Paper Citation Record · LEDGER

How Massive Can a Population III Starburst Be? Simulating the First Galaxies with High Lyman-Werner Background

As of 10 August 2026, this Paper Citation Record lists 100 of 112 outbound references and 9 inbound Pith citation observations for arXiv:2603.23209.

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

pith.paper-citation-record.v1
2603.23209 v3

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measured 100 of 112 reference resolution

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Source: paper_references, paper_reference_links, observed 2026-08-02T17:38:12.323044Z

measured 109 of 109 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-10T06:31:04.303077+00:00

measured 9 of 9 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-07-10T17:07:21.371604Z

measured 1 of 1 external citation measurements

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

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

Reference resolution

100 of 112 outbound references displayed

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

Outbound references

Observation b32b8113-10ae-4e0e-960b-208e9c70d839 · outbound

This paper cites R., Iliev, I.

How Massive Can a Population III Starburst Be? Simulating the First Galaxies with High Lyman-Werner Background R., Iliev, I

Reference 2

Resolution: unresolved; no resolver link, observed 2026-08-02T17:38:01.733294Z

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Observation 579e74f5-7262-4884-a2ef-54db518e660b · outbound

This paper cites L., Teyssier, R., & Dekel, A.

How Massive Can a Population III Starburst Be? Simulating the First Galaxies with High Lyman-Werner Background L., Teyssier, R., & Dekel, A

Reference 3

Resolution: unresolved; no resolver link, observed 2026-08-02T17:38:01.973609Z

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Observation 4f030ce0-5e04-45b6-af14-70b2ed83fc96 · outbound

This paper cites an unresolved cited work.

How Massive Can a Population III Starburst Be? Simulating the First Galaxies with High Lyman-Werner Background Unresolved cited work

Reference 4

Resolution: verified exact; doi, observed 2026-08-02T17:38:33.068486Z

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Observation 32f598c3-c5ae-4cde-924f-66fef85caf02 · outbound

This paper cites 2001, PhR, 349, 125, doi: 10.1016/S0370-1573(01)00019-9.

How Massive Can a Population III Starburst Be? Simulating the First Galaxies with High Lyman-Werner Background 2001, PhR, 349, 125, doi: 10.1016/S0370-1573(01)00019-9

Reference 5

Resolution: unresolved; no resolver link, observed 2026-08-02T17:38:02.195145Z

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Observation f6a0180a-339e-4240-9c8c-3a878663e840 · outbound

This paper cites D., Bolton, J.

How Massive Can a Population III Starburst Be? Simulating the First Galaxies with High Lyman-Werner Background D., Bolton, J

Reference 6

Resolution: unresolved; no resolver link, observed 2026-08-02T17:38:02.315587Z

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Observation c530eb46-2cf0-4803-aef4-e3490149a52a · outbound

This paper cites S., Wechsler, R.

How Massive Can a Population III Starburst Be? Simulating the First Galaxies with High Lyman-Werner Background S., Wechsler, R

Reference 7

Resolution: unresolved; no resolver link, observed 2026-08-02T17:38:02.433053Z

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Observation 8196f24c-682b-45dd-8fb5-c48443c7553e · outbound

This paper cites 2025, ApJ, 980, 41, doi: 10.3847/1538-4357/ada4a1.

How Massive Can a Population III Starburst Be? Simulating the First Galaxies with High Lyman-Werner Background 2025, ApJ, 980, 41, doi: 10.3847/1538-4357/ada4a1

Reference 8

Resolution: unresolved; no resolver link, observed 2026-08-02T17:38:02.565254Z

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Observation 61877082-7049-4890-830c-b5b017e688e4 · outbound

This paper cites 2013, Reports on Progress in Physics, 76, 112901, doi: 10.1088/0034-4885/76/11/112901.

How Massive Can a Population III Starburst Be? Simulating the First Galaxies with High Lyman-Werner Background 2013, Reports on Progress in Physics, 76, 112901, doi: 10.1088/0034-4885/76/11/112901

Reference 9

Resolution: unresolved; no resolver link, observed 2026-08-02T17:38:02.663749Z

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Observation f4ced34f-a4b2-4938-9b46-007ecd0323b8 · outbound

This paper cites P., & Loeb, A.

How Massive Can a Population III Starburst Be? Simulating the First Galaxies with High Lyman-Werner Background P., & Loeb, A

Reference 10

Resolution: unresolved; no resolver link, observed 2026-08-02T17:38:02.767138Z

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Observation 628babfd-2a4f-4e7c-9c18-eac5d9e0603f · outbound

This paper cites an unresolved cited work.

How Massive Can a Population III Starburst Be? Simulating the First Galaxies with High Lyman-Werner Background Unresolved cited work

Reference 11

Resolution: unresolved; no resolver link, observed 2026-08-02T17:38:02.856327Z

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Observation eb43ca3d-a218-4b50-a478-659f226b1bf0 · outbound

This paper cites J., Saxena, A., Cameron, A.

How Massive Can a Population III Starburst Be? Simulating the First Galaxies with High Lyman-Werner Background J., Saxena, A., Cameron, A

Reference 12

Resolution: unresolved; no resolver link, observed 2026-08-02T17:38:02.928464Z

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Observation bc326cc7-98be-4d00-ab6d-a909bd149846 · outbound

This paper cites 2025, arXiv e-prints, arXiv:2507.17820, doi: 10.48550/arXiv.2507.17820.

How Massive Can a Population III Starburst Be? Simulating the First Galaxies with High Lyman-Werner Background 2025, arXiv e-prints, arXiv:2507.17820, doi: 10.48550/arXiv.2507.17820

Reference 13

Resolution: unresolved; no resolver link, observed 2026-08-02T17:38:03.001825Z

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Observation 94fa7226-042d-458b-9b50-76888f6e6212 · outbound

This paper cites 2003, PASP, 115, 763, doi: 10.1086/376392.

How Massive Can a Population III Starburst Be? Simulating the First Galaxies with High Lyman-Werner Background 2003, PASP, 115, 763, doi: 10.1086/376392

Reference 14

Resolution: unresolved; no resolver link, observed 2026-08-02T17:38:03.074401Z

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Observation b7f128b6-394c-4c16-bfee-3fbb7862d5f3 · outbound

This paper cites 2024, ApJL, 976, L15, doi: 10.3847/2041-8213/ad8dc9.

How Massive Can a Population III Starburst Be? Simulating the First Galaxies with High Lyman-Werner Background 2024, ApJL, 976, L15, doi: 10.3847/2041-8213/ad8dc9

Reference 15

Resolution: unresolved; no resolver link, observed 2026-08-02T17:38:03.129658Z

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Observation 5ad99ae8-8d2e-40a9-a23c-806f1a739eed · outbound

This paper cites 2022, MNRAS, 514, 4639, doi: 10.1093/mnras/stac1549.

How Massive Can a Population III Starburst Be? Simulating the First Galaxies with High Lyman-Werner Background 2022, MNRAS, 514, 4639, doi: 10.1093/mnras/stac1549

Reference 16

Resolution: unresolved; no resolver link, observed 2026-08-02T17:38:03.224794Z

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Observation 03f59f2f-cd5f-4430-a226-ab1a081f45c5 · outbound

This paper cites C., Glover, S.

How Massive Can a Population III Starburst Be? Simulating the First Galaxies with High Lyman-Werner Background C., Glover, S

Reference 17

Resolution: unresolved; no resolver link, observed 2026-08-02T17:38:03.296409Z

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Observation 3c0e9183-32bf-46ee-b8d2-3a60bd696ee5 · outbound

This paper cites an unresolved cited work.

How Massive Can a Population III Starburst Be? Simulating the First Galaxies with High Lyman-Werner Background Unresolved cited work

Reference 18

Resolution: unresolved; no resolver link, observed 2026-08-02T17:38:03.356590Z

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Observation 77d8144d-5833-42f3-9743-30425606d41c · outbound

This paper cites J., McLeod, D.

How Massive Can a Population III Starburst Be? Simulating the First Galaxies with High Lyman-Werner Background J., McLeod, D

Reference 19

Resolution: unresolved; no resolver link, observed 2026-08-02T17:38:03.428012Z

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Observation d96c76f2-913d-4ae5-a0c8-af0a22f28522 · outbound

This paper cites C., Scholte, D., et al.

How Massive Can a Population III Starburst Be? Simulating the First Galaxies with High Lyman-Werner Background C., Scholte, D., et al

Reference 20

Resolution: unresolved; no resolver link, observed 2026-08-02T17:38:03.486353Z

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Observation d1a41093-50d4-49e6-9d17-5c62c6cda572 · outbound

This paper cites C., Birnboim, Y., Mandelker, N., & Li, Z.

How Massive Can a Population III Starburst Be? Simulating the First Galaxies with High Lyman-Werner Background C., Birnboim, Y., Mandelker, N., & Li, Z

Reference 21

Resolution: unresolved; no resolver link, observed 2026-08-02T17:38:03.576159Z

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Observation 9572c36b-b096-43e3-81a5-21b66b6e2bac · outbound

This paper cites 2014, MNRAS, 442, 2036, doi: 10.1093/mnras/stu1007.

How Massive Can a Population III Starburst Be? Simulating the First Galaxies with High Lyman-Werner Background 2014, MNRAS, 442, 2036, doi: 10.1093/mnras/stu1007

Reference 22

Resolution: unresolved; no resolver link, observed 2026-08-02T17:38:03.769842Z

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Observation 99dc4691-8f54-4146-bb9e-a01e668010db · outbound

This paper cites Overview of the JWST Advanced Deep Extragalactic Survey (JADES).

How Massive Can a Population III Starburst Be? Simulating the First Galaxies with High Lyman-Werner Background Overview of the JWST Advanced Deep Extragalactic Survey (JADES)

Reference 24

Resolution: unresolved; no resolver link, observed 2026-08-02T17:38:04.056669Z

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Observation e94157cb-4523-444e-836e-ee30429e2ca2 · outbound

This paper cites The 2017 Release of Cloudy.

How Massive Can a Population III Starburst Be? Simulating the First Galaxies with High Lyman-Werner Background The 2017 Release of Cloudy

Reference 25

Resolution: unresolved; no resolver link, observed 2026-08-02T17:38:04.122586Z

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Observation 5c31f5cc-e795-47fe-86d4-b28803b96f3a · outbound

This paper cites Population III star formation near high-redshift active galactic nuclei.

How Massive Can a Population III Starburst Be? Simulating the First Galaxies with High Lyman-Werner Background Population III star formation near high-redshift active galactic nuclei

Reference 26

Resolution: verified exact; local_arxiv, observed 2026-08-02T17:38:32.695502Z

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Observation 3fe9363c-c7bb-4fd6-a40b-65b183ae04b8 · outbound

This paper cites 2012, ApJ, 759, 115, doi: 10.1088/0004-637X/759/2/115.

How Massive Can a Population III Starburst Be? Simulating the First Galaxies with High Lyman-Werner Background 2012, ApJ, 759, 115, doi: 10.1088/0004-637X/759/2/115

Reference 27

Resolution: unresolved; no resolver link, observed 2026-08-02T17:38:04.382636Z

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Observation 9a91ff80-0687-4b8a-9863-6ded880acecc · outbound

This paper cites GLIMPSE: An ultra-faint $\simeq$ 10$^{5}$ $M_{\odot}$ Pop III Galaxy Candidate and First Constraints on the Pop III UV Luminosity Function at $z\simeq6-7$.

How Massive Can a Population III Starburst Be? Simulating the First Galaxies with High Lyman-Werner Background GLIMPSE: An ultra-faint $\simeq$ 10$^{5}$ $M_{\odot}$ Pop III Galaxy Candidate and First Constraints on the Pop III UV Luminosity Function at $z\simeq6-7$

Reference 28

Resolution: unresolved; no resolver link, observed 2026-08-02T17:38:04.514353Z

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Observation 41392e6a-9cf2-4e9f-b920-3fe400175191 · outbound

This paper cites P., et al.

How Massive Can a Population III Starburst Be? Simulating the First Galaxies with High Lyman-Werner Background P., et al

Reference 29

Resolution: unresolved; no resolver link, observed 2026-08-02T17:38:04.673358Z

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Observation 073f00be-644a-4660-8a55-070f84e02af7 · outbound

This paper cites H., & Bromm, V.

How Massive Can a Population III Starburst Be? Simulating the First Galaxies with High Lyman-Werner Background H., & Bromm, V

Reference 30

Resolution: unresolved; no resolver link, observed 2026-08-02T17:38:04.804830Z

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Observation 4504ddc7-3b66-4556-9d1a-5114171746c9 · outbound

This paper cites H., Springel, V., White, S.

How Massive Can a Population III Starburst Be? Simulating the First Galaxies with High Lyman-Werner Background H., Springel, V., White, S

Reference 32

Resolution: unresolved; no resolver link, observed 2026-08-02T17:38:04.996043Z

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Observation aa840069-23f7-4e36-9932-c9e0dd2dc000 · outbound

This paper cites 2012, ApJ, 746, 125, doi: 10.1088/0004-637X/746/2/125.

How Massive Can a Population III Starburst Be? Simulating the First Galaxies with High Lyman-Werner Background 2012, ApJ, 746, 125, doi: 10.1088/0004-637X/746/2/125

Reference 33

Resolution: unresolved; no resolver link, observed 2026-08-02T17:38:05.158042Z

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Observation 22e7cf56-d45b-4b34-a30e-01109124b400 · outbound

This paper cites J., & Loeb, A.

How Massive Can a Population III Starburst Be? Simulating the First Galaxies with High Lyman-Werner Background J., & Loeb, A

Reference 35

Resolution: unresolved; no resolver link, observed 2026-08-02T17:38:05.378056Z

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Observation aaa13951-fe28-4db7-8ec1-52ce02a1231b · outbound

This paper cites an unresolved cited work.

How Massive Can a Population III Starburst Be? Simulating the First Galaxies with High Lyman-Werner Background Unresolved cited work

Reference 36

Resolution: unresolved; no resolver link, observed 2026-08-02T17:38:05.505592Z

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Observation edbe3387-9393-4448-8f80-416843234168 · outbound

This paper cites L., Woosley, S.

How Massive Can a Population III Starburst Be? Simulating the First Galaxies with High Lyman-Werner Background L., Woosley, S

Reference 37

Resolution: unresolved; no resolver link, observed 2026-08-02T17:38:05.639558Z

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Observation 3bb5bb84-2d12-4e6a-ada8-b37261c8a3e3 · outbound

This paper cites an unresolved cited work.

How Massive Can a Population III Starburst Be? Simulating the First Galaxies with High Lyman-Werner Background Unresolved cited work

Reference 38

Resolution: unresolved; no resolver link, observed 2026-08-02T17:38:05.734489Z

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Observation d9d05d3f-e46a-450f-945a-e050b7cf5e2a · outbound

This paper cites 2017, MNRAS, 470, 898, doi: 10.1093/mnras/stx1220.

How Massive Can a Population III Starburst Be? Simulating the First Galaxies with High Lyman-Werner Background 2017, MNRAS, 470, 898, doi: 10.1093/mnras/stx1220

Reference 39

Resolution: unresolved; no resolver link, observed 2026-08-02T17:38:05.792467Z

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Observation bebc14f7-1d00-468f-8809-9930b6f1da6f · outbound

This paper cites SAPPHIRES: Extremely Metal-Poor Galaxy Candidates with $12+{\rm log(O/H)}<7.0$ at $z\sim5-7$ from Deep JWST/NIRCam Grism Observations.

How Massive Can a Population III Starburst Be? Simulating the First Galaxies with High Lyman-Werner Background SAPPHIRES: Extremely Metal-Poor Galaxy Candidates with $12+{\rm log(O/H)}<7.0$ at $z\sim5-7$ from Deep JWST/NIRCam Grism Observations

Reference 40

Resolution: unresolved; no resolver link, observed 2026-08-02T17:38:05.864843Z

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Observation b41481af-a838-4d58-a3ef-f584ddd0566f · outbound

This paper cites K., Shimizu, I., Iwata, I., & Tanaka, M.

How Massive Can a Population III Starburst Be? Simulating the First Galaxies with High Lyman-Werner Background K., Shimizu, I., Iwata, I., & Tanaka, M

Reference 41

Resolution: unresolved; no resolver link, observed 2026-08-02T17:38:05.947433Z

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Observation 62260b3e-1e72-4896-8f74-edb49720b8c3 · outbound

This paper cites L., & Bromm, V.

How Massive Can a Population III Starburst Be? Simulating the First Galaxies with High Lyman-Werner Background L., & Bromm, V

Reference 42

Resolution: unresolved; no resolver link, observed 2026-08-02T17:38:06.000179Z

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Observation 69c52079-9782-487c-a1ac-8934316fc2e5 · outbound

This paper cites an unresolved cited work.

How Massive Can a Population III Starburst Be? Simulating the First Galaxies with High Lyman-Werner Background Unresolved cited work

Reference 43

Resolution: unresolved; no resolver link, observed 2026-08-02T17:38:06.080912Z

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Observation 0de282ef-98f3-43c2-9ef1-896a70c26982 · outbound

This paper cites J., et al.

How Massive Can a Population III Starburst Be? Simulating the First Galaxies with High Lyman-Werner Background J., et al

Reference 44

Resolution: unresolved; no resolver link, observed 2026-08-02T17:38:06.136464Z

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Observation 0a7c88f2-dddb-4aa5-9dc5-7cd8528414be · outbound

This paper cites 2025c, arXiv e-prints, arXiv:2508.14155, doi: 10.48550/arXiv.2508.14155.

How Massive Can a Population III Starburst Be? Simulating the First Galaxies with High Lyman-Werner Background 2025c, arXiv e-prints, arXiv:2508.14155, doi: 10.48550/arXiv.2508.14155

Reference 45

Resolution: unresolved; no resolver link, observed 2026-08-02T17:38:06.216476Z

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Observation 129c379e-d346-4537-83e6-94b83d46f225 · outbound

This paper cites 2017, ApJ, 848, 85, doi: 10.3847/1538-4357/aa8c80.

How Massive Can a Population III Starburst Be? Simulating the First Galaxies with High Lyman-Werner Background 2017, ApJ, 848, 85, doi: 10.3847/1538-4357/aa8c80

Reference 46

Resolution: unresolved; no resolver link, observed 2026-08-02T17:38:06.276818Z

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Observation 1946f2e6-d3a6-4711-bc4f-7078c979da34 · outbound

This paper cites 2019, MNRAS, 485, 5939, doi: 10.1093/mnras/stz863.

How Massive Can a Population III Starburst Be? Simulating the First Galaxies with High Lyman-Werner Background 2019, MNRAS, 485, 5939, doi: 10.1093/mnras/stz863

Reference 47

Resolution: unresolved; no resolver link, observed 2026-08-02T17:38:06.381579Z

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Observation a2936d94-9611-496c-8715-aef8f95aa470 · outbound

This paper cites H., Bromm, V., & Milosavljević, M.

How Massive Can a Population III Starburst Be? Simulating the First Galaxies with High Lyman-Werner Background H., Bromm, V., & Milosavljević, M

Reference 48

Resolution: unresolved; no resolver link, observed 2026-08-02T17:38:06.464212Z

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Observation 18dffa73-145c-408f-ac08-ccd92f378c8f · outbound

This paper cites B., Jeon, M., Song, H., & Bromm, V.

How Massive Can a Population III Starburst Be? Simulating the First Galaxies with High Lyman-Werner Background B., Jeon, M., Song, H., & Bromm, V

Reference 49

Resolution: unresolved; no resolver link, observed 2026-08-02T17:38:06.548723Z

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Observation 674c734f-a00f-4b56-9464-7c4588cded0e · outbound

This paper cites P., Frebel, A., & Bromm, V.

How Massive Can a Population III Starburst Be? Simulating the First Galaxies with High Lyman-Werner Background P., Frebel, A., & Bromm, V

Reference 50

Resolution: unresolved; no resolver link, observed 2026-08-02T17:38:06.608301Z

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Observation 5d1f0f1b-35c9-4691-a931-a4c8ea2d509d · outbound

This paper cites L., Dalla Vecchia, C., & Khochfar, S.

How Massive Can a Population III Starburst Be? Simulating the First Galaxies with High Lyman-Werner Background L., Dalla Vecchia, C., & Khochfar, S

Reference 52

Resolution: unresolved; no resolver link, observed 2026-08-02T17:38:06.765269Z

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Observation 8d31219d-494e-4748-9088-d174e9826f9c · outbound

This paper cites L., Greif, T.

How Massive Can a Population III Starburst Be? Simulating the First Galaxies with High Lyman-Werner Background L., Greif, T

Reference 53

Resolution: unresolved; no resolver link, observed 2026-08-02T17:38:06.848569Z

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Observation ce2b2fd3-d59c-47a5-8abe-2e4c7794ba2b · outbound

This paper cites 2013, Reviews of Modern Physics, 85, 809, doi: 10.1103/RevModPhys.85.809.

How Massive Can a Population III Starburst Be? Simulating the First Galaxies with High Lyman-Werner Background 2013, Reviews of Modern Physics, 85, 809, doi: 10.1103/RevModPhys.85.809

Reference 55

Resolution: unresolved; no resolver link, observed 2026-08-02T17:38:07.011248Z

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Observation 1579b6f1-7ead-491b-afe3-f6e1a673a0b2 · outbound

This paper cites S., Devriendt, J., & Slyz, A.

How Massive Can a Population III Starburst Be? Simulating the First Galaxies with High Lyman-Werner Background S., Devriendt, J., & Slyz, A

Reference 56

Resolution: unresolved; no resolver link, observed 2026-08-02T17:38:07.094358Z

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Observation eaaf1e52-c495-47a5-baff-0f6545ada210 · outbound

This paper cites S., & Glover, S.

How Massive Can a Population III Starburst Be? Simulating the First Galaxies with High Lyman-Werner Background S., & Glover, S

Reference 57

Resolution: unresolved; no resolver link, observed 2026-08-02T17:38:07.179032Z

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Observation 9a19c2b9-685e-4eb2-b55b-8b99f32d14d8 · outbound

This paper cites A., Whalen, D., & Khochfar, S.

How Massive Can a Population III Starburst Be? Simulating the First Galaxies with High Lyman-Werner Background A., Whalen, D., & Khochfar, S

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Resolution: unresolved; no resolver link, observed 2026-08-02T17:38:07.268275Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f8460ded-57ef-455d-92eb-1805f63d0e9c · outbound

This paper cites 2024, MNRAS, 527, 1257, doi: 10.1093/mnras/stad3198.

How Massive Can a Population III Starburst Be? Simulating the First Galaxies with High Lyman-Werner Background 2024, MNRAS, 527, 1257, doi: 10.1093/mnras/stad3198

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Resolution: verified exact; doi, observed 2026-08-02T17:38:32.226680Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation 3b76ab3e-73bd-4738-9802-f58691101ca6 · outbound

This paper cites K., Walter, F., Brinks, E., et al.

How Massive Can a Population III Starburst Be? Simulating the First Galaxies with High Lyman-Werner Background K., Walter, F., Brinks, E., et al

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Resolution: unresolved; no resolver link, observed 2026-08-02T17:38:07.399904Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 06d3321c-fa97-4551-9072-63437915c5ae · outbound

This paper cites an unresolved cited work.

How Massive Can a Population III Starburst Be? Simulating the First Galaxies with High Lyman-Werner Background Unresolved cited work

Reference 61

Resolution: unresolved; no resolver link, observed 2026-08-02T17:38:07.475242Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 71399fc4-8971-4281-92f6-ccc5d8389f0c · outbound

This paper cites 2020, MNRAS, 497, 2839, doi: 10.1093/mnras/staa2143.

How Massive Can a Population III Starburst Be? Simulating the First Galaxies with High Lyman-Werner Background 2020, MNRAS, 497, 2839, doi: 10.1093/mnras/staa2143

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Resolution: unresolved; no resolver link, observed 2026-08-02T17:38:07.535824Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 06dc4a2c-2b8c-4d70-8872-195301b9a3ac · outbound

This paper cites 2024, A&A, 687, A67, doi: 10.1051/0004-6361/202347087.

How Massive Can a Population III Starburst Be? Simulating the First Galaxies with High Lyman-Werner Background 2024, A&A, 687, A67, doi: 10.1051/0004-6361/202347087

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Resolution: unresolved; no resolver link, observed 2026-08-02T17:38:07.696964Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7f44f5ae-8faf-4d64-8b04-d2fc542dca6c · outbound

This paper cites 2001, A&A, 370, 194, doi: 10.1051/0004-6361:20000247.

How Massive Can a Population III Starburst Be? Simulating the First Galaxies with High Lyman-Werner Background 2001, A&A, 370, 194, doi: 10.1051/0004-6361:20000247

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Resolution: unresolved; no resolver link, observed 2026-08-02T17:38:07.778103Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 77d89f4a-0465-419c-9aec-2952dab95457 · outbound

This paper cites 2025, ApJ, 988, 171, doi: 10.3847/1538-4357/ade2cd.

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Resolution: unresolved; no resolver link, observed 2026-08-02T17:38:07.864624Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 266b396e-8a7a-4385-aa42-c7222d04c0c1 · outbound

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How Massive Can a Population III Starburst Be? Simulating the First Galaxies with High Lyman-Werner Background Pristine Massive Star Formation Caught at the Break of Cosmic Dawn

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Resolution: unresolved; no resolver link, observed 2026-08-02T17:38:07.950527Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 6948346e-d191-4df2-881d-355b4f007fc4 · outbound

This paper cites All the Little Things in Abell 2744: $>$1000 Gravitationally Lensed Dwarf Galaxies at $z=0-9$ from JWST NIRCam Grism Spectroscopy.

How Massive Can a Population III Starburst Be? Simulating the First Galaxies with High Lyman-Werner Background All the Little Things in Abell 2744: $>$1000 Gravitationally Lensed Dwarf Galaxies at $z=0-9$ from JWST NIRCam Grism Spectroscopy

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Resolution: unresolved; no resolver link, observed 2026-08-02T17:38:08.017621Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 3a74bf1c-d435-455f-93a2-d936b5ad40e1 · outbound

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How Massive Can a Population III Starburst Be? Simulating the First Galaxies with High Lyman-Werner Background 2025, arXiv e-prints, arXiv:2506.11846, doi: 10.48550/arXiv.2506.11846

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Resolution: unresolved; no resolver link, observed 2026-08-02T17:38:08.088582Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 1ac4fddb-d594-47a5-9962-4d0ca619d509 · outbound

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Resolution: unresolved; no resolver link, observed 2026-08-02T17:38:08.148339Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7f1e6528-60a2-4dc0-ae63-cc3df52d39f1 · outbound

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Resolution: unresolved; no resolver link, observed 2026-08-02T17:38:08.246466Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 1a4ac02d-a465-4fd4-98a0-52bdec0bb0f7 · outbound

This paper cites 2014, MNRAS, 440, 2498, doi: 10.1093/mnras/stu451.

How Massive Can a Population III Starburst Be? Simulating the First Galaxies with High Lyman-Werner Background 2014, MNRAS, 440, 2498, doi: 10.1093/mnras/stu451

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Resolution: unresolved; no resolver link, observed 2026-08-02T17:38:08.365470Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 9c7e123e-fa39-4579-be61-c431971fbd3f · outbound

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How Massive Can a Population III Starburst Be? Simulating the First Galaxies with High Lyman-Werner Background H., Milosavljević, M., & Bromm, V

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Resolution: verified exact; doi, observed 2026-08-02T17:38:31.864995Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation b7321b79-248b-4b0c-b77b-2cf37b5abd82 · outbound

This paper cites Galactic chemical enrichment with new metallicity dependent yields.

How Massive Can a Population III Starburst Be? Simulating the First Galaxies with High Lyman-Werner Background Galactic chemical enrichment with new metallicity dependent yields

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Resolution: unresolved; no resolver link, observed 2026-08-02T17:38:08.782737Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 3e448146-afa0-4e33-b424-62e3d92ba09f · outbound

This paper cites R., Clark, P.

How Massive Can a Population III Starburst Be? Simulating the First Galaxies with High Lyman-Werner Background R., Clark, P

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Resolution: unresolved; no resolver link, observed 2026-08-02T17:38:08.941733Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 423a91f1-91dd-488e-b1f1-b7033cefff34 · outbound

This paper cites R., Regan, J.

How Massive Can a Population III Starburst Be? Simulating the First Galaxies with High Lyman-Werner Background R., Regan, J

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Resolution: unresolved; no resolver link, observed 2026-08-02T17:38:09.000874Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation b572fee5-39d3-4a7c-b992-4177466f13fd · outbound

This paper cites A., Johansson, P.

How Massive Can a Population III Starburst Be? Simulating the First Galaxies with High Lyman-Werner Background A., Johansson, P

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Resolution: unresolved; no resolver link, observed 2026-08-02T17:38:09.068066Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation fa4cda94-2ef0-4c1b-8d92-a99cb3f381ff · outbound

This paper cites an unresolved cited work.

How Massive Can a Population III Starburst Be? Simulating the First Galaxies with High Lyman-Werner Background Unresolved cited work

Reference 78

Resolution: unresolved; no resolver link, observed 2026-08-02T17:38:09.227940Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 15b1ba6a-d993-4ec0-bd38-c02f2da5bfb3 · outbound

This paper cites an unresolved cited work.

How Massive Can a Population III Starburst Be? Simulating the First Galaxies with High Lyman-Werner Background Unresolved cited work

Reference 79

Resolution: unresolved; no resolver link, observed 2026-08-02T17:38:09.408749Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ccb74d9a-0aca-43cc-bb0f-30b028550ad6 · outbound

This paper cites 2025, ApJL, 989, L32, doi: 10.3847/2041-8213/adf4e3.

How Massive Can a Population III Starburst Be? Simulating the First Galaxies with High Lyman-Werner Background 2025, ApJL, 989, L32, doi: 10.3847/2041-8213/adf4e3

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Resolution: unresolved; no resolver link, observed 2026-08-02T17:38:09.550746Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a0278905-e149-4c9a-a117-3f5d4a1633e8 · outbound

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How Massive Can a Population III Starburst Be? Simulating the First Galaxies with High Lyman-Werner Background 2014, MNRAS, 438, 1669, doi: 10.1093/mnras/stt2307 17

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Resolution: verified exact; doi, observed 2026-08-02T17:38:31.565538Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation 3fa2d2e4-6b4e-419c-91d5-47e424a7e531 · outbound

This paper cites 2016, MNRAS, 455, 3288, doi: 10.1093/mnras/stv2545.

How Massive Can a Population III Starburst Be? Simulating the First Galaxies with High Lyman-Werner Background 2016, MNRAS, 455, 3288, doi: 10.1093/mnras/stv2545

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Resolution: verified exact; doi, observed 2026-08-02T17:38:31.391955Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation ede4f695-728a-4a97-9a87-875b512cd6e4 · outbound

This paper cites 2002, A&A, 382, 28, doi: 10.1051/0004-6361:20011619 —.

How Massive Can a Population III Starburst Be? Simulating the First Galaxies with High Lyman-Werner Background 2002, A&A, 382, 28, doi: 10.1051/0004-6361:20011619 —

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Resolution: unresolved; no resolver link, observed 2026-08-02T17:38:09.901902Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e3d71a18-1727-4311-947d-d7b50b79282d · outbound

This paper cites an unresolved cited work.

How Massive Can a Population III Starburst Be? Simulating the First Galaxies with High Lyman-Werner Background Unresolved cited work

Reference 84

Resolution: unresolved; no resolver link, observed 2026-08-02T17:38:09.980613Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f8f5a803-af5c-4b06-8df0-7e6386984401 · outbound

This paper cites an unresolved cited work.

How Massive Can a Population III Starburst Be? Simulating the First Galaxies with High Lyman-Werner Background Unresolved cited work

Reference 85

Resolution: unresolved; no resolver link, observed 2026-08-02T17:38:10.083864Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 6eeedc2c-9017-487a-bfad-28a2adf84cae · outbound

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How Massive Can a Population III Starburst Be? Simulating the First Galaxies with High Lyman-Werner Background 1959, ApJ, 129, 243, doi: 10.1086/146614

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Resolution: unresolved; no resolver link, observed 2026-08-02T17:38:10.194032Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 3038e68d-b6a2-4a9d-9058-830e9f4ec96a · outbound

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How Massive Can a Population III Starburst Be? Simulating the First Galaxies with High Lyman-Werner Background H., Gerasimov, R., et al

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Resolution: unresolved; no resolver link, observed 2026-08-02T17:38:10.483573Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ef5f47f9-4cc1-4e24-82ef-b1c70c152e4b · outbound

This paper cites 2005, Monthly Notices of the Royal Astronomical Society, 364, 1105–1134, doi: 10.1111/j.1365-2966.2005.09655.x.

How Massive Can a Population III Starburst Be? Simulating the First Galaxies with High Lyman-Werner Background 2005, Monthly Notices of the Royal Astronomical Society, 364, 1105–1134, doi: 10.1111/j.1365-2966.2005.09655.x

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Resolution: unresolved; no resolver link, observed 2026-08-02T17:38:10.638709Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation fea40964-d453-45a0-9e5d-343e35587ccf · outbound

This paper cites an unresolved cited work.

How Massive Can a Population III Starburst Be? Simulating the First Galaxies with High Lyman-Werner Background Unresolved cited work

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Resolution: unresolved; no resolver link, observed 2026-08-02T17:38:10.800766Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f348d547-71f3-415e-81a2-a81a68f2bae8 · outbound

This paper cites an unresolved cited work.

How Massive Can a Population III Starburst Be? Simulating the First Galaxies with High Lyman-Werner Background Unresolved cited work

Reference 92

Resolution: unresolved; no resolver link, observed 2026-08-02T17:38:10.924825Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 2aa54b92-457e-458c-a959-ddbf60b82e80 · outbound

This paper cites MEGATRON: The environments of Population III stars at Cosmic Dawn and their connection to present day galaxies.

How Massive Can a Population III Starburst Be? Simulating the First Galaxies with High Lyman-Werner Background MEGATRON: The environments of Population III stars at Cosmic Dawn and their connection to present day galaxies

Reference 93

Resolution: unresolved; no resolver link, observed 2026-08-02T17:38:10.991885Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 2b4e68fc-01cb-4616-83ab-d5d6524eddeb · outbound

This paper cites A., Weaver, J.

How Massive Can a Population III Starburst Be? Simulating the First Galaxies with High Lyman-Werner Background A., Weaver, J

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Resolution: unresolved; no resolver link, observed 2026-08-02T17:38:11.053005Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation af1f7459-7933-4a5e-b6e8-935f570983d8 · outbound

This paper cites 2025, MNRAS, doi: 10.1093/mnras/staf1269.

How Massive Can a Population III Starburst Be? Simulating the First Galaxies with High Lyman-Werner Background 2025, MNRAS, doi: 10.1093/mnras/staf1269

Reference 95

Resolution: unresolved; no resolver link, observed 2026-08-02T17:38:11.265264Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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This paper cites V., Klypin, A., et al.

How Massive Can a Population III Starburst Be? Simulating the First Galaxies with High Lyman-Werner Background V., Klypin, A., et al

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Resolution: unresolved; no resolver link, observed 2026-08-02T17:38:11.357270Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 221af428-359b-4687-9e85-c4d8eb6dfb92 · outbound

This paper cites 2006, Revisiting the Supernova Ia Rate at z>1, HST Proposal ID 10980.

How Massive Can a Population III Starburst Be? Simulating the First Galaxies with High Lyman-Werner Background 2006, Revisiting the Supernova Ia Rate at z>1, HST Proposal ID 10980

Reference 97

Resolution: unresolved; no resolver link, observed 2026-08-02T17:38:11.488403Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e0d97fd7-eb1c-468c-83e5-5ae30fea2b0d · outbound

This paper cites 2007, MNRAS, 382, 945, doi: 10.1111/j.1365-2966.2007.12215.x.

How Massive Can a Population III Starburst Be? Simulating the First Galaxies with High Lyman-Werner Background 2007, MNRAS, 382, 945, doi: 10.1111/j.1365-2966.2007.12215.x

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Resolution: unresolved; no resolver link, observed 2026-08-02T17:38:11.667092Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 1d46aa63-07f9-41a5-8b1e-76e018343fdc · outbound

This paper cites 2022, ApJ, 935, 110, doi: 10.3847/1538-4357/ac8158.

How Massive Can a Population III Starburst Be? Simulating the First Galaxies with High Lyman-Werner Background 2022, ApJ, 935, 110, doi: 10.3847/1538-4357/ac8158

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Resolution: unresolved; no resolver link, observed 2026-08-02T17:38:11.785239Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7b0971e0-88a5-4f49-8171-7c5a01684fd5 · outbound

This paper cites Hunting the first Cosmic Giants: formation and detectability of Direct Collapse Black Holes around high-redshift quasars.

How Massive Can a Population III Starburst Be? Simulating the First Galaxies with High Lyman-Werner Background Hunting the first Cosmic Giants: formation and detectability of Direct Collapse Black Holes around high-redshift quasars

Reference 100

Resolution: unresolved; no resolver link, observed 2026-08-02T17:38:11.852003Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 388e1ed5-1ace-4025-839f-10b757e56ac7 · outbound

This paper cites an unresolved cited work.

How Massive Can a Population III Starburst Be? Simulating the First Galaxies with High Lyman-Werner Background Unresolved cited work

Reference 101

Resolution: verified exact; arxiv_id, observed 2026-08-02T17:38:31.050279Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation 9c1bd874-5134-4e74-bf7b-667c8640de79 · outbound

This paper cites 2023, A&A, 678, A173, doi: 10.1051/0004-6361/202346981.

How Massive Can a Population III Starburst Be? Simulating the First Galaxies with High Lyman-Werner Background 2023, A&A, 678, A173, doi: 10.1051/0004-6361/202346981

Reference 102

Resolution: unresolved; no resolver link, observed 2026-08-02T17:38:11.968047Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 900f8e15-40e9-406f-a900-7e039f6baad7 · outbound

This paper cites A hide-and-seek game: Looking for Population III stars during the Epoch of Reionization through the HeII$\lambda$1640 line.

How Massive Can a Population III Starburst Be? Simulating the First Galaxies with High Lyman-Werner Background A hide-and-seek game: Looking for Population III stars during the Epoch of Reionization through the HeII$\lambda$1640 line

Reference 103

Resolution: verified exact; local_arxiv, observed 2026-08-02T17:38:30.703833Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation 3f68a5f6-ce1c-408d-9cb3-8ba375bebd96 · outbound

This paper cites 2024b, MNRAS, 527, 5102, doi: 10.1093/mnras/stad3513.

How Massive Can a Population III Starburst Be? Simulating the First Galaxies with High Lyman-Werner Background 2024b, MNRAS, 527, 5102, doi: 10.1093/mnras/stad3513

Reference 104

Resolution: unresolved; no resolver link, observed 2026-08-02T17:38:12.093287Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 29df158e-93b3-4dfd-949f-715424d59957 · outbound

This paper cites 2023, MNRAS, 522, 3809, doi: 10.1093/mnras/stad1201.

How Massive Can a Population III Starburst Be? Simulating the First Galaxies with High Lyman-Werner Background 2023, MNRAS, 522, 3809, doi: 10.1093/mnras/stad1201

Reference 105

Resolution: unresolved; no resolver link, observed 2026-08-02T17:38:12.157806Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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This paper cites B., Bromm, V., et al.

How Massive Can a Population III Starburst Be? Simulating the First Galaxies with High Lyman-Werner Background B., Bromm, V., et al

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Resolution: unresolved; no resolver link, observed 2026-08-02T17:38:12.186590Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 21d51f7b-d8d8-4c12-bcca-4694c3532667 · outbound

This paper cites M., Qin, Y., Balu, S., & Wyithe, J.

How Massive Can a Population III Starburst Be? Simulating the First Galaxies with High Lyman-Werner Background M., Qin, Y., Balu, S., & Wyithe, J

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Resolution: unresolved; no resolver link, observed 2026-08-02T17:38:12.222052Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 5c328273-8678-4eef-b23b-90219315778f · outbound

This paper cites L., & Haiman, Z.

How Massive Can a Population III Starburst Be? Simulating the First Galaxies with High Lyman-Werner Background L., & Haiman, Z

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Resolution: unresolved; no resolver link, observed 2026-08-02T17:38:12.263277Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 238ffde4-b8d0-4efe-b396-6bd0b07a9ee5 · outbound

This paper cites 2024, ApJL, 967, L42, doi: 10.3847/2041-8213/ad4ced.

How Massive Can a Population III Starburst Be? Simulating the First Galaxies with High Lyman-Werner Background 2024, ApJL, 967, L42, doi: 10.3847/2041-8213/ad4ced

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Resolution: unresolved; no resolver link, observed 2026-08-02T17:38:12.323044Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Pith citing papers

Observation 0a32f062-a3da-4809-900e-7842398301b7 · inbound

The Pristine HeII Emitter near GN-z11: Constraining the Mass Distribution of the First Stars cites this paper.

The Pristine HeII Emitter near GN-z11: Constraining the Mass Distribution of the First Stars How Massive Can a Population III Starburst Be? Simulating the First Galaxies with High Lyman-Werner Background

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Resolution: verified exact; arxiv_id, observed 2026-07-23T01:23:34.971481Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation 6cb8d2ab-488f-41b7-9eed-03915d0288bc · inbound

What is Powering the Enigmatic He II Emitter Hebe: The First Stars or Black Holes? cites this paper.

What is Powering the Enigmatic He II Emitter Hebe: The First Stars or Black Holes? How Massive Can a Population III Starburst Be? Simulating the First Galaxies with High Lyman-Werner Background

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Resolution: verified exact; arxiv_id, observed 2026-07-23T01:23:34.971481Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation 2c5fa25b-6aed-4ecb-8950-ca7e0f38344a · inbound

What is Powering the Enigmatic He II Emitter Hebe: The First Stars or Black Holes? cites this paper.

What is Powering the Enigmatic He II Emitter Hebe: The First Stars or Black Holes? How Massive Can a Population III Starburst Be? Simulating the First Galaxies with High Lyman-Werner Background

Reference 33

Resolution: verified exact; arxiv_id, observed 2026-07-23T01:23:34.971481Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation 07bf67a9-896f-4e5c-a013-7a3a4d2d9712 · inbound

NEFERTITI: Linking early galaxy formation to the assembly of the Milky Way cites this paper.

NEFERTITI: Linking early galaxy formation to the assembly of the Milky Way How Massive Can a Population III Starburst Be? Simulating the First Galaxies with High Lyman-Werner Background

Reference 2

Resolution: metadata mismatch; arxiv_id, observed 2026-07-23T01:23:34.971481Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation 141ac0c4-e526-41bf-bf46-f179656bbc07 · inbound

A Pixel-by-Pixel Path to Population III Discovery with JWST cites this paper.

A Pixel-by-Pixel Path to Population III Discovery with JWST How Massive Can a Population III Starburst Be? Simulating the First Galaxies with High Lyman-Werner Background

Reference 25

Resolution: metadata mismatch; arxiv_id, observed 2026-07-23T01:23:34.971481Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation 3b805633-63da-4274-a3e5-f85c75706c04 · inbound

A Pixel-by-Pixel Path to Population III Discovery with JWST cites this paper.

A Pixel-by-Pixel Path to Population III Discovery with JWST How Massive Can a Population III Starburst Be? Simulating the First Galaxies with High Lyman-Werner Background

Reference 151

Resolution: verified exact; arxiv_id, observed 2026-07-23T01:23:34.971481Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation f6b3f3be-efd7-4953-bd16-c264e11a9e63 · inbound

Possible chemical signatures of first-star enrichment in a very metal-poor galaxy overdensity near the end of reionization cites this paper.

Possible chemical signatures of first-star enrichment in a very metal-poor galaxy overdensity near the end of reionization How Massive Can a Population III Starburst Be? Simulating the First Galaxies with High Lyman-Werner Background

Reference 62

Resolution: metadata mismatch; arxiv_id, observed 2026-07-23T01:23:34.971481Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation abf330b8-8075-4b34-a1ca-95e4f32873bf · inbound

How can we finally see the first light? Status and perspective in the search for Population III stars cites this paper.

How can we finally see the first light? Status and perspective in the search for Population III stars How Massive Can a Population III Starburst Be? Simulating the First Galaxies with High Lyman-Werner Background

Reference 168

Resolution: verified exact; arxiv_id, observed 2026-07-23T01:23:34.971481Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation 36e1a1b6-b5e3-4fc0-b2b1-1d7dc4c81a61 · inbound

On the detection of Population III galaxies: Emission Line Diagnostics for Hybrid Stellar Populations cites this paper.

On the detection of Population III galaxies: Emission Line Diagnostics for Hybrid Stellar Populations How Massive Can a Population III Starburst Be? Simulating the First Galaxies with High Lyman-Werner Background

Reference 39

Resolution: verified exact; arxiv_id, observed 2026-07-23T01:23:34.971481Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.