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Paper Citation Record · LEDGER

MUSEQuBES: Connecting HI absorption with Ly$\alpha$ emitters at $z \approx 3.3$

As of 20 August 2026, this Paper Citation Record lists 93 of 93 outbound references and 4 inbound Pith citation observations for arXiv:2411.11959.

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

pith.paper-citation-record.v1
2411.11959 v2

Coverage vector

measured 93 of 93 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links, observed 2026-08-12T18:15:24.727693Z

measured 97 of 97 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-20T06:33:59.587034+00:00

measured 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-11T21:31:36.828726Z

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

93 of 93 outbound references displayed

  • verified exact8
  • verified fuzzy0
  • unresolved85
  • parse uncertain0
  • malformed identifier0
  • metadata mismatch0

External citation measurements

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

Outbound references

Observation 7624147c-6db3-4353-94a5-cf05872d8903 · outbound

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

MUSEQuBES: Connecting HI absorption with Ly$\alpha$ emitters at $z \approx 3.3$ , " * write output.state after.block = add.period write newline

Reference 1

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source=arxiv_source observed=2026-08-12T18:15:24.083083Z digest=sha256:ca27423ffe16bbbe17c11e6bc63ca460489988e71a76eb505765894a7eecc261

Observation de0108de-c9aa-42ea-9c01-f087cddf9bc2 · outbound

This paper cites write newline.

MUSEQuBES: Connecting HI absorption with Ly$\alpha$ emitters at $z \approx 3.3$ write newline

Reference 2

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source=arxiv_source observed=2026-08-12T18:15:24.090262Z digest=sha256:0389454d486056cbe059238dfe3a0bd81d49c00a40d4bedf27d9de1977c8c1f2

Observation dec337f0-7b07-407b-923d-0a351fc991db · outbound

This paper cites PeF> 9T 6Gnd 1W9A> 9T 6Gkh. |s.l Kq!.

MUSEQuBES: Connecting HI absorption with Ly$\alpha$ emitters at $z \approx 3.3$ PeF> 9T 6Gnd 1W9A> 9T 6Gkh. |s.l Kq!

Reference 3

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source=arxiv_source observed=2026-08-12T18:15:24.098515Z digest=sha256:987865317465b3ad1faed023d9bc99d0825c74fd9eb2a1b8cd1dafaeca9cd68c

Observation 2ed84b04-9c5b-4fb5-9360-00ab5bf60219 · outbound

This paper cites L., Shapley A.

MUSEQuBES: Connecting HI absorption with Ly$\alpha$ emitters at $z \approx 3.3$ L., Shapley A

Reference 4

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source=arxiv_source observed=2026-08-12T18:15:24.137054Z digest=sha256:ebf7b05d2bcf5ded0d785d64f4e5f70691669b8a54e529a95d8735eaffb32e30

Observation 2f70a854-93fd-4adf-94ca-b4cce0f6b096 · outbound

This paper cites an unresolved cited work.

MUSEQuBES: Connecting HI absorption with Ly$\alpha$ emitters at $z \approx 3.3$ Unresolved cited work

Reference 5

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source=arxiv_source observed=2026-08-12T18:15:24.142555Z digest=sha256:95e1c01e8c5822db74a304c980e63a6f9a73003199e06da7fb494e2ad1d57b43

Observation 51fd4418-7d3b-4175-9157-7d566ee6ec21 · outbound

This paper cites F., Prochaska J.

MUSEQuBES: Connecting HI absorption with Ly$\alpha$ emitters at $z \approx 3.3$ F., Prochaska J

Reference 6

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source=arxiv_source observed=2026-08-12T18:15:24.148011Z digest=sha256:b0bda75393eb2c0087dc2b3090abe05753c67268cab78ac1d651bc9b631ec2fd

Observation b0bd7c13-34d5-458e-9c76-8c3fa884df61 · outbound

This paper cites an unresolved cited work.

MUSEQuBES: Connecting HI absorption with Ly$\alpha$ emitters at $z \approx 3.3$ Unresolved cited work

Reference 7

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source=arxiv_source observed=2026-08-12T18:15:24.154697Z digest=sha256:d868a8a6652637bf98c58b3f58c1fb6856a3bc90ab186ab4112d1b01a997815f

Observation 8b61b18c-1519-49bb-988d-cf467b8fe0dc · outbound

This paper cites an unresolved cited work.

MUSEQuBES: Connecting HI absorption with Ly$\alpha$ emitters at $z \approx 3.3$ Unresolved cited work

Reference 8

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source=arxiv_source observed=2026-08-12T18:15:24.160845Z digest=sha256:e76278edf743e0c46cc546f7f325c04b2e8349d3743c830b66381313968bb2c0

Observation 0d2f5b81-bca6-4629-b482-eb402a519714 · outbound

This paper cites The MUSE second-generation VLT instrument.

MUSEQuBES: Connecting HI absorption with Ly$\alpha$ emitters at $z \approx 3.3$ The MUSE second-generation VLT instrument

Reference 9

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source=arxiv_source observed=2026-08-12T18:15:24.167385Z digest=sha256:419a1bb262740da924cc30e18dfee6dd1aca0813fcc310b73babf8621bce329b

Observation a34ecbd6-5682-4226-8488-49d07a1a501e · outbound

This paper cites an unresolved cited work.

MUSEQuBES: Connecting HI absorption with Ly$\alpha$ emitters at $z \approx 3.3$ Unresolved cited work

Reference 10

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source=arxiv_source observed=2026-08-12T18:15:24.173741Z digest=sha256:d955534f88a32c4d5077a5128aa9cbed0c7b6a7fc1d1b346b247c4419b1cecf7

Observation 929ec0e4-4ce1-4a46-9add-6d24c51d5c56 · outbound

This paper cites D., Cantalupo S., 2023, @doi [ ] 10.1093/mnras/stad2022 , https://ui.adsabs.harvard.edu/abs/2023MNRAS.524.5148B 524, 5148.

MUSEQuBES: Connecting HI absorption with Ly$\alpha$ emitters at $z \approx 3.3$ D., Cantalupo S., 2023, @doi [ ] 10.1093/mnras/stad2022 , https://ui.adsabs.harvard.edu/abs/2023MNRAS.524.5148B 524, 5148

Reference 11

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source=arxiv_source observed=2026-08-12T18:15:24.178923Z digest=sha256:dc19a9c70ab0f656d3b8b120ec5d7ec36b0bf1b9e708b01fe3cb48922b0d1c0a

Observation 92c1c9cb-b822-43f5-94cf-a41e7ad02924 · outbound

This paper cites D., Bolton J.

MUSEQuBES: Connecting HI absorption with Ly$\alpha$ emitters at $z \approx 3.3$ D., Bolton J

Reference 12

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no resolver link, observed 2026-08-12T18:15:24.185208Z

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source=arxiv_source observed=2026-08-12T18:15:24.185208Z digest=sha256:0f8836be92c6a59000a5d8c4679d3e67f15b7d921f0a05fbc69cd189843f7313

Observation f4bc9d58-2f15-45ef-8deb-b86cfa419508 · outbound

This paper cites H., Hearin A.

MUSEQuBES: Connecting HI absorption with Ly$\alpha$ emitters at $z \approx 3.3$ H., Hearin A

Reference 13

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source=arxiv_source observed=2026-08-12T18:15:24.190283Z digest=sha256:c8a485be1c6fa2f4eb1bf6f812ef21d8827608743f989f0d96fca8b4cb94b0ed

Observation d12bbde7-3e17-45c6-a871-201f0324b592 · outbound

This paper cites an unresolved cited work.

MUSEQuBES: Connecting HI absorption with Ly$\alpha$ emitters at $z \approx 3.3$ Unresolved cited work

Reference 14

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source=arxiv_source observed=2026-08-12T18:15:24.195504Z digest=sha256:02fa2ca0067ba5846e773b168671e31c92618133f7abf3958dd9e5bbc23f41ee

Observation 9d9aa632-303c-454d-95d7-2471480e268a · outbound

This paper cites J., et al., 2014, @doi [ ] 10.1088/0004-637X/793/2/115 , https://ui.adsabs.harvard.edu/abs/2014ApJ...793..115B 793, 115.

MUSEQuBES: Connecting HI absorption with Ly$\alpha$ emitters at $z \approx 3.3$ J., et al., 2014, @doi [ ] 10.1088/0004-637X/793/2/115 , https://ui.adsabs.harvard.edu/abs/2014ApJ...793..115B 793, 115

Reference 15

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source=arxiv_source observed=2026-08-12T18:15:24.200619Z digest=sha256:715af709e194448e533de366828a5f76522b1684970ec1fde3608e8d849a6860

Observation 7939f697-5b6a-4502-a3e2-62040c9b474d · outbound

This paper cites X., Hennawi J.

MUSEQuBES: Connecting HI absorption with Ly$\alpha$ emitters at $z \approx 3.3$ X., Hennawi J

Reference 16

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source=arxiv_source observed=2026-08-12T18:15:24.206167Z digest=sha256:49fece583b3fb79fc0a41aa37f4d6c7ec9a1735c569f1b840819359ebffd228c

Observation 0e65f29d-572a-4651-a39d-d0442a26181a · outbound

This paper cites F., Webb J.

MUSEQuBES: Connecting HI absorption with Ly$\alpha$ emitters at $z \approx 3.3$ F., Webb J

Reference 17

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source=arxiv_source observed=2026-08-12T18:15:24.213550Z digest=sha256:1df838218d3cc707bf36a30ec584c692f7d6950d394c2f064b5e773da376ac47

Observation 4f67653e-7447-4ec7-aa56-758ab3efc268 · outbound

This paper cites an unresolved cited work.

MUSEQuBES: Connecting HI absorption with Ly$\alpha$ emitters at $z \approx 3.3$ Unresolved cited work

Reference 18

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source=arxiv_source observed=2026-08-12T18:15:24.219267Z digest=sha256:7b013e12212e01e33a65ceb853a5c426015797ebb9f5764a9991cf23a17578ab

Observation a1747eb9-f7b3-4a68-9e12-0e5a39e41a86 · outbound

This paper cites M., Webb J.

MUSEQuBES: Connecting HI absorption with Ly$\alpha$ emitters at $z \approx 3.3$ M., Webb J

Reference 19

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source=arxiv_source observed=2026-08-12T18:15:24.225771Z digest=sha256:f900093d736631ce41e90cace5fbd9c437b1d5a4eb4509516c75881ec7f387a4

Observation c3ab89b9-29fc-4acd-8759-10ca8142ea4a · outbound

This paper cites M., Webb J.

MUSEQuBES: Connecting HI absorption with Ly$\alpha$ emitters at $z \approx 3.3$ M., Webb J

Reference 20

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source=arxiv_source observed=2026-08-12T18:15:24.232579Z digest=sha256:4ef35503b9c1c1aad7c77a207f796fef57dc5d1094ff2af17d118e7ac7712b7b

Observation b3b85d35-3e54-4fd9-a3e5-3d72d3020f53 · outbound

This paper cites an unresolved cited work.

MUSEQuBES: Connecting HI absorption with Ly$\alpha$ emitters at $z \approx 3.3$ Unresolved cited work

Reference 21

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source=arxiv_source observed=2026-08-12T18:15:24.239175Z digest=sha256:d9adb5ba84596099ff04a05861f9989e0c04155c475dea9fbc30b54e49db8cd0

Observation 9a6b8f96-f9bc-4efc-ad39-a315bb04e1b9 · outbound

This paper cites M., 2015, @doi [ ] 10.1088/2041-8205/812/2/L27 , https://ui.adsabs.harvard.edu/abs/2015ApJ...812L..27C 812, L27.

MUSEQuBES: Connecting HI absorption with Ly$\alpha$ emitters at $z \approx 3.3$ M., 2015, @doi [ ] 10.1088/2041-8205/812/2/L27 , https://ui.adsabs.harvard.edu/abs/2015ApJ...812L..27C 812, L27

Reference 22

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source=arxiv_source observed=2026-08-12T18:15:24.244806Z digest=sha256:cc2dcbbe1b5d7488a684c65d508624df1a838dae80bb855019f69dc485e1ee41

Observation 07dbb6e6-62b7-40ee-8196-0a7dbb2e079f · outbound

This paper cites W., Stocke J.

MUSEQuBES: Connecting HI absorption with Ly$\alpha$ emitters at $z \approx 3.3$ W., Stocke J

Reference 24

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source=arxiv_source observed=2026-08-12T18:15:24.255371Z digest=sha256:cba3401e3056ea3b3405058b765dadd2528fe0543332663a521575db3893887d

Observation 7800d042-be93-4eb8-99b1-ea85e41d40b2 · outbound

This paper cites H., 1999, @doi [ ] 10.1086/306722 , https://ui.adsabs.harvard.edu/abs/1999ApJ...511..521D 511, 521.

MUSEQuBES: Connecting HI absorption with Ly$\alpha$ emitters at $z \approx 3.3$ H., 1999, @doi [ ] 10.1086/306722 , https://ui.adsabs.harvard.edu/abs/1999ApJ...511..521D 511, 521

Reference 25

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source=arxiv_source observed=2026-08-12T18:15:24.261081Z digest=sha256:5635511447f3afc8b20e9b31d7e2f2cb199d98e5452aea435b1c9a329edd65ca

Observation 78e387c6-eee5-4c54-865c-f6c0293005ed · outbound

This paper cites an unresolved cited work.

MUSEQuBES: Connecting HI absorption with Ly$\alpha$ emitters at $z \approx 3.3$ Unresolved cited work

Reference 26

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source=arxiv_source observed=2026-08-12T18:15:24.267273Z digest=sha256:5a778df8f32541b03a53cbd16ddaca99c118f8de1178d88eb82229d2cd869367

Observation 2040c565-34e5-4606-8e8c-7096a4356ba4 · outbound

This paper cites an unresolved cited work.

MUSEQuBES: Connecting HI absorption with Ly$\alpha$ emitters at $z \approx 3.3$ Unresolved cited work

Reference 27

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source=arxiv_source observed=2026-08-12T18:15:24.272429Z digest=sha256:3fff661b7cc866a7aa90f6f57175b1e55baa421382353e99db0f98740a0605ba

Observation 63926b28-1149-4637-937f-0c9cf80c4fb8 · outbound

This paper cites K., Steidel C.

MUSEQuBES: Connecting HI absorption with Ly$\alpha$ emitters at $z \approx 3.3$ K., Steidel C

Reference 28

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source=arxiv_source observed=2026-08-12T18:15:24.278849Z digest=sha256:87bc8ed4bdf385c163bc437c09f4b9bfdb9d796e24838f1a273febe6dc1696a4

Observation e9f81879-3fc1-41d9-afd9-b341b6637899 · outbound

This paper cites an unresolved cited work.

MUSEQuBES: Connecting HI absorption with Ly$\alpha$ emitters at $z \approx 3.3$ Unresolved cited work

Reference 29

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source=arxiv_source observed=2026-08-12T18:15:24.286160Z digest=sha256:3173c558b6ed9813810e1b40e65024ed925dd45b03258bbe38a055df6f848e61

Observation 6f214026-71d1-4b2b-ace6-90c7c2397cf0 · outbound

This paper cites an unresolved cited work.

MUSEQuBES: Connecting HI absorption with Ly$\alpha$ emitters at $z \approx 3.3$ Unresolved cited work

Reference 30

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source=arxiv_source observed=2026-08-12T18:15:24.291693Z digest=sha256:9491b4907d453adb4269f8d55072cec3906426043c8325210abcf3b69ab6c491

Observation 064e0ca1-fa07-4458-bf0d-21b1861f65f4 · outbound

This paper cites an unresolved cited work.

MUSEQuBES: Connecting HI absorption with Ly$\alpha$ emitters at $z \approx 3.3$ Unresolved cited work

Reference 31

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source=arxiv_source observed=2026-08-12T18:15:24.297699Z digest=sha256:d5a173540d13e7a30db5a61f8337ee2e9829d3a31388571beb318bdb6839d5e2

Observation ac1f8660-a438-49a7-9703-c002bed828b1 · outbound

This paper cites an unresolved cited work.

MUSEQuBES: Connecting HI absorption with Ly$\alpha$ emitters at $z \approx 3.3$ Unresolved cited work

Reference 32

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source=arxiv_source observed=2026-08-12T18:15:24.303750Z digest=sha256:2aad8c20904e3484071db4aa77eeccd25ef5798dd672e7532c3f3d47b68323a2

Observation a61cf2f5-cad3-4df4-88ff-a750266362f4 · outbound

This paper cites R., et al., 2020, @doi [ ] 10.1038/s41586-020-2649-2 , https://ui.adsabs.harvard.edu/abs/2020Natur.585..357H 585, 357.

MUSEQuBES: Connecting HI absorption with Ly$\alpha$ emitters at $z \approx 3.3$ R., et al., 2020, @doi [ ] 10.1038/s41586-020-2649-2 , https://ui.adsabs.harvard.edu/abs/2020Natur.585..357H 585, 357

Reference 33

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source=arxiv_source observed=2026-08-12T18:15:24.310776Z digest=sha256:31e0a8c10b081a2c7f69ef49fb1be04e05cdcc61189f29ba704e236526534519

Observation c44c4325-b38b-4724-90d8-e7ae2f06d7c3 · outbound

This paper cites H., 1998, @doi [ ] 10.1086/305622 , https://ui.adsabs.harvard.edu/abs/1998ApJ...499..172H 499, 172.

MUSEQuBES: Connecting HI absorption with Ly$\alpha$ emitters at $z \approx 3.3$ H., 1998, @doi [ ] 10.1086/305622 , https://ui.adsabs.harvard.edu/abs/1998ApJ...499..172H 499, 172

Reference 34

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source=arxiv_source observed=2026-08-12T18:15:24.317114Z digest=sha256:6340ae5934b614b530a065d23a1d5739a8ac8be282c0d00198904d70ea53f549

Observation 5ecf3b07-a4a2-4b43-9592-782748741bd8 · outbound

This paper cites an unresolved cited work.

MUSEQuBES: Connecting HI absorption with Ly$\alpha$ emitters at $z \approx 3.3$ Unresolved cited work

Reference 35

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source=arxiv_source observed=2026-08-12T18:15:24.323730Z digest=sha256:c7606a7772801e02ac9cfa0c2a049ac4c53540e4f904c6982605d1f807bec63d

Observation e6cd66f7-abbe-4ef3-bdad-a11ec90a54c4 · outbound

This paper cites D., 2007, @doi [Computing in Science and Engineering] 10.1109/MCSE.2007.55 , https://ui.adsabs.harvard.edu/abs/2007CSE.....9...90H 9, 90.

MUSEQuBES: Connecting HI absorption with Ly$\alpha$ emitters at $z \approx 3.3$ D., 2007, @doi [Computing in Science and Engineering] 10.1109/MCSE.2007.55 , https://ui.adsabs.harvard.edu/abs/2007CSE.....9...90H 9, 90

Reference 36

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source=arxiv_source observed=2026-08-12T18:15:24.329948Z digest=sha256:9debdab8bfa84ca5596edd11f2e7b72e8ed9f6a132d85b496cc898ba1e9346c4

Observation 3b61da6c-82d0-452e-9a5f-c7e2d48a32fb · outbound

This paper cites D., Chen H.-W., Mulchaey J.

MUSEQuBES: Connecting HI absorption with Ly$\alpha$ emitters at $z \approx 3.3$ D., Chen H.-W., Mulchaey J

Reference 37

Resolution
unresolved
no resolver link, observed 2026-08-12T18:15:24.337387Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-12T18:15:24.337387Z digest=sha256:5d03594bf19a501095e9bbda12976a08cefb5e86e21967427c3738e79ca7eff9

Observation 2c6cc850-0163-4f9f-9666-58546359468c · outbound

This paper cites Directly tracing cool filamentary accretion over >100 kpc into the interstellar medium of a quasar host at z=1.

MUSEQuBES: Connecting HI absorption with Ly$\alpha$ emitters at $z \approx 3.3$ Directly tracing cool filamentary accretion over >100 kpc into the interstellar medium of a quasar host at z=1

Reference 38

Resolution
unresolved
no resolver link, observed 2026-08-12T18:15:24.343272Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-12T18:15:24.343272Z digest=sha256:7191831f1887bed5e75a3e3bcdcc72d95b3688aee1b05d2c9caa0522ccb779b6

Observation ee343198-c859-484a-8d61-8297f9cba7b6 · outbound

This paper cites D., et al., 2024, @doi [ ] 10.3847/1538-4357/ad3911 , https://ui.adsabs.harvard.edu/abs/2024ApJ...966..218J 966, 218.

MUSEQuBES: Connecting HI absorption with Ly$\alpha$ emitters at $z \approx 3.3$ D., et al., 2024, @doi [ ] 10.3847/1538-4357/ad3911 , https://ui.adsabs.harvard.edu/abs/2024ApJ...966..218J 966, 218

Reference 39

Resolution
unresolved
no resolver link, observed 2026-08-12T18:15:24.349399Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-12T18:15:24.349399Z digest=sha256:1bbb3a6e61452753ab98b01fbcbd22fee445775bc5decb476d18bebe69184a74

Observation aaeff0d5-f289-4fd0-ae93-7335464df200 · outbound

This paper cites J., 1998, @doi [ ] 10.1146/annurev.astro.36.1.189 , https://ui.adsabs.harvard.edu/abs/1998ARA&A..36..189K 36, 189.

MUSEQuBES: Connecting HI absorption with Ly$\alpha$ emitters at $z \approx 3.3$ J., 1998, @doi [ ] 10.1146/annurev.astro.36.1.189 , https://ui.adsabs.harvard.edu/abs/1998ARA&A..36..189K 36, 189

Reference 40

Resolution
unresolved
no resolver link, observed 2026-08-12T18:15:24.354798Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-12T18:15:24.354798Z digest=sha256:39361cb0784afce21614d2c970f5916b4b04d5fa3708f8783e792dcbab110a1f

Observation 4800cef0-72c5-4444-8b20-a80a3c839b94 · outbound

This paper cites H., Dav \'e R., 2005, @doi [ ] 10.1111/j.1365-2966.2005.09451.x , https://ui.adsabs.harvard.edu/abs/2005MNRAS.363....2K 363, 2.

MUSEQuBES: Connecting HI absorption with Ly$\alpha$ emitters at $z \approx 3.3$ H., Dav \'e R., 2005, @doi [ ] 10.1111/j.1365-2966.2005.09451.x , https://ui.adsabs.harvard.edu/abs/2005MNRAS.363....2K 363, 2

Reference 41

Resolution
unresolved
no resolver link, observed 2026-08-12T18:15:24.361682Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-12T18:15:24.361682Z digest=sha256:5ff44d67003bfc07ae922b66553f33e1e3bbcb619132c16dbe0fb56bc670362c

Observation e1e30658-5443-4f7c-a82e-cbfb9f199b16 · outbound

This paper cites an unresolved cited work.

MUSEQuBES: Connecting HI absorption with Ly$\alpha$ emitters at $z \approx 3.3$ Unresolved cited work

Reference 42

Resolution
unresolved
no resolver link, observed 2026-08-12T18:15:24.367286Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-12T18:15:24.367286Z digest=sha256:18b83f5e7b8960fe0705c9c53bcf44157d695e791396573a97fdcb3ac8faca0b

Observation 639b12f7-a9bc-4483-b5d2-5db622085654 · outbound

This paper cites K., M ller P., Fynbo J.

MUSEQuBES: Connecting HI absorption with Ly$\alpha$ emitters at $z \approx 3.3$ K., M ller P., Fynbo J

Reference 43

Resolution
unresolved
no resolver link, observed 2026-08-12T18:15:24.373465Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-12T18:15:24.373465Z digest=sha256:51414ece3d697556791f364b4c6b6fe61e43c5309c28163e3cbfea6df1625037

Observation a3d8dedb-5551-4555-90a6-17eec8943584 · outbound

This paper cites an unresolved cited work.

MUSEQuBES: Connecting HI absorption with Ly$\alpha$ emitters at $z \approx 3.3$ Unresolved cited work

Reference 44

Resolution
unresolved
no resolver link, observed 2026-08-12T18:15:24.381144Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-12T18:15:24.381144Z digest=sha256:f039012d1d5ed682b6ffa646ec8f26d95b02b3ae78ef522cbf966dd8a2fcfcb9

Observation c5338b8c-b9c2-496f-8937-94300ea05a9f · outbound

This paper cites an unresolved cited work.

MUSEQuBES: Connecting HI absorption with Ly$\alpha$ emitters at $z \approx 3.3$ Unresolved cited work

Reference 45

Resolution
unresolved
no resolver link, observed 2026-08-12T18:15:24.387082Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-12T18:15:24.387082Z digest=sha256:19cc7d5b8a5698bf784f76e2b64a4ceb1fb63d760f195032c00bdfa0077e85e5

Observation 7e86f2fd-9435-460c-8788-cbaf718468fd · outbound

This paper cites an unresolved cited work.

MUSEQuBES: Connecting HI absorption with Ly$\alpha$ emitters at $z \approx 3.3$ Unresolved cited work

Reference 46

Resolution
verified exact
doi, observed 2026-08-12T18:15:25.433332Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=arxiv_source observed=2026-08-12T18:15:24.393419Z digest=sha256:f13c7478eec24caa269d86ae8a48c0016d7ca18d77aaa875905b5369feeab1e0

Observation 56d7394d-f3d6-4287-bcab-4a6198ebf28a · outbound

This paper cites an unresolved cited work.

MUSEQuBES: Connecting HI absorption with Ly$\alpha$ emitters at $z \approx 3.3$ Unresolved cited work

Reference 47

Resolution
verified exact
doi, observed 2026-08-12T18:15:25.416194Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=arxiv_source observed=2026-08-12T18:15:24.399841Z digest=sha256:aaacc51e6aaa2b5f42bdfcf2e1441295a152d7f9bcec25743a970985fd1c2a0f

Observation 5caaa4e7-d8ea-4918-9fe6-0f883b9072d4 · outbound

This paper cites K., et al., 2023, @doi [ ] 10.1093/mnras/stac3089 , https://ui.adsabs.harvard.edu/abs/2023MNRAS.518..305L 518, 305.

MUSEQuBES: Connecting HI absorption with Ly$\alpha$ emitters at $z \approx 3.3$ K., et al., 2023, @doi [ ] 10.1093/mnras/stac3089 , https://ui.adsabs.harvard.edu/abs/2023MNRAS.518..305L 518, 305

Reference 48

Resolution
unresolved
no resolver link, observed 2026-08-12T18:15:24.405989Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-12T18:15:24.405989Z digest=sha256:1b99c2879d0fa3ee7f626d4382d252c8de847e02ecbbb3c623b849bec9602904

Observation 5fe1d0f7-81ca-4d81-8d3c-b9c7d3aa39e4 · outbound

This paper cites an unresolved cited work.

MUSEQuBES: Connecting HI absorption with Ly$\alpha$ emitters at $z \approx 3.3$ Unresolved cited work

Reference 49

Resolution
unresolved
no resolver link, observed 2026-08-12T18:15:24.414786Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-12T18:15:24.414786Z digest=sha256:ce6b25d6a339803576c5904ac25e01b5c4873d894a11a04548963473b1b2c6eb

Observation 72076276-3d84-4147-835a-65a2084890bb · outbound

This paper cites an unresolved cited work.

MUSEQuBES: Connecting HI absorption with Ly$\alpha$ emitters at $z \approx 3.3$ Unresolved cited work

Reference 50

Resolution
unresolved
no resolver link, observed 2026-08-12T18:15:24.421663Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-12T18:15:24.421663Z digest=sha256:ef39d4274d497d7100d3bbca65bec5176918b5c44f7dc0ab5e0821b04bc39a78

Observation 99f72c80-734b-4257-87b8-7a79c108a6a2 · outbound

This paper cites an unresolved cited work.

MUSEQuBES: Connecting HI absorption with Ly$\alpha$ emitters at $z \approx 3.3$ Unresolved cited work

Reference 51

Resolution
unresolved
no resolver link, observed 2026-08-12T18:15:24.427904Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-12T18:15:24.427904Z digest=sha256:2d33159981f1615b42f177af0d5581a38a83e1906a7c567841b1039007823d92

Observation 26c84a3a-1c46-402e-9512-84b1590fe0a3 · outbound

This paper cites an unresolved cited work.

MUSEQuBES: Connecting HI absorption with Ly$\alpha$ emitters at $z \approx 3.3$ Unresolved cited work

Reference 52

Resolution
unresolved
no resolver link, observed 2026-08-12T18:15:24.434046Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-12T18:15:24.434046Z digest=sha256:b3363639b5e445f7bf70e496998d453c3d0228b1ced98f130781164d9a2cc2a2

Observation 1d2d6c65-ff1a-40ef-ac99-c66a6b1d7047 · outbound

This paper cites an unresolved cited work.

MUSEQuBES: Connecting HI absorption with Ly$\alpha$ emitters at $z \approx 3.3$ Unresolved cited work

Reference 53

Resolution
unresolved
no resolver link, observed 2026-08-12T18:15:24.440166Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-12T18:15:24.440166Z digest=sha256:f763f10a183b4f4e01666111f6d69dcd52964c2a8dbc97e498a21788162ee29c

Observation 59b7b34c-4813-423a-a29c-b2857e95c9e6 · outbound

This paper cites P., Naab T., White S.

MUSEQuBES: Connecting HI absorption with Ly$\alpha$ emitters at $z \approx 3.3$ P., Naab T., White S

Reference 54

Resolution
unresolved
no resolver link, observed 2026-08-12T18:15:24.449922Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-12T18:15:24.449922Z digest=sha256:791dc720f2a624ea2f37b282ad8ce480c8e103d42ab420ceadd8cd3c5ff6a030

Observation 60b92bd9-a673-436b-a580-ab2aa2b46bf0 · outbound

This paper cites an unresolved cited work.

MUSEQuBES: Connecting HI absorption with Ly$\alpha$ emitters at $z \approx 3.3$ Unresolved cited work

Reference 55

Resolution
unresolved
no resolver link, observed 2026-08-12T18:15:24.457332Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-12T18:15:24.457332Z digest=sha256:25126ac2c813a7b621ede16a0d59a9cdc532e06ff998d48075d22ae1c532851d

Observation 7d555b21-93d9-4d3a-a7b6-637bf560c618 · outbound

This paper cites an unresolved cited work.

MUSEQuBES: Connecting HI absorption with Ly$\alpha$ emitters at $z \approx 3.3$ Unresolved cited work

Reference 56

Resolution
unresolved
no resolver link, observed 2026-08-12T18:15:24.465914Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-12T18:15:24.465914Z digest=sha256:cba5c39b8d3c2e3ae91a99a9dcc6f86dcdaec8c1ab116b541ef8ff07bba3d34b

Observation 81b187f3-c681-4cbd-b453-9d0fecc04305 · outbound

This paper cites M., Prochaska J.

MUSEQuBES: Connecting HI absorption with Ly$\alpha$ emitters at $z \approx 3.3$ M., Prochaska J

Reference 57

Resolution
unresolved
no resolver link, observed 2026-08-12T18:15:24.472909Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-12T18:15:24.472909Z digest=sha256:25304e39a6ee7f5520f110028fd330222c3f9abbffd084d88adf524f490894c5

Observation 4ecc890c-2c63-4ea4-a31e-32066798b732 · outbound

This paper cites X., Rafelski M., Carilli C.

MUSEQuBES: Connecting HI absorption with Ly$\alpha$ emitters at $z \approx 3.3$ X., Rafelski M., Carilli C

Reference 58

Resolution
unresolved
no resolver link, observed 2026-08-12T18:15:24.479355Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-12T18:15:24.479355Z digest=sha256:465db16965a45a56a63df942162256865fb9f3243a88690cf48910fbce467d1a

Observation f95f5d2d-7bc6-4dd0-b30f-0bb8be91b8e8 · outbound

This paper cites X., Rafelski M.

MUSEQuBES: Connecting HI absorption with Ly$\alpha$ emitters at $z \approx 3.3$ X., Rafelski M

Reference 59

Resolution
unresolved
no resolver link, observed 2026-08-12T18:15:24.484930Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-12T18:15:24.484930Z digest=sha256:751e266e23367108dc59e96e2145ab88f215b2235ce7020b2724429579fe81f1

Observation a883d47a-0c50-44fa-ac03-0a04b2f07949 · outbound

This paper cites an unresolved cited work.

MUSEQuBES: Connecting HI absorption with Ly$\alpha$ emitters at $z \approx 3.3$ Unresolved cited work

Reference 60

Resolution
unresolved
no resolver link, observed 2026-08-12T18:15:24.490663Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-12T18:15:24.490663Z digest=sha256:9927de76f4f0856594d9ad4e4c104b55e031c00244080a9d91e635581b41d54b

Observation e349240b-909d-4e09-ad8d-54fe36919f45 · outbound

This paper cites an unresolved cited work.

MUSEQuBES: Connecting HI absorption with Ly$\alpha$ emitters at $z \approx 3.3$ Unresolved cited work

Reference 61

Resolution
unresolved
no resolver link, observed 2026-08-12T18:15:24.495870Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-12T18:15:24.495870Z digest=sha256:159b2eee96d4a17227a723cbfabc66d8afab9e314d8bfdc6e0e2545c6fbd9931

Observation 7d99ae2c-68a7-49d4-aee0-bd7f29f07f41 · outbound

This paper cites an unresolved cited work.

MUSEQuBES: Connecting HI absorption with Ly$\alpha$ emitters at $z \approx 3.3$ Unresolved cited work

Reference 62

Resolution
unresolved
no resolver link, observed 2026-08-12T18:15:24.501808Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-12T18:15:24.501808Z digest=sha256:3a678adfc8bc0a07c6f4497990cd19f256adff0ac7930e1b1ca2acbca2195cd8

Observation 15d544c8-c437-493e-8be5-f8ef26aa8797 · outbound

This paper cites C., 2020, @doi [ ] 10.1146/annurev-astro-021820-120014 , https://ui.adsabs.harvard.edu/abs/2020ARA&A..58..363P 58, 363.

MUSEQuBES: Connecting HI absorption with Ly$\alpha$ emitters at $z \approx 3.3$ C., 2020, @doi [ ] 10.1146/annurev-astro-021820-120014 , https://ui.adsabs.harvard.edu/abs/2020ARA&A..58..363P 58, 363

Reference 63

Resolution
unresolved
no resolver link, observed 2026-08-12T18:15:24.508618Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-12T18:15:24.508618Z digest=sha256:e6d7d192425fb7fd0e5daa9416c7d0102c7256b0e6ba32bd311c50ed8b2a6bee

Observation 80a87cb6-6892-4b80-906e-f7e5ee6800cc · outbound

This paper cites X., Weiner B., Chen H.-W., Mulchaey J., Cooksey K., 2011, @doi [The Astrophysical Journal] 10.1088/0004-637x/740/2/91 , 740, 91.

MUSEQuBES: Connecting HI absorption with Ly$\alpha$ emitters at $z \approx 3.3$ X., Weiner B., Chen H.-W., Mulchaey J., Cooksey K., 2011, @doi [The Astrophysical Journal] 10.1088/0004-637x/740/2/91 , 740, 91

Reference 65

Resolution
unresolved
no resolver link, observed 2026-08-12T18:15:24.523658Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-12T18:15:24.523658Z digest=sha256:4b36f18a5c12adbb179acdbdee776aee04826f15d44a302774a1a5537c97883a

Observation 7c9041b7-51ff-437d-a9c1-d7a65d98637c · outbound

This paper cites X., O'Meara J.

MUSEQuBES: Connecting HI absorption with Ly$\alpha$ emitters at $z \approx 3.3$ X., O'Meara J

Reference 66

Resolution
unresolved
no resolver link, observed 2026-08-12T18:15:24.531318Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-12T18:15:24.531318Z digest=sha256:42bd6416b01bc4d364116232d5d430a0f4e7dbf64ad7f5b87f75bc16f32a8aeb

Observation 2afeb855-fa70-4e5c-9c9d-29c3f3b028fc · outbound

This paper cites an unresolved cited work.

MUSEQuBES: Connecting HI absorption with Ly$\alpha$ emitters at $z \approx 3.3$ Unresolved cited work

Reference 67

Resolution
verified exact
doi, observed 2026-08-12T18:15:25.163696Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=arxiv_source observed=2026-08-12T18:15:24.536482Z digest=sha256:7a15d4bac45023d4a2fe9ceea1d87de47c3b8123e2ae99b9731116e091d0f660

Observation 037fa01e-9bc1-46c1-812a-63e28f1314e6 · outbound

This paper cites an unresolved cited work.

MUSEQuBES: Connecting HI absorption with Ly$\alpha$ emitters at $z \approx 3.3$ Unresolved cited work

Reference 68

Resolution
verified exact
doi, observed 2026-08-12T18:15:25.146324Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=arxiv_source observed=2026-08-12T18:15:24.542235Z digest=sha256:1d07786bc24b70782cfd7b826edecac7b0de33d59974ebc67b5a1def61131db1

Observation 6a0ff52b-82ab-49e8-a1ce-660d0e487953 · outbound

This paper cites C., Rudie G.

MUSEQuBES: Connecting HI absorption with Ly$\alpha$ emitters at $z \approx 3.3$ C., Rudie G

Reference 70

Resolution
unresolved
no resolver link, observed 2026-08-12T18:15:24.552969Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-12T18:15:24.552969Z digest=sha256:412fcd6a9a331df376d104037948bd59540871c078bc7ade77fa041a987c7c08

Observation 410c7c0f-c4b1-4a2a-a95b-ca0b8880e542 · outbound

This paper cites an unresolved cited work.

MUSEQuBES: Connecting HI absorption with Ly$\alpha$ emitters at $z \approx 3.3$ Unresolved cited work

Reference 71

Resolution
unresolved
no resolver link, observed 2026-08-12T18:15:24.558605Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-12T18:15:24.558605Z digest=sha256:667eeecd054b11833761e6593fed870c22727ac82e415952d0746977c5100ad0

Observation 8ea739eb-5234-455e-8ddf-2bc55cac7d2e · outbound

This paper cites C., et al., 2012, @doi [The Astrophysical Journal] 10.1088/0004-637x/750/1/67 , 750, 67.

MUSEQuBES: Connecting HI absorption with Ly$\alpha$ emitters at $z \approx 3.3$ C., et al., 2012, @doi [The Astrophysical Journal] 10.1088/0004-637x/750/1/67 , 750, 67

Reference 72

Resolution
unresolved
no resolver link, observed 2026-08-12T18:15:24.565641Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-12T18:15:24.565641Z digest=sha256:38f0c37c620369b29603430ac1cfbb2be30417e6ae683c62517133d486f024c4

Observation 9638173d-81cc-40ae-9149-c05fe0c4991f · outbound

This paper cites C., Steidel C.

MUSEQuBES: Connecting HI absorption with Ly$\alpha$ emitters at $z \approx 3.3$ C., Steidel C

Reference 73

Resolution
unresolved
no resolver link, observed 2026-08-12T18:15:24.571295Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-12T18:15:24.571295Z digest=sha256:56285c9ed6ad46ac27b61fbacd6d9ac3a6d69eef319c508e425fc26845fd189f

Observation c848ec73-f57a-499b-8473-0a6cec406046 · outbound

This paper cites C., Steidel C.

MUSEQuBES: Connecting HI absorption with Ly$\alpha$ emitters at $z \approx 3.3$ C., Steidel C

Reference 74

Resolution
unresolved
no resolver link, observed 2026-08-12T18:15:24.576577Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-12T18:15:24.576577Z digest=sha256:9c71d304bedc74d5f91bc34f5c87eb84c8b961107cf879d4b6357f40dd31324d

Observation 814ab7c4-ea8e-47cb-ab92-e7d257ebfaf4 · outbound

This paper cites an unresolved cited work.

MUSEQuBES: Connecting HI absorption with Ly$\alpha$ emitters at $z \approx 3.3$ Unresolved cited work

Reference 75

Resolution
unresolved
no resolver link, observed 2026-08-12T18:15:24.582392Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-12T18:15:24.582392Z digest=sha256:f7327da66771c2994d24abfef7c612cb41ab9e176000d7f06bc504fb1361801b

Observation 144f1435-ac0a-4a3f-bedc-316ee79f7d1e · outbound

This paper cites an unresolved cited work.

MUSEQuBES: Connecting HI absorption with Ly$\alpha$ emitters at $z \approx 3.3$ Unresolved cited work

Reference 76

Resolution
unresolved
no resolver link, observed 2026-08-12T18:15:24.588850Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-12T18:15:24.588850Z digest=sha256:087b870788801dfdfa3d1858eefdb889f6a1e9f3fdd0f3d3cc1cf99d05c2ca6b

Observation c98caf4a-5bd1-4b2a-a83d-ad687712489b · outbound

This paper cites M., et al., 2000, @doi [ ] 10.1086/312781 , https://ui.adsabs.harvard.edu/abs/2000ApJ...538L..13S 538, L13.

MUSEQuBES: Connecting HI absorption with Ly$\alpha$ emitters at $z \approx 3.3$ M., et al., 2000, @doi [ ] 10.1086/312781 , https://ui.adsabs.harvard.edu/abs/2000ApJ...538L..13S 538, L13

Reference 77

Resolution
verified exact
doi, observed 2026-08-12T18:15:25.045000Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=arxiv_source observed=2026-08-12T18:15:24.595469Z digest=sha256:ad293ebf11d1ef8167726244c1838399e87cd50eb65f6fe718a2c5690792df71

Observation c232cecf-c8ae-45e7-b7c9-44411d8eae0c · outbound

This paper cites an unresolved cited work.

MUSEQuBES: Connecting HI absorption with Ly$\alpha$ emitters at $z \approx 3.3$ Unresolved cited work

Reference 78

Resolution
verified exact
doi, observed 2026-08-12T18:15:25.025785Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=arxiv_source observed=2026-08-12T18:15:24.601095Z digest=sha256:4f240c0ac24256e6299d7706f679f5d5a66f72d56246cfa295fdeb2a4c0d74ab

Observation 3a3f9c63-88d1-4ca9-a3f7-b21ed58ab626 · outbound

This paper cites C., Erb D.

MUSEQuBES: Connecting HI absorption with Ly$\alpha$ emitters at $z \approx 3.3$ C., Erb D

Reference 79

Resolution
unresolved
no resolver link, observed 2026-08-12T18:15:24.606952Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-12T18:15:24.606952Z digest=sha256:c03a2a61133175b2624d70dd292d1473233bbd21769e4cd75dc2866cef14a193

Observation 4928b8b6-9738-47d3-b097-743ab7425849 · outbound

This paper cites C., Bogosavljevi \'c M., Shapley A.

MUSEQuBES: Connecting HI absorption with Ly$\alpha$ emitters at $z \approx 3.3$ C., Bogosavljevi \'c M., Shapley A

Reference 80

Resolution
unresolved
no resolver link, observed 2026-08-12T18:15:24.615151Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-12T18:15:24.615151Z digest=sha256:9ad3992e8f3847511ded46c84692cef421c6ffe371b9822c96ffc9baf3969e1c

Observation 8375ce78-efde-4a24-afb8-9d37fe42a8f6 · outbound

This paper cites an unresolved cited work.

MUSEQuBES: Connecting HI absorption with Ly$\alpha$ emitters at $z \approx 3.3$ Unresolved cited work

Reference 81

Resolution
unresolved
no resolver link, observed 2026-08-12T18:15:24.622524Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-12T18:15:24.622524Z digest=sha256:1d4c34ed220199876e7b6f8b23ce1c9d0c6186d4b4e625542c388fccf5d232c7

Observation 06365e93-367b-4632-8221-857c563b7af8 · outbound

This paper cites F., Steidel C.

MUSEQuBES: Connecting HI absorption with Ly$\alpha$ emitters at $z \approx 3.3$ F., Steidel C

Reference 82

Resolution
unresolved
no resolver link, observed 2026-08-12T18:15:24.629380Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-12T18:15:24.629380Z digest=sha256:7e1675e556537704ffffb173dd094480940b8e9cc2603ba123bcb57f87846182

Observation 9d862001-9887-4602-9082-3624aaaccdb3 · outbound

This paper cites an unresolved cited work.

MUSEQuBES: Connecting HI absorption with Ly$\alpha$ emitters at $z \approx 3.3$ Unresolved cited work

Reference 83

Resolution
unresolved
no resolver link, observed 2026-08-12T18:15:24.635508Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-12T18:15:24.635508Z digest=sha256:9794d7835712e59075f6989276bbbab196f2e6598c0b85bb2bfb2f512d95d0d9

Observation a8bf6e15-30ca-4dca-b50d-2fa0736139f0 · outbound

This paper cites an unresolved cited work.

MUSEQuBES: Connecting HI absorption with Ly$\alpha$ emitters at $z \approx 3.3$ Unresolved cited work

Reference 84

Resolution
unresolved
no resolver link, observed 2026-08-12T18:15:24.641380Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-12T18:15:24.641380Z digest=sha256:59ae03b48bd6bc9a54b7e28c50a1bc5e7bbfca679607e4d313bf009974130326

Observation 6ba7a53c-5e35-4aaa-85a2-63dd6c5f22f0 · outbound

This paper cites L., Schaye J., Steidel C.

MUSEQuBES: Connecting HI absorption with Ly$\alpha$ emitters at $z \approx 3.3$ L., Schaye J., Steidel C

Reference 85

Resolution
unresolved
no resolver link, observed 2026-08-12T18:15:24.648174Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-12T18:15:24.648174Z digest=sha256:2feee9b2895fb0b510c6659075cef3dc585491536b6448479e9be81e42dc9144

Observation 230b37a8-9aed-446d-af63-94a52708ad2f · outbound

This paper cites an unresolved cited work.

MUSEQuBES: Connecting HI absorption with Ly$\alpha$ emitters at $z \approx 3.3$ Unresolved cited work

Reference 86

Resolution
unresolved
no resolver link, observed 2026-08-12T18:15:24.655217Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-12T18:15:24.655217Z digest=sha256:ddd0f43794385cdfede93f7d8728693f428589a1979cec768c3e2467ce4553d1

Observation f7d5ef5d-f535-4d81-99b0-1fb9c6beecc5 · outbound

This paper cites an unresolved cited work.

MUSEQuBES: Connecting HI absorption with Ly$\alpha$ emitters at $z \approx 3.3$ Unresolved cited work

Reference 87

Resolution
unresolved
no resolver link, observed 2026-08-12T18:15:24.660300Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-12T18:15:24.660300Z digest=sha256:5b0dde00e3ead934e94b63b5e30f432b54784e2f2a8b07e95991feb165b68daf

Observation 7a86099a-fd21-4427-9685-29b5be29df0e · outbound

This paper cites X., Guseva N., 2017, @doi [ ] 10.1051/0004-6361/201629264 , https://ui.adsabs.harvard.edu/abs/2017A&A...597A..13V 597, A13.

MUSEQuBES: Connecting HI absorption with Ly$\alpha$ emitters at $z \approx 3.3$ X., Guseva N., 2017, @doi [ ] 10.1051/0004-6361/201629264 , https://ui.adsabs.harvard.edu/abs/2017A&A...597A..13V 597, A13

Reference 88

Resolution
unresolved
no resolver link, observed 2026-08-12T18:15:24.667031Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-12T18:15:24.667031Z digest=sha256:c501c525336c21795f387f057f396fc96c6df7175eeee60c9641ff7f0c2759c9

Observation 09f1a6f2-fded-4e34-b882-2b2115dfa1a0 · outbound

This paper cites an unresolved cited work.

MUSEQuBES: Connecting HI absorption with Ly$\alpha$ emitters at $z \approx 3.3$ Unresolved cited work

Reference 89

Resolution
unresolved
no resolver link, observed 2026-08-12T18:15:24.673594Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-12T18:15:24.673594Z digest=sha256:08c8288352c88943e05634a64c31efd5cd5190a4e899cfa114f9869483c71895

Observation 7dfdd966-eaeb-4607-9d09-913207aa05a4 · outbound

This paper cites an unresolved cited work.

MUSEQuBES: Connecting HI absorption with Ly$\alpha$ emitters at $z \approx 3.3$ Unresolved cited work

Reference 90

Resolution
unresolved
no resolver link, observed 2026-08-12T18:15:24.680071Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-12T18:15:24.680071Z digest=sha256:8bd67f263a8e7255561a0808f2efb0f48b674f9c34ab0962142e949ba884b59e

Observation 9f3699a4-e671-4ce6-be80-1b751ba53037 · outbound

This paper cites P., Savage B.

MUSEQuBES: Connecting HI absorption with Ly$\alpha$ emitters at $z \approx 3.3$ P., Savage B

Reference 91

Resolution
verified exact
doi, observed 2026-08-12T18:15:24.850500Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=arxiv_source observed=2026-08-12T18:15:24.686511Z digest=sha256:8ae30ed457379fa762418cef54a68e3ca5f918cc4b1fae92dd9dcf343d9a574d

Observation d54081b5-ad7c-48e6-9144-275c9e222adf · outbound

This paper cites C., et al., 2021, @doi [ ] 10.3847/1538-4357/abea14 , https://ui.adsabs.harvard.edu/abs/2021ApJ...912....9W 912, 9.

MUSEQuBES: Connecting HI absorption with Ly$\alpha$ emitters at $z \approx 3.3$ C., et al., 2021, @doi [ ] 10.3847/1538-4357/abea14 , https://ui.adsabs.harvard.edu/abs/2021ApJ...912....9W 912, 9

Reference 92

Resolution
unresolved
no resolver link, observed 2026-08-12T18:15:24.694217Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-12T18:15:24.694217Z digest=sha256:240bb5000235b50cc3d1206c4f41c3610965af0a86add63dd442cda5bd96386d

Observation 6deb2b36-6ce9-47d1-9a32-a65c83e1ac80 · outbound

This paper cites an unresolved cited work.

MUSEQuBES: Connecting HI absorption with Ly$\alpha$ emitters at $z \approx 3.3$ Unresolved cited work

Reference 93

Resolution
verified exact
doi, observed 2026-08-12T18:15:24.805886Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=arxiv_source observed=2026-08-12T18:15:24.701595Z digest=sha256:d760025256580715bf3ea0cf9325060ed9913228b66727f2566fb4ca7e3f550e

Observation f07280d7-78ee-4269-a340-c9476ee4113e · outbound

This paper cites an unresolved cited work.

MUSEQuBES: Connecting HI absorption with Ly$\alpha$ emitters at $z \approx 3.3$ Unresolved cited work

Reference 94

Resolution
unresolved
no resolver link, observed 2026-08-12T18:15:24.708646Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-12T18:15:24.708646Z digest=sha256:de1582c1fc05b74b2d8e9ae304f2875496ff790ac2b89034e92b98551ec13875

Observation 1dc5f61d-5492-44dc-8a0d-8700e9d043d2 · outbound

This paper cites M., Frank S., 2013, @doi [ ] 10.1051/0004-6361/201321154 , https://ui.adsabs.harvard.edu/abs/2013A&A...556A.141Z 556, A141.

MUSEQuBES: Connecting HI absorption with Ly$\alpha$ emitters at $z \approx 3.3$ M., Frank S., 2013, @doi [ ] 10.1051/0004-6361/201321154 , https://ui.adsabs.harvard.edu/abs/2013A&A...556A.141Z 556, A141

Reference 95

Resolution
unresolved
no resolver link, observed 2026-08-12T18:15:24.714458Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-12T18:15:24.714458Z digest=sha256:e9dbf02078fa11537ec41060c9be262a8a3d16f38aeeba907f17b70703496222

Observation c0ee7a0f-d191-4b1f-ab26-e439c98e36ca · outbound

This paper cites M., Dalla Vecchia C., 2011b, @doi [ ] 10.1111/j.1365-2966.2011.18896.x , https://ui.adsabs.harvard.edu/abs/2011MNRAS.415.2782V 415, 2782.

MUSEQuBES: Connecting HI absorption with Ly$\alpha$ emitters at $z \approx 3.3$ M., Dalla Vecchia C., 2011b, @doi [ ] 10.1111/j.1365-2966.2011.18896.x , https://ui.adsabs.harvard.edu/abs/2011MNRAS.415.2782V 415, 2782

Reference 97

Resolution
unresolved
no resolver link, observed 2026-08-12T18:15:24.727693Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-12T18:15:24.727693Z digest=sha256:6530efdcbbf14de08b3ac63e72a1b629b5c5fd0260d0d31adce58b729e9e3c5d

Pith citing papers

Observation 1b3a882c-2439-4540-85fc-044a8a31f045 · inbound

MUSEQuBES: Unveiling Cosmic Web Filaments at $z\approx3.6$ through Dual Absorption and Emission Line Analysis cites this paper.

MUSEQuBES: Unveiling Cosmic Web Filaments at $z\approx3.6$ through Dual Absorption and Emission Line Analysis MUSEQuBES: Connecting HI absorption with Ly$\alpha$ emitters at $z \approx 3.3$

Reference 5

Resolution
unresolved
no resolver link, observed 2026-08-11T21:31:36.828726Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-11T21:31:36.828726Z digest=sha256:3a135f55a48b3cb2bec2378bdfe08a95e7a1177092904a23bb51d89e93000add

Observation 04314702-d872-4487-b819-2508da4d042b · inbound

The connection between high-redshift galaxies and Lyman ${\alpha}$ transmission in the Sherwood-Relics simulations of patchy reionisation cites this paper.

The connection between high-redshift galaxies and Lyman ${\alpha}$ transmission in the Sherwood-Relics simulations of patchy reionisation MUSEQuBES: Connecting HI absorption with Ly$\alpha$ emitters at $z \approx 3.3$

Reference 8

Resolution
unresolved
no resolver link, observed 2026-08-09T10:27:52.236184Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-09T10:27:52.236184Z digest=sha256:cb4f86e57971f44a46a8509206b9bcf8e498877f46c6c1f0e37f60d6a5f86088

Observation dd9dd484-ef0d-4517-873f-854eadd24c31 · inbound

The impact of source and survey modelling on the connection between [O III] emitters and Ly $\alpha$ forest transmission at z ~ 6 cites this paper.

The impact of source and survey modelling on the connection between [O III] emitters and Ly $\alpha$ forest transmission at z ~ 6 MUSEQuBES: Connecting HI absorption with Ly$\alpha$ emitters at $z \approx 3.3$

Reference 30

Resolution
verified exact
arxiv_id, observed 2026-06-28T08:31:48.288422Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=arxiv_source observed=2026-06-28T08:30:12.037696Z digest=sha256:8c661daf45d38c21d6547be2f447e4172c6259db46efafed5e79fc82f4735f9e

Observation 16bd547d-20b4-4f93-8702-9cd83aa5c14f · inbound

The 3D clustering of Lyman Alpha Emitters measured with DESI cites this paper.

The 3D clustering of Lyman Alpha Emitters measured with DESI MUSEQuBES: Connecting HI absorption with Ly$\alpha$ emitters at $z \approx 3.3$

Reference 54

Resolution
verified exact
arxiv_id, observed 2026-07-04T18:10:01.328688Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.

source=pdf_text observed=2026-06-25T23:02:45.609207Z digest=sha256:c5585d98514b0ff8588a063510ddfcd05f52e0367449e5dcf5597e736e7e3c66