bf691df2894b8f985e2e5a0fc3517c100f318438269650fa3a30

Observation 3afb21c0-7d51-4204-86c7-26cf1f8c4475 · outbound

This paper cites R¨ as¨ anen, Journal of Cosmology and Astroparticle Physics 2010 (03), 018.

Constraining the Hubble parameter with the 21 cm brightness temperature signal in a universe with inhomogeneities R¨ as¨ anen, Journal of Cosmology and Astroparticle Physics 2010 (03), 018

Reference 53

Resolution
unresolved
no resolver link, observed 2026-08-07T13:18:47.669355Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T13:18:47.669355Z digest=sha256:d748534ec6989b3f60d50445e9a33cdf4fc68c079928b4fcbfe3ba7119681460

Observation 7632a7d7-e92f-4426-8814-4c70cb4c2a4a · outbound

This paper cites Koksbang, Journal of Cosmology and Astroparticle Physics 2019 (10), 036.

Constraining the Hubble parameter with the 21 cm brightness temperature signal in a universe with inhomogeneities Koksbang, Journal of Cosmology and Astroparticle Physics 2019 (10), 036

Reference 54

Resolution
unresolved
no resolver link, observed 2026-08-07T13:18:47.878893Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T13:18:47.878893Z digest=sha256:cc549ae3773d4b8fa41b4146e2e7ec97734813c9603cb121cc5b37721c95d112

Observation dee706e0-5111-4a3b-af5b-1bcac4bd62e8 · outbound

This paper cites an unresolved cited work.

Constraining the Hubble parameter with the 21 cm brightness temperature signal in a universe with inhomogeneities Unresolved cited work

Reference 55

Resolution
unresolved
no resolver link, observed 2026-08-07T13:18:48.004946Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T13:18:48.004946Z digest=sha256:10ab559079b83328597a97cdfbf13c286da8ba37c4abf255d68caa519fbda0e1

Observation 4db39e7b-6172-49be-9b7b-a9324b611442 · outbound

This paper cites an unresolved cited work.

Constraining the Hubble parameter with the 21 cm brightness temperature signal in a universe with inhomogeneities Unresolved cited work

Reference 56

Resolution
unresolved
raw_fallback, observed 2026-08-07T13:19:11.093825Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

source=pdf_text observed=2026-08-07T13:18:48.083559Z digest=sha256:a2a34a00c221f0f3e1fe47bce986a371cc7a572079f76d4352441edceab6d6c5

Observation 3e51b3c1-f7cf-4425-933e-ed2cd4bfda80 · outbound

This paper cites Koksbang, Journal of Cosmology and Astroparticle Physics 2020 (11), 061.

Constraining the Hubble parameter with the 21 cm brightness temperature signal in a universe with inhomogeneities Koksbang, Journal of Cosmology and Astroparticle Physics 2020 (11), 061

Reference 57

Resolution
verified fuzzy
raw_fallback, observed 2026-08-07T13:19:10.931330Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

source=pdf_text observed=2026-08-07T13:18:48.189854Z digest=sha256:9b86fd18ffd6e2a05d5df70d12ed8ce5d66120586adc23af0f4211aac6b2ce02

Observation b2711ab8-8782-47ff-be27-d5aba208d04c · outbound

This paper cites an unresolved cited work.

Constraining the Hubble parameter with the 21 cm brightness temperature signal in a universe with inhomogeneities Unresolved cited work

Reference 58

Resolution
unresolved
raw_fallback, observed 2026-08-07T13:19:10.776355Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

source=pdf_text observed=2026-08-07T13:18:48.257940Z digest=sha256:74bd2763aca3f51b8e81b9c7466b71b471d801d647a333dce677902b4f382e50

Observation 70f65791-7946-4e52-b1b7-10b7fcc13cc0 · outbound

This paper cites Korzy´ nski, Classical and Quantum Gravity 27, 105015 (2010).

Constraining the Hubble parameter with the 21 cm brightness temperature signal in a universe with inhomogeneities Korzy´ nski, Classical and Quantum Gravity 27, 105015 (2010)

Reference 59

Resolution
verified fuzzy
raw_fallback, observed 2026-08-07T13:19:10.571295Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

source=pdf_text observed=2026-08-07T13:18:48.368570Z digest=sha256:73c98f70d4d1b1ca72145e8f08edf831cda0570100d2109395b119f5639b0f36

Observation 336eedef-7ff4-4e57-b41c-8d26cdc87789 · outbound

This paper cites Clifton, K.

Constraining the Hubble parameter with the 21 cm brightness temperature signal in a universe with inhomogeneities Clifton, K

Reference 60

Resolution
verified fuzzy
raw_fallback, observed 2026-08-07T13:19:10.325690Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

source=pdf_text observed=2026-08-07T13:18:48.441009Z digest=sha256:c763317b4b51f4bc4413870f6705b6b1f019c20cd2933f86c8b25804b8d35b68

Observation e9630b1d-2e3f-41da-b6b6-eb6c79449bce · outbound

This paper cites Skarke, Phys.

Constraining the Hubble parameter with the 21 cm brightness temperature signal in a universe with inhomogeneities Skarke, Phys

Reference 61

Resolution
verified fuzzy
raw_fallback, observed 2026-08-07T13:19:10.128672Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

source=pdf_text observed=2026-08-07T13:18:48.530590Z digest=sha256:05a8f1005b5a3827173c6774516cde287b92286bd90bf78c74c4990c1524adc4

Observation ccbc318d-0b11-41e6-86e9-dbf850f41572 · outbound

This paper cites Buchert, M.

Constraining the Hubble parameter with the 21 cm brightness temperature signal in a universe with inhomogeneities Buchert, M

Reference 62

Resolution
verified fuzzy
raw_fallback, observed 2026-08-07T13:19:09.951967Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

source=pdf_text observed=2026-08-07T13:18:48.604594Z digest=sha256:e67f23cbecbe169be3fa9887ee13678a6610f8c42524d3b3fb4160947a3742cf

Observation 9f0091a5-419a-4204-aa5c-50e4bd0e3b40 · outbound

This paper cites Buchert, A.

Constraining the Hubble parameter with the 21 cm brightness temperature signal in a universe with inhomogeneities Buchert, A

Reference 63

Resolution
verified fuzzy
raw_fallback, observed 2026-08-07T13:19:09.740534Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

source=pdf_text observed=2026-08-07T13:18:48.769937Z digest=sha256:d47d9fe757a7b11b3798e454b32ab927be5e6fa6fe29349ec25b97f2deb0011a

Observation 53c1d9fb-1643-480d-a2e9-eae2b30c8bb7 · outbound

This paper cites Wiegand and T.

Constraining the Hubble parameter with the 21 cm brightness temperature signal in a universe with inhomogeneities Wiegand and T

Reference 64

Resolution
verified fuzzy
raw_fallback, observed 2026-08-07T13:19:09.542257Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

source=pdf_text observed=2026-08-07T13:18:48.968839Z digest=sha256:7ed90e6296da97ca20207bd1c9112d85cc82fb062d13ab231b99dacac0c6b888

Observation 247b6d1c-6cad-476d-8a75-31e30ee2693e · outbound

This paper cites R¨ as¨ anen, Journal of Cosmology and Astroparticle Physics 2004 (02), 003.

Constraining the Hubble parameter with the 21 cm brightness temperature signal in a universe with inhomogeneities R¨ as¨ anen, Journal of Cosmology and Astroparticle Physics 2004 (02), 003

Reference 65

Resolution
verified fuzzy
raw_fallback, observed 2026-08-07T13:19:09.324011Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

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Observation 982971b4-4269-46db-a0eb-1946a86575de · outbound

This paper cites an unresolved cited work.

Constraining the Hubble parameter with the 21 cm brightness temperature signal in a universe with inhomogeneities Unresolved cited work

Reference 66

Resolution
unresolved
raw_fallback, observed 2026-08-07T13:19:09.121382Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

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Observation 564a7ddf-b0ba-41b0-b85f-ea9d2f215609 · outbound

This paper cites an unresolved cited work.

Constraining the Hubble parameter with the 21 cm brightness temperature signal in a universe with inhomogeneities Unresolved cited work

Reference 67

Resolution
unresolved
raw_fallback, observed 2026-08-07T13:19:08.886944Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

source=pdf_text observed=2026-08-07T13:18:49.328677Z digest=sha256:4092a5bc9469a2478dd05fd8c0c20d5d1a1acf03eef9433813765ea318bdae09

Observation 88ed8f02-61f4-4102-a50d-fee4811e4a76 · outbound

This paper cites an unresolved cited work.

Constraining the Hubble parameter with the 21 cm brightness temperature signal in a universe with inhomogeneities Unresolved cited work

Reference 68

Resolution
unresolved
raw_fallback, observed 2026-08-07T13:19:08.645246Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

source=pdf_text observed=2026-08-07T13:18:49.443656Z digest=sha256:49e043afc27d3d135cb80efd1c3af5d5a81262e6e45fd8e8ca432d242a258909

Observation e4fb5258-b08e-4d2e-bfb3-cc6ec914f3b2 · outbound

This paper cites R¨ as¨ anen, Journal of Cosmology and Astroparticle Physics 2008 (04), 026.

Constraining the Hubble parameter with the 21 cm brightness temperature signal in a universe with inhomogeneities R¨ as¨ anen, Journal of Cosmology and Astroparticle Physics 2008 (04), 026

Reference 69

Resolution
verified fuzzy
raw_fallback, observed 2026-08-07T13:19:08.421439Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

source=pdf_text observed=2026-08-07T13:18:49.549180Z digest=sha256:2fc72a23650ab774ca5f5497272bad68f459a88e6dbce8bc930453ffdf7e22f2

Observation a42048d6-6b5f-4f53-a70e-441a4ae6cd28 · outbound

This paper cites Bose and A.

Constraining the Hubble parameter with the 21 cm brightness temperature signal in a universe with inhomogeneities Bose and A

Reference 70

Resolution
verified fuzzy
raw_fallback, observed 2026-08-07T13:19:08.174348Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

source=pdf_text observed=2026-08-07T13:18:49.612175Z digest=sha256:9df4b059c337fd6573651d6e5bcc3b152db679d4c7259fb32079341cfb4dc947

Observation e0fa6ebd-761e-4a1a-873f-bf4d3a08e2cb · outbound

This paper cites Bose and A.

Constraining the Hubble parameter with the 21 cm brightness temperature signal in a universe with inhomogeneities Bose and A

Reference 71

Resolution
verified fuzzy
raw_fallback, observed 2026-08-07T13:19:07.936912Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

source=pdf_text observed=2026-08-07T13:18:49.685882Z digest=sha256:60bcf5fbd7b6312e0ad74d5a4038f86ddb8ec214564cf5cec613218bed0d8a04

Observation dddef3ea-a37d-46db-afe4-55d1a1a7da89 · outbound

This paper cites Ali and A.

Constraining the Hubble parameter with the 21 cm brightness temperature signal in a universe with inhomogeneities Ali and A

Reference 72

Resolution
verified fuzzy
raw_fallback, observed 2026-08-07T13:19:07.794376Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

source=pdf_text observed=2026-08-07T13:18:49.749469Z digest=sha256:3ad395279365e0b4b9192648b1a33229a19b4afb32d55f169ba410779daeae06

Observation 81601a52-15f9-4862-9c28-07eb055a9513 · outbound

This paper cites an unresolved cited work.

Constraining the Hubble parameter with the 21 cm brightness temperature signal in a universe with inhomogeneities Unresolved cited work

Reference 73

Resolution
unresolved
raw_fallback, observed 2026-08-07T13:19:07.595801Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

source=pdf_text observed=2026-08-07T13:18:49.815021Z digest=sha256:26acbac54af5d253ce970735d560d04729e8c899aa585b7dcc2ed453f2a44e4c

Observation aaaa96a3-0596-481a-9e20-63bf424c714a · outbound

This paper cites an unresolved cited work.

Constraining the Hubble parameter with the 21 cm brightness temperature signal in a universe with inhomogeneities Unresolved cited work

Reference 74

Resolution
unresolved
raw_fallback, observed 2026-08-07T13:19:07.384824Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

source=pdf_text observed=2026-08-07T13:18:49.922180Z digest=sha256:46d250528d40be7aa8557752a8453aca7cabd567eb9f3408f5b33d384be7c966

Observation 6dcd1431-9bbe-4122-854c-f19aa192e15b · outbound

This paper cites Koksbang and S.

Constraining the Hubble parameter with the 21 cm brightness temperature signal in a universe with inhomogeneities Koksbang and S

Reference 75

Resolution
verified fuzzy
raw_fallback, observed 2026-08-07T13:19:07.126096Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

source=pdf_text observed=2026-08-07T13:18:50.000360Z digest=sha256:ad7316856e5dbcb56092b1541fb3765639d1f347c5f2ddd41fbb9f7d7ec34049

Observation b744ad51-38cb-43be-8705-5575de92cd4c · outbound

This paper cites an unresolved cited work.

Constraining the Hubble parameter with the 21 cm brightness temperature signal in a universe with inhomogeneities Unresolved cited work

Reference 76

Resolution
unresolved
raw_fallback, observed 2026-08-07T13:19:06.894888Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

source=pdf_text observed=2026-08-07T13:18:50.024143Z digest=sha256:a0b12f49082fa4f0bd8a5465dfcae298fe6c13f54448d3f0a5710906108eb4b8

Observation 2e90e786-d2dc-492e-ab0f-195ede6c72cb · outbound

This paper cites an unresolved cited work.

Constraining the Hubble parameter with the 21 cm brightness temperature signal in a universe with inhomogeneities Unresolved cited work

Reference 78

Resolution
unresolved
raw_fallback, observed 2026-08-07T13:19:06.407274Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

source=pdf_text observed=2026-08-07T13:18:50.097247Z digest=sha256:d718b974836da4f389045c70e639498e60a58d3784d8bc3fc7da4d851d8401f5

Observation bf39b7e6-c84e-46a5-8676-abd9ba6b9426 · outbound

This paper cites Halder, S.

Constraining the Hubble parameter with the 21 cm brightness temperature signal in a universe with inhomogeneities Halder, S

Reference 79

Resolution
verified fuzzy
raw_fallback, observed 2026-08-07T13:19:06.243943Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

source=pdf_text observed=2026-08-07T13:18:50.147856Z digest=sha256:7ccbb97e5d9da741d916ba1cf796553d2e151843a59dbab10ed10c44bcd98c5d

Observation e9aca9f3-bcf3-4af2-92f9-36a0dffec85d · outbound

This paper cites an unresolved cited work.

Constraining the Hubble parameter with the 21 cm brightness temperature signal in a universe with inhomogeneities Unresolved cited work

Reference 80

Resolution
unresolved
raw_fallback, observed 2026-08-07T13:19:06.610545Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

source=pdf_text observed=2026-08-07T13:18:50.152001Z digest=sha256:7afee13e1128348821df3d5f7104f4a9db7ef0d9ad8f7024bb23dddafc872f4b

Observation 50d2d2c9-9cc8-4248-beb7-efeb9659d7f6 · outbound

This paper cites an unresolved cited work.

Constraining the Hubble parameter with the 21 cm brightness temperature signal in a universe with inhomogeneities Unresolved cited work

Reference 81

Resolution
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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

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Observation 86610fbe-ec92-4749-b365-64157df83649 · outbound

This paper cites an unresolved cited work.

Constraining the Hubble parameter with the 21 cm brightness temperature signal in a universe with inhomogeneities Unresolved cited work

Reference 82

Resolution
unresolved
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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

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Observation ff0d9a75-cb4a-44ca-9f91-437692192a6f · outbound

This paper cites an unresolved cited work.

Constraining the Hubble parameter with the 21 cm brightness temperature signal in a universe with inhomogeneities Unresolved cited work

Reference 83

Resolution
unresolved
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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

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Observation 65e3d108-de15-4e81-81d2-71a9826a2c04 · outbound

This paper cites Meiksin, MNRAS 370, 2025 (2006).

Constraining the Hubble parameter with the 21 cm brightness temperature signal in a universe with inhomogeneities Meiksin, MNRAS 370, 2025 (2006)

Reference 84

Resolution
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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

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Observation f3b6790e-41ea-4cec-b5b1-d359bf688b8a · outbound

This paper cites Meiksin and P.

Constraining the Hubble parameter with the 21 cm brightness temperature signal in a universe with inhomogeneities Meiksin and P

Reference 85

Resolution
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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

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Observation 28bab244-de96-4d51-874d-d9ca30b5adf4 · outbound

This paper cites Chen and J.

Constraining the Hubble parameter with the 21 cm brightness temperature signal in a universe with inhomogeneities Chen and J

Reference 86

Resolution
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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

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Observation c0e1eeec-5faf-4875-be51-0ad460348eca · outbound

This paper cites Chuzhoy and P.

Constraining the Hubble parameter with the 21 cm brightness temperature signal in a universe with inhomogeneities Chuzhoy and P

Reference 87

Resolution
verified fuzzy
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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

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Observation 8aec6fa2-d64f-4915-9e83-fdcef6e1c931 · outbound

This paper cites Ghara and G.

Constraining the Hubble parameter with the 21 cm brightness temperature signal in a universe with inhomogeneities Ghara and G

Reference 88

Resolution
verified fuzzy
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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

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Observation 2b4a3349-0940-453d-93dd-6ce7ae4f03cb · outbound

This paper cites Mittal and G.

Constraining the Hubble parameter with the 21 cm brightness temperature signal in a universe with inhomogeneities Mittal and G

Reference 89

Resolution
verified fuzzy
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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

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Observation ac2d0960-633e-44f0-8087-a9ab8dbd2e19 · outbound

This paper cites Haario, M.

Constraining the Hubble parameter with the 21 cm brightness temperature signal in a universe with inhomogeneities Haario, M

Reference 90

Resolution
verified fuzzy
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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

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Observation 2e5ba488-9a63-4c45-8a53-ddf1dbd97062 · outbound

This paper cites Haario, E.

Constraining the Hubble parameter with the 21 cm brightness temperature signal in a universe with inhomogeneities Haario, E

Reference 91

Resolution
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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

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Observation 53f7fcf7-0526-4fa5-bf64-095f57827dcd · outbound

This paper cites Suzuki et al., The Astrophysical Journal 746, 85 (2012).

Constraining the Hubble parameter with the 21 cm brightness temperature signal in a universe with inhomogeneities Suzuki et al., The Astrophysical Journal 746, 85 (2012)

Reference 92

Resolution
unresolved
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Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation c425e584-7d43-4152-a38a-1a3a98e321b2 · outbound

This paper cites an unresolved cited work.

Constraining the Hubble parameter with the 21 cm brightness temperature signal in a universe with inhomogeneities Unresolved cited work

Reference 93

Resolution
unresolved
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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

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Observation ba24daa5-c098-45f1-9a01-54dcb34b2840 · outbound

This paper cites Halder and S.

Constraining the Hubble parameter with the 21 cm brightness temperature signal in a universe with inhomogeneities Halder and S

Reference 94

Resolution
verified fuzzy
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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

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Observation e0f34a85-7184-40a4-8049-893b47d830b5 · outbound

This paper cites an unresolved cited work.

Constraining the Hubble parameter with the 21 cm brightness temperature signal in a universe with inhomogeneities Unresolved cited work

Reference 95

Resolution
unresolved
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Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation aff88e95-5623-42a5-b79c-37f9721dd3f6 · outbound

This paper cites Ali-Ha ¨ ımoud and C.

Constraining the Hubble parameter with the 21 cm brightness temperature signal in a universe with inhomogeneities Ali-Ha ¨ ımoud and C

Reference 96

Resolution
verified fuzzy
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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

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Observation 6d08e847-e429-41f6-86f3-aefe72a173b6 · outbound

This paper cites Zaldarriaga, S.

Constraining the Hubble parameter with the 21 cm brightness temperature signal in a universe with inhomogeneities Zaldarriaga, S

Reference 97

Resolution
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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

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Observation ee9b69d2-6f6c-4802-a6aa-a6e9d87f3d82 · outbound

This paper cites an unresolved cited work.

Constraining the Hubble parameter with the 21 cm brightness temperature signal in a universe with inhomogeneities Unresolved cited work

Reference 98

Resolution
unresolved
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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

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Observation 7506577a-865f-41c1-8a4f-c681044750f6 · outbound

This paper cites an unresolved cited work.

Constraining the Hubble parameter with the 21 cm brightness temperature signal in a universe with inhomogeneities Unresolved cited work

Reference 99

Resolution
unresolved
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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

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Observation 91e84c18-63a7-4bec-b6d4-f27649394ca1 · outbound

This paper cites Kuhlen, P.

Constraining the Hubble parameter with the 21 cm brightness temperature signal in a universe with inhomogeneities Kuhlen, P

Reference 100

Resolution
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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

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Observation 6de85487-4083-4b9d-b959-15497534622c · outbound

This paper cites an unresolved cited work.

Constraining the Hubble parameter with the 21 cm brightness temperature signal in a universe with inhomogeneities Unresolved cited work

Reference 101

Resolution
unresolved
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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

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Observation fe35464d-68ee-480f-9da0-8a1c9bca32a3 · outbound

This paper cites Ciardi and P.

Constraining the Hubble parameter with the 21 cm brightness temperature signal in a universe with inhomogeneities Ciardi and P

Reference 102

Resolution
verified fuzzy
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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

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Observation 484aa619-0bf1-4d33-9ce4-5eb353335576 · outbound

This paper cites Ali-Ha ¨ ımoud and C.

Constraining the Hubble parameter with the 21 cm brightness temperature signal in a universe with inhomogeneities Ali-Ha ¨ ımoud and C

Reference 103

Resolution
verified fuzzy
raw_fallback, observed 2026-08-07T13:19:02.161881Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

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Observation b790b232-099f-4148-b61d-4e579686f78b · outbound

This paper cites an unresolved cited work.

Constraining the Hubble parameter with the 21 cm brightness temperature signal in a universe with inhomogeneities Unresolved cited work

Reference 104

Resolution
unresolved
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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

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Pith citing papers

Observation 89878c57-51fc-4e6e-8f79-bef65fddf31c · inbound

Constraining the Hubble parameter with the 21 cm brightness temperature signal in a universe with inhomogeneities cites this paper.

Constraining the Hubble parameter with the 21 cm brightness temperature signal in a universe with inhomogeneities Constraining the Hubble parameter with the 21 cm brightness temperature signal in a universe with inhomogeneities

Reference 23

Resolution
unresolved
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Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 86f46052-de60-4277-b4b8-86bf57dcd211 · inbound

Interpretation of the binned SNe Ia Master Sample data via a scalar quintessence component: phantom transition? cites this paper.

Interpretation of the binned SNe Ia Master Sample data via a scalar quintessence component: phantom transition? Constraining the Hubble parameter with the 21 cm brightness temperature signal in a universe with inhomogeneities

Reference 9

Resolution
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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

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Observation 64cf7296-e322-4aad-8835-03b4ccc72975 · inbound

Interpretation of the binned SNe Ia Master Sample data via a scalar quintessence component: phantom transition? cites this paper.

Interpretation of the binned SNe Ia Master Sample data via a scalar quintessence component: phantom transition? Constraining the Hubble parameter with the 21 cm brightness temperature signal in a universe with inhomogeneities

Reference 9

Resolution
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Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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