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Paper Citation Record · LEDGER

Constraints on the state of the IGM at $z\sim 8-10$ using redshifted 21-cm observations with LOFAR

As of 19 August 2026, this Paper Citation Record lists 100 of 150 outbound references and 5 inbound Pith citation observations for arXiv:2505.00373.

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

pith.paper-citation-record.v1
2505.00373 v1

Coverage vector

measured 100 of 150 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links, observed 2026-08-16T04:51:30.103141Z

measured 105 of 105 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-19T06:32:44.657259+00:00

measured 5 of 5 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-06T17:35:29.464923Z

measured 1 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-08-05T02:28:24.338817Z

Reference resolution

100 of 150 outbound references displayed

  • verified exact1
  • verified fuzzy22
  • unresolved77
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  • malformed identifier0
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External citation measurements

1
arxiv_reference, observed 2026-08-05T02:28:24.338817Z

Outbound references

Observation bdb1cecc-724e-476f-a776-18fef97e8ad2 · outbound

This paper cites , " * write output.state after.block = add.period write newline.

Constraints on the state of the IGM at $z\sim 8-10$ using redshifted 21-cm observations with LOFAR , " * write output.state after.block = add.period write newline

Reference 1

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Observation 0c7b1753-1e82-4c37-abaf-15c848948306 · outbound

This paper cites write newline.

Constraints on the state of the IGM at $z\sim 8-10$ using redshifted 21-cm observations with LOFAR write newline

Reference 2

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Observation a2ca3afe-dfc1-4169-9835-bf6b13f92513 · outbound

This paper cites an unresolved cited work.

Constraints on the state of the IGM at $z\sim 8-10$ using redshifted 21-cm observations with LOFAR Unresolved cited work

Reference 3

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Observation 42885145-e3a1-41aa-8c4c-e6c0915b1463 · outbound

This paper cites E., Alexander , P., et al.

Constraints on the state of the IGM at $z\sim 8-10$ using redshifted 21-cm observations with LOFAR E., Alexander , P., et al

Reference 4

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Observation 52d1e059-327c-4923-8b50-29cbea4c3a26 · outbound

This paper cites K., et al.

Constraints on the state of the IGM at $z\sim 8-10$ using redshifted 21-cm observations with LOFAR K., et al

Reference 5

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Observation a8a0867c-b627-429f-9b2d-b419208e3780 · outbound

This paper cites 2024 b , , 527, 7835.

Constraints on the state of the IGM at $z\sim 8-10$ using redshifted 21-cm observations with LOFAR 2024 b , , 527, 7835

Reference 6

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Observation 22a362e5-017f-4ec5-a455-63a2d58d5dc6 · outbound

This paper cites 2024 c , , 534, L30.

Constraints on the state of the IGM at $z\sim 8-10$ using redshifted 21-cm observations with LOFAR 2024 c , , 534, L30

Reference 7

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Observation beabafd1-19a0-44fb-9170-17e493812fbe · outbound

This paper cites S., Parsons , A.

Constraints on the state of the IGM at $z\sim 8-10$ using redshifted 21-cm observations with LOFAR S., Parsons , A

Reference 8

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Observation 1de3fbd7-9009-4243-8a86-d5e397b2f127 · outbound

This paper cites P., Mazzucchelli , C., et al.

Constraints on the state of the IGM at $z\sim 8-10$ using redshifted 21-cm observations with LOFAR P., Mazzucchelli , C., et al

Reference 9

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Observation 50872943-ea87-4d6f-9823-3e7138bf93cd · outbound

This paper cites 2018, , 555, 71.

Constraints on the state of the IGM at $z\sim 8-10$ using redshifted 21-cm observations with LOFAR 2018, , 555, 71

Reference 10

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Observation f9e7a02b-1225-4713-9a6d-2ec80fa6517a · outbound

This paper cites & Loeb , A.

Constraints on the state of the IGM at $z\sim 8-10$ using redshifted 21-cm observations with LOFAR & Loeb , A

Reference 11

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Observation 6d85bad4-4a6e-4b3e-b1e7-d70f9b94846b · outbound

This paper cites & Loeb , A.

Constraints on the state of the IGM at $z\sim 8-10$ using redshifted 21-cm observations with LOFAR & Loeb , A

Reference 12

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Observation d153d90e-9b84-418a-9913-4f4d26db53bd · outbound

This paper cites F., & Pober , J.

Constraints on the state of the IGM at $z\sim 8-10$ using redshifted 21-cm observations with LOFAR F., & Pober , J

Reference 13

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Observation 6e68b002-70f8-4254-b6e6-f086ca19cab9 · outbound

This paper cites M., et al.

Constraints on the state of the IGM at $z\sim 8-10$ using redshifted 21-cm observations with LOFAR M., et al

Reference 14

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Observation 99d8de7c-e140-4f35-a5cd-4b12d53d2076 · outbound

This paper cites P., Hazelton , B.

Constraints on the state of the IGM at $z\sim 8-10$ using redshifted 21-cm observations with LOFAR P., Hazelton , B

Reference 15

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Observation 51d98a9b-e543-4d85-8203-43c2394e3dea · outbound

This paper cites D., Bolton, J.

Constraints on the state of the IGM at $z\sim 8-10$ using redshifted 21-cm observations with LOFAR D., Bolton, J

Reference 16

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Observation bcba8175-479a-4079-83c2-cf6f2b17292e · outbound

This paper cites D., Davies , F.

Constraints on the state of the IGM at $z\sim 8-10$ using redshifted 21-cm observations with LOFAR D., Davies , F

Reference 17

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Observation 0af24591-710a-42f9-95d3-0dd35ab75c00 · outbound

This paper cites an unresolved cited work.

Constraints on the state of the IGM at $z\sim 8-10$ using redshifted 21-cm observations with LOFAR Unresolved cited work

Reference 18

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Observation b361d206-5cba-42cc-b599-24eb6f86a74b · outbound

This paper cites K., & Samui , S.

Constraints on the state of the IGM at $z\sim 8-10$ using redshifted 21-cm observations with LOFAR K., & Samui , S

Reference 19

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Observation 5f1c82d0-dc1a-4978-a33e-b0b5daf1e119 · outbound

This paper cites an unresolved cited work.

Constraints on the state of the IGM at $z\sim 8-10$ using redshifted 21-cm observations with LOFAR Unresolved cited work

Reference 20

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Observation 5f5b6240-c6b0-4a09-b893-8d686a2a2e45 · outbound

This paper cites & Brown , M.

Constraints on the state of the IGM at $z\sim 8-10$ using redshifted 21-cm observations with LOFAR & Brown , M

Reference 21

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Observation 965ca1f1-30d1-4f48-b548-3b8dd6d09980 · outbound

This paper cites an unresolved cited work.

Constraints on the state of the IGM at $z\sim 8-10$ using redshifted 21-cm observations with LOFAR Unresolved cited work

Reference 22

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Observation 27bc3d43-17de-4af0-bbc9-a0813b534063 · outbound

This paper cites D., Rogers , A.

Constraints on the state of the IGM at $z\sim 8-10$ using redshifted 21-cm observations with LOFAR D., Rogers , A

Reference 23

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Observation 936f8c86-267e-4be5-99c9-5597cd9851ec · outbound

This paper cites F., Tauscher , K., Rapetti , D., & Burns , J.

Constraints on the state of the IGM at $z\sim 8-10$ using redshifted 21-cm observations with LOFAR F., Tauscher , K., Rapetti , D., & Burns , J

Reference 24

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Observation 4ea100de-f0db-4619-8287-e3398f2de938 · outbound

This paper cites 2023, The Astrophysical Journal Letters, 948, L14.

Constraints on the state of the IGM at $z\sim 8-10$ using redshifted 21-cm observations with LOFAR 2023, The Astrophysical Journal Letters, 948, L14

Reference 25

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Observation 77f7d490-27b1-4d4b-b8b1-aac0a7fba784 · outbound

This paper cites Spectral modelling of Cygnus A between 110 and 250 MHz. Impact on the LOFAR 21-cm signal power spectrum.

Constraints on the state of the IGM at $z\sim 8-10$ using redshifted 21-cm observations with LOFAR Spectral modelling of Cygnus A between 110 and 250 MHz. Impact on the LOFAR 21-cm signal power spectrum

Reference 26

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Observation 0b68242e-a7a5-46b4-8135-ab149a5656f9 · outbound

This paper cites B., et al.

Constraints on the state of the IGM at $z\sim 8-10$ using redshifted 21-cm observations with LOFAR B., et al

Reference 27

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Observation a4a34f0b-decc-4a29-8485-3b964b93bf0d · outbound

This paper cites R., & Hutter , A.

Constraints on the state of the IGM at $z\sim 8-10$ using redshifted 21-cm observations with LOFAR R., & Hutter , A

Reference 28

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Observation 2f55db16-6c34-4df3-8e7b-6d83f342009c · outbound

This paper cites R., & Schneider , R.

Constraints on the state of the IGM at $z\sim 8-10$ using redshifted 21-cm observations with LOFAR R., & Schneider , R

Reference 29

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Observation 37f0ebb2-6524-46f9-9df0-0d799966f684 · outbound

This paper cites R., Kolopanis , M., et al.

Constraints on the state of the IGM at $z\sim 8-10$ using redshifted 21-cm observations with LOFAR R., Kolopanis , M., et al

Reference 30

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Observation 6a3dc966-9c76-4cab-bbcf-d1b80164d38d · outbound

This paper cites Inferring IGM parameters from the redshifted 21-cm Power Spectrum using Artificial Neural Networks.

Constraints on the state of the IGM at $z\sim 8-10$ using redshifted 21-cm observations with LOFAR Inferring IGM parameters from the redshifted 21-cm Power Spectrum using Artificial Neural Networks

Reference 31

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Observation 6e65a80d-aad6-4228-ba52-376f4e73ee80 · outbound

This paper cites an unresolved cited work.

Constraints on the state of the IGM at $z\sim 8-10$ using redshifted 21-cm observations with LOFAR Unresolved cited work

Reference 32

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Observation 61a731da-62b2-49e3-9f96-1e1df4bb9ca2 · outbound

This paper cites D., & Carilli , C.

Constraints on the state of the IGM at $z\sim 8-10$ using redshifted 21-cm observations with LOFAR D., & Carilli , C

Reference 33

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Observation b0290acc-619f-4046-8bc0-46209f8a2c25 · outbound

This paper cites K., Bharadwaj , S., & Choudhury , T.

Constraints on the state of the IGM at $z\sim 8-10$ using redshifted 21-cm observations with LOFAR K., Bharadwaj , S., & Choudhury , T

Reference 34

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Observation e0dc6bf1-86aa-4ffd-a24d-fde40e39a05a · outbound

This paper cites an unresolved cited work.

Constraints on the state of the IGM at $z\sim 8-10$ using redshifted 21-cm observations with LOFAR Unresolved cited work

Reference 35

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Observation 07551f03-df06-4afa-844a-60cc7679ba58 · outbound

This paper cites R., Parsons , A.

Constraints on the state of the IGM at $z\sim 8-10$ using redshifted 21-cm observations with LOFAR R., Parsons , A

Reference 36

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Observation f560fba4-f3fd-4b6f-8387-73bf03aa641e · outbound

This paper cites T., McLeod, D.

Constraints on the state of the IGM at $z\sim 8-10$ using redshifted 21-cm observations with LOFAR T., McLeod, D

Reference 37

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source=arxiv_source observed=2026-08-16T04:51:29.879212Z digest=sha256:a0229ffe31954bf8ddabd3e888bba3806f90f27f9365a4451c9007b133b9527d

Observation 0fe921dd-5629-4237-a3d9-5b915ff81f74 · outbound

This paper cites & Taylor , G.

Constraints on the state of the IGM at $z\sim 8-10$ using redshifted 21-cm observations with LOFAR & Taylor , G

Reference 38

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source=arxiv_source observed=2026-08-16T04:51:29.882655Z digest=sha256:054be58aaec24b250cfa2e267088a023367cba8946e822ddc93dad7b841f75df

Observation 8d5b69f5-344c-4b71-9115-4702b2950147 · outbound

This paper cites an unresolved cited work.

Constraints on the state of the IGM at $z\sim 8-10$ using redshifted 21-cm observations with LOFAR Unresolved cited work

Reference 39

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source=arxiv_source observed=2026-08-16T04:51:29.886235Z digest=sha256:5c3237a6d12d0f24502135596087fb8788a8c235b8d83bb6d20371cbab81ba50

Observation a5d52f92-086b-4346-a420-53736539bb3c · outbound

This paper cites W., Anderson , M.

Constraints on the state of the IGM at $z\sim 8-10$ using redshifted 21-cm observations with LOFAR W., Anderson , M

Reference 40

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source=arxiv_source observed=2026-08-16T04:51:29.889612Z digest=sha256:e5289d279159819b51aab38bed27d86fc55973fd5af3c0183d6500ab2d4591ac

Observation 501ca49d-2faa-452b-90e7-796849b940b3 · outbound

This paper cites W., de Gasperin , F., & Rafferty , D.

Constraints on the state of the IGM at $z\sim 8-10$ using redshifted 21-cm observations with LOFAR W., de Gasperin , F., & Rafferty , D

Reference 41

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source=arxiv_source observed=2026-08-16T04:51:29.892795Z digest=sha256:9159c853c8819714f2e365b1a094db93f0c731c7d040ae273d8c2058c01517dd

Observation efc6e395-0b01-4b7a-a1e3-3eadcfaf0eb8 · outbound

This paper cites B., Ciardi , B., Graziani , L., et al.

Constraints on the state of the IGM at $z\sim 8-10$ using redshifted 21-cm observations with LOFAR B., Ciardi , B., Graziani , L., et al

Reference 42

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source=arxiv_source observed=2026-08-16T04:51:29.897421Z digest=sha256:48351daf45cfae59b261a3e795893aec759d29f972ae7ba192c6b1c342ca9d63

Observation 8f0b9b66-0c6a-47e7-92dc-9343056613ff · outbound

This paper cites B., & Hennawi , J.

Constraints on the state of the IGM at $z\sim 8-10$ using redshifted 21-cm observations with LOFAR B., & Hennawi , J

Reference 43

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source=arxiv_source observed=2026-08-16T04:51:29.900977Z digest=sha256:cfe4ed3e6d10674e49a090d4cc8c8e1bb737f5feab5620518f17e7fc24aa613e

Observation c8ea2ac5-4a43-4474-9ede-99690ca64bb0 · outbound

This paper cites S., Liu, A., & Hewitt, J.

Constraints on the state of the IGM at $z\sim 8-10$ using redshifted 21-cm observations with LOFAR S., Liu, A., & Hewitt, J

Reference 44

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source=arxiv_source observed=2026-08-16T04:51:29.904410Z digest=sha256:42e54944f8022b74ceb26613a4d1178ba49f7f52febf5ebd417dcc77be45b75e

Observation b9bda66e-9ef8-4084-8635-f8f6ecef7b92 · outbound

This paper cites 2016, , 458, 2710.

Constraints on the state of the IGM at $z\sim 8-10$ using redshifted 21-cm observations with LOFAR 2016, , 458, 2710

Reference 45

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no resolver link, observed 2026-08-16T04:51:29.908018Z

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source=arxiv_source observed=2026-08-16T04:51:29.908018Z digest=sha256:86aca57c6a4cbbbfd82f9d903f371ecc1a9fcc9418f888d51b9093c45ea8694d

Observation ed121d84-d84e-433b-b7b0-90fbbe8ee50c · outbound

This paper cites A., Becker , R.

Constraints on the state of the IGM at $z\sim 8-10$ using redshifted 21-cm observations with LOFAR A., Becker , R

Reference 46

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source=arxiv_source observed=2026-08-16T04:51:29.911565Z digest=sha256:7b092808d7ffa5d308f0c2a71bea394ec6e0247fcdbd05a19644ef78c7f04a7b

Observation 4b57ab5f-cfa1-424f-9b95-0f7426b253e1 · outbound

This paper cites & Barkana , R.

Constraints on the state of the IGM at $z\sim 8-10$ using redshifted 21-cm observations with LOFAR & Barkana , R

Reference 47

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no resolver link, observed 2026-08-16T04:51:29.915076Z

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source=arxiv_source observed=2026-08-16T04:51:29.915076Z digest=sha256:65edf2158a345c79795fcb7974831171fd4e90b72bc4bee7ae55cbe0721e03e1

Observation 44b8e4ad-4f25-47c7-8c1b-9466e742191a · outbound

This paper cites 2018, Physical Review Letters, 121, 011101.

Constraints on the state of the IGM at $z\sim 8-10$ using redshifted 21-cm observations with LOFAR 2018, Physical Review Letters, 121, 011101

Reference 48

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source=arxiv_source observed=2026-08-16T04:51:29.918600Z digest=sha256:3a01c91e3a674b9809682729a67df657f6a0dab25de36db59d8d74fead42f720

Observation 4534de08-dc21-4d5b-931a-8d010166de5e · outbound

This paper cites J., Kogut , A., Levin , S., et al.

Constraints on the state of the IGM at $z\sim 8-10$ using redshifted 21-cm observations with LOFAR J., Kogut , A., Levin , S., et al

Reference 49

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no resolver link, observed 2026-08-16T04:51:29.922010Z

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source=arxiv_source observed=2026-08-16T04:51:29.922010Z digest=sha256:77a78634890f1c7d2fe66dcff9f128c7013249f2d9379e43e73c94cf0ac83f6c

Observation 2668b16e-4c0d-4cc9-8f2c-ac4715539463 · outbound

This paper cites R., Oh , S.

Constraints on the state of the IGM at $z\sim 8-10$ using redshifted 21-cm observations with LOFAR R., Oh , S

Reference 50

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no resolver link, observed 2026-08-16T04:51:29.925648Z

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source=arxiv_source observed=2026-08-16T04:51:29.925648Z digest=sha256:f630bf2790d2dddfbd06cb45ee0491b17f388ab7e4a98906d4029df5b6717388

Observation a6f52ee9-8437-42c6-a59f-206ab6ee3d13 · outbound

This paper cites an unresolved cited work.

Constraints on the state of the IGM at $z\sim 8-10$ using redshifted 21-cm observations with LOFAR Unresolved cited work

Reference 51

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no resolver link, observed 2026-08-16T04:51:29.928757Z

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source=arxiv_source observed=2026-08-16T04:51:29.928757Z digest=sha256:7dec2bfdb223261ea53d38706e44db0e7ba95fc95835288ac46324c99a026861

Observation 154e09b6-e651-4725-91db-63a09003fd83 · outbound

This paper cites G., Koopmans , L.

Constraints on the state of the IGM at $z\sim 8-10$ using redshifted 21-cm observations with LOFAR G., Koopmans , L

Reference 52

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no resolver link, observed 2026-08-16T04:51:29.932753Z

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source=arxiv_source observed=2026-08-16T04:51:29.932753Z digest=sha256:4f67de53214ff60a806bc0b7f9143cbfe2595198a76e0510dfc016468ddf1b16

Observation 6cf7a18b-7c99-4d84-b73a-bb94e867ec27 · outbound

This paper cites Extracting the Epoch of Reionization Signal with 3D U-Net Neural Networks Using Data-driven Systematic Effect Model.

Constraints on the state of the IGM at $z\sim 8-10$ using redshifted 21-cm observations with LOFAR Extracting the Epoch of Reionization Signal with 3D U-Net Neural Networks Using Data-driven Systematic Effect Model

Reference 53

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verified exact
local_arxiv, observed 2026-08-16T04:51:30.353749Z

Source-reported events for the cited work

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source=arxiv_source observed=2026-08-16T04:51:29.935978Z digest=sha256:3c112488f5d8a0a21014355febcd509f04c57e2281e2f86425400adc1b334827

Observation fc478f14-ab18-4527-b972-3aa86bd8d573 · outbound

This paper cites K., Mertens , F.

Constraints on the state of the IGM at $z\sim 8-10$ using redshifted 21-cm observations with LOFAR K., Mertens , F

Reference 54

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source=arxiv_source observed=2026-08-16T04:51:29.939460Z digest=sha256:c5f64c2d9c620f010a50ae1d1409a7f72770aee9e4e4519706b1665b14c0d8c1

Observation f794d274-ac07-418a-b401-c1a37b8101dd · outbound

This paper cites R., & Datta , K.

Constraints on the state of the IGM at $z\sim 8-10$ using redshifted 21-cm observations with LOFAR R., & Datta , K

Reference 55

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no resolver link, observed 2026-08-16T04:51:29.942501Z

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source=arxiv_source observed=2026-08-16T04:51:29.942501Z digest=sha256:61026b95a9ebd68c44f63ae666962de19844773fc0e36415a640a8dd2dce13cf

Observation 914e9487-d6bb-435c-b90c-be7f2250644f · outbound

This paper cites R., & Datta , K.

Constraints on the state of the IGM at $z\sim 8-10$ using redshifted 21-cm observations with LOFAR R., & Datta , K

Reference 56

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no resolver link, observed 2026-08-16T04:51:29.945800Z

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source=arxiv_source observed=2026-08-16T04:51:29.945800Z digest=sha256:833004962fa7c80c0fb500320832da4dc06e2e863aa16134a0f87615949c2352

Observation b97132ea-2368-4ef6-9642-5393a42e88dd · outbound

This paper cites R., Datta , K.

Constraints on the state of the IGM at $z\sim 8-10$ using redshifted 21-cm observations with LOFAR R., Datta , K

Reference 57

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no resolver link, observed 2026-08-16T04:51:29.949282Z

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source=arxiv_source observed=2026-08-16T04:51:29.949282Z digest=sha256:5c98878c7c8a58a4e21cff17e0984fc41ee30f85297793a310217407fc2696f5

Observation 299cdbc8-bb93-4933-a340-7d59f0ed1cc2 · outbound

This paper cites K., & Choudhury , T.

Constraints on the state of the IGM at $z\sim 8-10$ using redshifted 21-cm observations with LOFAR K., & Choudhury , T

Reference 58

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no resolver link, observed 2026-08-16T04:51:29.952264Z

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source=arxiv_source observed=2026-08-16T04:51:29.952264Z digest=sha256:a09485038c924dc5028a25a4179e739fe927831c0267cfaf17845d87fdb79772

Observation f90dde2f-7111-497a-aee8-98f77c8099dc · outbound

This paper cites K., Ciardi , B., Mellema , G., & Zaroubi , S.

Constraints on the state of the IGM at $z\sim 8-10$ using redshifted 21-cm observations with LOFAR K., Ciardi , B., Mellema , G., & Zaroubi , S

Reference 59

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source=arxiv_source observed=2026-08-16T04:51:29.955076Z digest=sha256:b1a8296a9cd07fab81a309bd72416c48d20df88d56703ff41538098d4c80f483

Observation e4dab977-6bcd-4413-b178-94110affcccf · outbound

This paper cites K., Mellema , G., et al.

Constraints on the state of the IGM at $z\sim 8-10$ using redshifted 21-cm observations with LOFAR K., Mellema , G., et al

Reference 60

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source=arxiv_source observed=2026-08-16T04:51:29.957877Z digest=sha256:782ce3f50956055fda247b46a960521e89f970eb7d29ec0bc0ce5dc7b61ee1d7

Observation 3a8832ac-5066-4a2b-9430-5fa1fb96305e · outbound

This paper cites & Mellema , G.

Constraints on the state of the IGM at $z\sim 8-10$ using redshifted 21-cm observations with LOFAR & Mellema , G

Reference 61

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source=arxiv_source observed=2026-08-16T04:51:29.960517Z digest=sha256:4c3ca26da34360676edfa1112120f78fda161beb516ea0762fc6496724230ddc

Observation 293af0c1-9b64-4c4b-8f81-180293fc7677 · outbound

This paper cites K., et al.

Constraints on the state of the IGM at $z\sim 8-10$ using redshifted 21-cm observations with LOFAR K., et al

Reference 62

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source=arxiv_source observed=2026-08-16T04:51:29.963443Z digest=sha256:48675d029a9155b9997fd679bea6814f61c8a9e4ce9c0a1482ba657c435f5b13

Observation f5bb0422-5ab0-495e-8a1d-01f19aebd7d7 · outbound

This paper cites 2022, , 2022, 055.

Constraints on the state of the IGM at $z\sim 8-10$ using redshifted 21-cm observations with LOFAR 2022, , 2022, 055

Reference 63

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no resolver link, observed 2026-08-16T04:51:29.966342Z

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source=arxiv_source observed=2026-08-16T04:51:29.966342Z digest=sha256:ce85d529ceb1a6b59b0744c40014daab8e26e7a1df37c8442918ae33c88c65b6

Observation 65bd6728-1df8-49ff-9ff1-a8a48aaf0826 · outbound

This paper cites K., Zaroubi , S., et al.

Constraints on the state of the IGM at $z\sim 8-10$ using redshifted 21-cm observations with LOFAR K., Zaroubi , S., et al

Reference 64

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no resolver link, observed 2026-08-16T04:51:29.969958Z

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source=arxiv_source observed=2026-08-16T04:51:29.969958Z digest=sha256:076f8b17e059aa012c5cb913ca68933ae4f1acb7400c0e7056c174089882f016

Observation 91e3554f-8f8c-482f-86bc-bfc728e99359 · outbound

This paper cites S., & Chengalur , J.

Constraints on the state of the IGM at $z\sim 8-10$ using redshifted 21-cm observations with LOFAR S., & Chengalur , J

Reference 65

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no resolver link, observed 2026-08-16T04:51:29.973124Z

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source=arxiv_source observed=2026-08-16T04:51:29.973124Z digest=sha256:bd439612836d8ccbb4674dceba880ede50b464ec8d7e975e0c1ac34a2c13d401

Observation 2d2aa3a8-5dd7-4958-aaa4-8f7cf96be717 · outbound

This paper cites K., D'Aloisio , A., Mellema , G., et al.

Constraints on the state of the IGM at $z\sim 8-10$ using redshifted 21-cm observations with LOFAR K., D'Aloisio , A., Mellema , G., et al

Reference 66

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source=arxiv_source observed=2026-08-16T04:51:29.976541Z digest=sha256:8456f04675493340f1e1d7b422abae977f9fa37c40aa10d96567128d80bceac3

Observation dad3d879-fbae-498d-98b8-dae9bf26f5e5 · outbound

This paper cites K., Mellema , G., Aldheimer , T., Dixon , K.

Constraints on the state of the IGM at $z\sim 8-10$ using redshifted 21-cm observations with LOFAR K., Mellema , G., Aldheimer , T., Dixon , K

Reference 67

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source=arxiv_source observed=2026-08-16T04:51:29.980348Z digest=sha256:b1401de0aca30ffc0cb781b54049a1adc953992955a1e047b12617a55d3cc4af

Observation 8bf2d273-b6a0-456a-ad6e-27bc960df0a9 · outbound

This paper cites an unresolved cited work.

Constraints on the state of the IGM at $z\sim 8-10$ using redshifted 21-cm observations with LOFAR Unresolved cited work

Reference 68

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source=arxiv_source observed=2026-08-16T04:51:29.983770Z digest=sha256:2c64d638092697771995aa35f4bd0644df14be3fb52f98a19d3400c9bea7ca3c

Observation fcb011c1-3460-49fd-bd06-719f0cb080bf · outbound

This paper cites 2009, , 397, 1138.

Constraints on the state of the IGM at $z\sim 8-10$ using redshifted 21-cm observations with LOFAR 2009, , 397, 1138

Reference 69

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source=arxiv_source observed=2026-08-16T04:51:29.987167Z digest=sha256:19b6aa7e25920c97d71481d24caec5db72521c240d4dc503f90ad07ff3a2a616

Observation e46762ad-cad3-4fc5-ad74-8fe60de1e6ea · outbound

This paper cites T., et al.

Constraints on the state of the IGM at $z\sim 8-10$ using redshifted 21-cm observations with LOFAR T., et al

Reference 70

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source=arxiv_source observed=2026-08-16T04:51:29.990418Z digest=sha256:18c004fae5ec180fd955e602cf5cb5ca02599d4c54d6aa2d948d271c3d991f94

Observation a85caeb3-87a6-4886-ade4-59cb9bd2d140 · outbound

This paper cites D., & Puchwein , E.

Constraints on the state of the IGM at $z\sim 8-10$ using redshifted 21-cm observations with LOFAR D., & Puchwein , E

Reference 71

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source=arxiv_source observed=2026-08-16T04:51:29.993897Z digest=sha256:eb2ac677858f8da357d91e2e6b46da0583a12b415a767c616794f4c4f883cdac

Observation 3645adda-e78c-4e8c-8845-eb62f60b4346 · outbound

This paper cites 2013, , 208, 19.

Constraints on the state of the IGM at $z\sim 8-10$ using redshifted 21-cm observations with LOFAR 2013, , 208, 19

Reference 72

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source=arxiv_source observed=2026-08-16T04:51:29.997673Z digest=sha256:2b414dddf84b9ee0e2f85b5ce41f55cf6acb298859e9ce8de8c4d21a49f5d471

Observation b2103c77-4bb1-4ee4-ba09-f7a40a8b1792 · outbound

This paper cites R., et al.

Constraints on the state of the IGM at $z\sim 8-10$ using redshifted 21-cm observations with LOFAR R., et al

Reference 73

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no resolver link, observed 2026-08-16T04:51:30.001176Z

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source=arxiv_source observed=2026-08-16T04:51:30.001176Z digest=sha256:8162acc7226a2a913b59d10a28a4e2d5346e3d79b4f53a195cbe35c0b7c0fbff

Observation 7674d185-bec0-4a93-914d-24719fc37c39 · outbound

This paper cites M., Cowie , L.

Constraints on the state of the IGM at $z\sim 8-10$ using redshifted 21-cm observations with LOFAR M., Cowie , L

Reference 74

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source=arxiv_source observed=2026-08-16T04:51:30.005674Z digest=sha256:f085e2e4460a90a9a339c26a80c75fe5b311c143f27735ec5ae602dbf97bf98f

Observation 0991cba1-e6a2-40b1-b37f-a64d638c68e8 · outbound

This paper cites R., & Nath , B.

Constraints on the state of the IGM at $z\sim 8-10$ using redshifted 21-cm observations with LOFAR R., & Nath , B

Reference 75

Resolution
verified fuzzy
raw_fallback, observed 2026-08-16T04:51:31.174803Z

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=arxiv_source observed=2026-08-16T04:51:30.010363Z digest=sha256:f84919761d2b0903093d6318370da8d0f23a5c8364e6577d71ec4f45eee42e75

Observation eca344e0-6e26-48e3-9215-28d1b28f9a1b · outbound

This paper cites 2010, , 409, 1647.

Constraints on the state of the IGM at $z\sim 8-10$ using redshifted 21-cm observations with LOFAR 2010, , 409, 1647

Reference 76

Resolution
verified fuzzy
raw_fallback, observed 2026-08-16T04:51:31.165341Z

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=arxiv_source observed=2026-08-16T04:51:30.014182Z digest=sha256:52ceb1ce5209bde3146ef24304e8a07d5487d0cf03418384202eb17035ed33a8

Observation a372d86f-adb8-4fa1-8488-419e9e418a31 · outbound

This paper cites S., Parsons , A.

Constraints on the state of the IGM at $z\sim 8-10$ using redshifted 21-cm observations with LOFAR S., Parsons , A

Reference 77

Resolution
verified fuzzy
raw_fallback, observed 2026-08-16T04:51:31.154960Z

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=arxiv_source observed=2026-08-16T04:51:30.017811Z digest=sha256:0d0c5a1daecdc0d52a8d1ed6418eb610322162466e36c86576ad15039538ad08

Observation e8afb6b4-728b-454d-b0ec-10c1631c5261 · outbound

This paper cites S., Parsons , A.

Constraints on the state of the IGM at $z\sim 8-10$ using redshifted 21-cm observations with LOFAR S., Parsons , A

Reference 78

Resolution
verified fuzzy
raw_fallback, observed 2026-08-16T04:51:31.145119Z

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=arxiv_source observed=2026-08-16T04:51:30.021837Z digest=sha256:968b7cc5a3c9bcdbbaa9875a9dbdbec37ff334a69a437e300ebf0a0e796c4e4d

Observation 0e3d3207-9e89-45f8-a05a-111cadb35e35 · outbound

This paper cites C., Cheng , C., et al.

Constraints on the state of the IGM at $z\sim 8-10$ using redshifted 21-cm observations with LOFAR C., Cheng , C., et al

Reference 79

Resolution
verified fuzzy
raw_fallback, observed 2026-08-16T04:51:31.135347Z

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=arxiv_source observed=2026-08-16T04:51:30.025545Z digest=sha256:b032e7b9b7f202ed04a958de1897b06c8fa316c4b58a128595d27d61dbd48465

Observation 4a972d7e-6c51-4274-9fbb-e2d4bbd9821b · outbound

This paper cites 2015, in Proceedings of Advancing Astrophysics with the Square Kilometre Array — PoS(AASKA14), AASKA14 (Sissa Medialab).

Constraints on the state of the IGM at $z\sim 8-10$ using redshifted 21-cm observations with LOFAR 2015, in Proceedings of Advancing Astrophysics with the Square Kilometre Array — PoS(AASKA14), AASKA14 (Sissa Medialab)

Reference 80

Resolution
verified fuzzy
raw_fallback, observed 2026-08-16T04:51:31.126441Z

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=arxiv_source observed=2026-08-16T04:51:30.028632Z digest=sha256:b726cb55e315568d0102e3d88e250ff47243ae92a93c173960959a6d1ace7104

Observation 7a0baf67-06e7-4f5a-872d-2637c103583c · outbound

This paper cites M., Zaroubi , S., & Abdalla , F.

Constraints on the state of the IGM at $z\sim 8-10$ using redshifted 21-cm observations with LOFAR M., Zaroubi , S., & Abdalla , F

Reference 81

Resolution
verified fuzzy
raw_fallback, observed 2026-08-16T04:51:31.116440Z

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=arxiv_source observed=2026-08-16T04:51:30.032144Z digest=sha256:889dd4e5f0e88ec8e97b90b3bbf02105b4173872229c7a1acf9db8bc27b39b24

Observation 265182f0-b623-450d-a304-8a2d95fdcd3f · outbound

This paper cites & Bridle , S.

Constraints on the state of the IGM at $z\sim 8-10$ using redshifted 21-cm observations with LOFAR & Bridle , S

Reference 82

Resolution
verified fuzzy
raw_fallback, observed 2026-08-16T04:51:31.106257Z

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=arxiv_source observed=2026-08-16T04:51:30.036795Z digest=sha256:751fa25d547bebeb116f7335314d11f91ccfdc6beada73748e097b6225b3edd8

Observation 7341a015-7171-402a-90f0-1bff2bf1b454 · outbound

This paper cites R., & Trott , C.

Constraints on the state of the IGM at $z\sim 8-10$ using redshifted 21-cm observations with LOFAR R., & Trott , C

Reference 83

Resolution
verified fuzzy
raw_fallback, observed 2026-08-16T04:51:31.096181Z

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=arxiv_source observed=2026-08-16T04:51:30.040461Z digest=sha256:d492220d3c5934935484b6e5b8c509fee2e54f157e60a39f31adb972188dd53c

Observation 2f69b29b-12ad-4704-9d14-d2c6a06474c3 · outbound

This paper cites 2023, , 522, 3284.

Constraints on the state of the IGM at $z\sim 8-10$ using redshifted 21-cm observations with LOFAR 2023, , 522, 3284

Reference 84

Resolution
verified fuzzy
raw_fallback, observed 2026-08-16T04:51:31.085718Z

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=arxiv_source observed=2026-08-16T04:51:30.044248Z digest=sha256:43084da814adaaf7a25ffcccf4a285b4bec59d722961bd66403abbfb42a81bbc

Observation 20679c25-3fd2-4966-a778-472ebe061f24 · outbound

This paper cites an unresolved cited work.

Constraints on the state of the IGM at $z\sim 8-10$ using redshifted 21-cm observations with LOFAR Unresolved cited work

Reference 85

Resolution
unresolved
raw_fallback, observed 2026-08-16T04:51:31.075386Z

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=arxiv_source observed=2026-08-16T04:51:30.047883Z digest=sha256:69c67830d01b6929184c97c3fe198830ec7cecc057d311ebf0fb4c5a82e3d12e

Observation 18634025-9f8f-43cc-ab63-ac694ea14b8a · outbound

This paper cites R., Mellema , G., et al.

Constraints on the state of the IGM at $z\sim 8-10$ using redshifted 21-cm observations with LOFAR R., Mellema , G., et al

Reference 86

Resolution
verified fuzzy
raw_fallback, observed 2026-08-16T04:51:31.064771Z

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=arxiv_source observed=2026-08-16T04:51:30.051483Z digest=sha256:8360859c4c561f361afe8c9f970faa044742e8eb66b79b7a8d039d1a6f57254c

Observation db6bf678-6314-489d-9eed-a437f0d0da6e · outbound

This paper cites 2015, Advancing Astrophysics with the Square Kilometre Array (AASKA14), 10.

Constraints on the state of the IGM at $z\sim 8-10$ using redshifted 21-cm observations with LOFAR 2015, Advancing Astrophysics with the Square Kilometre Array (AASKA14), 10

Reference 87

Resolution
verified fuzzy
raw_fallback, observed 2026-08-16T04:51:31.054257Z

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=arxiv_source observed=2026-08-16T04:51:30.055044Z digest=sha256:212e2a555bbce9ba957004dfc433ffb94779ab414e339a70c16f7449006e0c9d

Observation 1a7e0ffc-3a4f-41c6-b37e-5a954c883e63 · outbound

This paper cites an unresolved cited work.

Constraints on the state of the IGM at $z\sim 8-10$ using redshifted 21-cm observations with LOFAR Unresolved cited work

Reference 88

Resolution
unresolved
raw_fallback, observed 2026-08-16T04:51:31.043990Z

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=arxiv_source observed=2026-08-16T04:51:30.059157Z digest=sha256:0bcf72ab45ef2df21df5fd81db509d9a4ed073a055e02aa4b05acbee35093071

Observation e6f3042a-3378-4f88-b119-cae7e1885ecd · outbound

This paper cites G., Bobin , J., & Carucci , I.

Constraints on the state of the IGM at $z\sim 8-10$ using redshifted 21-cm observations with LOFAR G., Bobin , J., & Carucci , I

Reference 89

Resolution
verified fuzzy
raw_fallback, observed 2026-08-16T04:51:31.033211Z

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=arxiv_source observed=2026-08-16T04:51:30.063299Z digest=sha256:7d01681048ee1508c012e9fdaaa9e3af8e1aba552ee781babde319be53eab9a0

Observation 783fd113-3439-469e-bcff-bc232f0abf93 · outbound

This paper cites G., Ghosh , A., & Koopmans , L.

Constraints on the state of the IGM at $z\sim 8-10$ using redshifted 21-cm observations with LOFAR G., Ghosh , A., & Koopmans , L

Reference 90

Resolution
verified fuzzy
raw_fallback, observed 2026-08-16T04:51:31.021559Z

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=arxiv_source observed=2026-08-16T04:51:30.067408Z digest=sha256:a19a8b2e7e555638cd9a9c21ad8b68a02f9c6d7fa39c99acb0c74ee709e33b16

Observation dc9c0ca8-670d-4fab-b657-b61cdd991302 · outbound

This paper cites G., Mevius , M., Koopmans , L.

Constraints on the state of the IGM at $z\sim 8-10$ using redshifted 21-cm observations with LOFAR G., Mevius , M., Koopmans , L

Reference 91

Resolution
verified fuzzy
raw_fallback, observed 2026-08-16T04:51:31.011870Z

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=arxiv_source observed=2026-08-16T04:51:30.071356Z digest=sha256:5e3f5ee8b3018b7d4f23bd5a8163787e87cc712914ea46e8599d434213cad6dd

Observation 88f53fbd-dd33-4c25-a12d-bd24e6d7acbe · outbound

This paper cites Deeper multi-redshift upper limits on the Epoch of Reionization 21-cm signal power spectrum from LOFAR between z=8.3 and z=10.1.

Constraints on the state of the IGM at $z\sim 8-10$ using redshifted 21-cm observations with LOFAR Deeper multi-redshift upper limits on the Epoch of Reionization 21-cm signal power spectrum from LOFAR between z=8.3 and z=10.1

Reference 92

Resolution
unresolved
no resolver link, observed 2026-08-16T04:51:30.075040Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T04:51:30.075040Z digest=sha256:fb529c3f08872d60d8df047f3dd2becd1ac5597b3fe6cb1b13a25fea301d8692

Observation 69342532-de2f-450a-8481-bd2cac7a0005 · outbound

This paper cites & Furlanetto , S.

Constraints on the state of the IGM at $z\sim 8-10$ using redshifted 21-cm observations with LOFAR & Furlanetto , S

Reference 93

Resolution
verified fuzzy
raw_fallback, observed 2026-08-16T04:51:31.001818Z

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=arxiv_source observed=2026-08-16T04:51:30.079434Z digest=sha256:da5608099b8cb573e6a0abd3ed8bd1cb512449b97020caaf5d1b69cfca17a38f

Observation bd32cdcf-a821-452f-bfdf-7cc3440f8cb8 · outbound

This paper cites an unresolved cited work.

Constraints on the state of the IGM at $z\sim 8-10$ using redshifted 21-cm observations with LOFAR Unresolved cited work

Reference 94

Resolution
unresolved
raw_fallback, observed 2026-08-16T04:51:30.991899Z

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=arxiv_source observed=2026-08-16T04:51:30.082819Z digest=sha256:dd4b581e6fb1e5e7d3fe6b202591f7c3a20dae7abb14ebfee8b6a6bdccb8697c

Observation 244ddb09-1489-4d9a-a6c9-655b777a09b4 · outbound

This paper cites N., et al.

Constraints on the state of the IGM at $z\sim 8-10$ using redshifted 21-cm observations with LOFAR N., et al

Reference 95

Resolution
verified fuzzy
raw_fallback, observed 2026-08-16T04:51:30.981860Z

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=arxiv_source observed=2026-08-16T04:51:30.085870Z digest=sha256:8892d31dbc209d03b5f2efdf95517153a70cc9827fb687a2ba1d10441a8ea9f8

Observation fedb320e-d1c9-4089-89d1-e306a0aa9a20 · outbound

This paper cites 2012, , 419, 2095.

Constraints on the state of the IGM at $z\sim 8-10$ using redshifted 21-cm observations with LOFAR 2012, , 419, 2095

Reference 96

Resolution
verified fuzzy
raw_fallback, observed 2026-08-16T04:51:30.971324Z

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=arxiv_source observed=2026-08-16T04:51:30.088775Z digest=sha256:13b1fd8d8fc82bcac372db24b576ca113191ef391a011e446bee52c8b8ff5e1a

Observation b2353ac7-7926-43c6-9b69-230dab0dcef1 · outbound

This paper cites B., Furlanetto , S.

Constraints on the state of the IGM at $z\sim 8-10$ using redshifted 21-cm observations with LOFAR B., Furlanetto , S

Reference 97

Resolution
verified fuzzy
raw_fallback, observed 2026-08-16T04:51:30.960328Z

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=arxiv_source observed=2026-08-16T04:51:30.091937Z digest=sha256:100e8c8959733dc27edffe0bb20fc50e1f8affcdc939d64ac3ccd0d0483d2f99

Observation 906a3ece-ef80-441f-9a7a-4671c1d22449 · outbound

This paper cites 2020, , 498, 4178.

Constraints on the state of the IGM at $z\sim 8-10$ using redshifted 21-cm observations with LOFAR 2020, , 498, 4178

Reference 98

Resolution
verified fuzzy
raw_fallback, observed 2026-08-16T04:51:30.949791Z

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=arxiv_source observed=2026-08-16T04:51:30.095676Z digest=sha256:b37eaad89e0a210aee137a56a98e3f14aec0926f611ba2c916c2644bdf655072

Observation a9509062-a82c-47dc-8238-0ff9e2c58206 · outbound

This paper cites A., Altamirano, C., Bidula, V., et al.

Constraints on the state of the IGM at $z\sim 8-10$ using redshifted 21-cm observations with LOFAR A., Altamirano, C., Bidula, V., et al

Reference 99

Resolution
verified fuzzy
raw_fallback, observed 2026-08-16T04:51:30.939932Z

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=arxiv_source observed=2026-08-16T04:51:30.099160Z digest=sha256:bcaaef673b0288a8bf02c39c1b45a905efed04d9850449908c605c586965c556

Observation 383284c5-e39d-43f9-981c-333f33857f5f · outbound

This paper cites A., Fialkov , A., Bowman , J.

Constraints on the state of the IGM at $z\sim 8-10$ using redshifted 21-cm observations with LOFAR A., Fialkov , A., Bowman , J

Reference 100

Resolution
verified fuzzy
raw_fallback, observed 2026-08-16T04:51:30.929517Z

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=arxiv_source observed=2026-08-16T04:51:30.103141Z digest=sha256:a4e890e85dab9503c5f13628f269c4d80768b8815f903a4d5a9631bb3880fb77

Pith citing papers

Observation f12d9b75-0afe-465c-8447-5548e4a1cc67 · inbound

Improved upper limits on the 21-cm signal power spectrum at $z=17.0$ and $z=20.3$ from an optimal field observed with NenuFAR cites this paper.

Improved upper limits on the 21-cm signal power spectrum at $z=17.0$ and $z=20.3$ from an optimal field observed with NenuFAR Constraints on the state of the IGM at $z\sim 8-10$ using redshifted 21-cm observations with LOFAR

Reference 50

Resolution
unresolved
no resolver link, observed 2026-08-06T17:35:29.464923Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-06T17:35:29.464923Z digest=sha256:5567a82581c2279b3350df909ea3fac78195f28e3df011831191c95acbaa4c77

Observation 230afebf-ff7a-4e85-81d0-aecd8e83fca5 · inbound

Rapid late-time reionization: constraints and cosmological implications cites this paper.

Rapid late-time reionization: constraints and cosmological implications Constraints on the state of the IGM at $z\sim 8-10$ using redshifted 21-cm observations with LOFAR

Reference 57

Resolution
unresolved
no resolver link, observed 2026-08-05T14:41:15.384679Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-05T14:41:15.384679Z digest=sha256:48460b3451e85fa2259e5fa1b76749e9469fe78ffcc98e049df4984ca6423413

Observation a28758b3-c666-46ca-ab02-723e98c1942f · inbound

Into the Gompverse: A robust Gompertzian reionization model for CMB analyses cites this paper.

Into the Gompverse: A robust Gompertzian reionization model for CMB analyses Constraints on the state of the IGM at $z\sim 8-10$ using redshifted 21-cm observations with LOFAR

Reference 112

Resolution
verified exact
arxiv_id, observed 2026-05-10T13:45:28.817898Z

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=2026-05-10T13:00:40.627560Z digest=sha256:6ac8905e04f03c0be0711d64eea0cfee4cb1ef6cdcb7385043c8af92660e0d1e

Observation 60592962-32d9-412a-ab7b-14c8a1d825a3 · inbound

21cmEMUv3: a hybrid diffusion-LSTM emulator of 21cmFAST summary observables cites this paper.

21cmEMUv3: a hybrid diffusion-LSTM emulator of 21cmFAST summary observables Constraints on the state of the IGM at $z\sim 8-10$ using redshifted 21-cm observations with LOFAR

Reference 294

Resolution
metadata mismatch
arxiv_id, observed 2026-06-28T21:02:38.549576Z

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=arxiv_source observed=2026-06-28T20:53:04.280649Z digest=sha256:ee6223e31f94244c516329d6a03288d2ae502a726a672ce5ccbcca37b211f485

Observation 674fd1ab-4c6d-4115-852e-e2bc3c3444a4 · inbound

When galaxies burst II. Implications of enhanced burstiness for the 21-cm Cosmic Dawn signal cites this paper.

When galaxies burst II. Implications of enhanced burstiness for the 21-cm Cosmic Dawn signal Constraints on the state of the IGM at $z\sim 8-10$ using redshifted 21-cm observations with LOFAR

Reference 89

Resolution
unresolved
no resolver link, observed 2026-08-01T09:49:27.833856Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T09:49:27.833856Z digest=sha256:b41021ae23fa931639718942a3b36c857ad7c54df2e2da6ce95f8ce80718d092