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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 5 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 2026-08-05T06:32:48.257954+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

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  • verified fuzzy0
  • unresolved84
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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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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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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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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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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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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:f3a71d263a8dab4b21f61d45be3e27658a1f933d443c5e34d6b726833cd5edd9

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 2026-08-05T06:32:48.257954+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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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=sha256:14fd0adf6b48bd6d2d84f66cc473ffe0c03decd8b51ee329cbc86c71c41f5e84

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

Reference 36

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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=sha256:596419b8e4c036ee6683b7e58a219afb3410ae034b20cd1f22c92f685e2d99d2

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=sha256:0664fb4f452ae8250c54fe5bd7fdad77c1815454de1fc525efd889fa65bc528c

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

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source=arxiv_source observed=2026-08-04T11:03:29.934748Z digest=sha256:f3209fa76d78926430ab59182e07d95f7929c350c727b430e1caa20abf4f4390

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=sha256:50ff50eae96fbb3d776e50d14dd7dda97b890b7a9ae89d0e76031b69b74aa1e8

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

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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=sha256:2a914c239d63d0c9c2b67e557661a9be09fe5fc5b727e6a7000fab1fedf5099e

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=sha256:8e8a90af56e0b0e17a4e7194e251cd61cde5a55af5733c661339cc4712e2b307

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:fcb58366b8de971ca2de2a278e059b13e2ca9cd12603d5c506a5be636869b4ab

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

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

Source-reported events for the cited work

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source=arxiv_source observed=2026-08-04T11:03:30.425421Z digest=sha256:fc13a540c80b19f53328c49b8fbcf9197145076e8b66f48801d706887980aa0b

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

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source=arxiv_source observed=2026-08-04T11:03:30.561039Z digest=sha256:043c4d4b35f940677c84bb931d3e23b588cd735f117675982f6de4121ae977c3

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:d9fcaffc5418f06f0e508f25b56b040b12e1092cd2b7584547e17ce889c6d6de

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:be73a9e7feaa0e55fd28ab1f62fe0a537c8dcf0d5f9420d0c2787e5e0c761d32

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 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-08-04T11:03:30.885820Z digest=sha256:871b7c45cb929c93020035be1abbdae4aceb03824bf60972d8b57aed2172dff2

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:b11048808227767ad7e2f8453e85004699a58eea3f031d18384d266543e6631e

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:e47978f54136ce2711aae13ab28aa3b0e9da07e20b6ff089a09fc700bfa08688

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:cb76659d42ab973acffee80667e6a848969014e84ef30b50487940c094c91030

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 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-08-04T11:03:31.664885Z digest=sha256:7096ffa7d90abef126fb1e4b6295a32bad215d779cc892dc2a267d5d3d70c42f

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=sha256:8957fd745a4f82a3c82176f167026e3523677a7f3a12b49c2ddc2e55b5cf451a

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:ae52d3c7e25daee4029c1be32cb3e88af029f1f43b3366d32bf4476cb2822694

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:beddd779e030a725a1a2b2827ec7ea44eebd212562f634ba4fdaa3afec3196ee

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 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-08-04T11:03:32.303151Z digest=sha256:2a3907b2f822a98c2c7c5f633ce5b4186d07a189386eda01e98426fc5128e5f4

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:b5f37873d9f89e18a267771971120a0cae7e98a574c403529b440d318913994e

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

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source=arxiv_source observed=2026-08-04T11:03:32.606063Z digest=sha256:e71eb1d5ac7e2d34679a02af8badb2a2f9b4459ca1335e3e197decb6b06fcb0d

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

Reference 58

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

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-04T11:03:32.768173Z digest=sha256:02e4a3325e06f8926f513ddbc1e5f36581422ce979078ac2aa53d16fd4756c02

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

Reference 59

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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=sha256:53b3c11b7b40c7d4355902f96ecb48f74129c76ff5f8e65755cf35e576dc7d96

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

Reference 60

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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=sha256:1669c51019945df5b16e170e877cf8ea005fa4b3195c8b211b27e921ebbc70e6

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=sha256:3151ef1d3de83425633bc0001cd29dd64d9d15ece1c031ac562a215567d4b5ea

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

Reference 62

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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=sha256:4d52877c0746fce513ed54a9d9ebb5a783ca347a06945b58f7af6cefd4a1de44

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

Reference 63

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=sha256:96f2b169e6ad400c33f0952354e7ff30c28eaf2d571fb046a0f3d41cc8d77c28

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

Reference 64

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=sha256:16c8d0f3bbaefad360adca662e8bee30979ee0970c0168db1aa39fd7e021ef85

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

Reference 65

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=sha256:0a384af9d84b60dee2c81ecaf4225c7d0347123263562a3cc2ac18bfde9f9768

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

Reference 66

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=sha256:7cc0db869e049ae8ee798e5ee76d12389c4264c6875e955274f914cb07a7cfb4

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

Reference 67

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 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-08-04T11:03:33.505366Z digest=sha256:efac5353294e7a791f56f18c045d04f2fa27407c55067846b1892d3672492b9f

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

Reference 68

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=sha256:923251bb3ff44c68b41279a3e32f1c2ce415c320cac6e1ccfbd5249eaea9a9bb

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

Reference 69

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source=arxiv_source observed=2026-08-04T11:03:33.635402Z digest=sha256:56e3610892c2ed846c6b78fdedab8a9252729f5c4426239d5b8270a0c691610c

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

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Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-04T11:03:33.713656Z digest=sha256:7dc9d5c9f727656b9755749f7bce49944fd19674df0e5cddaecbf69f5996fb8b

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

Reference 71

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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:e8ec6e3b14a5e7a4d601361258ccbcf616ea3184be582ef14fb9804ceeadded7

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

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Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-04T11:03:33.838160Z digest=sha256:d88107de976bd571744e113966eee04e1f468bc6e9787c1c17ad39f8be77ce7c

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

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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 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-08-04T11:03:33.878449Z digest=sha256:822bfeb900c2616681647c10ac9c86a891d75d314b72bd6400b00cbf6e78a19c

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

Reference 74

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

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Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-04T11:03:33.924835Z digest=sha256:5c0b9d89641db104be675281db871c94415200828cca8b970b33dc5d156c64ac

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

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source=arxiv_source observed=2026-08-04T11:03:33.972190Z digest=sha256:c51ae8d19315b25480dd62e8a9261b0d47a8a3d57364abf45de57e444c235faf

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

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source=arxiv_source observed=2026-08-04T11:03:34.058904Z digest=sha256:2b11cdb9909b4bf2b5be26b3b14932f50a0f947a94bf7f66d43d343f69eaf5cc

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=sha256:41493e9de64700ad185f6143ee544bcca0c691336ee4b4aab9d12697164182a1

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

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source=arxiv_source observed=2026-08-04T11:03:34.189766Z digest=sha256:bb15298a890303537776903ed3c944dbde55c67e5f904343dda21ab5e92c5726

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

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source=arxiv_source observed=2026-08-04T11:03:34.241780Z digest=sha256:56ab96f83ed5e670dfc11c9608e0a8d6f0633a13889b68f222c484a777072cd2

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

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

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source=arxiv_source observed=2026-08-04T11:03:34.315405Z digest=sha256:d7b794ad92863804d05e970b2067913553a6fcd3f669bb8dc58d3f4a3a5b9f19

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

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

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source=arxiv_source observed=2026-08-04T11:03:34.362042Z digest=sha256:7f664d9fe8bad2a9c160a8860f9e959764d82b321f9a10cb39195dcffbc7b36e

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

Reference 82

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

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source=arxiv_source observed=2026-08-04T11:03:34.409459Z digest=sha256:e77c2c8e0a3538423899cb648573f41196cbdf313b0cfd15eb3cf246e36e8e5b

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

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

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source=arxiv_source observed=2026-08-04T11:03:34.460594Z digest=sha256:50b4bacec5f1f978a199a64ca7ece2b99a195c4ef5cc93b3367d3b045fc78d22

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 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-08-04T11:03:34.514137Z digest=sha256:64782e6fed17f788be8be297e105aab6217461cfc1f53227f848d650cc6f0f51

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 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-08-04T11:03:34.561100Z digest=sha256:e1cc5134a2fc5e4097aba5101d1e65e6142ad0919518ce1f386cf3b52533c89e

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=sha256:56e242ad16ac20ce81ea821b229c4b8cf75ebf93e6e2a443e2d136f6b3f2ca28

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

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

Source-reported events for the cited work

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source=arxiv_source observed=2026-08-04T11:03:34.667989Z digest=sha256:f635e803c969f38a86cf26e4e0fbaabc6038b982b77dddb0b6b6d56cc6514e9a

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=sha256:334a348f23d01caa08da87895df7bf06cb0fce3c638e9bc85b3ba919ed85a114

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=sha256:208af2b3a78e0eb81135b84b4a76b2da1fcd5c6120b680e003044337c30ce1f3

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:c399a6476aecc12de15cbf81b85f10fa60ac9a9f954b5616522ff81d512d436f

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 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-08-04T11:03:34.922646Z digest=sha256:2dac8a5f8ec7763ecac793d0a81a1901badba2a87db6892bb57b6881cba271e3

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=sha256:1b32c769cf73a5b4340c63020a4125bab61ad5a06bea49c63dbd782b6533a3b5

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 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-08-04T11:03:35.069622Z digest=sha256:95ff7c4ed8631f1aa8559bd0c726f624f16a77ae730bb7c664806ab949da2f1d

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

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

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Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-04T11:03:35.250729Z digest=sha256:9441e5aaa6b8c3add006d90dcbe6eff1ad76f85a509c7ecf9c570892b7499277

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 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-08-04T11:03:35.345880Z digest=sha256:c5561b7b511edd86c5cb0c7dca432dbccebe52001e4fdbd0e216d0167176f0c4

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:e4d028c579b29198b357d85388c21abb1edef9dca73f4200a8b46c3d1431777a

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=sha256:757f98ccc9c7a90806d3fb6f9d6123a8efe510c13f1ae5f809cb028fcfcefbc5

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 2026-08-05T06:32:48.257954+00:00.

source=arxiv_source observed=2026-08-04T11:03:35.762701Z digest=sha256:ada9b77d510d33c4fa2b1390ae15a07d39241a640563213961b7b8cb9a7e46f5

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=sha256:1f211a88ce7ba414a7e9430cc19088a41910839c64c55cfe0bcd28cb0d9c4fee

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

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Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-04T11:03:35.973176Z digest=sha256:b1513fe40cbfef5e01bcbd0071cfa110efd4b67d28bba4f00ab52b462e3872c9

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

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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:b17c79658643c879d91f194e9c22cdf4cfbe77c00c8de5ef3279bca0b71c3565

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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

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