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Paper Citation Record · LEDGER

Can Dark Stars account for the star formation efficiency excess at very high redshifts?

As of 13 August 2026, this Paper Citation Record lists 100 of 111 outbound references and 0 inbound Pith citation observations for arXiv:2501.07119.

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

pith.paper-citation-record.v1
2501.07119 v3

Coverage vector

measured 100 of 111 reference resolution

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Pith citing papers itemized under the disclosed page cap.

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Reference resolution

100 of 111 outbound references displayed

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External citation measurements

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Outbound references

Observation bdac7170-d885-434e-b461-745db3c1f043 · outbound

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

Can Dark Stars account for the star formation efficiency excess at very high redshifts? , " * write output.state after.block = add.period write newline

Reference 1

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Observation b2722cd9-5170-482c-a510-6af894e96878 · outbound

This paper cites write newline.

Can Dark Stars account for the star formation efficiency excess at very high redshifts? write newline

Reference 2

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Observation 819457d2-06fd-4e28-a60f-8c4d550b3849 · outbound

This paper cites Dark matter annihilation effects on the first stars.

Can Dark Stars account for the star formation efficiency excess at very high redshifts? Dark matter annihilation effects on the first stars

Reference 3

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Observation 31292fbd-b86b-4013-a85f-802d07f6b3d2 · outbound

This paper cites J., Conselice , C.

Can Dark Stars account for the star formation efficiency excess at very high redshifts? J., Conselice , C

Reference 4

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Observation 67454c89-a28d-414f-a946-1fecc4abf1e4 · outbound

This paper cites A., Mukhopadhyay , U., Sen , A.

Can Dark Stars account for the star formation efficiency excess at very high redshifts? A., Mukhopadhyay , U., Sen , A

Reference 5

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Observation 215d9f89-71ff-4abf-a1c9-20381907be6f · outbound

This paper cites P., Tollerud , E.

Can Dark Stars account for the star formation efficiency excess at very high redshifts? P., Tollerud , E

Reference 6

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This paper cites M., Sip o cz , B.

Can Dark Stars account for the star formation efficiency excess at very high redshifts? M., Sip o cz , B

Reference 7

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Observation 44046dd5-dfbe-48bb-a786-afffa1db33a4 · outbound

This paper cites M., Lim , P.

Can Dark Stars account for the star formation efficiency excess at very high redshifts? M., Lim , P

Reference 8

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Observation aba0822b-fa1d-453c-99c4-54bde26a3b3c · outbound

This paper cites S., & Silk , J.

Can Dark Stars account for the star formation efficiency excess at very high redshifts? S., & Silk , J

Reference 9

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Observation 1bc731d4-830f-454a-ae51-ff548641a3e8 · outbound

This paper cites 2024, Physics Letters B, 858, 139062, 10.1016/j.physletb.2024.139062.

Can Dark Stars account for the star formation efficiency excess at very high redshifts? 2024, Physics Letters B, 858, 139062, 10.1016/j.physletb.2024.139062

Reference 10

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Observation 49c7f7c0-8aa5-4a4b-a2c7-7808438185cf · outbound

This paper cites 2023 a , MNRAS, 523, 1009, 10.1093/mnras/stad1014.

Can Dark Stars account for the star formation efficiency excess at very high redshifts? 2023 a , MNRAS, 523, 1009, 10.1093/mnras/stad1014

Reference 11

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Observation 48a8730a-faff-408c-9c36-11b73a013b51 · outbound

This paper cites J., Oesch , P.

Can Dark Stars account for the star formation efficiency excess at very high redshifts? J., Oesch , P

Reference 12

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Observation 0aee5195-384c-40a7-994f-c2b6c418406c · outbound

This paper cites J., Stefanon , M., Brammer , G., et al.

Can Dark Stars account for the star formation efficiency excess at very high redshifts? J., Stefanon , M., Brammer , G., et al

Reference 13

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Can Dark Stars account for the star formation efficiency excess at very high redshifts? Unresolved cited work

Reference 14

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This paper cites 2023, Nature Astronomy, 7, 731, 10.1038/s41550-023-01937-7.

Can Dark Stars account for the star formation efficiency excess at very high redshifts? 2023, Nature Astronomy, 7, 731, 10.1038/s41550-023-01937-7

Reference 15

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Observation 6f7abe8b-2363-4ca6-b56b-99df32075eb1 · outbound

This paper cites 2014, , 564, A125, 10.1051/0004-6361/201322971.

Can Dark Stars account for the star formation efficiency excess at very high redshifts? 2014, , 564, A125, 10.1051/0004-6361/201322971

Reference 17

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Observation 121e7bc7-fa7f-427c-a12f-1636706489f7 · outbound

This paper cites J., Cameron , A.

Can Dark Stars account for the star formation efficiency excess at very high redshifts? J., Cameron , A

Reference 18

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Observation cbad6820-e50a-4b1b-b05c-5b9b6c894a7d · outbound

This paper cites C., McLure , R.

Can Dark Stars account for the star formation efficiency excess at very high redshifts? C., McLure , R

Reference 19

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This paper cites C., McLure , R.

Can Dark Stars account for the star formation efficiency excess at very high redshifts? C., McLure , R

Reference 20

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Observation 952d4b19-b0dc-4d92-969b-75afe7b8bd12 · outbound

This paper cites 2021, Rept.

Can Dark Stars account for the star formation efficiency excess at very high redshifts? 2021, Rept

Reference 21

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Observation 0bf345cb-5ed8-48de-aa4c-eb2364090044 · outbound

This paper cites M., Akins , H.

Can Dark Stars account for the star formation efficiency excess at very high redshifts? M., Akins , H

Reference 22

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Observation 56c083a4-8d6c-42d2-b7fc-98267ee9a8d8 · outbound

This paper cites 2022, Science, 376, 170, 10.1126/science.abk1781.

Can Dark Stars account for the star formation efficiency excess at very high redshifts? 2022, Science, 376, 170, 10.1126/science.abk1781

Reference 23

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This paper cites Do high redshift QSOs and GRBs corroborate JWST?.

Can Dark Stars account for the star formation efficiency excess at very high redshifts? Do high redshift QSOs and GRBs corroborate JWST?

Reference 24

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Observation 2d9f4ed8-a927-432a-a525-c1e37660ea69 · outbound

This paper cites S., & Fan , Y.-Z.

Can Dark Stars account for the star formation efficiency excess at very high redshifts? S., & Fan , Y.-Z

Reference 25

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This paper cites 2023, Nature Astronomy, 7, 622, 10.1038/s41550-023-01918-w.

Can Dark Stars account for the star formation efficiency excess at very high redshifts? 2023, Nature Astronomy, 7, 622, 10.1038/s41550-023-01918-w

Reference 26

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

Can Dark Stars account for the star formation efficiency excess at very high redshifts? C., Birnboim , Y., Mandelker , N., & Li , Z

Reference 27

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This paper cites JADES Data Release 3 -- NIRSpec/MSA spectroscopy for 4,000 galaxies in the GOODS fields.

Can Dark Stars account for the star formation efficiency excess at very high redshifts? JADES Data Release 3 -- NIRSpec/MSA spectroscopy for 4,000 galaxies in the GOODS fields

Reference 28

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Can Dark Stars account for the star formation efficiency excess at very high redshifts? T., McLeod , D

Reference 29

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Can Dark Stars account for the star formation efficiency excess at very high redshifts? Overview of the JWST Advanced Deep Extragalactic Survey (JADES)

Reference 30

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This paper cites K., Lupton , R.

Can Dark Stars account for the star formation efficiency excess at very high redshifts? K., Lupton , R

Reference 31

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Can Dark Stars account for the star formation efficiency excess at very high redshifts? S., & Wu , L

Reference 32

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This paper cites P., & Bridges , M.

Can Dark Stars account for the star formation efficiency excess at very high redshifts? P., & Bridges , M

Reference 33

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This paper cites L., Bagley , M.

Can Dark Stars account for the star formation efficiency excess at very high redshifts? L., Bagley , M

Reference 34

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Can Dark Stars account for the star formation efficiency excess at very high redshifts? L., Leung , G

Reference 35

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This paper cites 2008, in American Institute of Physics Conference Series, Vol.

Can Dark Stars account for the star formation efficiency excess at very high redshifts? 2008, in American Institute of Physics Conference Series, Vol

Reference 36

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Can Dark Stars account for the star formation efficiency excess at very high redshifts? 2010, ApJ, 716, 1397, 10.1088/0004-637X/716/2/1397

Reference 37

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Can Dark Stars account for the star formation efficiency excess at very high redshifts? 2016, Reports on Progress in Physics, 79, 066902, 10.1088/0034-4885/79/6/066902

Reference 38

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Observation a6521eeb-e418-4a72-a3d9-3251daa0eeb4 · outbound

This paper cites 2013, in Astrophysics and Space Science Library, Vol.

Can Dark Stars account for the star formation efficiency excess at very high redshifts? 2013, in Astrophysics and Space Science Library, Vol

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Resolution
unresolved
no resolver link, observed 2026-08-10T20:58:09.386560Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T20:58:09.386560Z digest=sha256:35046199c08311d3a705d22ff04693e4d1427e42b6c880fb99702c5061c43462

Observation 81de7bb9-4e84-47e1-8110-0d0a9666a69b · outbound

This paper cites 2022, , 935, 11, 10.3847/1538-4357/ac7fea.

Can Dark Stars account for the star formation efficiency excess at very high redshifts? 2022, , 935, 11, 10.3847/1538-4357/ac7fea

Reference 40

Resolution
verified exact
doi, observed 2026-08-10T20:58:10.242044Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.

source=arxiv_source observed=2026-08-10T20:58:09.390126Z digest=sha256:0cc851cadceced949657fbb9f08b7ec9552f13f3abf1e2f3e66588a79fb4dcb9

Observation 28efe33f-1a71-4a8b-a160-d7186a5c5ff9 · outbound

This paper cites 2023, ApJ, 947, 28, 10.3847/1538-4357/acc109.

Can Dark Stars account for the star formation efficiency excess at very high redshifts? 2023, ApJ, 947, 28, 10.3847/1538-4357/acc109

Reference 41

Resolution
unresolved
no resolver link, observed 2026-08-10T20:58:09.393387Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T20:58:09.393387Z digest=sha256:85272338ef2059170b10669357c9d05a6db15e23379d8e8880c500d26a44b007

Observation 53733b62-459c-4ce3-92cc-873ca9f1b482 · outbound

This paper cites W., & Ramani , H.

Can Dark Stars account for the star formation efficiency excess at very high redshifts? W., & Ramani , H

Reference 42

Resolution
verified exact
doi, observed 2026-08-10T20:58:10.222681Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.

source=arxiv_source observed=2026-08-10T20:58:09.396973Z digest=sha256:a0f4e575b995a0220ce6eeafef17443d54676a8040177cb2fc235618ec0988d4

Observation 832c587c-4a5b-49ca-a9cf-e81d192f356c · outbound

This paper cites E., Strader , J., & Ho , L.

Can Dark Stars account for the star formation efficiency excess at very high redshifts? E., Strader , J., & Ho , L

Reference 43

Resolution
unresolved
no resolver link, observed 2026-08-10T20:58:09.400908Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T20:58:09.400908Z digest=sha256:1e76a70ba37536e7305805e64f077a10265c2e4db7c13069327d964c5ddee1fb

Observation 345666bf-28cb-4e2b-92b2-980033443b8f · outbound

This paper cites 2024, , 960, 56, 10.3847/1538-4357/ad0b7e.

Can Dark Stars account for the star formation efficiency excess at very high redshifts? 2024, , 960, 56, 10.3847/1538-4357/ad0b7e

Reference 44

Resolution
unresolved
no resolver link, observed 2026-08-10T20:58:09.405131Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T20:58:09.405131Z digest=sha256:c9c94b20a9ef3c47bc4847784c5dd1ee2a0f20465d416b59993fe88035558aaa

Observation bafd4a50-9552-44ee-8bdc-06ee15c592fa · outbound

This paper cites 2022 a , ApJS, 259, 20, 10.3847/1538-4365/ac3dfc.

Can Dark Stars account for the star formation efficiency excess at very high redshifts? 2022 a , ApJS, 259, 20, 10.3847/1538-4365/ac3dfc

Reference 45

Resolution
unresolved
no resolver link, observed 2026-08-10T20:58:09.408529Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T20:58:09.408529Z digest=sha256:3652e1865c29a8a71dc70c24ee23656c8bd67f1f42349bb086771f006b5e0a0a

Observation e160233e-616d-4afd-943c-af1364eeacb1 · outbound

This paper cites K., Mawatari , K., et al.

Can Dark Stars account for the star formation efficiency excess at very high redshifts? K., Mawatari , K., et al

Reference 46

Resolution
unresolved
no resolver link, observed 2026-08-10T20:58:09.412216Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T20:58:09.412216Z digest=sha256:c01a148479aaf19cc48d572077ea93777c12ff40730568bd43e24f97ffe5b08a

Observation 32722107-efb0-42e6-b8ed-b52d8bcbd7ce · outbound

This paper cites 2023, ApJS, 265, 5, 10.3847/1538-4365/acaaa9.

Can Dark Stars account for the star formation efficiency excess at very high redshifts? 2023, ApJS, 265, 5, 10.3847/1538-4365/acaaa9

Reference 47

Resolution
unresolved
no resolver link, observed 2026-08-10T20:58:09.416351Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T20:58:09.416351Z digest=sha256:a1113ebb35de479b1c9f7cebe430117e0a889cfdc594688b1ddb65654c2f18a0

Observation 3c880b93-eb23-432e-8b9c-d65bc4895033 · outbound

This paper cites R., Millman, K.

Can Dark Stars account for the star formation efficiency excess at very high redshifts? R., Millman, K

Reference 48

Resolution
unresolved
no resolver link, observed 2026-08-10T20:58:09.420063Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T20:58:09.420063Z digest=sha256:4531ac4d5231a5f7234738f865c26ae086e03d6cefcc5c310bd1e000e918c11d

Observation 32b03d15-f309-4f2d-ad86-c552a5eb73eb · outbound

This paper cites H., & Haghi , H.

Can Dark Stars account for the star formation efficiency excess at very high redshifts? H., & Haghi , H

Reference 49

Resolution
unresolved
no resolver link, observed 2026-08-10T20:58:09.424026Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T20:58:09.424026Z digest=sha256:7a7da751b16712c4926c638e3563d790cfe981f0a11dd943a7d1376d46fdcfbf

Observation 84f06aee-9e42-4990-9554-e29d643f2fe3 · outbound

This paper cites 2011, Physics Letters B, 697, 412, 10.1016/j.physletb.2011.02.029.

Can Dark Stars account for the star formation efficiency excess at very high redshifts? 2011, Physics Letters B, 697, 412, 10.1016/j.physletb.2011.02.029

Reference 50

Resolution
unresolved
no resolver link, observed 2026-08-10T20:58:09.427903Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T20:58:09.427903Z digest=sha256:f6141b80ea6c8b269b77b0abec8dfb6b8a0ba273ce1bf10f298faf99ad11c1b9

Observation 933972f0-c236-46b7-8660-030fda1b1dc9 · outbound

This paper cites an unresolved cited work.

Can Dark Stars account for the star formation efficiency excess at very high redshifts? Unresolved cited work

Reference 51

Resolution
unresolved
no resolver link, observed 2026-08-10T20:58:09.432573Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T20:58:09.432573Z digest=sha256:444ae4f1f272f4d1d7c57a2f6182cbafb944e3de6a2096baa9fb2e35583c424b

Observation 62771956-8a1d-4ce0-b3ce-3b559f797840 · outbound

This paper cites UHZ1 and the other three most distant quasars observed: possible evidence for Supermassive Dark Stars.

Can Dark Stars account for the star formation efficiency excess at very high redshifts? UHZ1 and the other three most distant quasars observed: possible evidence for Supermassive Dark Stars

Reference 52

Resolution
unresolved
no resolver link, observed 2026-08-10T20:58:09.436896Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T20:58:09.436896Z digest=sha256:dc8f6e0fe30be578c349a19a076fffa276b85851a50528bb349f06e3ce4d4352

Observation 178de0de-1c7d-401b-a8e2-aa7a6daca2c4 · outbound

This paper cites T., & Shapiro , P.

Can Dark Stars account for the star formation efficiency excess at very high redshifts? T., & Shapiro , P

Reference 53

Resolution
unresolved
no resolver link, observed 2026-08-10T20:58:09.440753Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T20:58:09.440753Z digest=sha256:051826488ff49fa17718a04a06d8f6ea1d5e32b93909603ef9637c8866b4f5f8

Observation 86718a7a-0a15-4f5b-a707-4ff5237a9fd9 · outbound

This paper cites 2023, Proceedings of the National Academy of Science, 120, e2305762120, 10.1073/pnas.2305762120.

Can Dark Stars account for the star formation efficiency excess at very high redshifts? 2023, Proceedings of the National Academy of Science, 120, e2305762120, 10.1073/pnas.2305762120

Reference 54

Resolution
unresolved
no resolver link, observed 2026-08-10T20:58:09.444913Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T20:58:09.444913Z digest=sha256:4f5a45c4507aadff2d66fa9b2a2383ed3fa305ccbaa6bd46ad379f561b2444c6

Observation 2bb99acf-788c-4a45-ac26-d93c2b5f0e2f · outbound

This paper cites K., Li , W., & Ho , L.

Can Dark Stars account for the star formation efficiency excess at very high redshifts? K., Li , W., & Ho , L

Reference 55

Resolution
unresolved
no resolver link, observed 2026-08-10T20:58:09.448770Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T20:58:09.448770Z digest=sha256:89efdd16ce0f1d1402b910135b0679573ceb5977f97730a580aa996df56f3daf

Observation 9a78850a-63e0-4138-a501-723c600c792f · outbound

This paper cites 2010, PoS, CRF2010, 018, 10.22323/1.121.0018.

Can Dark Stars account for the star formation efficiency excess at very high redshifts? 2010, PoS, CRF2010, 018, 10.22323/1.121.0018

Reference 56

Resolution
verified exact
doi, observed 2026-08-10T20:58:10.130909Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.

source=arxiv_source observed=2026-08-10T20:58:09.452794Z digest=sha256:e1167f453978bffe33af061c5feb208669689e97533e024083a78b0a8f07308d

Observation a786e15e-701d-4d03-b23f-9127892aeb87 · outbound

This paper cites 2008, MNRAS, 390, 1655, 10.1111/j.1365-2966.2008.13853.x.

Can Dark Stars account for the star formation efficiency excess at very high redshifts? 2008, MNRAS, 390, 1655, 10.1111/j.1365-2966.2008.13853.x

Reference 58

Resolution
unresolved
no resolver link, observed 2026-08-10T20:58:09.460779Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T20:58:09.460779Z digest=sha256:b667305295c5154466c3151868185a9d0b9e5e67de27ea69bb548e586f35cacb

Observation a2641e7e-89c3-4c06-b55f-00db9da715be · outbound

This paper cites 2024, Phys.

Can Dark Stars account for the star formation efficiency excess at very high redshifts? 2024, Phys

Reference 59

Resolution
unresolved
no resolver link, observed 2026-08-10T20:58:09.464182Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T20:58:09.464182Z digest=sha256:d7e170d0226e463d3e0e150411270b48ce11e44d03c026e7d8726e2982c34d0b

Observation dadb773c-339b-4bcb-b39c-af3bdad25afd · outbound

This paper cites 2023, , 108, 043510, 10.1103/PhysRevD.108.043510.

Can Dark Stars account for the star formation efficiency excess at very high redshifts? 2023, , 108, 043510, 10.1103/PhysRevD.108.043510

Reference 60

Resolution
unresolved
no resolver link, observed 2026-08-10T20:58:09.467967Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T20:58:09.467967Z digest=sha256:9f4271f7bc2a31c978b2588ddc304bfa7c56a4b3c7957b2bd881f7521dd6f08a

Observation 3a47be25-6711-42e7-af6d-cda28e7b5082 · outbound

This paper cites an unresolved cited work.

Can Dark Stars account for the star formation efficiency excess at very high redshifts? Unresolved cited work

Reference 61

Resolution
verified exact
doi, observed 2026-08-10T20:58:10.111561Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.

source=arxiv_source observed=2026-08-10T20:58:09.471623Z digest=sha256:89afe1c3dd10605a5f4933d040638a338500a54a838ca385f3e79bf86bbaea7e

Observation 649f5125-75ad-4ff9-8f4d-42195498a683 · outbound

This paper cites an unresolved cited work.

Can Dark Stars account for the star formation efficiency excess at very high redshifts? Unresolved cited work

Reference 62

Resolution
unresolved
no resolver link, observed 2026-08-10T20:58:09.475436Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T20:58:09.475436Z digest=sha256:bdbd4ae50f09809371810286d8015338438e70fecde755f365bd7bbc164c2aef

Observation 4a8e04eb-c556-4c05-a99e-b463ff8f30bf · outbound

This paper cites S., & Glover , S.

Can Dark Stars account for the star formation efficiency excess at very high redshifts? S., & Glover , S

Reference 63

Resolution
unresolved
no resolver link, observed 2026-08-10T20:58:09.479982Z

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Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T20:58:09.479982Z digest=sha256:d3c1a181583f1a320034055508516335554e1f4acf90ceef4e2414d1116aeae1

Observation 9a71ff7a-9407-48ea-88bf-4ee68d2c775e · outbound

This paper cites 2023, , 616, 266, 10.1038/s41586-023-05786-2.

Can Dark Stars account for the star formation efficiency excess at very high redshifts? 2023, , 616, 266, 10.1038/s41586-023-05786-2

Reference 64

Resolution
unresolved
no resolver link, observed 2026-08-10T20:58:09.483870Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T20:58:09.483870Z digest=sha256:ba7f0e49c2729e02ceccfc30204d40c20cf95a1e0bd0bf3b28a7069c0f9f30aa

Observation e2883916-18c6-4a39-be53-95b5bc0d1884 · outbound

This paper cites 2000, ApJ, 538, 473, 10.1086/309179.

Can Dark Stars account for the star formation efficiency excess at very high redshifts? 2000, ApJ, 538, 473, 10.1086/309179

Reference 65

Resolution
unresolved
no resolver link, observed 2026-08-10T20:58:09.487782Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T20:58:09.487782Z digest=sha256:de61c9136d0ff4b25af432b1a01157eb4477e871471af4b6a3088cd28c9ee7dd

Observation a6e4dc45-ef4e-4abd-97ea-a53bcedea8a5 · outbound

This paper cites C., et al.

Can Dark Stars account for the star formation efficiency excess at very high redshifts? C., et al

Reference 66

Resolution
unresolved
no resolver link, observed 2026-08-10T20:58:09.491815Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T20:58:09.491815Z digest=sha256:855109a571e10835d75d9b605332246b6cc106157636a7aebc0e9c8799caeeb1

Observation aca4e74a-0fbf-4b4a-bb93-d77bb1f29c36 · outbound

This paper cites 2024, Research in Astronomy and Astrophysics, 24, 015009, 10.1088/1674-4527/ad0864.

Can Dark Stars account for the star formation efficiency excess at very high redshifts? 2024, Research in Astronomy and Astrophysics, 24, 015009, 10.1088/1674-4527/ad0864

Reference 67

Resolution
unresolved
no resolver link, observed 2026-08-10T20:58:09.496276Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T20:58:09.496276Z digest=sha256:738fdc86d816be29cb3c8efc5b7d011077ab422bb55f014d74fb8fca45400f1a

Observation e06e9a6e-1fe6-425a-b544-ddec6fa5c3c8 · outbound

This paper cites C., Harrison , I., Harikane , Y., Tacchella , S., & Wilkins , S.

Can Dark Stars account for the star formation efficiency excess at very high redshifts? C., Harrison , I., Harikane , Y., Tacchella , S., & Wilkins , S

Reference 68

Resolution
unresolved
no resolver link, observed 2026-08-10T20:58:09.500253Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T20:58:09.500253Z digest=sha256:d834f666c9f15a61b17dec2f94ed017ef2bdcc50bab80b76b7e10b4076786f69

Observation 9547bb72-2212-49c8-b0a0-17ce01d50ad7 · outbound

This paper cites 2014, ARA&A, 52, 415, 10.1146/annurev-astro-081811-125615.

Can Dark Stars account for the star formation efficiency excess at very high redshifts? 2014, ARA&A, 52, 415, 10.1146/annurev-astro-081811-125615

Reference 69

Resolution
unresolved
no resolver link, observed 2026-08-10T20:58:09.504420Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T20:58:09.504420Z digest=sha256:7a1aaeea15baa0da6978da45dd50b131c51e30dc0caf24e3a8dab07a862184e8

Observation 9d3666ac-2db2-4207-a57a-a51b65d81a2c · outbound

This paper cites 2012, , 745, 166, 10.1088/0004-637X/745/2/166.

Can Dark Stars account for the star formation efficiency excess at very high redshifts? 2012, , 745, 166, 10.1088/0004-637X/745/2/166

Reference 70

Resolution
unresolved
no resolver link, observed 2026-08-10T20:58:09.508192Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T20:58:09.508192Z digest=sha256:1d142768ccc946575e0432b999182a5b3f6a0f9185ff5b1d498035b4975aa315

Observation 276e8cb9-7997-42b3-a533-c2403f358a10 · outbound

This paper cites J., Donnan , C.

Can Dark Stars account for the star formation efficiency excess at very high redshifts? J., Donnan , C

Reference 71

Resolution
unresolved
no resolver link, observed 2026-08-10T20:58:09.511685Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T20:58:09.511685Z digest=sha256:3ca029c484e384d0ad1f1691f8b91abe7beb29ea48841c925dde7227b1dc84fe

Observation af4d4a2f-bc6a-4761-ae22-cbd96bb4ae2f · outbound

This paper cites A., Mukhopadhyay, U., Sen, A.

Can Dark Stars account for the star formation efficiency excess at very high redshifts? A., Mukhopadhyay, U., Sen, A

Reference 72

Resolution
unresolved
no resolver link, observed 2026-08-10T20:58:09.515238Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T20:58:09.515238Z digest=sha256:d95ff19f2f30f83cc5e63e4ac7f1290dac6a73b3a295392178fcfb3575a828a0

Observation 93caa018-6bd5-4e6d-8dbe-4668c6c95470 · outbound

This paper cites 1998, , 501, 15, 10.1086/305799.

Can Dark Stars account for the star formation efficiency excess at very high redshifts? 1998, , 501, 15, 10.1086/305799

Reference 73

Resolution
unresolved
no resolver link, observed 2026-08-10T20:58:09.519192Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T20:58:09.519192Z digest=sha256:dd875deb5e12017cabc0f932b40f3b7309eaf054a324009a9ab47ff3e9fd0b6c

Observation 7bdb149c-c2eb-45a4-bc71-a53b97ac8d38 · outbound

This paper cites 2023, ApJL, 946, L35, 10.3847/2041-8213/acbf50.

Can Dark Stars account for the star formation efficiency excess at very high redshifts? 2023, ApJL, 946, L35, 10.3847/2041-8213/acbf50

Reference 74

Resolution
unresolved
no resolver link, observed 2026-08-10T20:58:09.523490Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T20:58:09.523490Z digest=sha256:7b3cd414e11b7898a27c04016a09ae97ef04fd8d0a99eb3b735c22248eed9982

Observation a0d16748-cab4-4a1d-9d72-e1e705619771 · outbound

This paper cites G., Power , C., & Robotham , A.

Can Dark Stars account for the star formation efficiency excess at very high redshifts? G., Power , C., & Robotham , A

Reference 75

Resolution
unresolved
no resolver link, observed 2026-08-10T20:58:09.528447Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T20:58:09.528447Z digest=sha256:f95f395cff15127b5fbc71659d159821e131bbfeed4053e50bed4804d0dd487a

Observation cd80ac56-598b-4508-b7aa-2505bba1225b · outbound

This paper cites P., Oesch , P.

Can Dark Stars account for the star formation efficiency excess at very high redshifts? P., Oesch , P

Reference 76

Resolution
unresolved
no resolver link, observed 2026-08-10T20:58:09.532179Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T20:58:09.532179Z digest=sha256:b7e12a919b2ca3528545d4af081c689ec05c4709ae6f8d682a82f8267956c627

Observation e2e35faa-ecc4-49c3-9417-381881869a5d · outbound

This paper cites C., & O'Shea , B.

Can Dark Stars account for the star formation efficiency excess at very high redshifts? C., & O'Shea , B

Reference 77

Resolution
unresolved
no resolver link, observed 2026-08-10T20:58:09.535831Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T20:58:09.535831Z digest=sha256:0334f28358f499d99822ed6b6f128fd48cdb1b593adff82f08d7c4ff74e5bff7

Observation 146a4ae7-8266-4498-b1d9-8a9736a8e2d2 · outbound

This paper cites 2023, Astronomy, 2, 90, 10.3390/astronomy2020007.

Can Dark Stars account for the star formation efficiency excess at very high redshifts? 2023, Astronomy, 2, 90, 10.3390/astronomy2020007

Reference 78

Resolution
verified exact
doi, observed 2026-08-10T20:58:09.989100Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.

source=arxiv_source observed=2026-08-10T20:58:09.539513Z digest=sha256:e63b758ca61b08d30457b03af4d69f3fbb697110114e575fa634cfb55643e701

Observation d10009f5-af42-43f1-8e39-1a02d09d1c5c · outbound

This paper cites M., Kaiser , N., Kelly , P.

Can Dark Stars account for the star formation efficiency excess at very high redshifts? M., Kaiser , N., Kelly , P

Reference 79

Resolution
unresolved
no resolver link, observed 2026-08-10T20:58:09.543529Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T20:58:09.543529Z digest=sha256:a59bd061c945b925991021383cf3e27fd6b2fe41e6dc6a3e72b50c0e52c129fe

Observation fa861f58-b0b1-494c-80c6-b021228f0a5a · outbound

This paper cites B., & Gunn , J.

Can Dark Stars account for the star formation efficiency excess at very high redshifts? B., & Gunn , J

Reference 80

Resolution
unresolved
no resolver link, observed 2026-08-10T20:58:09.547553Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T20:58:09.547553Z digest=sha256:ecdd4cfecab7782936fc8af13730e89fc31d9a79f849b9d90a39ffc631b30e63

Observation 453bd315-98fe-4a3d-a992-8decc0f62bfd · outbound

This paper cites G., Costantin , L., Langeroodi , D., et al.

Can Dark Stars account for the star formation efficiency excess at very high redshifts? G., Costantin , L., Langeroodi , D., et al

Reference 81

Resolution
unresolved
no resolver link, observed 2026-08-10T20:58:09.551604Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T20:58:09.551604Z digest=sha256:df443676bac1469b7689ae82d2f890e8a2c0a17d530b3cd78113b3edeaf24203

Observation 8f07828d-f442-448e-a869-736cf4beb32f · outbound

This paper cites 2020, A&A, 641, A6, 10.1051/0004-6361/201833910.

Can Dark Stars account for the star formation efficiency excess at very high redshifts? 2020, A&A, 641, A6, 10.1051/0004-6361/201833910

Reference 82

Resolution
unresolved
no resolver link, observed 2026-08-10T20:58:09.555380Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T20:58:09.555380Z digest=sha256:d162d49ae4d08a09e30f882413dfdfb4c2021d9ebafe8da62f9671ce680e2595

Observation 6766cf11-ddb4-4661-9a95-9ae7ec7de7bc · outbound

This paper cites B., Liu , H., & Slatyer , T.

Can Dark Stars account for the star formation efficiency excess at very high redshifts? B., Liu , H., & Slatyer , T

Reference 83

Resolution
verified exact
doi, observed 2026-08-10T20:58:09.947617Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.

source=arxiv_source observed=2026-08-10T20:58:09.558756Z digest=sha256:8735273805e95203d0aeab3e171602e8715ce037f25fc2796ecf50feae371545

Observation f6519e44-1bc8-4d02-9f09-f5e75a2b6490 · outbound

This paper cites S., Bower , R., Frenk , C.

Can Dark Stars account for the star formation efficiency excess at very high redshifts? S., Bower , R., Frenk , C

Reference 84

Resolution
unresolved
no resolver link, observed 2026-08-10T20:58:09.562616Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T20:58:09.562616Z digest=sha256:1287079f50fa0e6fe75cc085c6daf989cfac5f47643f08cecb6bcb69d11964ec

Observation 125c5c29-0f45-4686-8e6a-ab5e0f391d35 · outbound

This paper cites 2023, Data from the JWST Advanced Deep Extragalactic Survey (JADES), STScI/MAST, 10.17909/8TDJ-8N28.

Can Dark Stars account for the star formation efficiency excess at very high redshifts? 2023, Data from the JWST Advanced Deep Extragalactic Survey (JADES), STScI/MAST, 10.17909/8TDJ-8N28

Reference 85

Resolution
unresolved
no resolver link, observed 2026-08-10T20:58:09.566136Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T20:58:09.566136Z digest=sha256:2e33b67b284b2ca32fb33eb483b46ba25f3502df2c4bc0259ef44c687835ce39

Observation d385a439-7bd8-4d1b-9667-64f28cf72c96 · outbound

This paper cites an unresolved cited work.

Can Dark Stars account for the star formation efficiency excess at very high redshifts? Unresolved cited work

Reference 86

Resolution
unresolved
no resolver link, observed 2026-08-10T20:58:09.570192Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T20:58:09.570192Z digest=sha256:25d78f0e13b23b2d7394c50dc8e2206331d2c0272881d47fd2c261c970126be6

Observation 3679558e-7f92-4d9a-b3cb-3a472b063912 · outbound

This paper cites 2011, , 2011, 018, 10.1088/1475-7516/2011/01/018.

Can Dark Stars account for the star formation efficiency excess at very high redshifts? 2011, , 2011, 018, 10.1088/1475-7516/2011/01/018

Reference 87

Resolution
verified exact
doi, observed 2026-08-10T20:58:09.919972Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.

source=arxiv_source observed=2026-08-10T20:58:09.574307Z digest=sha256:838bc65f31b02af9fbcd9aebdc317cda8e3778920c0bed6696875fff0f72e429

Observation ee85f8b8-ff33-49df-a475-7e4f23761062 · outbound

This paper cites 2012, , 85, 083519, 10.1103/PhysRevD.85.083519.

Can Dark Stars account for the star formation efficiency excess at very high redshifts? 2012, , 85, 083519, 10.1103/PhysRevD.85.083519

Reference 88

Resolution
verified exact
doi, observed 2026-08-10T20:58:09.908526Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.

source=arxiv_source observed=2026-08-10T20:58:09.578271Z digest=sha256:ffd4918513ee21b3797e4a6696e8d002cee27d9d7b2050b1695d7b15bfa36fd3

Observation 3be580ca-8717-4ab5-b4b6-50597878e052 · outbound

This paper cites an unresolved cited work.

Can Dark Stars account for the star formation efficiency excess at very high redshifts? Unresolved cited work

Reference 89

Resolution
verified exact
doi, observed 2026-08-10T20:58:09.897011Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.

source=arxiv_source observed=2026-08-10T20:58:09.582239Z digest=sha256:87c8f14452f97d968203c1326185e3d248e05e09b15a2ba19c28968cb9cf6a8b

Observation eae18191-b5a6-44ed-9679-68c3457ef2d0 · outbound

This paper cites 2011, , 742, 129, 10.1088/0004-637X/742/2/129.

Can Dark Stars account for the star formation efficiency excess at very high redshifts? 2011, , 742, 129, 10.1088/0004-637X/742/2/129

Reference 90

Resolution
verified exact
doi, observed 2026-08-10T20:58:09.884258Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.

source=arxiv_source observed=2026-08-10T20:58:09.585978Z digest=sha256:3c175106d95fedad435159c772b3b1539aca0d9003fd9a53aabf785885362e93

Observation 67d999b6-44cb-4759-be6f-0778514490bc · outbound

This paper cites J., Iocco , F., Glover , S.

Can Dark Stars account for the star formation efficiency excess at very high redshifts? J., Iocco , F., Glover , S

Reference 91

Resolution
verified exact
doi, observed 2026-08-10T20:58:09.872062Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.

source=arxiv_source observed=2026-08-10T20:58:09.589389Z digest=sha256:6c085daa79e958391a1943eb14ba5c003773e3843043a855d19cff3fe4e161ec

Observation 3b350511-f213-4754-b835-4aaf9d909de0 · outbound

This paper cites S., & Dav \'e , R.

Can Dark Stars account for the star formation efficiency excess at very high redshifts? S., & Dav \'e , R

Reference 92

Resolution
unresolved
no resolver link, observed 2026-08-10T20:58:09.593098Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T20:58:09.593098Z digest=sha256:778bd06276878bbbb977a6c7ed921b905f120b19a1cb3126412d955425dc8bd0

Observation e2398ac6-8591-45f6-9d9e-d1bb0ec728e5 · outbound

This paper cites An inflation model for massive primordial black holes to interpret the JWST observations.

Can Dark Stars account for the star formation efficiency excess at very high redshifts? An inflation model for massive primordial black holes to interpret the JWST observations

Reference 93

Resolution
unresolved
no resolver link, observed 2026-08-10T20:58:09.597047Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T20:58:09.597047Z digest=sha256:c643ae85d06e37af3b85bedd3eda462fcd86621b04d2e384da1cf78b16926812

Observation f0b67104-4a7b-4669-9c7d-06769aeff9a7 · outbound

This paper cites L., Graziani , L., & Schneider , R.

Can Dark Stars account for the star formation efficiency excess at very high redshifts? L., Graziani , L., & Schneider , R

Reference 94

Resolution
unresolved
no resolver link, observed 2026-08-10T20:58:09.601230Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T20:58:09.601230Z digest=sha256:3f75efb6f004a27e9d80f6c5e55f2632e95936fe724bd424fe177a0d74946a94

Observation c9d3c9db-66f5-47f3-9197-69b3844e6de3 · outbound

This paper cites E., et al.

Can Dark Stars account for the star formation efficiency excess at very high redshifts? E., et al

Reference 95

Resolution
unresolved
no resolver link, observed 2026-08-10T20:58:09.605817Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T20:58:09.605817Z digest=sha256:884500c452d440d0fb14e57e97a883065eecaacecde540103e98b422c00c5f6c

Observation 1b7d847f-91dd-478b-9857-c59294985a7a · outbound

This paper cites 2021, Nature Reviews Physics, 3, 732, 10.1038/s42254-021-00364-9.

Can Dark Stars account for the star formation efficiency excess at very high redshifts? 2021, Nature Reviews Physics, 3, 732, 10.1038/s42254-021-00364-9

Reference 96

Resolution
unresolved
no resolver link, observed 2026-08-10T20:58:09.610067Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T20:58:09.610067Z digest=sha256:3c4ade26cc010e580fc33b4bc6d418ffcd83964e4ada67754327db9f4aa93ee9

Observation efecb5f9-bb86-4b90-9764-cbc1998702b1 · outbound

This paper cites 2024 a , Research in Astronomy and Astrophysics, 24, 045001, 10.1088/1674-4527/ad2cd3.

Can Dark Stars account for the star formation efficiency excess at very high redshifts? 2024 a , Research in Astronomy and Astrophysics, 24, 045001, 10.1088/1674-4527/ad2cd3

Reference 97

Resolution
unresolved
no resolver link, observed 2026-08-10T20:58:09.613827Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T20:58:09.613827Z digest=sha256:10e3b31ab42b6beb08a5298ad2703aedaa53d3d2e5ae8b1c8f0aa44e2f01ac31

Observation 700f0391-c61f-4513-9f28-570976f143e6 · outbound

This paper cites 2024 b , European Physical Journal Plus, 139, 711, 10.1140/epjp/s13360-024-05276-y.

Can Dark Stars account for the star formation efficiency excess at very high redshifts? 2024 b , European Physical Journal Plus, 139, 711, 10.1140/epjp/s13360-024-05276-y

Reference 98

Resolution
unresolved
no resolver link, observed 2026-08-10T20:58:09.617706Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T20:58:09.617706Z digest=sha256:10d98f1d5d3c9c805e6acb0a9472a8539d730f9648335fa77d7fae4e1085726d

Observation 7027f71a-68fb-4981-af48-5c6555dee74b · outbound

This paper cites 2023 a , ApJL, 954, L48, 10.3847/2041-8213/acf46c.

Can Dark Stars account for the star formation efficiency excess at very high redshifts? 2023 a , ApJL, 954, L48, 10.3847/2041-8213/acf46c

Reference 99

Resolution
unresolved
no resolver link, observed 2026-08-10T20:58:09.621172Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T20:58:09.621172Z digest=sha256:1bb89e732534d8b6de36523a44085a1b44f8299472afd6a03bcf7a1be1eda26c

Observation 4c7f45ab-dde1-4e35-a579-e15a892fa488 · outbound

This paper cites 2023 b , Science China Physics, Mechanics, and Astronomy, 66, 120403, 10.1007/s11433-023-2262-0.

Can Dark Stars account for the star formation efficiency excess at very high redshifts? 2023 b , Science China Physics, Mechanics, and Astronomy, 66, 120403, 10.1007/s11433-023-2262-0

Reference 100

Resolution
unresolved
no resolver link, observed 2026-08-10T20:58:09.624736Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T20:58:09.624736Z digest=sha256:390f1aba963cd94d796404b6d83cd0dc70b44bcbb2dabb8785c1f3bfbace2e18

Observation a725ad7a-60af-43d7-8d2a-586e5938feea · outbound

This paper cites H., & Tinker , J.

Can Dark Stars account for the star formation efficiency excess at very high redshifts? H., & Tinker , J

Reference 101

Resolution
unresolved
no resolver link, observed 2026-08-10T20:58:09.628907Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-10T20:58:09.628907Z digest=sha256:203cd3258ca6b55b580705d6c3ae95b9f77ca9470f084be24594e9077ecab930

Pith citing papers

No inbound Pith citation observations are available.