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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 19 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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measured 103 of 103 standing notices

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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=sha256:64c5da9e2e2a394b497f3914377dfcbaa983851c5e2fee02ecacb2c92c1494d2

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 2026-08-19T06:32:44.657259+00:00.

source=pdf_text observed=2026-08-07T13:18:48.083559Z digest=sha256:b660b5ff4f963dc60925b4db53796c45b3d2be8c07bf74d747781c90265f1bb9

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 2026-08-19T06:32:44.657259+00:00.

source=pdf_text observed=2026-08-07T13:18:48.189854Z digest=sha256:ae87118f32c5b5786fef7a8f934cd620679eed2e2b3f8a22997c08a69e776736

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 2026-08-19T06:32:44.657259+00:00.

source=pdf_text observed=2026-08-07T13:18:48.257940Z digest=sha256:a77fa9e44abd78ce79f8733e245b76dc842df53bef3124d112f58f0c78f9770a

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 2026-08-19T06:32:44.657259+00:00.

source=pdf_text observed=2026-08-07T13:18:48.368570Z digest=sha256:678af980d8342e14a96d68376f383810726d995babc0f3b14279e17c911240af

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 2026-08-19T06:32:44.657259+00:00.

source=pdf_text observed=2026-08-07T13:18:48.441009Z digest=sha256:337956b591722f913595c1a6fd37ef7e577aa3e96da005c2197cba311c263833

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 2026-08-19T06:32:44.657259+00:00.

source=pdf_text observed=2026-08-07T13:18:48.530590Z digest=sha256:e9775cdbbfe7f322861c06dc94541f47571a5b530744a65bffe256ca36f3694a

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 2026-08-19T06:32:44.657259+00:00.

source=pdf_text observed=2026-08-07T13:18:48.604594Z digest=sha256:d6654922874d35d026876fc766c46809f7fab9963c176e7a57ac30bfa2a1381d

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 2026-08-19T06:32:44.657259+00:00.

source=pdf_text observed=2026-08-07T13:18:48.769937Z digest=sha256:227827970ff7dab4e62872b8369133740015da278594355bd4d0b7cb03b53a57

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 2026-08-19T06:32:44.657259+00:00.

source=pdf_text observed=2026-08-07T13:18:48.968839Z digest=sha256:822127f07a537e8ca9aaafec1a97a38c68d959c1e09c66bed9788a4390e9b626

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 2026-08-19T06:32:44.657259+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 2026-08-19T06:32:44.657259+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 2026-08-19T06:32:44.657259+00:00.

source=pdf_text observed=2026-08-07T13:18:49.328677Z digest=sha256:b482f856b6c85b2f955592dd84a679436deb33acdae01649c04e58cf1794ea6d

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 2026-08-19T06:32:44.657259+00:00.

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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 2026-08-19T06:32:44.657259+00:00.

source=pdf_text observed=2026-08-07T13:18:49.549180Z digest=sha256:63c26f5aa0c8e29718897f4984137c3a311ca7761520affd797a9658d555b3a5

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 2026-08-19T06:32:44.657259+00:00.

source=pdf_text observed=2026-08-07T13:18:49.612175Z digest=sha256:1bb2e0497390f22ea00da38d20fb6a511d517dae721b48be768a99d18e7318a8

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 2026-08-19T06:32:44.657259+00:00.

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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 2026-08-19T06:32:44.657259+00:00.

source=pdf_text observed=2026-08-07T13:18:49.749469Z digest=sha256:f48b8b843ec1a611a39d4ca4443685627514fe20ef5a7f25403f052c7666e2be

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 2026-08-19T06:32:44.657259+00:00.

source=pdf_text observed=2026-08-07T13:18:49.815021Z digest=sha256:4edd2b4f83163b2c618eef49a232d4d50e6146427159127f9fdcfc9cd3eb98c5

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 2026-08-19T06:32:44.657259+00:00.

source=pdf_text observed=2026-08-07T13:18:49.922180Z digest=sha256:334230762b55374c8fcf804c237c60fbbb9e2057372dd43360e9b3d4d6f0f48a

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 2026-08-19T06:32:44.657259+00:00.

source=pdf_text observed=2026-08-07T13:18:50.000360Z digest=sha256:5454fc6e721b7cf4a827c6d13e36331975d0b66bee6d03988497f871af53a716

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 2026-08-19T06:32:44.657259+00:00.

source=pdf_text observed=2026-08-07T13:18:50.024143Z digest=sha256:7a1252f3d24cf069bf7cdca2d5bcc3b895a6b89447292bd01fa9ff89a2ece4ec

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 2026-08-19T06:32:44.657259+00:00.

source=pdf_text observed=2026-08-07T13:18:50.097247Z digest=sha256:f52d607fb7a9348ac12d5032d7dce681f938b6e85615f2d256f92526e1e782e7

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 2026-08-19T06:32:44.657259+00:00.

source=pdf_text observed=2026-08-07T13:18:50.147856Z digest=sha256:673065227322c25c7977410f5053b6e34dc95fa04005c9c226b58e0978b405dd

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 2026-08-19T06:32:44.657259+00:00.

source=pdf_text observed=2026-08-07T13:18:50.152001Z digest=sha256:e2cc12d457921c7c5499b55535a2d9bfa25d72d7754bf16b67492df95045328c

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
unresolved
raw_fallback, observed 2026-08-07T13:19:06.099234Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+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
raw_fallback, observed 2026-08-07T13:19:05.960403Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+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
raw_fallback, observed 2026-08-07T13:19:05.826367Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+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
verified fuzzy
raw_fallback, observed 2026-08-07T13:19:05.676930Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+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
verified fuzzy
raw_fallback, observed 2026-08-07T13:19:05.524385Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+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
verified fuzzy
raw_fallback, observed 2026-08-07T13:19:05.337899Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+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
raw_fallback, observed 2026-08-07T13:19:05.130532Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+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
raw_fallback, observed 2026-08-07T13:19:04.904181Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+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
raw_fallback, observed 2026-08-07T13:19:04.687594Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+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
raw_fallback, observed 2026-08-07T13:19:04.471993Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+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
verified fuzzy
raw_fallback, observed 2026-08-07T13:19:04.254567Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+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
no resolver link, observed 2026-08-07T13:18:51.369245Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T13:18:51.369245Z digest=sha256:bd9e18955540df5b5f43cf8488531e8329e332596d9390f16f257abd459d3274

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
raw_fallback, observed 2026-08-07T13:19:04.034881Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+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
raw_fallback, observed 2026-08-07T13:19:03.837149Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+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
no resolver link, observed 2026-08-07T13:18:51.842083Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T13:18:51.842083Z digest=sha256:cef2f67fa240b35a781c316f4c18c16f4ef42001ca1f58fac265a7239aec0882

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
raw_fallback, observed 2026-08-07T13:19:03.683772Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+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
verified fuzzy
raw_fallback, observed 2026-08-07T13:19:03.500214Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

source=pdf_text observed=2026-08-07T13:18:52.173927Z digest=sha256:a8147b21bab4e715a2d31953e57895c193ff8b4fe05d8a6d294eb1a16f6917b4

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
raw_fallback, observed 2026-08-07T13:19:03.285923Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+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
raw_fallback, observed 2026-08-07T13:19:03.049399Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

source=pdf_text observed=2026-08-07T13:18:52.416514Z digest=sha256:f9f9edf4e1dafe92593ac57d3bc0d34ae4507ee65ded4dbad50d505b68e7f13e

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
verified fuzzy
raw_fallback, observed 2026-08-07T13:19:02.800495Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+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
raw_fallback, observed 2026-08-07T13:19:02.585045Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+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
raw_fallback, observed 2026-08-07T13:19:02.439165Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+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 2026-08-19T06:32:44.657259+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
raw_fallback, observed 2026-08-07T13:19:01.995066Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+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
no resolver link, observed 2026-08-07T13:18:42.676548Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T13:18:42.676548Z digest=sha256:9c6cdcc53572c0a90d02d0225345a094cb6ca934e67bcde603f5b8eefab89ad0

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
malformed identifier
arxiv_id, observed 2026-07-02T06:36:43.764570Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+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
malformed identifier
no resolver link, observed 2026-07-12T08:56:43.854989Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-07-12T08:56:43.854989Z digest=sha256:d7926a1b7dd60d552b63039a12e63487fe24ff6b51c4b83c7dbeb9eefe89d94a