Paper Citation Record · LEDGER

How probable is the Lyman-$\alpha$ damping wing in the spectrum of the redshift z = 5.9896 quasar ULAS J0148+0600?

As of 22 August 2026, this Paper Citation Record lists 66 of 66 outbound references and 2 inbound Pith citation observations for arXiv:2502.03085.

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

pith.paper-citation-record.v1
2502.03085 v3

Coverage vector

measured 66 of 66 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links, observed 2026-08-09T06:06:10.051422Z

measured 68 of 68 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-22T06:32:14.747728+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-16T04:22:25.668338Z

measured 1 of 1 external citation measurements

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

Source: pith, observed 2026-08-10T05:30:23.456663Z

Reference resolution

66 of 66 outbound references displayed

verified exact3
verified fuzzy0
unresolved63
parse uncertain0
malformed identifier0
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External citation measurements

0
pith, observed 2026-08-10T05:30:23.456663Z

Outbound references

Observation de8a5dc3-c7f4-4715-bd40-2b103765cb94 · outbound

This paper cites The First Billion Years, According to JWST.

How probable is the Lyman-$\alpha$ damping wing in the spectrum of the redshift z = 5.9896 quasar ULAS J0148+0600? The First Billion Years, According to JWST

Reference 1

Resolution: unresolved; no resolver link, observed 2026-08-09T06:06:09.829362Z

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Observation 397bb8be-9994-45d6-ad5e-84446ca7161c · outbound

This paper cites J., et al., 2023, @doi [ ] 10.1093/mnras/stac3347 , https://ui.adsabs.harvard.edu/abs/2023MNRAS.518.4755A 518, 4755.

How probable is the Lyman-$\alpha$ damping wing in the spectrum of the redshift z = 5.9896 quasar ULAS J0148+0600? J., et al., 2023, @doi [ ] 10.1093/mnras/stac3347 , https://ui.adsabs.harvard.edu/abs/2023MNRAS.518.4755A 518, 4755

Reference 2

Resolution: unresolved; no resolver link, observed 2026-08-09T06:06:09.833921Z

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Observation b17b2e16-7ccc-4cfd-959b-a34fd166b548 · outbound

This paper cites G., Kulkarni G., Bolton J.

How probable is the Lyman-$\alpha$ damping wing in the spectrum of the redshift z = 5.9896 quasar ULAS J0148+0600? G., Kulkarni G., Bolton J

Reference 3

Resolution: unresolved; no resolver link, observed 2026-08-09T06:06:09.836908Z

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Observation 25d34ba9-4a12-4676-bf35-36f3b39a9096 · outbound

This paper cites an unresolved cited work.

How probable is the Lyman-$\alpha$ damping wing in the spectrum of the redshift z = 5.9896 quasar ULAS J0148+0600? Unresolved cited work

Reference 4

Resolution: unresolved; no resolver link, observed 2026-08-09T06:06:09.841260Z

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Observation 7d08ee6f-60b1-4baf-b81e-fc6baa77a76c · outbound

This paper cites an unresolved cited work.

How probable is the Lyman-$\alpha$ damping wing in the spectrum of the redshift z = 5.9896 quasar ULAS J0148+0600? Unresolved cited work

Reference 5

Resolution: unresolved; no resolver link, observed 2026-08-09T06:06:09.844276Z

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Unavailable: canonical work link unavailable.

Observation a7cfcd41-9c4c-4afc-b848-0f993b22eabf · outbound

This paper cites D., Bolton J.

How probable is the Lyman-$\alpha$ damping wing in the spectrum of the redshift z = 5.9896 quasar ULAS J0148+0600? D., Bolton J

Reference 6

Resolution: unresolved; no resolver link, observed 2026-08-09T06:06:09.847180Z

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Observation 3c5d1883-25d6-40aa-96e9-7c381330922e · outbound

This paper cites D., D'Aloisio A., Christenson H.

How probable is the Lyman-$\alpha$ damping wing in the spectrum of the redshift z = 5.9896 quasar ULAS J0148+0600? D., D'Aloisio A., Christenson H

Reference 7

Resolution: unresolved; no resolver link, observed 2026-08-09T06:06:09.850458Z

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Observation c7931f41-ebc3-4bba-947b-e4c88526607e · outbound

This paper cites D., Bolton J.

How probable is the Lyman-$\alpha$ damping wing in the spectrum of the redshift z = 5.9896 quasar ULAS J0148+0600? D., Bolton J

Reference 8

Resolution: unresolved; no resolver link, observed 2026-08-09T06:06:09.853258Z

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Observation 29fd7326-40e8-4664-89e0-7cd2e5ac3246 · outbound

This paper cites an unresolved cited work.

How probable is the Lyman-$\alpha$ damping wing in the spectrum of the redshift z = 5.9896 quasar ULAS J0148+0600? Unresolved cited work

Reference 9

Resolution: unresolved; no resolver link, observed 2026-08-09T06:06:09.856862Z

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Observation c5d9b6b1-fe9e-4a48-86f6-fe3fe44f04b5 · outbound

This paper cites S., Haehnelt M.

How probable is the Lyman-$\alpha$ damping wing in the spectrum of the redshift z = 5.9896 quasar ULAS J0148+0600? S., Haehnelt M

Reference 11

Resolution: unresolved; no resolver link, observed 2026-08-09T06:06:09.863338Z

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Observation 0dfbf7b0-503f-4f0c-b4f6-6b02ccd8a83b · outbound

This paper cites S., Becker G.

How probable is the Lyman-$\alpha$ damping wing in the spectrum of the redshift z = 5.9896 quasar ULAS J0148+0600? S., Becker G

Reference 12

Resolution: unresolved; no resolver link, observed 2026-08-09T06:06:09.866581Z

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Observation e671ff73-8edd-4967-8112-5106126e7b77 · outbound

This paper cites an unresolved cited work.

How probable is the Lyman-$\alpha$ damping wing in the spectrum of the redshift z = 5.9896 quasar ULAS J0148+0600? Unresolved cited work

Reference 13

Resolution: unresolved; no resolver link, observed 2026-08-09T06:06:09.869883Z

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Observation a430037a-35af-4fec-a56a-77c95726f4e0 · outbound

This paper cites an unresolved cited work.

How probable is the Lyman-$\alpha$ damping wing in the spectrum of the redshift z = 5.9896 quasar ULAS J0148+0600? Unresolved cited work

Reference 14

Resolution: unresolved; no resolver link, observed 2026-08-09T06:06:09.873189Z

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Observation d9c35acc-6bc9-484d-9ded-aae91ca543a1 · outbound

This paper cites an unresolved cited work.

How probable is the Lyman-$\alpha$ damping wing in the spectrum of the redshift z = 5.9896 quasar ULAS J0148+0600? Unresolved cited work

Reference 15

Resolution: unresolved; no resolver link, observed 2026-08-09T06:06:09.876403Z

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Observation 3ef0287d-6b3d-4923-9b73-d4a497def3a2 · outbound

This paper cites an unresolved cited work.

How probable is the Lyman-$\alpha$ damping wing in the spectrum of the redshift z = 5.9896 quasar ULAS J0148+0600? Unresolved cited work

Reference 16

Resolution: unresolved; no resolver link, observed 2026-08-09T06:06:09.879668Z

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Observation 7a74f529-70e5-42ae-9dd8-d7c76708decd · outbound

This paper cites Y., 2021, @doi [ ] 10.3847/1538-4357/abe7e7 , https://ui.adsabs.harvard.edu/abs/2021ApJ...911...60C 911, 60.

How probable is the Lyman-$\alpha$ damping wing in the spectrum of the redshift z = 5.9896 quasar ULAS J0148+0600? Y., 2021, @doi [ ] 10.3847/1538-4357/abe7e7 , https://ui.adsabs.harvard.edu/abs/2021ApJ...911...60C 911, 60

Reference 17

Resolution: unresolved; no resolver link, observed 2026-08-09T06:06:09.882987Z

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Observation 1005d66a-b261-44e5-bb95-85917a5bd8c2 · outbound

This paper cites an unresolved cited work.

How probable is the Lyman-$\alpha$ damping wing in the spectrum of the redshift z = 5.9896 quasar ULAS J0148+0600? Unresolved cited work

Reference 18

Resolution: unresolved; no resolver link, observed 2026-08-09T06:06:09.886239Z

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Observation 10ad7dcd-8de4-471a-ba08-935f70b5ed17 · outbound

This paper cites B., et al., 2018, @doi [ ] 10.3847/1538-4357/aad6dc , https://ui.adsabs.harvard.edu/abs/2018ApJ...864..142D 864, 142.

How probable is the Lyman-$\alpha$ damping wing in the spectrum of the redshift z = 5.9896 quasar ULAS J0148+0600? B., et al., 2018, @doi [ ] 10.3847/1538-4357/aad6dc , https://ui.adsabs.harvard.edu/abs/2018ApJ...864..142D 864, 142

Reference 19

Resolution: unresolved; no resolver link, observed 2026-08-09T06:06:09.889544Z

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Observation 18e5bc11-f578-4d69-b435-ceeaac98599f · outbound

This paper cites B., Hennawi J.

How probable is the Lyman-$\alpha$ damping wing in the spectrum of the redshift z = 5.9896 quasar ULAS J0148+0600? B., Hennawi J

Reference 20

Resolution: unresolved; no resolver link, observed 2026-08-09T06:06:09.892982Z

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Observation db2c4252-a3a0-45ff-a5fa-ac2b4c14b31e · outbound

This paper cites B., et al., 2024, @doi [ ] 10.3847/1538-4357/ad1d5d , https://ui.adsabs.harvard.edu/abs/2024ApJ...965..134D 965, 134.

How probable is the Lyman-$\alpha$ damping wing in the spectrum of the redshift z = 5.9896 quasar ULAS J0148+0600? B., et al., 2024, @doi [ ] 10.3847/1538-4357/ad1d5d , https://ui.adsabs.harvard.edu/abs/2024ApJ...965..134D 965, 134

Reference 21

Resolution: unresolved; no resolver link, observed 2026-08-09T06:06:09.896514Z

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Observation a3e1cfc6-b5d8-4b4a-9329-2b0c7da06254 · outbound

This paper cites UNCOVERing the contribution of black holes to reionization in the JWST era.

How probable is the Lyman-$\alpha$ damping wing in the spectrum of the redshift z = 5.9896 quasar ULAS J0148+0600? UNCOVERing the contribution of black holes to reionization in the JWST era

Reference 22

Resolution: unresolved; no resolver link, observed 2026-08-09T06:06:09.899878Z

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Observation b1fd2d24-994c-446e-a19e-34549e8eca9c · outbound

This paper cites B., Hennawi J.

How probable is the Lyman-$\alpha$ damping wing in the spectrum of the redshift z = 5.9896 quasar ULAS J0148+0600? B., Hennawi J

Reference 23

Resolution: unresolved; no resolver link, observed 2026-08-09T06:06:09.903639Z

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Unavailable: canonical work link unavailable.

Observation 9dbe350e-c382-4317-9e21-add0708b2150 · outbound

This paper cites B., Hennawi J.

How probable is the Lyman-$\alpha$ damping wing in the spectrum of the redshift z = 5.9896 quasar ULAS J0148+0600? B., Hennawi J

Reference 24

Resolution: unresolved; no resolver link, observed 2026-08-09T06:06:09.907099Z

Source-reported events for the cited work

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Observation e3f99d37-17df-442c-abe2-61853e91abd0 · outbound

This paper cites an unresolved cited work.

How probable is the Lyman-$\alpha$ damping wing in the spectrum of the redshift z = 5.9896 quasar ULAS J0148+0600? Unresolved cited work

Reference 25

Resolution: unresolved; no resolver link, observed 2026-08-09T06:06:09.910595Z

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Observation 0f1cb56e-fa0c-4c1c-b06f-535971e39d6c · outbound

This paper cites IPAW 2020 Preprint: Efficient Computation of Provenance for Query Result Exploration.

How probable is the Lyman-$\alpha$ damping wing in the spectrum of the redshift z = 5.9896 quasar ULAS J0148+0600? IPAW 2020 Preprint: Efficient Computation of Provenance for Query Result Exploration

Reference 26

Resolution: unresolved; no resolver link, observed 2026-08-09T06:06:09.913840Z

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Observation d51d264e-f733-4c49-b2a2-f416a169c68a · outbound

This paper cites B., Wang F., Yang J., Hennawi J.

How probable is the Lyman-$\alpha$ damping wing in the spectrum of the redshift z = 5.9896 quasar ULAS J0148+0600? B., Wang F., Yang J., Hennawi J

Reference 27

Resolution: unresolved; no resolver link, observed 2026-08-09T06:06:09.917479Z

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Observation 1025fa37-e7ab-44ed-ac36-9a93cb287907 · outbound

This paper cites E., Peterson B.

How probable is the Lyman-$\alpha$ damping wing in the spectrum of the redshift z = 5.9896 quasar ULAS J0148+0600? E., Peterson B

Reference 28

Resolution: unresolved; no resolver link, observed 2026-08-09T06:06:09.920834Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 59681610-3dfc-4d99-b0c3-c787db20b4a8 · outbound

This paper cites an unresolved cited work.

How probable is the Lyman-$\alpha$ damping wing in the spectrum of the redshift z = 5.9896 quasar ULAS J0148+0600? Unresolved cited work

Reference 29

Resolution: unresolved; no resolver link, observed 2026-08-09T06:06:09.924499Z

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Unavailable: canonical work link unavailable.

Observation fb570796-bbb3-4211-b22a-faab03257eb5 · outbound

This paper cites Precisely Measuring the Cosmic Reionization History from IGM Damping Wings Towards Quasars.

How probable is the Lyman-$\alpha$ damping wing in the spectrum of the redshift z = 5.9896 quasar ULAS J0148+0600? Precisely Measuring the Cosmic Reionization History from IGM Damping Wings Towards Quasars

Reference 30

Resolution: unresolved; no resolver link, observed 2026-08-09T06:06:09.927716Z

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Observation ce5e36ca-0a42-474d-b656-7ce0a50ccc3e · outbound

This paper cites an unresolved cited work.

How probable is the Lyman-$\alpha$ damping wing in the spectrum of the redshift z = 5.9896 quasar ULAS J0148+0600? Unresolved cited work

Reference 31

Resolution: unresolved; no resolver link, observed 2026-08-09T06:06:09.931285Z

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Observation 6eb2599a-4cd3-4a6b-a2c9-815c6a5f1b16 · outbound

This paper cites C., Haehnelt M.

How probable is the Lyman-$\alpha$ damping wing in the spectrum of the redshift z = 5.9896 quasar ULAS J0148+0600? C., Haehnelt M

Reference 32

Resolution: verified exact; doi, observed 2026-08-09T06:06:10.288655Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

Observation 39dc9131-b0ac-4c1e-a782-063c9a02e759 · outbound

This paper cites C., Weinberger L.

How probable is the Lyman-$\alpha$ damping wing in the spectrum of the redshift z = 5.9896 quasar ULAS J0148+0600? C., Weinberger L

Reference 33

Resolution: unresolved; no resolver link, observed 2026-08-09T06:06:09.936887Z

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Observation 80739c6e-fe48-473e-9f3e-5843b9166e7e · outbound

This paper cites C., Kulkarni G., Haehnelt M.

How probable is the Lyman-$\alpha$ damping wing in the spectrum of the redshift z = 5.9896 quasar ULAS J0148+0600? C., Kulkarni G., Haehnelt M

Reference 34

Resolution: unresolved; no resolver link, observed 2026-08-09T06:06:09.939883Z

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Observation f0ced7d1-0487-4fc0-b95a-d4f23a79ca88 · outbound

This paper cites C., Haehnelt M.

How probable is the Lyman-$\alpha$ damping wing in the spectrum of the redshift z = 5.9896 quasar ULAS J0148+0600? C., Haehnelt M

Reference 35

Resolution: unresolved; no resolver link, observed 2026-08-09T06:06:09.942931Z

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Observation bf2225f7-93a0-4bcb-8a31-9d29bf849d96 · outbound

This paper cites an unresolved cited work.

How probable is the Lyman-$\alpha$ damping wing in the spectrum of the redshift z = 5.9896 quasar ULAS J0148+0600? Unresolved cited work

Reference 36

Resolution: unresolved; no resolver link, observed 2026-08-09T06:06:09.945888Z

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Observation 6e2c652d-50ac-41ef-bf66-294d47d28afa · outbound

This paper cites an unresolved cited work.

How probable is the Lyman-$\alpha$ damping wing in the spectrum of the redshift z = 5.9896 quasar ULAS J0148+0600? Unresolved cited work

Reference 37

Resolution: unresolved; no resolver link, observed 2026-08-09T06:06:09.948581Z

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Unavailable: canonical work link unavailable.

Observation 358657a5-3a90-4546-804c-570d23f618cb · outbound

This paper cites F., Prochaska J.

How probable is the Lyman-$\alpha$ damping wing in the spectrum of the redshift z = 5.9896 quasar ULAS J0148+0600? F., Prochaska J

Reference 38

Resolution: unresolved; no resolver link, observed 2026-08-09T06:06:09.951504Z

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Unavailable: canonical work link unavailable.

Observation 9a81ebb2-78dd-4b45-8052-059eea0acaf5 · outbound

This paper cites an unresolved cited work.

How probable is the Lyman-$\alpha$ damping wing in the spectrum of the redshift z = 5.9896 quasar ULAS J0148+0600? Unresolved cited work

Reference 39

Resolution: unresolved; no resolver link, observed 2026-08-09T06:06:09.954757Z

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Unavailable: canonical work link unavailable.

Observation 744dd82c-11b2-4a8e-960f-15c615b2b17c · outbound

This paper cites an unresolved cited work.

How probable is the Lyman-$\alpha$ damping wing in the spectrum of the redshift z = 5.9896 quasar ULAS J0148+0600? Unresolved cited work

Reference 40

Resolution: unresolved; no resolver link, observed 2026-08-09T06:06:09.958257Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 60cc57b9-f23b-49a1-b576-cba8f93e7314 · outbound

This paper cites an unresolved cited work.

How probable is the Lyman-$\alpha$ damping wing in the spectrum of the redshift z = 5.9896 quasar ULAS J0148+0600? Unresolved cited work

Reference 41

Resolution: verified exact; doi, observed 2026-08-09T06:06:10.228452Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

Observation 354527dd-fa7b-4a19-9669-0aefd0adc7d6 · outbound

This paper cites an unresolved cited work.

How probable is the Lyman-$\alpha$ damping wing in the spectrum of the redshift z = 5.9896 quasar ULAS J0148+0600? Unresolved cited work

Reference 42

Resolution: unresolved; no resolver link, observed 2026-08-09T06:06:09.964625Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 3b774573-2f5f-41aa-932f-f0d0dfc9629c · outbound

This paper cites an unresolved cited work.

How probable is the Lyman-$\alpha$ damping wing in the spectrum of the redshift z = 5.9896 quasar ULAS J0148+0600? Unresolved cited work

Reference 43

Resolution: unresolved; no resolver link, observed 2026-08-09T06:06:09.967856Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 62ec174c-f4b7-438d-aeff-28566facd277 · outbound

This paper cites an unresolved cited work.

How probable is the Lyman-$\alpha$ damping wing in the spectrum of the redshift z = 5.9896 quasar ULAS J0148+0600? Unresolved cited work

Reference 44

Resolution: unresolved; no resolver link, observed 2026-08-09T06:06:09.971432Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 29b72e99-6435-4c57-b2a6-9391681e480e · outbound

This paper cites A., Eilers A.-C., Davies F.

How probable is the Lyman-$\alpha$ damping wing in the spectrum of the redshift z = 5.9896 quasar ULAS J0148+0600? A., Eilers A.-C., Davies F

Reference 45

Resolution: unresolved; no resolver link, observed 2026-08-09T06:06:09.974688Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a1b632d7-4462-4054-afe3-211902576303 · outbound

This paper cites J., et al., 2011, @doi [ ] 10.1038/nature10159 , https://ui.adsabs.harvard.edu/abs/2011Natur.474..616M 474, 616.

How probable is the Lyman-$\alpha$ damping wing in the spectrum of the redshift z = 5.9896 quasar ULAS J0148+0600? J., et al., 2011, @doi [ ] 10.1038/nature10159 , https://ui.adsabs.harvard.edu/abs/2011Natur.474..616M 474, 616

Reference 46

Resolution: unresolved; no resolver link, observed 2026-08-09T06:06:09.978012Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c1d817e0-fb05-40fe-96d5-91f48e1211f8 · outbound

This paper cites B., Mirocha J., Chisholm J., Furlanetto S.

How probable is the Lyman-$\alpha$ damping wing in the spectrum of the redshift z = 5.9896 quasar ULAS J0148+0600? B., Mirocha J., Chisholm J., Furlanetto S

Reference 47

Resolution: unresolved; no resolver link, observed 2026-08-09T06:06:09.981392Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation bee7b832-9f97-4c90-a577-1773ee0315e0 · outbound

This paper cites an unresolved cited work.

How probable is the Lyman-$\alpha$ damping wing in the spectrum of the redshift z = 5.9896 quasar ULAS J0148+0600? Unresolved cited work

Reference 48

Resolution: unresolved; no resolver link, observed 2026-08-09T06:06:09.985047Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 42835945-0f9a-4db2-9d96-b49ab4f61877 · outbound

This paper cites an unresolved cited work.

How probable is the Lyman-$\alpha$ damping wing in the spectrum of the redshift z = 5.9896 quasar ULAS J0148+0600? Unresolved cited work

Reference 49

Resolution: unresolved; no resolver link, observed 2026-08-09T06:06:09.988805Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f2c3648e-c9e1-4701-ae6e-f26b4602966b · outbound

This paper cites C., Haehnelt M.

How probable is the Lyman-$\alpha$ damping wing in the spectrum of the redshift z = 5.9896 quasar ULAS J0148+0600? C., Haehnelt M

Reference 50

Resolution: unresolved; no resolver link, observed 2026-08-09T06:06:09.992284Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d068aa71-49eb-4fe0-a310-3ed8af2e9161 · outbound

This paper cites an unresolved cited work.

How probable is the Lyman-$\alpha$ damping wing in the spectrum of the redshift z = 5.9896 quasar ULAS J0148+0600? Unresolved cited work

Reference 51

Resolution: unresolved; no resolver link, observed 2026-08-09T06:06:09.995959Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation bf4c622a-ba2f-45bc-9843-096cb8c84c3c · outbound

This paper cites an unresolved cited work.

How probable is the Lyman-$\alpha$ damping wing in the spectrum of the redshift z = 5.9896 quasar ULAS J0148+0600? Unresolved cited work

Reference 52

Resolution: unresolved; no resolver link, observed 2026-08-09T06:06:09.999992Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 360c4004-d444-48e7-b736-9ad119417cd1 · outbound

This paper cites F., Faucher-Gigu \`e re C.-A., Alexander D.

How probable is the Lyman-$\alpha$ damping wing in the spectrum of the redshift z = 5.9896 quasar ULAS J0148+0600? F., Faucher-Gigu \`e re C.-A., Alexander D

Reference 53

Resolution: unresolved; no resolver link, observed 2026-08-09T06:06:10.003613Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a3442d78-0087-486a-b511-8ba5997c4f34 · outbound

This paper cites an unresolved cited work.

How probable is the Lyman-$\alpha$ damping wing in the spectrum of the redshift z = 5.9896 quasar ULAS J0148+0600? Unresolved cited work

Reference 54

Resolution: unresolved; no resolver link, observed 2026-08-09T06:06:10.007173Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 5369c764-75c8-49d1-9a99-7c07e5cc1431 · outbound

This paper cites an unresolved cited work.

How probable is the Lyman-$\alpha$ damping wing in the spectrum of the redshift z = 5.9896 quasar ULAS J0148+0600? Unresolved cited work

Reference 55

Resolution: unresolved; no resolver link, observed 2026-08-09T06:06:10.010637Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ff466efa-eec1-4259-a6bb-1fa0b78af214 · outbound

This paper cites an unresolved cited work.

How probable is the Lyman-$\alpha$ damping wing in the spectrum of the redshift z = 5.9896 quasar ULAS J0148+0600? Unresolved cited work

Reference 56

Resolution: unresolved; no resolver link, observed 2026-08-09T06:06:10.014026Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 4fec1242-5319-4148-87e3-65e2a64f8bfd · outbound

This paper cites an unresolved cited work.

How probable is the Lyman-$\alpha$ damping wing in the spectrum of the redshift z = 5.9896 quasar ULAS J0148+0600? Unresolved cited work

Reference 57

Resolution: unresolved; no resolver link, observed 2026-08-09T06:06:10.017603Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation dda1e75f-74d5-4eae-bdfd-ebb03052b1a9 · outbound

This paper cites an unresolved cited work.

How probable is the Lyman-$\alpha$ damping wing in the spectrum of the redshift z = 5.9896 quasar ULAS J0148+0600? Unresolved cited work

Reference 58

Resolution: unresolved; no resolver link, observed 2026-08-09T06:06:10.021089Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 82d12c32-76a2-4b92-9b96-dc1eae354337 · outbound

This paper cites D., Ni Y., Croft R.

How probable is the Lyman-$\alpha$ damping wing in the spectrum of the redshift z = 5.9896 quasar ULAS J0148+0600? D., Ni Y., Croft R

Reference 59

Resolution: verified exact; doi, observed 2026-08-09T06:06:10.129117Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

Observation d386a973-6b85-4957-a83d-f66f42d4e623 · outbound

This paper cites an unresolved cited work.

How probable is the Lyman-$\alpha$ damping wing in the spectrum of the redshift z = 5.9896 quasar ULAS J0148+0600? Unresolved cited work

Reference 60

Resolution: unresolved; no resolver link, observed 2026-08-09T06:06:10.028385Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a33865c1-c82b-412d-a265-f39e6e7fde78 · outbound

This paper cites an unresolved cited work.

How probable is the Lyman-$\alpha$ damping wing in the spectrum of the redshift z = 5.9896 quasar ULAS J0148+0600? Unresolved cited work

Reference 61

Resolution: unresolved; no resolver link, observed 2026-08-09T06:06:10.032221Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 6ed7faf9-03bd-4ea7-a46b-e1587c3b9121 · outbound

This paper cites an unresolved cited work.

How probable is the Lyman-$\alpha$ damping wing in the spectrum of the redshift z = 5.9896 quasar ULAS J0148+0600? Unresolved cited work

Reference 62

Resolution: unresolved; no resolver link, observed 2026-08-09T06:06:10.035806Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ad4976dd-35f0-4114-8689-56716443e48e · outbound

This paper cites an unresolved cited work.

How probable is the Lyman-$\alpha$ damping wing in the spectrum of the redshift z = 5.9896 quasar ULAS J0148+0600? Unresolved cited work

Reference 63

Resolution: unresolved; no resolver link, observed 2026-08-09T06:06:10.039224Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c265dee6-435d-46c2-9330-4f531ad09f3f · outbound

This paper cites an unresolved cited work.

How probable is the Lyman-$\alpha$ damping wing in the spectrum of the redshift z = 5.9896 quasar ULAS J0148+0600? Unresolved cited work

Reference 64

Resolution: unresolved; no resolver link, observed 2026-08-09T06:06:10.042674Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a07e5023-43be-41ea-a054-72d3ff9f33c9 · outbound

This paper cites S., Molaro M., Hatch N., Haehnelt M.

How probable is the Lyman-$\alpha$ damping wing in the spectrum of the redshift z = 5.9896 quasar ULAS J0148+0600? S., Molaro M., Hatch N., Haehnelt M

Reference 65

Resolution: unresolved; no resolver link, observed 2026-08-09T06:06:10.045411Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation dc6f975c-e227-4513-a0df-cdac134ad776 · outbound

This paper cites P., Bolton J.

How probable is the Lyman-$\alpha$ damping wing in the spectrum of the redshift z = 5.9896 quasar ULAS J0148+0600? P., Bolton J

Reference 66

Resolution: unresolved; no resolver link, observed 2026-08-09T06:06:10.048380Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 528292d4-e933-4e0f-945f-9d67e7c0b580 · outbound

This paper cites write newline.

How probable is the Lyman-$\alpha$ damping wing in the spectrum of the redshift z = 5.9896 quasar ULAS J0148+0600? write newline

Reference 67

Resolution: unresolved; no resolver link, observed 2026-08-09T06:06:10.051422Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Pith citing papers

Observation a0850fc1-9ad6-4968-ad89-350812b0c509 · inbound

An extremely metal-poor Lyman $\alpha$ emitter candidate at $z=6$ revealed through absorption spectroscopy cites this paper.

An extremely metal-poor Lyman $\alpha$ emitter candidate at $z=6$ revealed through absorption spectroscopy How probable is the Lyman-$\alpha$ damping wing in the spectrum of the redshift z = 5.9896 quasar ULAS J0148+0600?

Reference 67

Resolution: unresolved; no resolver link, observed 2026-08-16T04:22:25.668338Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 9f433ba0-5e2e-4c49-b5a8-fa393438218c · inbound

The Lyman-$\alpha$ emitter bispectrum as a probe of reionization morphology cites this paper.

The Lyman-$\alpha$ emitter bispectrum as a probe of reionization morphology How probable is the Lyman-$\alpha$ damping wing in the spectrum of the redshift z = 5.9896 quasar ULAS J0148+0600?

Reference 123

Resolution: verified exact; local_arxiv, observed 2026-08-07T14:55:49.637147Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.