Semi-analytic modelling of Pop. III star formation and metallicity evolution -- II. Impact on 21cm power spectrum | Paper Citation Record

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Semi-analytic modelling of Pop. III star formation and metallicity evolution -- II. Impact on 21cm power spectrum write newline

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Semi-analytic modelling of Pop. III star formation and metallicity evolution -- II. Impact on 21cm power spectrum Unresolved cited work

Reference 2

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Observation 00768574-72c2-4f39-abe2-9d23dd72c0be · outbound

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Semi-analytic modelling of Pop. III star formation and metallicity evolution -- II. Impact on 21cm power spectrum Unresolved cited work

Reference 3

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Observation 39975306-3ce4-410f-acde-2c771c3632dd · outbound

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Semi-analytic modelling of Pop. III star formation and metallicity evolution -- II. Impact on 21cm power spectrum Unresolved cited work

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Observation 31ffce00-6924-49a9-b681-824d6dc47e6c · outbound

This paper cites K., Samui S., 2020, @doi [ ] 10.1093/mnras/staa1529 , https://ui.adsabs.harvard.edu/abs/2020MNRAS.498..918B 498, 918.

Semi-analytic modelling of Pop. III star formation and metallicity evolution -- II. Impact on 21cm power spectrum K., Samui S., 2020, @doi [ ] 10.1093/mnras/staa1529 , https://ui.adsabs.harvard.edu/abs/2020MNRAS.498..918B 498, 918

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Observation 45660595-fbe4-48f2-aeab-fb6f262e8c41 · outbound

This paper cites K., 2023, @doi [ ] 10.1093/mnras/stac3814 , https://ui.adsabs.harvard.edu/abs/2023MNRAS.519.4869B 519, 4869.

Semi-analytic modelling of Pop. III star formation and metallicity evolution -- II. Impact on 21cm power spectrum K., 2023, @doi [ ] 10.1093/mnras/stac3814 , https://ui.adsabs.harvard.edu/abs/2023MNRAS.519.4869B 519, 4869

Reference 6

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Semi-analytic modelling of Pop. III star formation and metallicity evolution -- II. Impact on 21cm power spectrum Unresolved cited work

Reference 7

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Observation bb728344-1cbb-4120-8944-b4566f653166 · outbound

This paper cites R., Schneider R., 2020, @doi [ ] 10.1093/mnras/staa1609 , 496, 1445.

Semi-analytic modelling of Pop. III star formation and metallicity evolution -- II. Impact on 21cm power spectrum R., Schneider R., 2020, @doi [ ] 10.1093/mnras/staa1609 , 496, 1445

Reference 8

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Observation b6792b80-e201-4826-982b-75cf2e2e4422 · outbound

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Semi-analytic modelling of Pop. III star formation and metallicity evolution -- II. Impact on 21cm power spectrum Unresolved cited work

Reference 9

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Observation 849c0bae-7f62-4da7-a142-af0883ce85d1 · outbound

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Semi-analytic modelling of Pop. III star formation and metallicity evolution -- II. Impact on 21cm power spectrum Unresolved cited work

Reference 10

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Semi-analytic modelling of Pop. III star formation and metallicity evolution -- II. Impact on 21cm power spectrum Unresolved cited work

Reference 11

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Observation b0feb078-12a4-4a1c-b5a5-884cf0072ed9 · outbound

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Semi-analytic modelling of Pop. III star formation and metallicity evolution -- II. Impact on 21cm power spectrum Unresolved cited work

Reference 12

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Observation 19b3f969-4d69-44ab-9ca2-fee1c41574c0 · outbound

This paper cites The First Billion Years in Seconds: An Effective Model for the 21-cm Signal with Population III Stars.

Semi-analytic modelling of Pop. III star formation and metallicity evolution -- II. Impact on 21cm power spectrum The First Billion Years in Seconds: An Effective Model for the 21-cm Signal with Population III Stars

Reference 13

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Observation 149e861e-22c5-4b5b-99e3-aa6c6e521697 · outbound

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Semi-analytic modelling of Pop. III star formation and metallicity evolution -- II. Impact on 21cm power spectrum Unresolved cited work

Reference 14

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Observation c15f7c32-c968-472c-8d3a-56864fa40273 · outbound

This paper cites H., 2017, @doi [ ] 10.1093/mnras/stx943 , https://ui.adsabs.harvard.edu/abs/2017MNRAS.469.1166D 469, 1166.

Semi-analytic modelling of Pop. III star formation and metallicity evolution -- II. Impact on 21cm power spectrum H., 2017, @doi [ ] 10.1093/mnras/stx943 , https://ui.adsabs.harvard.edu/abs/2017MNRAS.469.1166D 469, 1166

Reference 15

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Observation f124892b-142d-4ac1-8121-cd34c6176ce1 · outbound

This paper cites D., Carilli C.

Semi-analytic modelling of Pop. III star formation and metallicity evolution -- II. Impact on 21cm power spectrum D., Carilli C

Reference 16

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Observation 9a4115b0-9faa-4e09-a587-d309e828ff4d · outbound

This paper cites B., et al., 2018, @doi [The Astrophysical Journal] 10.3847/1538-4357/aad6dc , 864, 142.

Semi-analytic modelling of Pop. III star formation and metallicity evolution -- II. Impact on 21cm power spectrum B., et al., 2018, @doi [The Astrophysical Journal] 10.3847/1538-4357/aad6dc , 864, 142

Reference 17

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Observation 79de75f2-699c-4a09-8491-c9081a95dc7c · outbound

This paper cites an unresolved cited work.

Semi-analytic modelling of Pop. III star formation and metallicity evolution -- II. Impact on 21cm power spectrum Unresolved cited work

Reference 18

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Observation bde66d0a-3348-4b00-ae1a-7307a4707919 · outbound

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

Semi-analytic modelling of Pop. III star formation and metallicity evolution -- II. Impact on 21cm power spectrum IPAW 2020 Preprint: Efficient Computation of Provenance for Query Result Exploration

Reference 19

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Observation f3f6bef2-f5fb-4ee7-be66-670635dcc57b · outbound

This paper cites R., Kulkarni M., Visbal E., Hazlett R., 2024, @doi [ ] 10.3847/1538-4357/ad1688 , https://ui.adsabs.harvard.edu/abs/2024ApJ...962...62F 962, 62.

Semi-analytic modelling of Pop. III star formation and metallicity evolution -- II. Impact on 21cm power spectrum R., Kulkarni M., Visbal E., Hazlett R., 2024, @doi [ ] 10.3847/1538-4357/ad1688 , https://ui.adsabs.harvard.edu/abs/2024ApJ...962...62F 962, 62

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Observation 867c21a3-7b15-4d5d-acbd-706e985fe69a · outbound

This paper cites an unresolved cited work.

Semi-analytic modelling of Pop. III star formation and metallicity evolution -- II. Impact on 21cm power spectrum Unresolved cited work

Reference 21

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Observation 1d48b3e5-f069-4ad3-b6ec-6f4bbd826201 · outbound

This paper cites R., Loeb A., 2004, @doi [ ] 10.1086/422242 , https://ui.adsabs.harvard.edu/abs/2004ApJ...611..642F 611, 642.

Semi-analytic modelling of Pop. III star formation and metallicity evolution -- II. Impact on 21cm power spectrum R., Loeb A., 2004, @doi [ ] 10.1086/422242 , https://ui.adsabs.harvard.edu/abs/2004ApJ...611..642F 611, 642

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Observation 3667d8d8-c21c-44cb-b293-355b10a9db98 · outbound

This paper cites R., Peng Oh S., Briggs F.

Semi-analytic modelling of Pop. III star formation and metallicity evolution -- II. Impact on 21cm power spectrum R., Peng Oh S., Briggs F

Reference 23

Resolution: unresolved; no resolver link, observed 2026-08-07T23:09:26.771264Z

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Observation 49a23f8a-c72e-4a0f-9d30-f9fde39496c2 · outbound

This paper cites an unresolved cited work.

Semi-analytic modelling of Pop. III star formation and metallicity evolution -- II. Impact on 21cm power spectrum Unresolved cited work

Reference 24

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Observation d1ddf51b-4878-4276-8d7b-76cefdfb6ef3 · outbound

This paper cites The mass distribution of the first stars can be determined via the 21-cm signal.

Semi-analytic modelling of Pop. III star formation and metallicity evolution -- II. Impact on 21cm power spectrum The mass distribution of the first stars can be determined via the 21-cm signal

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Resolution: verified exact; local_arxiv, observed 2026-08-07T23:09:27.540029Z

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Observation 567c3dad-7de8-4e33-ad2a-ac05a71a6ce8 · outbound

This paper cites Y., Shaver P.

Semi-analytic modelling of Pop. III star formation and metallicity evolution -- II. Impact on 21cm power spectrum Y., Shaver P

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Resolution: verified exact; doi, observed 2026-08-07T23:09:27.527626Z

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Observation ab09bf32-9aed-496a-be87-ea0aaca82d85 · outbound

This paper cites H., White S.

Semi-analytic modelling of Pop. III star formation and metallicity evolution -- II. Impact on 21cm power spectrum H., White S

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Observation 262d9c1c-21c5-46d1-b325-3bf84b853768 · outbound

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

Semi-analytic modelling of Pop. III star formation and metallicity evolution -- II. Impact on 21cm power spectrum B., Wang F., Yang J., Hennawi J

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Observation 26ff2179-5301-413a-9348-633b0dd3a921 · outbound

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Semi-analytic modelling of Pop. III star formation and metallicity evolution -- II. Impact on 21cm power spectrum Unresolved cited work

Reference 29

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Observation db08f342-29f8-4183-b164-1a4dcf86d8f5 · outbound

This paper cites A Framework to Calibrate a Semi-analytic Model of the First Stars and Galaxies to the Renaissance Simulations.

Semi-analytic modelling of Pop. III star formation and metallicity evolution -- II. Impact on 21cm power spectrum A Framework to Calibrate a Semi-analytic Model of the First Stars and Galaxies to the Renaissance Simulations

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Observation 37bdb753-1916-4b9e-99b3-d7cd5febb407 · outbound

This paper cites R., 2023, @doi [ ] 10.1093/mnras/stad2308 , https://ui.adsabs.harvard.edu/abs/2023MNRAS.525..428H 525, 428.

Semi-analytic modelling of Pop. III star formation and metallicity evolution -- II. Impact on 21cm power spectrum R., 2023, @doi [ ] 10.1093/mnras/stad2308 , https://ui.adsabs.harvard.edu/abs/2023MNRAS.525..428H 525, 428

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Observation 9dd254ed-8ca8-4059-8542-06d0d132f363 · outbound

This paper cites S., 2018, @doi [ ] 10.3847/1538-4357/aaaaba , https://ui.adsabs.harvard.edu/abs/2018ApJ...855...17H 855, 17.

Semi-analytic modelling of Pop. III star formation and metallicity evolution -- II. Impact on 21cm power spectrum S., 2018, @doi [ ] 10.3847/1538-4357/aaaaba , https://ui.adsabs.harvard.edu/abs/2018ApJ...855...17H 855, 17

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Observation 82550497-1d1a-426e-800a-4b74191f2e16 · outbound

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Semi-analytic modelling of Pop. III star formation and metallicity evolution -- II. Impact on 21cm power spectrum Unresolved cited work

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Observation 6309967e-b03d-4baf-80ae-30e087d99a5e · outbound

This paper cites The Effects of Dark Matter Annihilation and Dark Matter-Baryon Velocity Offsets at Cosmic Dawn.

Semi-analytic modelling of Pop. III star formation and metallicity evolution -- II. Impact on 21cm power spectrum The Effects of Dark Matter Annihilation and Dark Matter-Baryon Velocity Offsets at Cosmic Dawn

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Observation 849a9280-8f68-49cc-8c25-1a4469f0ec24 · outbound

This paper cites T., Mellema G., Ahn K., Shapiro P.

Semi-analytic modelling of Pop. III star formation and metallicity evolution -- II. Impact on 21cm power spectrum T., Mellema G., Ahn K., Shapiro P

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Observation 2cb1e11c-9a4b-4d16-9d4b-3a8d860069c5 · outbound

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Semi-analytic modelling of Pop. III star formation and metallicity evolution -- II. Impact on 21cm power spectrum Unresolved cited work

Reference 36

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Observation 99add4e7-7a9d-4961-9645-a007de45ae70 · outbound

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Semi-analytic modelling of Pop. III star formation and metallicity evolution -- II. Impact on 21cm power spectrum Unresolved cited work

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Observation 2350b97e-89b7-49ce-9c1f-c6fcb42a7ce4 · outbound

This paper cites D., Gillet N., Mesinger A., 2020, @doi [ ] 10.1093/mnras/staa1323 , https://ui.adsabs.harvard.edu/abs/2020MNRAS.495.2354K 495, 2354.

Semi-analytic modelling of Pop. III star formation and metallicity evolution -- II. Impact on 21cm power spectrum D., Gillet N., Mesinger A., 2020, @doi [ ] 10.1093/mnras/staa1323 , https://ui.adsabs.harvard.edu/abs/2020MNRAS.495.2354K 495, 2354

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Observation 4f83b054-1601-48f4-aa59-dba451c79279 · outbound

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Semi-analytic modelling of Pop. III star formation and metallicity evolution -- II. Impact on 21cm power spectrum D., Qin Y., Mesinger A., Pallottini A., Fragos T., Basu-Zych A., 2022, @doi [ ] 10.1093/mnras/stac1226 , https://ui.adsabs.harvard.edu/abs/2022MNRAS.513.5097K 513, 5097

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Observation 2d803ce1-e3ff-4d82-8588-4703904b59b5 · outbound

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Semi-analytic modelling of Pop. III star formation and metallicity evolution -- II. Impact on 21cm power spectrum Unresolved cited work

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Observation 4fe6ba3c-5511-4ffe-b8da-01d233c2c75e · outbound

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Semi-analytic modelling of Pop. III star formation and metallicity evolution -- II. Impact on 21cm power spectrum Unresolved cited work

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Observation 1c511ed2-272f-4f29-9c00-36e5a7cc4936 · outbound

This paper cites L., 2021, @doi [ ] 10.3847/1538-4357/ac08a3 , https://ui.adsabs.harvard.edu/abs/2021ApJ...917...40K 917, 40.

Semi-analytic modelling of Pop. III star formation and metallicity evolution -- II. Impact on 21cm power spectrum L., 2021, @doi [ ] 10.3847/1538-4357/ac08a3 , https://ui.adsabs.harvard.edu/abs/2021ApJ...917...40K 917, 40

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Observation 62fe2ab8-bc75-4859-b741-5e5de34c46b1 · outbound

This paper cites R., 2020, @doi [Publications of the Astronomical Society of the Pacific] 10.1088/1538-3873/ab5bfd , 132, 062001.

Semi-analytic modelling of Pop. III star formation and metallicity evolution -- II. Impact on 21cm power spectrum R., 2020, @doi [Publications of the Astronomical Society of the Pacific] 10.1088/1538-3873/ab5bfd , 132, 062001

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Observation 40ac0d60-3a95-4f66-91e6-dff6ec3a361e · outbound

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Semi-analytic modelling of Pop. III star formation and metallicity evolution -- II. Impact on 21cm power spectrum R., 2018, @doi [ ] 10.1103/PhysRevD.98.023501 , https://ui.adsabs.harvard.edu/abs/2018PhRvD..98b3501L 98, 023501

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Observation 57e7933b-c7c8-439a-a2c0-fc3b47d41e0b · outbound

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Semi-analytic modelling of Pop. III star formation and metallicity evolution -- II. Impact on 21cm power spectrum Towards a universal analytical model for Population III star formation: interplay between feedback and fragmentation

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Resolution: verified exact; local_arxiv, observed 2026-08-07T23:09:27.418642Z

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Observation 1d81e0d6-bc2c-4deb-890a-9f04173af9b1 · outbound

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Semi-analytic modelling of Pop. III star formation and metallicity evolution -- II. Impact on 21cm power spectrum B., Busch P., Mao Y., Zhi Q.-J., 2021, @doi [ ] 10.3847/1538-4357/abefd5 , 912, 143

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Observation 6b537497-b05a-4113-9ce2-0635571c6d3c · outbound

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Semi-analytic modelling of Pop. III star formation and metallicity evolution -- II. Impact on 21cm power spectrum Unresolved cited work

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Observation cb199869-d423-4134-aba9-816d7d66a08e · outbound

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Semi-analytic modelling of Pop. III star formation and metallicity evolution -- II. Impact on 21cm power spectrum Unresolved cited work

Reference 48

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Observation c5eccc72-3c87-40d1-b206-eace9f34875b · outbound

This paper cites A., et al., 2019, @doi [Monthly Notices of the Royal Astronomical Society] 10.1093/mnras/stz632 , 485, 3947.

Semi-analytic modelling of Pop. III star formation and metallicity evolution -- II. Impact on 21cm power spectrum A., et al., 2019, @doi [Monthly Notices of the Royal Astronomical Society] 10.1093/mnras/stz632 , 485, 3947

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Observation d57cf1d8-c9b3-4a9c-9854-57d66c5b7f9e · outbound

This paper cites D., Mesinger A., D'Odorico V., 2015, @doi [ ] 10.1093/mnras/stu2449 , https://ui.adsabs.harvard.edu/abs/2015MNRAS.447..499M 447, 499.

Semi-analytic modelling of Pop. III star formation and metallicity evolution -- II. Impact on 21cm power spectrum D., Mesinger A., D'Odorico V., 2015, @doi [ ] 10.1093/mnras/stu2449 , https://ui.adsabs.harvard.edu/abs/2015MNRAS.447..499M 447, 499

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Observation abe532bf-73e0-4c88-af0e-aeeb80a671f5 · outbound

This paper cites R., 2006, @doi [ ] 10.1086/505167 , https://ui.adsabs.harvard.edu/abs/2006ApJ...653..815M 653, 815.

Semi-analytic modelling of Pop. III star formation and metallicity evolution -- II. Impact on 21cm power spectrum R., 2006, @doi [ ] 10.1086/505167 , https://ui.adsabs.harvard.edu/abs/2006ApJ...653..815M 653, 815

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Observation de6cd306-0d35-4b80-b73c-aab7abc08fec · outbound

This paper cites H., Mirocha J., Furlanetto S.

Semi-analytic modelling of Pop. III star formation and metallicity evolution -- II. Impact on 21cm power spectrum H., Mirocha J., Furlanetto S

Reference 52

Resolution: unresolved; no resolver link, observed 2026-08-07T23:09:26.878500Z

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Observation c7f1d5f7-7701-4761-b22c-3397bcae6563 · outbound

This paper cites G., et al., 2020, @doi [Monthly Notices of the Royal Astronomical Society] 10.1093/mnras/staa327 , 493, 1662.

Semi-analytic modelling of Pop. III star formation and metallicity evolution -- II. Impact on 21cm power spectrum G., et al., 2020, @doi [Monthly Notices of the Royal Astronomical Society] 10.1093/mnras/staa327 , 493, 1662

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Resolution: unresolved; no resolver link, observed 2026-08-07T23:09:26.881834Z

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Observation d6789d04-ab06-4ed7-ac23-46c1027e977b · outbound

This paper cites Deeper multi-redshift upper limits on the Epoch of Reionization 21-cm signal power spectrum from LOFAR between z=8.3 and z=10.1.

Semi-analytic modelling of Pop. III star formation and metallicity evolution -- II. Impact on 21cm power spectrum Deeper multi-redshift upper limits on the Epoch of Reionization 21-cm signal power spectrum from LOFAR between z=8.3 and z=10.1

Reference 54

Resolution: unresolved; no resolver link, observed 2026-08-07T23:09:26.886131Z

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Observation 37b56f0d-493e-4160-95c8-d3db340eb8cd · outbound

This paper cites an unresolved cited work.

Semi-analytic modelling of Pop. III star formation and metallicity evolution -- II. Impact on 21cm power spectrum Unresolved cited work

Reference 55

Resolution: unresolved; no resolver link, observed 2026-08-07T23:09:26.889727Z

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Observation 1d7e4c8f-047d-4b43-a4e2-fa808a6e83cf · outbound

This paper cites an unresolved cited work.

Semi-analytic modelling of Pop. III star formation and metallicity evolution -- II. Impact on 21cm power spectrum Unresolved cited work

Reference 56

Resolution: unresolved; no resolver link, observed 2026-08-07T23:09:26.892632Z

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Observation bb8f15cd-8456-45f4-95a6-794e1ff35d99 · outbound

This paper cites an unresolved cited work.

Semi-analytic modelling of Pop. III star formation and metallicity evolution -- II. Impact on 21cm power spectrum Unresolved cited work

Reference 57

Resolution: unresolved; no resolver link, observed 2026-08-07T23:09:26.895846Z

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Observation 5a6afc6f-e608-4f69-b4b7-db6b91578032 · outbound

This paper cites an unresolved cited work.

Semi-analytic modelling of Pop. III star formation and metallicity evolution -- II. Impact on 21cm power spectrum Unresolved cited work

Reference 58

Resolution: verified exact; doi, observed 2026-08-07T23:09:27.343252Z

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Observation afafc70a-047e-4a42-b85b-8a4780c4a556 · outbound

This paper cites F., 2005, @doi [The Astrophysical Journal] 10.1086/426730 , 619, 678.

Semi-analytic modelling of Pop. III star formation and metallicity evolution -- II. Impact on 21cm power spectrum F., 2005, @doi [The Astrophysical Journal] 10.1086/426730 , 619, 678

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Resolution: unresolved; no resolver link, observed 2026-08-07T23:09:26.903596Z

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Observation f1e20bbf-5ec4-4bd4-b90c-fcaf5f4f577e · outbound

This paper cites F., Wyithe J.

Semi-analytic modelling of Pop. III star formation and metallicity evolution -- II. Impact on 21cm power spectrum F., Wyithe J

Reference 60

Resolution: unresolved; no resolver link, observed 2026-08-07T23:09:26.906643Z

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Observation 1d23edd7-337d-48ab-8ea1-081e519b646d · outbound

This paper cites B., 2023, @doi [ ] 10.1093/mnras/stad1512 , https://ui.adsabs.harvard.edu/abs/2023MNRAS.523.2587M 523, 2587.

Semi-analytic modelling of Pop. III star formation and metallicity evolution -- II. Impact on 21cm power spectrum B., 2023, @doi [ ] 10.1093/mnras/stad1512 , https://ui.adsabs.harvard.edu/abs/2023MNRAS.523.2587M 523, 2587

Reference 61

Resolution: unresolved; no resolver link, observed 2026-08-07T23:09:26.909958Z

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Observation 47cd3f64-cb82-45d5-9087-e53c9518cc17 · outbound

This paper cites B., Qin Y., Mesinger A., Murray S.

Semi-analytic modelling of Pop. III star formation and metallicity evolution -- II. Impact on 21cm power spectrum B., Qin Y., Mesinger A., Murray S

Reference 62

Resolution: unresolved; no resolver link, observed 2026-08-07T23:09:26.913055Z

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Observation 52542303-ca9a-46d8-be6c-8ca33c707114 · outbound

This paper cites J., Geil P.

Semi-analytic modelling of Pop. III star formation and metallicity evolution -- II. Impact on 21cm power spectrum J., Geil P

Reference 63

Resolution: unresolved; no resolver link, observed 2026-08-07T23:09:26.916609Z

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Observation f76889f9-5fc3-4b6a-b888-5bb55b7f380a · outbound

This paper cites J., Greig B., Qin Y., Poole G.

Semi-analytic modelling of Pop. III star formation and metallicity evolution -- II. Impact on 21cm power spectrum J., Greig B., Qin Y., Poole G

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Resolution: verified exact; doi, observed 2026-08-07T23:09:27.309028Z

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Observation 1928ff27-a5f9-437a-9758-fb55c460550d · outbound

This paper cites K., Mellema G., 2023, @doi [ ] 10.1093/mnras/stad1852 , https://ui.adsabs.harvard.edu/abs/2023MNRAS.524.2290N 524, 2290.

Semi-analytic modelling of Pop. III star formation and metallicity evolution -- II. Impact on 21cm power spectrum K., Mellema G., 2023, @doi [ ] 10.1093/mnras/stad1852 , https://ui.adsabs.harvard.edu/abs/2023MNRAS.524.2290N 524, 2290

Reference 65

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Observation d18fbb84-1d77-401c-829d-8428cccb7b68 · outbound

This paper cites an unresolved cited work.

Semi-analytic modelling of Pop. III star formation and metallicity evolution -- II. Impact on 21cm power spectrum Unresolved cited work

Reference 66

Resolution: unresolved; no resolver link, observed 2026-08-07T23:09:26.926279Z

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Observation c4768d32-cbbf-4a4a-b82b-7083afed9830 · outbound

This paper cites an unresolved cited work.

Semi-analytic modelling of Pop. III star formation and metallicity evolution -- II. Impact on 21cm power spectrum Unresolved cited work

Reference 67

Resolution: unresolved; no resolver link, observed 2026-08-07T23:09:26.930353Z

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Observation b062b3ee-d440-4a89-9cb7-891f02f0beab · outbound

This paper cites an unresolved cited work.

Semi-analytic modelling of Pop. III star formation and metallicity evolution -- II. Impact on 21cm power spectrum Unresolved cited work

Reference 68

Resolution: unresolved; no resolver link, observed 2026-08-07T23:09:26.934478Z

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Observation 021d8087-9165-42a1-b5a6-9096599eb727 · outbound

This paper cites an unresolved cited work.

Semi-analytic modelling of Pop. III star formation and metallicity evolution -- II. Impact on 21cm power spectrum Unresolved cited work

Reference 69

Resolution: unresolved; no resolver link, observed 2026-08-07T23:09:26.938438Z

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Observation 45cba503-b93a-4412-8c27-4f98b1f3cf17 · outbound

This paper cites R., et al., 2014, @doi [The Astrophysical Journal] 10.1088/0004-637X/788/2/106 , 788, 106.

Semi-analytic modelling of Pop. III star formation and metallicity evolution -- II. Impact on 21cm power spectrum R., et al., 2014, @doi [The Astrophysical Journal] 10.1088/0004-637X/788/2/106 , 788, 106

Reference 70

Resolution: unresolved; no resolver link, observed 2026-08-07T23:09:26.942384Z

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Observation c44316d9-ae61-459e-acf1-4ef2a8376ad4 · outbound

This paper cites an unresolved cited work.

Semi-analytic modelling of Pop. III star formation and metallicity evolution -- II. Impact on 21cm power spectrum Unresolved cited work

Reference 71

Resolution: unresolved; no resolver link, observed 2026-08-07T23:09:26.946248Z

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Observation 362bd239-9f39-4aa7-99ba-d2ea42e0d718 · outbound

This paper cites an unresolved cited work.

Semi-analytic modelling of Pop. III star formation and metallicity evolution -- II. Impact on 21cm power spectrum Unresolved cited work

Reference 72

Resolution: unresolved; no resolver link, observed 2026-08-07T23:09:26.950154Z

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Observation c8ad777e-a113-47c5-a482-de26b6c56c9c · outbound

This paper cites C., et al., 2013, @doi [ ] 10.1088/2041-8205/768/2/L36 , https://ui.adsabs.harvard.edu/abs/2013ApJ...768L..36P 768, L36.

Semi-analytic modelling of Pop. III star formation and metallicity evolution -- II. Impact on 21cm power spectrum C., et al., 2013, @doi [ ] 10.1088/2041-8205/768/2/L36 , https://ui.adsabs.harvard.edu/abs/2013ApJ...768L..36P 768, L36

Reference 73

Resolution: unresolved; no resolver link, observed 2026-08-07T23:09:26.953988Z

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Observation 114db967-8e83-49fa-aa2a-b616ffbadb98 · outbound

This paper cites C., et al., 2014, @doi [ ] 10.1088/0004-637X/788/1/96 , https://ui.adsabs.harvard.edu/abs/2014ApJ...788...96P 788, 96.

Semi-analytic modelling of Pop. III star formation and metallicity evolution -- II. Impact on 21cm power spectrum C., et al., 2014, @doi [ ] 10.1088/0004-637X/788/1/96 , https://ui.adsabs.harvard.edu/abs/2014ApJ...788...96P 788, 96

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Resolution: verified exact; doi, observed 2026-08-07T23:09:27.252835Z

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Observation fab618f6-43a8-45b7-8135-a60ddbb64ded · outbound

This paper cites an unresolved cited work.

Semi-analytic modelling of Pop. III star formation and metallicity evolution -- II. Impact on 21cm power spectrum Unresolved cited work

Reference 75

Resolution: unresolved; no resolver link, observed 2026-08-07T23:09:26.961202Z

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Observation 90c5cc8a-41d3-4f88-8888-9ac5337e4c97 · outbound

This paper cites R., Loeb A., 2012, @doi [Reports on Progress in Physics] 10.1088/0034-4885/75/8/086901 , https://ui.adsabs.harvard.edu/abs/2012RPPh...75h6901P 75, 086901.

Semi-analytic modelling of Pop. III star formation and metallicity evolution -- II. Impact on 21cm power spectrum R., Loeb A., 2012, @doi [Reports on Progress in Physics] 10.1088/0034-4885/75/8/086901 , https://ui.adsabs.harvard.edu/abs/2012RPPh...75h6901P 75, 086901

Reference 76

Resolution: unresolved; no resolver link, observed 2026-08-07T23:09:26.964216Z

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Observation 0ecc58ec-f8f9-4f22-ad2d-d2d1c41c97c9 · outbound

This paper cites an unresolved cited work.

Semi-analytic modelling of Pop. III star formation and metallicity evolution -- II. Impact on 21cm power spectrum Unresolved cited work

Reference 77

Resolution: unresolved; no resolver link, observed 2026-08-07T23:09:26.968221Z

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Observation c2064cd0-11f6-48a4-a901-2a2b5e852c97 · outbound

This paper cites B., 2020, @doi [ ] 10.1093/mnras/staa1131 , https://ui.adsabs.harvard.edu/abs/2020MNRAS.495..123Q 495, 123.

Semi-analytic modelling of Pop. III star formation and metallicity evolution -- II. Impact on 21cm power spectrum B., 2020, @doi [ ] 10.1093/mnras/staa1131 , https://ui.adsabs.harvard.edu/abs/2020MNRAS.495..123Q 495, 123

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Resolution: unresolved; no resolver link, observed 2026-08-07T23:09:26.972174Z

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Observation 402e858b-e125-4fd0-b133-45acf4c36e88 · outbound

This paper cites an unresolved cited work.

Semi-analytic modelling of Pop. III star formation and metallicity evolution -- II. Impact on 21cm power spectrum Unresolved cited work

Reference 79

Resolution: unresolved; no resolver link, observed 2026-08-07T23:09:26.975686Z

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Observation c1416d93-6b3d-42ea-83a5-52cbd16ee096 · outbound

This paper cites an unresolved cited work.

Semi-analytic modelling of Pop. III star formation and metallicity evolution -- II. Impact on 21cm power spectrum Unresolved cited work

Reference 80

Resolution: unresolved; no resolver link, observed 2026-08-07T23:09:26.979174Z

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Observation 94549caf-aa36-456e-90fa-76f2a0666846 · outbound

This paper cites an unresolved cited work.

Semi-analytic modelling of Pop. III star formation and metallicity evolution -- II. Impact on 21cm power spectrum Unresolved cited work

Reference 81

Resolution: unresolved; no resolver link, observed 2026-08-07T23:09:26.982249Z

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Observation a6326925-80a6-4144-a549-84c11d4c0f14 · outbound

This paper cites Percent-level timing of reionization: self-consistent, implicit-likelihood inference from XQR-30+ Ly$\alpha$ forest data.

Semi-analytic modelling of Pop. III star formation and metallicity evolution -- II. Impact on 21cm power spectrum Percent-level timing of reionization: self-consistent, implicit-likelihood inference from XQR-30+ Ly$\alpha$ forest data

Reference 82

Resolution: unresolved; no resolver link, observed 2026-08-07T23:09:26.986170Z

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Observation 9e8c54f0-b0ac-4234-9e97-54212b221b83 · outbound

This paper cites J., da Cunha E., Poole G.

Semi-analytic modelling of Pop. III star formation and metallicity evolution -- II. Impact on 21cm power spectrum J., da Cunha E., Poole G

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Resolution: verified exact; doi, observed 2026-08-07T23:09:27.201243Z

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Observation ee9e734e-1cb0-4ed7-8850-108f6b1c93f2 · outbound

This paper cites an unresolved cited work.

Semi-analytic modelling of Pop. III star formation and metallicity evolution -- II. Impact on 21cm power spectrum Unresolved cited work

Reference 84

Resolution: unresolved; no resolver link, observed 2026-08-07T23:09:26.993550Z

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Observation 0b35f383-081a-487c-965a-b273621ec77d · outbound

This paper cites an unresolved cited work.

Semi-analytic modelling of Pop. III star formation and metallicity evolution -- II. Impact on 21cm power spectrum Unresolved cited work

Reference 85

Resolution: unresolved; no resolver link, observed 2026-08-07T23:09:26.996671Z

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Observation b214813c-8e22-47ef-8133-ce1402184cf5 · outbound

This paper cites an unresolved cited work.

Semi-analytic modelling of Pop. III star formation and metallicity evolution -- II. Impact on 21cm power spectrum Unresolved cited work

Reference 86

Resolution: verified exact; doi, observed 2026-08-07T23:09:27.180656Z

Source-reported events for the cited work

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

Observation 79234cb7-5c8f-447c-a380-c16772d39fa4 · outbound

This paper cites E., Omukai K., Sugimura K., Matsumoto T., Tomida K., 2024, @doi [ ] 10.1093/pasj/psae051 , https://ui.adsabs.harvard.edu/abs/2024PASJ...76..823S 76, 823.

Semi-analytic modelling of Pop. III star formation and metallicity evolution -- II. Impact on 21cm power spectrum E., Omukai K., Sugimura K., Matsumoto T., Tomida K., 2024, @doi [ ] 10.1093/pasj/psae051 , https://ui.adsabs.harvard.edu/abs/2024PASJ...76..823S 76, 823

Reference 87

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Observation 7a9fec4b-2eaa-4bb2-90ca-e8feacdd0dab · outbound

This paper cites S., et al., 2023, @doi [ ] 10.1093/mnras/stad697 , https://ui.adsabs.harvard.edu/abs/2023MNRAS.521.4039S 521, 4039.

Semi-analytic modelling of Pop. III star formation and metallicity evolution -- II. Impact on 21cm power spectrum S., et al., 2023, @doi [ ] 10.1093/mnras/stad697 , https://ui.adsabs.harvard.edu/abs/2023MNRAS.521.4039S 521, 4039

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Resolution: unresolved; no resolver link, observed 2026-08-07T23:09:27.008317Z

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Observation 1c10d208-8f00-48c6-8c36-ce8a6f882bff · outbound

This paper cites an unresolved cited work.

Semi-analytic modelling of Pop. III star formation and metallicity evolution -- II. Impact on 21cm power spectrum Unresolved cited work

Reference 89

Resolution: unresolved; no resolver link, observed 2026-08-07T23:09:27.012240Z

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Observation ce67d146-22c7-4ed8-801f-80cf7f75cbfb · outbound

This paper cites an unresolved cited work.

Semi-analytic modelling of Pop. III star formation and metallicity evolution -- II. Impact on 21cm power spectrum Unresolved cited work

Reference 90

Resolution: unresolved; no resolver link, observed 2026-08-07T23:09:27.016184Z

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Observation d86feddf-c5f7-403c-9b4c-7176440363f4 · outbound

This paper cites an unresolved cited work.

Semi-analytic modelling of Pop. III star formation and metallicity evolution -- II. Impact on 21cm power spectrum Unresolved cited work

Reference 91

Resolution: unresolved; no resolver link, observed 2026-08-07T23:09:27.020160Z

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Observation c00486f1-9210-4a6d-90ad-6f2df50279d8 · outbound

This paper cites Inhomogeneous Energy Injection in the 21-cm Power Spectrum: Sensitivity to Dark Matter Decay.

Semi-analytic modelling of Pop. III star formation and metallicity evolution -- II. Impact on 21cm power spectrum Inhomogeneous Energy Injection in the 21-cm Power Spectrum: Sensitivity to Dark Matter Decay

Reference 92

Resolution: unresolved; no resolver link, observed 2026-08-07T23:09:27.023880Z

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Observation 19c107bc-b600-4a2c-ab5e-7fc54a3b20ea · outbound

This paper cites an unresolved cited work.

Semi-analytic modelling of Pop. III star formation and metallicity evolution -- II. Impact on 21cm power spectrum Unresolved cited work

Reference 93

Resolution: unresolved; no resolver link, observed 2026-08-07T23:09:27.027822Z

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Observation 4b6cc333-33a5-49e3-af7b-6a43ba86016a · outbound

This paper cites M., et al., 2020, @doi [ ] 10.1093/mnras/staa414 , https://ui.adsabs.harvard.edu/abs/2020MNRAS.493.4711T 493, 4711.

Semi-analytic modelling of Pop. III star formation and metallicity evolution -- II. Impact on 21cm power spectrum M., et al., 2020, @doi [ ] 10.1093/mnras/staa414 , https://ui.adsabs.harvard.edu/abs/2020MNRAS.493.4711T 493, 4711

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Resolution: unresolved; no resolver link, observed 2026-08-07T23:09:27.031512Z

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Observation ccad1218-eef8-4205-a03f-eab748f24413 · outbound

This paper cites an unresolved cited work.

Semi-analytic modelling of Pop. III star formation and metallicity evolution -- II. Impact on 21cm power spectrum Unresolved cited work

Reference 95

Resolution: unresolved; no resolver link, observed 2026-08-07T23:09:27.035398Z

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Observation bd53d356-28df-4392-8b13-f254b70cd3a6 · outbound

This paper cites M., Trinca A., Schneider R., Graziani L., Valiante R., Wyithe J.

Semi-analytic modelling of Pop. III star formation and metallicity evolution -- II. Impact on 21cm power spectrum M., Trinca A., Schneider R., Graziani L., Valiante R., Wyithe J

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Resolution: unresolved; no resolver link, observed 2026-08-07T23:09:27.039585Z

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Observation 46d5a671-9413-4b41-90fe-707a2b853396 · outbound

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

Semi-analytic modelling of Pop. III star formation and metallicity evolution -- II. Impact on 21cm power spectrum M., Qin Y., Balu S., Wyithe J

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Resolution: unresolved; no resolver link, observed 2026-08-07T23:09:27.043430Z

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Observation c5ea5b00-f8e2-4edb-b6b5-70d417cf24b1 · outbound

This paper cites L., 2015, @doi [ ] 10.1093/mnras/stv1941 , https://ui.adsabs.harvard.edu/abs/2015MNRAS.453.4456V 453, 4456.

Semi-analytic modelling of Pop. III star formation and metallicity evolution -- II. Impact on 21cm power spectrum L., 2015, @doi [ ] 10.1093/mnras/stv1941 , https://ui.adsabs.harvard.edu/abs/2015MNRAS.453.4456V 453, 4456

Reference 98

Resolution: unresolved; no resolver link, observed 2026-08-07T23:09:27.047300Z

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Observation d98ab3ca-5afa-4095-bfdb-8ecdb1468869 · outbound

This paper cites L., Haiman Z., 2020, @doi [ ] 10.3847/1538-4357/ab994e , https://ui.adsabs.harvard.edu/abs/2020ApJ...897...95V 897, 95.

Semi-analytic modelling of Pop. III star formation and metallicity evolution -- II. Impact on 21cm power spectrum L., Haiman Z., 2020, @doi [ ] 10.3847/1538-4357/ab994e , https://ui.adsabs.harvard.edu/abs/2020ApJ...897...95V 897, 95

Reference 99

Resolution: unresolved; no resolver link, observed 2026-08-07T23:09:27.051342Z

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Observation e34774a1-d519-46d3-a944-fe72274289f8 · outbound

This paper cites an unresolved cited work.

Semi-analytic modelling of Pop. III star formation and metallicity evolution -- II. Impact on 21cm power spectrum Unresolved cited work

Reference 100

Resolution: unresolved; no resolver link, observed 2026-08-07T23:09:27.055124Z

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Outbound references

Pith citing papers