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Paper Citation Record · LEDGER

The cosmic web's Lyman-$\alpha$ glow at $z \approx 2.5$; hydrodynamic models, dust, and wide-field, narrow-band detection

As of 8 August 2026, this Paper Citation Record lists 100 of 153 outbound references and 1 inbound Pith citation observation for arXiv:2510.07259.

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

pith.paper-citation-record.v1
2510.07259 v2

Coverage vector

measured 100 of 153 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links, observed 2026-08-04T11:03:36.212947Z

measured 101 of 101 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-08T06:32:00.761636+00:00

measured 1 of 1 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-02T19:24:52.522960Z

measured 0 of 1 external citation measurements

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

Source: cited_works

Reference resolution

100 of 153 outbound references displayed

  • verified exact16
  • verified fuzzy0
  • unresolved84
  • parse uncertain0
  • malformed identifier0
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External citation measurements

No source-named external measurement is stored.

Outbound references

Observation d0b2b308-6415-4c9a-9cf2-dd4841bf4a98 · outbound

This paper cites an unresolved cited work.

The cosmic web's Lyman-$\alpha$ glow at $z \approx 2.5$; hydrodynamic models, dust, and wide-field, narrow-band detection Unresolved cited work

Reference 1

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Unavailable: canonical work link unavailable.

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Observation ca823e1c-d06b-44c3-a202-c47fdcbd93c2 · outbound

This paper cites W., Darling D.

The cosmic web's Lyman-$\alpha$ glow at $z \approx 2.5$; hydrodynamic models, dust, and wide-field, narrow-band detection W., Darling D

Reference 2

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Observation e39f42f7-d14c-46e4-a247-e00c9213d01b · outbound

This paper cites & Astrophys.] 10.1051/0004-6361/202039887 , https://ui.adsabs.harvard.edu/abs/2021A&A...647A.107B 647, A107.

The cosmic web's Lyman-$\alpha$ glow at $z \approx 2.5$; hydrodynamic models, dust, and wide-field, narrow-band detection & Astrophys.] 10.1051/0004-6361/202039887 , https://ui.adsabs.harvard.edu/abs/2021A&A...647A.107B 647, A107

Reference 5

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Observation 646ec615-52ce-4993-9220-01a008d5d164 · outbound

This paper cites an unresolved cited work.

The cosmic web's Lyman-$\alpha$ glow at $z \approx 2.5$; hydrodynamic models, dust, and wide-field, narrow-band detection Unresolved cited work

Reference 6

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Observation dd8be199-7bc1-48e4-b123-73e8154085a7 · outbound

This paper cites an unresolved cited work.

The cosmic web's Lyman-$\alpha$ glow at $z \approx 2.5$; hydrodynamic models, dust, and wide-field, narrow-band detection Unresolved cited work

Reference 7

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source=arxiv_source observed=2026-08-04T11:03:26.699135Z digest=sha256:510afb7088d92324a1d666fd9f9f040b7f2754f51d0b3be7ed0e6b80e3633720

Observation b1ef762d-9e22-49b7-82c5-7490c43f548a · outbound

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

The cosmic web's Lyman-$\alpha$ glow at $z \approx 2.5$; hydrodynamic models, dust, and wide-field, narrow-band detection MUSEQuBES: Unveiling Cosmic Web Filaments at $z\approx3.6$ through Dual Absorption and Emission Line Analysis

Reference 8

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Observation ec164716-2a40-4a55-ad36-23cb68b108ec · outbound

This paper cites an unresolved cited work.

The cosmic web's Lyman-$\alpha$ glow at $z \approx 2.5$; hydrodynamic models, dust, and wide-field, narrow-band detection Unresolved cited work

Reference 9

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Observation 690df445-df66-44c6-93c0-89cb4f0db533 · outbound

This paper cites an unresolved cited work.

The cosmic web's Lyman-$\alpha$ glow at $z \approx 2.5$; hydrodynamic models, dust, and wide-field, narrow-band detection Unresolved cited work

Reference 10

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Observation ba177ce7-d41c-4ae9-9102-5079594d567e · outbound

This paper cites an unresolved cited work.

The cosmic web's Lyman-$\alpha$ glow at $z \approx 2.5$; hydrodynamic models, dust, and wide-field, narrow-band detection Unresolved cited work

Reference 11

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Observation e53b5532-3e7f-4c09-899d-6661aa24a7e8 · outbound

This paper cites Distinguish dark matter theories with the cosmic web and next-generation surveys I: an alternative theory of gravity.

The cosmic web's Lyman-$\alpha$ glow at $z \approx 2.5$; hydrodynamic models, dust, and wide-field, narrow-band detection Distinguish dark matter theories with the cosmic web and next-generation surveys I: an alternative theory of gravity

Reference 12

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Observation 09e034ae-e43c-43d6-9bf8-a4dd324568cb · outbound

This paper cites S., Puchwein E., Sijacki D., Haehnelt M.

The cosmic web's Lyman-$\alpha$ glow at $z \approx 2.5$; hydrodynamic models, dust, and wide-field, narrow-band detection S., Puchwein E., Sijacki D., Haehnelt M

Reference 13

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Observation d6511c2d-34c0-4d1b-b5af-55648865780f · outbound

This paper cites an unresolved cited work.

The cosmic web's Lyman-$\alpha$ glow at $z \approx 2.5$; hydrodynamic models, dust, and wide-field, narrow-band detection Unresolved cited work

Reference 14

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source=arxiv_source observed=2026-08-04T11:03:27.324670Z digest=sha256:3e8f8cd3c11e47c6aad2c903f380cd6bfbcd913b68f6dcd57a3a16670ef7daca

Observation 43b9637f-e0d2-491f-99c5-fea69df4ad24 · outbound

This paper cites R., Kofman L., Pogosyan D., 1996, @doi [Nature] 10.1038/380603a0 , https://ui.adsabs.harvard.edu/abs/1996Natur.380..603B 380, 603.

The cosmic web's Lyman-$\alpha$ glow at $z \approx 2.5$; hydrodynamic models, dust, and wide-field, narrow-band detection R., Kofman L., Pogosyan D., 1996, @doi [Nature] 10.1038/380603a0 , https://ui.adsabs.harvard.edu/abs/1996Natur.380..603B 380, 603

Reference 15

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Observation 8513229b-3090-4840-adb4-6edf289b4a25 · outbound

This paper cites an unresolved cited work.

The cosmic web's Lyman-$\alpha$ glow at $z \approx 2.5$; hydrodynamic models, dust, and wide-field, narrow-band detection Unresolved cited work

Reference 16

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Observation d3edb551-f62c-4f14-964e-d06254b087a9 · outbound

This paper cites N., Elek O., Tejos N., Prochaska J.

The cosmic web's Lyman-$\alpha$ glow at $z \approx 2.5$; hydrodynamic models, dust, and wide-field, narrow-band detection N., Elek O., Tejos N., Prochaska J

Reference 17

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verified exact
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No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

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Observation af1f2503-8d84-4386-aa9c-426109d91fea · outbound

This paper cites an unresolved cited work.

The cosmic web's Lyman-$\alpha$ glow at $z \approx 2.5$; hydrodynamic models, dust, and wide-field, narrow-band detection Unresolved cited work

Reference 18

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Observation 041c0ee2-0084-475f-9089-86fa70a948a5 · outbound

This paper cites an unresolved cited work.

The cosmic web's Lyman-$\alpha$ glow at $z \approx 2.5$; hydrodynamic models, dust, and wide-field, narrow-band detection Unresolved cited work

Reference 19

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Observation 301e5972-18bf-41a4-ad2b-0fae95b0deb8 · outbound

This paper cites an unresolved cited work.

The cosmic web's Lyman-$\alpha$ glow at $z \approx 2.5$; hydrodynamic models, dust, and wide-field, narrow-band detection Unresolved cited work

Reference 20

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Observation 6245abeb-027f-4730-b0fe-42409a8a9310 · outbound

This paper cites J., Miniati F., 2005, @doi [ApJ] 10.1086/430758 , https://ui.adsabs.harvard.edu/abs/2005ApJ...628...61C 628, 61.

The cosmic web's Lyman-$\alpha$ glow at $z \approx 2.5$; hydrodynamic models, dust, and wide-field, narrow-band detection J., Miniati F., 2005, @doi [ApJ] 10.1086/430758 , https://ui.adsabs.harvard.edu/abs/2005ApJ...628...61C 628, 61

Reference 21

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Observation 9db1e985-540d-4a94-93e2-6ffe090fd02f · outbound

This paper cites J., 2008, @doi [Astrophysical Journal] 10.1086/523298 , https://ui.adsabs.harvard.edu/abs/2008ApJ...672...48C 672, 48.

The cosmic web's Lyman-$\alpha$ glow at $z \approx 2.5$; hydrodynamic models, dust, and wide-field, narrow-band detection J., 2008, @doi [Astrophysical Journal] 10.1086/523298 , https://ui.adsabs.harvard.edu/abs/2008ApJ...672...48C 672, 48

Reference 22

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Observation 4ad9f080-9a08-4d1b-9504-b52997c51cc0 · outbound

This paper cites X., Hennawi J.

The cosmic web's Lyman-$\alpha$ glow at $z \approx 2.5$; hydrodynamic models, dust, and wide-field, narrow-band detection X., Hennawi J

Reference 23

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Observation d7459ef3-b37c-4d21-8ce8-0808368e5142 · outbound

This paper cites F., 2024, VPFIT homepage: https://people.ast.cam.ac.uk/ rfc/, https://people.ast.cam.ac.uk/ rfc/.

The cosmic web's Lyman-$\alpha$ glow at $z \approx 2.5$; hydrodynamic models, dust, and wide-field, narrow-band detection F., 2024, VPFIT homepage: https://people.ast.cam.ac.uk/ rfc/, https://people.ast.cam.ac.uk/ rfc/

Reference 24

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Observation 65dc3ea8-74d5-4b0a-a30e-c73f6a6ecb16 · outbound

This paper cites F., Webb J.

The cosmic web's Lyman-$\alpha$ glow at $z \approx 2.5$; hydrodynamic models, dust, and wide-field, narrow-band detection F., Webb J

Reference 25

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Observation 5a937983-6a0f-457e-a2ae-8021a5bbaa49 · outbound

This paper cites an unresolved cited work.

The cosmic web's Lyman-$\alpha$ glow at $z \approx 2.5$; hydrodynamic models, dust, and wide-field, narrow-band detection Unresolved cited work

Reference 26

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Observation 9b3cddf4-802a-4e1b-91fb-dd77fb4bacd1 · outbound

This paper cites G., 2018, @doi [MNRAS] 10.1093/mnras/sty992 , https://ui.adsabs.harvard.edu/abs/2018MNRAS.478.1065C 478, 1065.

The cosmic web's Lyman-$\alpha$ glow at $z \approx 2.5$; hydrodynamic models, dust, and wide-field, narrow-band detection G., 2018, @doi [MNRAS] 10.1093/mnras/sty992 , https://ui.adsabs.harvard.edu/abs/2018MNRAS.478.1065C 478, 1065

Reference 27

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Observation 2f9a80ee-0248-4014-8666-505e55353ad2 · outbound

This paper cites The Dragonfly Spectral Line Mapper: Completion of the 120-lens array.

The cosmic web's Lyman-$\alpha$ glow at $z \approx 2.5$; hydrodynamic models, dust, and wide-field, narrow-band detection The Dragonfly Spectral Line Mapper: Completion of the 120-lens array

Reference 28

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verified exact
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No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

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Observation fc7447fb-b432-4f96-b342-6e3352fe20d1 · outbound

This paper cites an unresolved cited work.

The cosmic web's Lyman-$\alpha$ glow at $z \approx 2.5$; hydrodynamic models, dust, and wide-field, narrow-band detection Unresolved cited work

Reference 29

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Observation 459554d5-2c88-4220-8816-787fcfa92461 · outbound

This paper cites an unresolved cited work.

The cosmic web's Lyman-$\alpha$ glow at $z \approx 2.5$; hydrodynamic models, dust, and wide-field, narrow-band detection Unresolved cited work

Reference 30

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Observation 11d82441-acbc-4390-b96b-238824e9d24c · outbound

This paper cites an unresolved cited work.

The cosmic web's Lyman-$\alpha$ glow at $z \approx 2.5$; hydrodynamic models, dust, and wide-field, narrow-band detection Unresolved cited work

Reference 31

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no resolver link, observed 2026-08-04T11:03:29.193338Z

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Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-04T11:03:29.193338Z digest=sha256:870e4ea51e762487447ea5b72b09a2abc12f7cc93e7c5a3a9df22ec5d3a0a0cc

Observation bea2330e-da08-4b52-93da-f2cc0a829a74 · outbound

This paper cites A gas-rich cosmic web revealed by the partitioning of the missing baryons.

The cosmic web's Lyman-$\alpha$ glow at $z \approx 2.5$; hydrodynamic models, dust, and wide-field, narrow-band detection A gas-rich cosmic web revealed by the partitioning of the missing baryons

Reference 32

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no resolver link, observed 2026-08-04T11:03:29.246669Z

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Observation 0371b3e9-dc1e-4502-bb2a-c6d8bf621e51 · outbound

This paper cites Science Cases for the Keck Wide-Field Imager.

The cosmic web's Lyman-$\alpha$ glow at $z \approx 2.5$; hydrodynamic models, dust, and wide-field, narrow-band detection Science Cases for the Keck Wide-Field Imager

Reference 33

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verified exact
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No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

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Observation 4d3a9476-e386-4f03-af1d-0ed053ff504b · outbound

This paper cites A., et al., 2015, @doi [MNRAS] 10.1093/mnras/stv725 , https://ui.adsabs.harvard.edu/abs/2015MNRAS.450.1937C 450, 1937.

The cosmic web's Lyman-$\alpha$ glow at $z \approx 2.5$; hydrodynamic models, dust, and wide-field, narrow-band detection A., et al., 2015, @doi [MNRAS] 10.1093/mnras/stv725 , https://ui.adsabs.harvard.edu/abs/2015MNRAS.450.1937C 450, 1937

Reference 34

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no resolver link, observed 2026-08-04T11:03:29.417846Z

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Observation 4ec6410c-b161-4ede-ad6a-f4df2a7d1345 · outbound

This paper cites A., et al., 2017, @doi [MNRAS] 10.1093/mnras/stw2586 , https://ui.adsabs.harvard.edu/abs/2017MNRAS.464.4204C 464, 4204.

The cosmic web's Lyman-$\alpha$ glow at $z \approx 2.5$; hydrodynamic models, dust, and wide-field, narrow-band detection A., et al., 2017, @doi [MNRAS] 10.1093/mnras/stw2586 , https://ui.adsabs.harvard.edu/abs/2017MNRAS.464.4204C 464, 4204

Reference 35

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source=arxiv_source observed=2026-08-04T11:03:29.503904Z digest=sha256:7494ce777f4a17453f9aaa00c644283a4af004e05d6818ca6777da623078de7e

Observation 052a387c-82b9-4f66-a09a-c2ea6ddba8bb · outbound

This paper cites & Astrophys.] 10.1051/0004-6361/201833655 , https://ui.adsabs.harvard.edu/abs/2018A&A...619A..49C 619, A49.

The cosmic web's Lyman-$\alpha$ glow at $z \approx 2.5$; hydrodynamic models, dust, and wide-field, narrow-band detection & Astrophys.] 10.1051/0004-6361/201833655 , https://ui.adsabs.harvard.edu/abs/2018A&A...619A..49C 619, A49

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no resolver link, observed 2026-08-04T11:03:29.635486Z

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source=arxiv_source observed=2026-08-04T11:03:29.635486Z digest=sha256:f5100e07ccb49ca3fe875537882d3aee714e72f7a062eafd52c25f6624066c1b

Observation 3a9e1a85-409b-4e64-a30d-b04991e0b850 · outbound

This paper cites H., Katz N., 1997, @doi [ ] 10.1086/303712 , https://ui.adsabs.harvard.edu/abs/1997ApJ...477...21D 477, 21.

The cosmic web's Lyman-$\alpha$ glow at $z \approx 2.5$; hydrodynamic models, dust, and wide-field, narrow-band detection H., Katz N., 1997, @doi [ ] 10.1086/303712 , https://ui.adsabs.harvard.edu/abs/1997ApJ...477...21D 477, 21

Reference 37

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no resolver link, observed 2026-08-04T11:03:29.835038Z

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source=arxiv_source observed=2026-08-04T11:03:29.835038Z digest=sha256:a3be0b8c01d6509c3a1f853e6994f54613cd227aa919dd46731bed9872255426

Observation c1602af9-bcde-4ebb-8d8a-77393a900bb0 · outbound

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

The cosmic web's Lyman-$\alpha$ glow at $z \approx 2.5$; hydrodynamic models, dust, and wide-field, narrow-band detection H., 1999, @doi [ ] 10.1086/306722 , https://ui.adsabs.harvard.edu/abs/1999ApJ...511..521D 511, 521

Reference 38

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unresolved
no resolver link, observed 2026-08-04T11:03:29.934748Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-04T11:03:29.934748Z digest=sha256:6765dd6600903ed9c41240be53acd4375464b3234c598bd81314210cf964558c

Observation 3dacce12-1bf3-4373-bd4e-8666ba8bee16 · outbound

This paper cites H., Appleby S., 2019, @doi [MNRAS] 10.1093/mnras/stz937 , https://ui.adsabs.harvard.edu/abs/2019MNRAS.486.2827D 486, 2827.

The cosmic web's Lyman-$\alpha$ glow at $z \approx 2.5$; hydrodynamic models, dust, and wide-field, narrow-band detection H., Appleby S., 2019, @doi [MNRAS] 10.1093/mnras/stz937 , https://ui.adsabs.harvard.edu/abs/2019MNRAS.486.2827D 486, 2827

Reference 39

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unresolved
no resolver link, observed 2026-08-04T11:03:30.031241Z

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source=arxiv_source observed=2026-08-04T11:03:30.031241Z digest=sha256:e8963e6ddc0af719c52027899c089436a4f161f9e531b2e616cc14e3932b230c

Observation e4cb44a5-0861-4327-9ab9-b6209cecdba6 · outbound

This paper cites S., White S.

The cosmic web's Lyman-$\alpha$ glow at $z \approx 2.5$; hydrodynamic models, dust, and wide-field, narrow-band detection S., White S

Reference 40

Resolution
unresolved
no resolver link, observed 2026-08-04T11:03:30.174747Z

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source=arxiv_source observed=2026-08-04T11:03:30.174747Z digest=sha256:0ecf15ffc88171d02066c8054b9537fb185d5d5ac04ba1784355653235a521f4

Observation 4dd681f7-aa09-4236-83f2-dedf7c7ac43d · outbound

This paper cites B., 2016, @doi [ ] 10.1051/0004-6361/201527895 , https://ui.adsabs.harvard.edu/abs/2016A&A...596A..97D 596, A97.

The cosmic web's Lyman-$\alpha$ glow at $z \approx 2.5$; hydrodynamic models, dust, and wide-field, narrow-band detection B., 2016, @doi [ ] 10.1051/0004-6361/201527895 , https://ui.adsabs.harvard.edu/abs/2016A&A...596A..97D 596, A97

Reference 41

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unresolved
no resolver link, observed 2026-08-04T11:03:30.302307Z

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source=arxiv_source observed=2026-08-04T11:03:30.302307Z digest=sha256:e2a541a588d0d660f7ac4d851413d4129d1b272036931997d60667eaa8d4f816

Observation 58ee0203-b678-4c85-b3cd-90c47fd0d2c9 · outbound

This paper cites an unresolved cited work.

The cosmic web's Lyman-$\alpha$ glow at $z \approx 2.5$; hydrodynamic models, dust, and wide-field, narrow-band detection Unresolved cited work

Reference 42

Resolution
unresolved
no resolver link, observed 2026-08-04T11:03:30.363881Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-04T11:03:30.363881Z digest=sha256:05071e2c7db7824a2c59b436234edca62efbeabbebaab77dbcb7f604d1348991

Observation 3b6d1f14-b772-4642-a2e4-0530fd0e18ad · outbound

This paper cites an unresolved cited work.

The cosmic web's Lyman-$\alpha$ glow at $z \approx 2.5$; hydrodynamic models, dust, and wide-field, narrow-band detection Unresolved cited work

Reference 43

Resolution
unresolved
no resolver link, observed 2026-08-04T11:03:30.425421Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-04T11:03:30.425421Z digest=sha256:6d9aa24ef33e5cdfa3e2cc9a138e23f0e3097691b3d16a1d5953064529b93242

Observation 7ef7dce3-bce8-40e9-8081-45c330c17cc4 · outbound

This paper cites an unresolved cited work.

The cosmic web's Lyman-$\alpha$ glow at $z \approx 2.5$; hydrodynamic models, dust, and wide-field, narrow-band detection Unresolved cited work

Reference 44

Resolution
unresolved
no resolver link, observed 2026-08-04T11:03:30.561039Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-04T11:03:30.561039Z digest=sha256:95365e6e811c331cefacb458e7786111a29e79104cead99723e4b682cbab9237

Observation bb46a627-ab47-42ad-8047-02987af105b4 · outbound

This paper cites T., 2011, Physics of the Interstellar and Intergalactic Medium.

The cosmic web's Lyman-$\alpha$ glow at $z \approx 2.5$; hydrodynamic models, dust, and wide-field, narrow-band detection T., 2011, Physics of the Interstellar and Intergalactic Medium

Reference 45

Resolution
unresolved
no resolver link, observed 2026-08-04T11:03:30.686641Z

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source=arxiv_source observed=2026-08-04T11:03:30.686641Z digest=sha256:6b6f4aff46e209d0b1cc57d7560fbc23377956087c7268ae9c41ebee33f644d0

Observation 470e5070-d9d7-44fe-aafa-329efb03b843 · outbound

This paper cites an unresolved cited work.

The cosmic web's Lyman-$\alpha$ glow at $z \approx 2.5$; hydrodynamic models, dust, and wide-field, narrow-band detection Unresolved cited work

Reference 46

Resolution
unresolved
no resolver link, observed 2026-08-04T11:03:30.824752Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-04T11:03:30.824752Z digest=sha256:0872623e492c662016f62ae1d7b976d381a0337b371f37fcf7fb8b611f79052e

Observation 8c764a4f-3e1f-487d-b60c-95868d5538aa · outbound

This paper cites A., 2015, @doi [ ] 10.1093/mnrasl/slv085 , https://ui.adsabs.harvard.edu/abs/2015MNRAS.452L..36D 452, L36.

The cosmic web's Lyman-$\alpha$ glow at $z \approx 2.5$; hydrodynamic models, dust, and wide-field, narrow-band detection A., 2015, @doi [ ] 10.1093/mnrasl/slv085 , https://ui.adsabs.harvard.edu/abs/2015MNRAS.452L..36D 452, L36

Reference 47

Resolution
verified exact
doi, observed 2026-08-04T11:08:57.295608Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

source=arxiv_source observed=2026-08-04T11:03:30.885820Z digest=sha256:a9b587138a7868f5bc300d3976cada23a777d3169d49dae43557775671879cbd

Observation c1f3f931-f04e-4bf0-be83-475d1f39af39 · outbound

This paper cites an unresolved cited work.

The cosmic web's Lyman-$\alpha$ glow at $z \approx 2.5$; hydrodynamic models, dust, and wide-field, narrow-band detection Unresolved cited work

Reference 48

Resolution
unresolved
no resolver link, observed 2026-08-04T11:03:30.994841Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-04T11:03:30.994841Z digest=sha256:aa7fe24f46f81e12f278765400309b3b272d8d7ee95f3827629feef64ecebd8e

Observation 21528b70-3508-49ee-9f48-c0b7ee7239d7 · outbound

This paper cites an unresolved cited work.

The cosmic web's Lyman-$\alpha$ glow at $z \approx 2.5$; hydrodynamic models, dust, and wide-field, narrow-band detection Unresolved cited work

Reference 49

Resolution
unresolved
no resolver link, observed 2026-08-04T11:03:31.132061Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-04T11:03:31.132061Z digest=sha256:9da3f4c5ee8bd0d154a52f96fb4d6dd3a9871dc73cff7cfbce248fcbfacf20b1

Observation e3e45c54-d7c7-4f36-8d57-617c838e3b86 · outbound

This paper cites J., Stanway E.

The cosmic web's Lyman-$\alpha$ glow at $z \approx 2.5$; hydrodynamic models, dust, and wide-field, narrow-band detection J., Stanway E

Reference 50

Resolution
unresolved
no resolver link, observed 2026-08-04T11:03:31.416116Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-04T11:03:31.416116Z digest=sha256:71e571e1905f31d8628c3c60029c7e42f94b18662872e8c75efdd58c9e835ed2

Observation 432e4d98-fdb0-4b6a-a134-70bbc697eaec · outbound

This paper cites an unresolved cited work.

The cosmic web's Lyman-$\alpha$ glow at $z \approx 2.5$; hydrodynamic models, dust, and wide-field, narrow-band detection Unresolved cited work

Reference 51

Resolution
verified exact
doi, observed 2026-08-04T11:08:57.052374Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

source=arxiv_source observed=2026-08-04T11:03:31.664885Z digest=sha256:dd5895658588e6e268b698f909b8300865bc4e8c29768e25dd43250bb1e118f0

Observation b2fef80f-2143-479c-9247-a905fcd0c902 · outbound

This paper cites an unresolved cited work.

The cosmic web's Lyman-$\alpha$ glow at $z \approx 2.5$; hydrodynamic models, dust, and wide-field, narrow-band detection Unresolved cited work

Reference 52

Resolution
unresolved
no resolver link, observed 2026-08-04T11:03:31.803355Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-04T11:03:31.803355Z digest=sha256:9f45afa01f74fe0941a4ab5b18115768422f20c6c045a43bd9e3bce9c6431e31

Observation 7bdf746d-00e1-42a4-9087-94a5d0002691 · outbound

This paper cites an unresolved cited work.

The cosmic web's Lyman-$\alpha$ glow at $z \approx 2.5$; hydrodynamic models, dust, and wide-field, narrow-band detection Unresolved cited work

Reference 53

Resolution
unresolved
no resolver link, observed 2026-08-04T11:03:32.017597Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-04T11:03:32.017597Z digest=sha256:95e87b9ff2ff3741d909560900cc10153f01b98c0011c897d1f0a7091b2cba14

Observation 66624cf9-1229-46e3-8ffb-672734111c4e · outbound

This paper cites an unresolved cited work.

The cosmic web's Lyman-$\alpha$ glow at $z \approx 2.5$; hydrodynamic models, dust, and wide-field, narrow-band detection Unresolved cited work

Reference 54

Resolution
unresolved
no resolver link, observed 2026-08-04T11:03:32.144754Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-04T11:03:32.144754Z digest=sha256:bbef8cca045d4b926bad52c5660f36fcb531b19738e6c560a17de42056c0a0ef

Observation bbcd3e23-b6f2-4dfa-ab95-d894e6763897 · outbound

This paper cites R., Schaye J., Springel V., Hernquist L., 2003, @doi [ ] 10.1086/381140 , https://ui.adsabs.harvard.edu/abs/2003ApJ...599L...1F 599, L1.

The cosmic web's Lyman-$\alpha$ glow at $z \approx 2.5$; hydrodynamic models, dust, and wide-field, narrow-band detection R., Schaye J., Springel V., Hernquist L., 2003, @doi [ ] 10.1086/381140 , https://ui.adsabs.harvard.edu/abs/2003ApJ...599L...1F 599, L1

Reference 55

Resolution
verified exact
doi, observed 2026-08-04T11:08:56.735161Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

source=arxiv_source observed=2026-08-04T11:03:32.303151Z digest=sha256:dda3b77763d75d44cc4881e3c8c94be425379d4797280262995040f1afae8048

Observation c81b7d85-ac1f-4762-9947-418bc73d6315 · outbound

This paper cites an unresolved cited work.

The cosmic web's Lyman-$\alpha$ glow at $z \approx 2.5$; hydrodynamic models, dust, and wide-field, narrow-band detection Unresolved cited work

Reference 56

Resolution
unresolved
no resolver link, observed 2026-08-04T11:03:32.426046Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-04T11:03:32.426046Z digest=sha256:433d6c786214f03345de0c3b585aa59a1894db6bcdae02fd595cd540c4b51a90

Observation 162fe815-a9bf-4719-91ad-2f830495a908 · outbound

This paper cites J., Huchra J.

The cosmic web's Lyman-$\alpha$ glow at $z \approx 2.5$; hydrodynamic models, dust, and wide-field, narrow-band detection J., Huchra J

Reference 57

Resolution
unresolved
no resolver link, observed 2026-08-04T11:03:32.606063Z

Source-reported events for the cited work

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source=arxiv_source observed=2026-08-04T11:03:32.606063Z digest=sha256:24faf1f20ce1f355ca91dc0ca70a5eac3270d70cee8e8df1cb0ec55c3992777a

Observation 4823b6cd-940a-403d-afde-da9550e5a20a · outbound

This paper cites Y., Kravtsov A.

The cosmic web's Lyman-$\alpha$ glow at $z \approx 2.5$; hydrodynamic models, dust, and wide-field, narrow-band detection Y., Kravtsov A

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Resolution
unresolved
no resolver link, observed 2026-08-04T11:03:32.768173Z

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Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-04T11:03:32.768173Z digest=sha256:0cb5801c29455b0655d720d9cb7d356f6f2ebb10ee1a95d07bfc5196a67083cd

Observation eaa40a5e-dd60-4540-b760-5ab8166673ad · outbound

This paper cites H., 1996, @doi [ApJ] 10.1086/177707 , https://ui.adsabs.harvard.edu/abs/1996ApJ...468..462G 468, 462.

The cosmic web's Lyman-$\alpha$ glow at $z \approx 2.5$; hydrodynamic models, dust, and wide-field, narrow-band detection H., 1996, @doi [ApJ] 10.1086/177707 , https://ui.adsabs.harvard.edu/abs/1996ApJ...468..462G 468, 462

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Resolution
unresolved
no resolver link, observed 2026-08-04T11:03:32.875496Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-04T11:03:32.875496Z digest=sha256:306f9235528d1431b8d2816033b92df739edb0f3b14276dda183ee6e40e6c2dd

Observation bdef7519-3ff5-4636-bba1-49375c559471 · outbound

This paper cites J.] 10.3847/1538-4357/835/2/175 , https://ui.adsabs.harvard.edu/abs/2017ApJ...835..175G 835, 175.

The cosmic web's Lyman-$\alpha$ glow at $z \approx 2.5$; hydrodynamic models, dust, and wide-field, narrow-band detection J.] 10.3847/1538-4357/835/2/175 , https://ui.adsabs.harvard.edu/abs/2017ApJ...835..175G 835, 175

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Resolution
unresolved
no resolver link, observed 2026-08-04T11:03:32.983369Z

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Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-04T11:03:32.983369Z digest=sha256:a2aee7375fceb65bfccd95038b5c3ee4b82ef0e4c7b2c07726556c6e357117fe

Observation ba69da2d-3eb1-4b92-97b8-6c3e1b2bd144 · outbound

This paper cites an unresolved cited work.

The cosmic web's Lyman-$\alpha$ glow at $z \approx 2.5$; hydrodynamic models, dust, and wide-field, narrow-band detection Unresolved cited work

Reference 61

Resolution
unresolved
no resolver link, observed 2026-08-04T11:03:33.075297Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-04T11:03:33.075297Z digest=sha256:53ef3437228c8e7ba0e8bcd52c09d33f603cf1837482a30a85ed34f2dd331cd2

Observation 7d9cf12a-c11c-4030-b851-a598e5cf48fa · outbound

This paper cites J., 1968, Bulletin of the Astronomical Institutes of the Netherlands, https://ui.adsabs.harvard.edu/abs/1968BAN....19..421H 19, 421.

The cosmic web's Lyman-$\alpha$ glow at $z \approx 2.5$; hydrodynamic models, dust, and wide-field, narrow-band detection J., 1968, Bulletin of the Astronomical Institutes of the Netherlands, https://ui.adsabs.harvard.edu/abs/1968BAN....19..421H 19, 421

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Resolution
unresolved
no resolver link, observed 2026-08-04T11:03:33.185689Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-04T11:03:33.185689Z digest=sha256:d717c8d2743a15110a69bb36574bd2df0d1f068bdd53e00baf8fcc54898e0fe5

Observation 66cac24d-fe38-4d3f-9db7-f8d643128c14 · outbound

This paper cites R., et al., 2020, @doi [Nature] 10.1038/s41586-020-2649-2 , 585, 357.

The cosmic web's Lyman-$\alpha$ glow at $z \approx 2.5$; hydrodynamic models, dust, and wide-field, narrow-band detection R., et al., 2020, @doi [Nature] 10.1038/s41586-020-2649-2 , 585, 357

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Resolution
unresolved
no resolver link, observed 2026-08-04T11:03:33.243002Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-04T11:03:33.243002Z digest=sha256:fabb3af9b2bde8666fc14f734f36a8689fc110a07e1afa1e0e744859a493aebf

Observation f2c93664-65a7-4b4e-8d4b-bb9b0d75fe61 · outbound

This paper cites M., Atek H., Kunth D., 2011, @doi [ ] 10.1088/0004-637X/730/1/8 , https://ui.adsabs.harvard.edu/abs/2011ApJ...730....8H 730, 8.

The cosmic web's Lyman-$\alpha$ glow at $z \approx 2.5$; hydrodynamic models, dust, and wide-field, narrow-band detection M., Atek H., Kunth D., 2011, @doi [ ] 10.1088/0004-637X/730/1/8 , https://ui.adsabs.harvard.edu/abs/2011ApJ...730....8H 730, 8

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Resolution
unresolved
no resolver link, observed 2026-08-04T11:03:33.294630Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-04T11:03:33.294630Z digest=sha256:0ff83c2a602c87af50349d41a505ad92023419949a2e1124a2858f35e6950ec8

Observation d454e447-4bd5-4fca-87fc-066fd8d965cf · outbound

This paper cites H., Miralda-Escud \'e J., 1996, @doi [ ] 10.1086/309899 , https://ui.adsabs.harvard.edu/abs/1996ApJ...457L..51H 457, L51.

The cosmic web's Lyman-$\alpha$ glow at $z \approx 2.5$; hydrodynamic models, dust, and wide-field, narrow-band detection H., Miralda-Escud \'e J., 1996, @doi [ ] 10.1086/309899 , https://ui.adsabs.harvard.edu/abs/1996ApJ...457L..51H 457, L51

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Resolution
unresolved
no resolver link, observed 2026-08-04T11:03:33.369977Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-04T11:03:33.369977Z digest=sha256:46992dbd77555a0cc343057ff5bc7e3dbc60b61e23e0a5aa6b79116f43627273

Observation 8a5eb340-d207-47eb-a08b-5a43e9b52e9f · outbound

This paper cites F., O \ n orbe J., O'Meara J.

The cosmic web's Lyman-$\alpha$ glow at $z \approx 2.5$; hydrodynamic models, dust, and wide-field, narrow-band detection F., O \ n orbe J., O'Meara J

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Resolution
unresolved
no resolver link, observed 2026-08-04T11:03:33.456390Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-04T11:03:33.456390Z digest=sha256:09dd5487dcbb099b034227e2fbd5e77a34749a5af45d2ead2a6f9ce9d488581b

Observation ad47d5fb-0714-41e8-b2ea-520940a088da · outbound

This paper cites J., Weymann R.

The cosmic web's Lyman-$\alpha$ glow at $z \approx 2.5$; hydrodynamic models, dust, and wide-field, narrow-band detection J., Weymann R

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Resolution
verified exact
doi, observed 2026-08-04T11:08:56.396335Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

source=arxiv_source observed=2026-08-04T11:03:33.505366Z digest=sha256:b249bec63109c04e206bd3833383d09cf2970e8a3120e4b5407011a27be7d9c4

Observation 314c5524-2319-45a2-aa49-f047b8f2de7a · outbound

This paper cites Y., 1997, @doi [ ] 10.1093/mnras/292.1.27 , https://ui.adsabs.harvard.edu/abs/1997MNRAS.292...27H 292, 27.

The cosmic web's Lyman-$\alpha$ glow at $z \approx 2.5$; hydrodynamic models, dust, and wide-field, narrow-band detection Y., 1997, @doi [ ] 10.1093/mnras/292.1.27 , https://ui.adsabs.harvard.edu/abs/1997MNRAS.292...27H 292, 27

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Resolution
unresolved
no resolver link, observed 2026-08-04T11:03:33.598051Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-04T11:03:33.598051Z digest=sha256:4f10516d99e0f28ef0d06cc787f36b605b286893e12e10b4d18c4618c59aea6a

Observation 012c663d-77ff-4f1b-b9dc-77742c6e58ba · outbound

This paper cites D., 2007, @doi [Computing in Science & Engineering] 10.1109/MCSE.2007.55 , 9, 90.

The cosmic web's Lyman-$\alpha$ glow at $z \approx 2.5$; hydrodynamic models, dust, and wide-field, narrow-band detection D., 2007, @doi [Computing in Science & Engineering] 10.1109/MCSE.2007.55 , 9, 90

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no resolver link, observed 2026-08-04T11:03:33.635402Z

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source=arxiv_source observed=2026-08-04T11:03:33.635402Z digest=sha256:d35fc64f88fbaf985bd9ee30cf7021d8fb8b6702769bf84ef2538b061413dbce

Observation 1135d960-e7f9-455e-b821-d157fe9f9651 · outbound

This paper cites an unresolved cited work.

The cosmic web's Lyman-$\alpha$ glow at $z \approx 2.5$; hydrodynamic models, dust, and wide-field, narrow-band detection Unresolved cited work

Reference 70

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no resolver link, observed 2026-08-04T11:03:33.713656Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-04T11:03:33.713656Z digest=sha256:7eefa65ea4b93ea2ff0f0c78649ca4cb068b64399f0cfc429bcf2e2c84372887

Observation eb9b4f46-c166-44cb-8d0d-34991e4c48f1 · outbound

This paper cites H., Hernquist L., 1996, @doi [Astrophysical Journal Supplements] 10.1086/192305 , https://ui.adsabs.harvard.edu/abs/1996ApJS..105...19K 105, 19.

The cosmic web's Lyman-$\alpha$ glow at $z \approx 2.5$; hydrodynamic models, dust, and wide-field, narrow-band detection H., Hernquist L., 1996, @doi [Astrophysical Journal Supplements] 10.1086/192305 , https://ui.adsabs.harvard.edu/abs/1996ApJS..105...19K 105, 19

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unresolved
no resolver link, observed 2026-08-04T11:03:33.784757Z

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source=arxiv_source observed=2026-08-04T11:03:33.784757Z digest=sha256:dfa26abe2a529cb93d7dae38f74e0e5d1f5574dfe2a464c28858066306e814c9

Observation c83f176d-8d51-4f74-b516-83dfb5ef3bf0 · outbound

This paper cites S., Partl A.

The cosmic web's Lyman-$\alpha$ glow at $z \approx 2.5$; hydrodynamic models, dust, and wide-field, narrow-band detection S., Partl A

Reference 72

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unresolved
no resolver link, observed 2026-08-04T11:03:33.838160Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-04T11:03:33.838160Z digest=sha256:e5278dd1b0e9302ec4becdef5965e65cfeb51afe227a632340fc44fac394017f

Observation e0b422a6-871d-46ba-8855-8d25aa8e7be6 · outbound

This paper cites an unresolved cited work.

The cosmic web's Lyman-$\alpha$ glow at $z \approx 2.5$; hydrodynamic models, dust, and wide-field, narrow-band detection Unresolved cited work

Reference 73

Resolution
verified exact
doi, observed 2026-08-04T11:08:56.129762Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

source=arxiv_source observed=2026-08-04T11:03:33.878449Z digest=sha256:7cc91b7e801c79638ccd020a03084be795da1af6438949787c0c9e526885793b

Observation 0ad17a06-c120-4a23-b4b8-a7848fdb1f27 · outbound

This paper cites S., Sinigaglia F., Balaguera-Antol \' nez A., Favole G., 2024, @doi [AAP] 10.1051/0004-6361/202345876 , https://ui.adsabs.harvard.edu/abs/2024A&A...683A.215K 683, A215.

The cosmic web's Lyman-$\alpha$ glow at $z \approx 2.5$; hydrodynamic models, dust, and wide-field, narrow-band detection S., Sinigaglia F., Balaguera-Antol \' nez A., Favole G., 2024, @doi [AAP] 10.1051/0004-6361/202345876 , https://ui.adsabs.harvard.edu/abs/2024A&A...683A.215K 683, A215

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Resolution
unresolved
no resolver link, observed 2026-08-04T11:03:33.924835Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-04T11:03:33.924835Z digest=sha256:dc94b7ca270ee2c7dfa407f012b9e80ce7d9b1db98bb46f92fd32185f5f128e4

Observation 1c394041-3a8f-4113-beb0-2022b04e5681 · outbound

This paper cites A., Shandarin S.

The cosmic web's Lyman-$\alpha$ glow at $z \approx 2.5$; hydrodynamic models, dust, and wide-field, narrow-band detection A., Shandarin S

Reference 75

Resolution
unresolved
no resolver link, observed 2026-08-04T11:03:33.972190Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-04T11:03:33.972190Z digest=sha256:92484134b1dbba63e66c351234cce8e1f9a20940510f53234b50719dff439b4b

Observation 763d13c8-61c6-4e8e-bd0f-905d5723d934 · outbound

This paper cites A., Zasowski G., Rix H.-W., Johns M., Anderson S.

The cosmic web's Lyman-$\alpha$ glow at $z \approx 2.5$; hydrodynamic models, dust, and wide-field, narrow-band detection A., Zasowski G., Rix H.-W., Johns M., Anderson S

Reference 76

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unresolved
no resolver link, observed 2026-08-04T11:03:34.058904Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-04T11:03:34.058904Z digest=sha256:9b4077c1f6143dd3b3b7ec440c0273d5869af16362ea8bc05c24f8d6894e44cf

Observation 9d3322bf-4a7e-4c76-8f91-45f9f1aa894b · outbound

This paper cites Cosmic Web Dynamics: Forces and Strains.

The cosmic web's Lyman-$\alpha$ glow at $z \approx 2.5$; hydrodynamic models, dust, and wide-field, narrow-band detection Cosmic Web Dynamics: Forces and Strains

Reference 77

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unresolved
no resolver link, observed 2026-08-04T11:03:34.113495Z

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source=arxiv_source observed=2026-08-04T11:03:34.113495Z digest=sha256:896c44092bf0418fd29adaba1c234a53dbf0263e02087790ee45e7151f9016a2

Observation abc31e70-4e6a-46b3-86b4-4fb53e055211 · outbound

This paper cites an unresolved cited work.

The cosmic web's Lyman-$\alpha$ glow at $z \approx 2.5$; hydrodynamic models, dust, and wide-field, narrow-band detection Unresolved cited work

Reference 78

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unresolved
no resolver link, observed 2026-08-04T11:03:34.189766Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-04T11:03:34.189766Z digest=sha256:1160723fc7ed690be6f0c827ea99a7425cc613098fca2eac31378ad37457a840

Observation b2a11c49-ad00-4196-954a-6b04651c4864 · outbound

This paper cites M., Bowen D.

The cosmic web's Lyman-$\alpha$ glow at $z \approx 2.5$; hydrodynamic models, dust, and wide-field, narrow-band detection M., Bowen D

Reference 79

Resolution
unresolved
no resolver link, observed 2026-08-04T11:03:34.241780Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-04T11:03:34.241780Z digest=sha256:be86e126e61c50042539f6e84892510c359431cd644a397c8179beb317423fc0

Observation 71ddd794-ce13-442d-ae37-232e7e89e0cb · outbound

This paper cites M., Gromoll S., Shara M.

The cosmic web's Lyman-$\alpha$ glow at $z \approx 2.5$; hydrodynamic models, dust, and wide-field, narrow-band detection M., Gromoll S., Shara M

Reference 80

Resolution
unresolved
no resolver link, observed 2026-08-04T11:03:34.315405Z

Source-reported events for the cited work

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source=arxiv_source observed=2026-08-04T11:03:34.315405Z digest=sha256:237cd353196d665c9b490c804dd47f515cf4a4cfa7c387ae399f8ea0c280facc

Observation e1115f0e-f40d-481c-bff4-0fe205dcc30b · outbound

This paper cites Direct Images of the Cosmic Web of Intergalactic and Circumgalactic Gas in the Distant Universe.

The cosmic web's Lyman-$\alpha$ glow at $z \approx 2.5$; hydrodynamic models, dust, and wide-field, narrow-band detection Direct Images of the Cosmic Web of Intergalactic and Circumgalactic Gas in the Distant Universe

Reference 81

Resolution
unresolved
no resolver link, observed 2026-08-04T11:03:34.362042Z

Source-reported events for the cited work

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source=arxiv_source observed=2026-08-04T11:03:34.362042Z digest=sha256:cdae62409ec1a507671af2a40007e2d45f5bd97bf1234b0efcc7456fe72c4c40

Observation ba067e56-f2fa-43f8-bb2c-44edd3363159 · outbound

This paper cites O., Sommer-Larsen J., 2009a, @doi [Astrophysical Journal] 10.1088/0004-637X/696/1/853 , https://ui.adsabs.harvard.edu/abs/2009ApJ...696..853L 696, 853.

The cosmic web's Lyman-$\alpha$ glow at $z \approx 2.5$; hydrodynamic models, dust, and wide-field, narrow-band detection O., Sommer-Larsen J., 2009a, @doi [Astrophysical Journal] 10.1088/0004-637X/696/1/853 , https://ui.adsabs.harvard.edu/abs/2009ApJ...696..853L 696, 853

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unresolved
no resolver link, observed 2026-08-04T11:03:34.409459Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-04T11:03:34.409459Z digest=sha256:84a34e197832149391c6e74d8dd916a511c1341a1f567709f346cf5c1c72e187

Observation a2c230a7-57e5-4d32-835a-128e2c1aeb87 · outbound

This paper cites C., 2009b, @doi [Astrophysical Journal] 10.1088/0004-637X/704/2/1640 , https://ui.adsabs.harvard.edu/abs/2009ApJ...704.1640L 704, 1640.

The cosmic web's Lyman-$\alpha$ glow at $z \approx 2.5$; hydrodynamic models, dust, and wide-field, narrow-band detection C., 2009b, @doi [Astrophysical Journal] 10.1088/0004-637X/704/2/1640 , https://ui.adsabs.harvard.edu/abs/2009ApJ...704.1640L 704, 1640

Reference 83

Resolution
unresolved
no resolver link, observed 2026-08-04T11:03:34.460594Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-04T11:03:34.460594Z digest=sha256:efd311d81ebb512cd6e4061272eb6ef3605053c33c42b173e82b421d4b069e80

Observation 1f2f137a-7505-481d-83de-7cdc9457253c · outbound

This paper cites K., Carswell R.

The cosmic web's Lyman-$\alpha$ glow at $z \approx 2.5$; hydrodynamic models, dust, and wide-field, narrow-band detection K., Carswell R

Reference 84

Resolution
verified exact
doi, observed 2026-08-04T11:08:55.776596Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

source=arxiv_source observed=2026-08-04T11:03:34.514137Z digest=sha256:9ceaf4cab911e1c5680f3c50511c45956c8611120b8c18c3ad3fee3eb49cdc44

Observation ef705286-1af4-403f-b29a-df40177a060c · outbound

This paper cites K., Carswell R.

The cosmic web's Lyman-$\alpha$ glow at $z \approx 2.5$; hydrodynamic models, dust, and wide-field, narrow-band detection K., Carswell R

Reference 85

Resolution
verified exact
doi, observed 2026-08-04T11:08:55.491324Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

source=arxiv_source observed=2026-08-04T11:03:34.561100Z digest=sha256:e482004edd22c16c9b80f79d9945ba700ffde0cbd258419d437a824318fee432

Observation 8745ae64-5f38-4958-b5fd-34d7225d6c18 · outbound

This paper cites an unresolved cited work.

The cosmic web's Lyman-$\alpha$ glow at $z \approx 2.5$; hydrodynamic models, dust, and wide-field, narrow-band detection Unresolved cited work

Reference 86

Resolution
unresolved
no resolver link, observed 2026-08-04T11:03:34.626793Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-04T11:03:34.626793Z digest=sha256:75576ba9a433fbda587351593baf075db38c2548722ce27eaef3f71496efa190

Observation b46e0e1b-d5ad-4c8f-8ccc-5579955e4315 · outbound

This paper cites T., 2001, @doi [ ] 10.1086/323147 , https://ui.adsabs.harvard.edu/abs/2001ApJ...554..778L 554, 778.

The cosmic web's Lyman-$\alpha$ glow at $z \approx 2.5$; hydrodynamic models, dust, and wide-field, narrow-band detection T., 2001, @doi [ ] 10.1086/323147 , https://ui.adsabs.harvard.edu/abs/2001ApJ...554..778L 554, 778

Reference 87

Resolution
unresolved
no resolver link, observed 2026-08-04T11:03:34.667989Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-04T11:03:34.667989Z digest=sha256:9fa872cf4fe616da51a7e86cb86854f5c87c091c6d7ff36fc6686d1783b90948

Observation dcfcbc4f-babc-4b5a-8627-8baf6f2d87ce · outbound

This paper cites F., Yajima H., Zhu Q., Maji M., 2020, @doi [MNRAS] 10.1093/mnras/staa733 , https://ui.adsabs.harvard.edu/abs/2020MNRAS.494.1919L 494, 1919.

The cosmic web's Lyman-$\alpha$ glow at $z \approx 2.5$; hydrodynamic models, dust, and wide-field, narrow-band detection F., Yajima H., Zhu Q., Maji M., 2020, @doi [MNRAS] 10.1093/mnras/staa733 , https://ui.adsabs.harvard.edu/abs/2020MNRAS.494.1919L 494, 1919

Reference 88

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unresolved
no resolver link, observed 2026-08-04T11:03:34.725579Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-04T11:03:34.725579Z digest=sha256:00b90004ae3f2312293ef2dd42e69e3e4ac65c0f656b1336b000ad046b91954a

Observation 100091d3-d2d5-48e0-85a0-a914aae3a5bc · outbound

This paper cites an unresolved cited work.

The cosmic web's Lyman-$\alpha$ glow at $z \approx 2.5$; hydrodynamic models, dust, and wide-field, narrow-band detection Unresolved cited work

Reference 89

Resolution
unresolved
no resolver link, observed 2026-08-04T11:03:34.786801Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-04T11:03:34.786801Z digest=sha256:9118b7401e43a41eeb0a975096359cdd2a7af7ff96f07769c0e340e7b45784c4

Observation 3791f2a7-cf5c-4462-b357-821f38f15822 · outbound

This paper cites I., et al., 2018, @doi [MNRAS] 10.1093/mnras/stx1976 , https://ui.adsabs.harvard.edu/abs/2018MNRAS.473.1195L 473, 1195.

The cosmic web's Lyman-$\alpha$ glow at $z \approx 2.5$; hydrodynamic models, dust, and wide-field, narrow-band detection I., et al., 2018, @doi [MNRAS] 10.1093/mnras/stx1976 , https://ui.adsabs.harvard.edu/abs/2018MNRAS.473.1195L 473, 1195

Reference 90

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unresolved
no resolver link, observed 2026-08-04T11:03:34.861297Z

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Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-04T11:03:34.861297Z digest=sha256:4e9d1552193fb29cf3419acdceb9d4eeba35fdbb320ac9fba8c6729733caa1b1

Observation 9da6610d-43b4-4a06-8f8c-33d5fecd1b59 · outbound

This paper cites H., Mo H.

The cosmic web's Lyman-$\alpha$ glow at $z \approx 2.5$; hydrodynamic models, dust, and wide-field, narrow-band detection H., Mo H

Reference 91

Resolution
verified exact
doi, observed 2026-08-04T11:08:55.225617Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

source=arxiv_source observed=2026-08-04T11:03:34.922646Z digest=sha256:a47e8a4fd7862cd3678d47930e376a8aa1e04ba408c8f081835bb2d22be55320

Observation b22ee3c1-d2f5-4902-a5ff-d0ce2a9cabbf · outbound

This paper cites an unresolved cited work.

The cosmic web's Lyman-$\alpha$ glow at $z \approx 2.5$; hydrodynamic models, dust, and wide-field, narrow-band detection Unresolved cited work

Reference 92

Resolution
unresolved
no resolver link, observed 2026-08-04T11:03:34.997818Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-04T11:03:34.997818Z digest=sha256:754762c641ac06f0540bfebc36dd99c0101ae9a4fd92811a1c714bc91c60aafb

Observation fde1495e-3434-4ee7-8b64-bec524b93bb6 · outbound

This paper cites an unresolved cited work.

The cosmic web's Lyman-$\alpha$ glow at $z \approx 2.5$; hydrodynamic models, dust, and wide-field, narrow-band detection Unresolved cited work

Reference 93

Resolution
verified exact
doi, observed 2026-08-04T11:08:54.955793Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

source=arxiv_source observed=2026-08-04T11:03:35.069622Z digest=sha256:6320d4c2190e5e9d17f9fbe88f07a2aa8c00bee92ac2b0298c88d33e2723d1ba

Observation a82536b1-7d62-430f-97ae-39b7ed7b6204 · outbound

This paper cites W., Nugent P., White M., Meiksin A.

The cosmic web's Lyman-$\alpha$ glow at $z \approx 2.5$; hydrodynamic models, dust, and wide-field, narrow-band detection W., Nugent P., White M., Meiksin A

Reference 94

Resolution
unresolved
no resolver link, observed 2026-08-04T11:03:35.250729Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-04T11:03:35.250729Z digest=sha256:fd1bb257fc50e7577bb1e189bb09eed8c3981f9088874e831272dceef57d41e8

Observation a8ea66ec-7dbb-40a1-aae2-4ec990e5add6 · outbound

This paper cites C., Darvish B., Lin Z., Cen R., Matuszewski M., Morrissey P., Neill J.

The cosmic web's Lyman-$\alpha$ glow at $z \approx 2.5$; hydrodynamic models, dust, and wide-field, narrow-band detection C., Darvish B., Lin Z., Cen R., Matuszewski M., Morrissey P., Neill J

Reference 95

Resolution
verified exact
doi, observed 2026-08-04T11:08:54.672043Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

source=arxiv_source observed=2026-08-04T11:03:35.345880Z digest=sha256:0f18fc77ff179e8bd455c1d07399b165f1f6766efbda85436f9c0f2c007399b0

Observation 1228a4c2-098d-4a7d-ae3b-f354c13d65cc · outbound

This paper cites R., 2010, @doi [ ] 10.1111/j.1365-2966.2010.17272.x , https://ui.adsabs.harvard.edu/abs/2010MNRAS.408.1945M 408, 1945.

The cosmic web's Lyman-$\alpha$ glow at $z \approx 2.5$; hydrodynamic models, dust, and wide-field, narrow-band detection R., 2010, @doi [ ] 10.1111/j.1365-2966.2010.17272.x , https://ui.adsabs.harvard.edu/abs/2010MNRAS.408.1945M 408, 1945

Reference 96

Resolution
unresolved
no resolver link, observed 2026-08-04T11:03:35.444035Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-04T11:03:35.444035Z digest=sha256:bb6467a70604630b7042d9f74e99c11c6d02dc1cbbf0bb3d5b147b4f1176817b

Observation 50b706d5-e6b7-4548-bc2e-55ab0587e2b9 · outbound

This paper cites & Astrophys.] 10.1051/0004-6361/201834961 , https://ui.adsabs.harvard.edu/abs/2020A&A...635A.154M 635, A154.

The cosmic web's Lyman-$\alpha$ glow at $z \approx 2.5$; hydrodynamic models, dust, and wide-field, narrow-band detection & Astrophys.] 10.1051/0004-6361/201834961 , https://ui.adsabs.harvard.edu/abs/2020A&A...635A.154M 635, A154

Reference 97

Resolution
unresolved
no resolver link, observed 2026-08-04T11:03:35.581584Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-04T11:03:35.581584Z digest=sha256:5b2f72274568e74ab6fd036ba7e2889137fcc2bfd4ef62130e68d8d3f477af0f

Observation 6604ea1f-83cb-4dd3-b6d9-74b600512c8a · outbound

This paper cites U., 2001, @doi [A&A] 10.1051/0004-6361:20010606 , https://ui.adsabs.harvard.edu/abs/2001A&A...372L..57M 372, L57.

The cosmic web's Lyman-$\alpha$ glow at $z \approx 2.5$; hydrodynamic models, dust, and wide-field, narrow-band detection U., 2001, @doi [A&A] 10.1051/0004-6361:20010606 , https://ui.adsabs.harvard.edu/abs/2001A&A...372L..57M 372, L57

Reference 98

Resolution
verified exact
doi, observed 2026-08-04T11:08:54.344614Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

source=arxiv_source observed=2026-08-04T11:03:35.762701Z digest=sha256:aa3c46853d9b163c65988fe7711b5c051d4d257bcecef309b20fb9d894915a75

Observation fb91bcad-542d-44f8-8532-4e857c6eb10b · outbound

This paper cites an unresolved cited work.

The cosmic web's Lyman-$\alpha$ glow at $z \approx 2.5$; hydrodynamic models, dust, and wide-field, narrow-band detection Unresolved cited work

Reference 99

Resolution
unresolved
no resolver link, observed 2026-08-04T11:03:35.868210Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-04T11:03:35.868210Z digest=sha256:4e0e72a5fff1748259481105a0270f496a1ab1d2086bfecc570da7eb1c56e893

Observation b6762fcc-e2e3-4bde-bb46-36114399a896 · outbound

This paper cites A., 1990, @doi [ ] 10.1086/168375 , https://ui.adsabs.harvard.edu/abs/1990ApJ...350..216N 350, 216.

The cosmic web's Lyman-$\alpha$ glow at $z \approx 2.5$; hydrodynamic models, dust, and wide-field, narrow-band detection A., 1990, @doi [ ] 10.1086/168375 , https://ui.adsabs.harvard.edu/abs/1990ApJ...350..216N 350, 216

Reference 100

Resolution
unresolved
no resolver link, observed 2026-08-04T11:03:35.973176Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-04T11:03:35.973176Z digest=sha256:ef0ba6050b17602a8aa7bdf1bae63481891223998c5fc395e38927394b22a865

Observation 687eb239-5cf6-4422-8c80-99c51d011fcc · outbound

This paper cites & Astrophys.] 10.1051/0004-6361/201220259 , https://ui.adsabs.harvard.edu/abs/2012A&A...547L...1N 547, L1.

The cosmic web's Lyman-$\alpha$ glow at $z \approx 2.5$; hydrodynamic models, dust, and wide-field, narrow-band detection & Astrophys.] 10.1051/0004-6361/201220259 , https://ui.adsabs.harvard.edu/abs/2012A&A...547L...1N 547, L1

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source=arxiv_source observed=2026-08-04T11:03:36.104244Z digest=sha256:d100a8b06f21688047956f1690e64d307763ba8fe7b59d07f3ca027fcbe9d458

Observation 9f65e0ab-e1a1-4729-9d97-585ed5a52124 · outbound

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The cosmic web's Lyman-$\alpha$ glow at $z \approx 2.5$; hydrodynamic models, dust, and wide-field, narrow-band detection Unresolved cited work

Reference 102

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source=arxiv_source observed=2026-08-04T11:03:36.212947Z digest=sha256:4d25e146b835f584298396abb315474868db136af8d4300e05fad51d70221fb5

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Observation 5b718c4b-aba5-4e8c-b706-a120151c671b · inbound

FEASTS and MHONGOOSE: HI Column Density Distribution at $z=0$ for $N_\mathrm{HI}>10^{17.8}\, \mathrm{cm}^{-2}$ cites this paper.

FEASTS and MHONGOOSE: HI Column Density Distribution at $z=0$ for $N_\mathrm{HI}>10^{17.8}\, \mathrm{cm}^{-2}$ The cosmic web's Lyman-$\alpha$ glow at $z \approx 2.5$; hydrodynamic models, dust, and wide-field, narrow-band detection

Reference 88

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source=arxiv_source observed=2026-08-02T19:24:52.522960Z digest=sha256:bb42ea777678eaab7e936515acc75d6fb58ddd2bbe25f02d079dcf4cd8b4d163