Paper Citation Record · LEDGER

No evidence (yet) for increased star-formation efficiency at early times

As of 14 August 2026, this Paper Citation Record lists 100 of 121 outbound references and 8 inbound Pith citation observations for arXiv:2501.03217.

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

pith.paper-citation-record.v1
2501.03217 v2

Coverage vector

measured 100 of 121 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links, observed 2026-08-10T21:58:22.257434Z

measured 108 of 108 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-14T06:32:32.682623+00:00

measured 8 of 8 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-12T00:06:12.089404Z

measured 1 of 1 external citation measurements

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

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

Reference resolution

100 of 121 outbound references displayed

verified exact1
verified fuzzy0
unresolved98
parse uncertain0
malformed identifier0
metadata mismatch1

External citation measurements

1
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

Observation 1f3b03b7-1336-45c3-8fd5-037827b868f3 · outbound

This paper cites write newline.

No evidence (yet) for increased star-formation efficiency at early times write newline

Reference 1

Resolution: unresolved; no resolver link, observed 2026-08-10T21:58:21.566906Z

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Unavailable: canonical work link unavailable.

Observation d48a5694-7b0e-4a76-96a4-10f035cb7bac · outbound

This paper cites The total rest-frame UV luminosity function from $3 < z < 5$: A simultaneous study of AGN and galaxies from $-28<M_{\rm UV}<-16$.

No evidence (yet) for increased star-formation efficiency at early times The total rest-frame UV luminosity function from $3 < z < 5$: A simultaneous study of AGN and galaxies from $-28<M_{\rm UV}<-16$

Reference 2

Resolution: unresolved; no resolver link, observed 2026-08-10T21:58:21.586078Z

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Observation 4398e36c-e294-4346-a6d5-b82379da7cd0 · outbound

This paper cites EPOCHS Paper II: The Ultraviolet Luminosity Function from $7.5<z<13.5$ using 180 square arcminutes of deep, blank-fields from the PEARLS Survey and Public JWST data.

No evidence (yet) for increased star-formation efficiency at early times EPOCHS Paper II: The Ultraviolet Luminosity Function from $7.5<z<13.5$ using 180 square arcminutes of deep, blank-fields from the PEARLS Survey and Public JWST data

Reference 3

Resolution: unresolved; no resolver link, observed 2026-08-10T21:58:21.597518Z

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Unavailable: canonical work link unavailable.

Observation 732b0073-4cf4-4c43-921b-aa7d7371f563 · outbound

This paper cites an unresolved cited work.

No evidence (yet) for increased star-formation efficiency at early times Unresolved cited work

Reference 4

Resolution: unresolved; no resolver link, observed 2026-08-10T21:58:21.602759Z

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Observation 2bc9f56b-48e9-4aa9-8bd4-d295205086e2 · outbound

This paper cites an unresolved cited work.

No evidence (yet) for increased star-formation efficiency at early times Unresolved cited work

Reference 5

Resolution: unresolved; no resolver link, observed 2026-08-10T21:58:21.608098Z

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Observation 5035eb66-a7c9-4e8f-b873-52fe8dbde518 · outbound

This paper cites The Next Generation Deep Extragalactic Exploratory Public (NGDEEP) Survey.

No evidence (yet) for increased star-formation efficiency at early times The Next Generation Deep Extragalactic Exploratory Public (NGDEEP) Survey

Reference 6

Resolution: unresolved; no resolver link, observed 2026-08-10T21:58:21.614940Z

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Unavailable: canonical work link unavailable.

Observation 5155af1e-e834-4963-9540-7401268d3c67 · outbound

This paper cites B., et al., 2024, @doi [ ] 10.3847/2041-8213/ad2f31 , https://ui.adsabs.harvard.edu/abs/2024ApJ...965L...6B 965, L6.

No evidence (yet) for increased star-formation efficiency at early times B., et al., 2024, @doi [ ] 10.3847/2041-8213/ad2f31 , https://ui.adsabs.harvard.edu/abs/2024ApJ...965L...6B 965, L6

Reference 7

Resolution: unresolved; no resolver link, observed 2026-08-10T21:58:21.619727Z

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Observation 5f9fcffd-cc8d-4398-9216-2ff6607ffe30 · outbound

This paper cites an unresolved cited work.

No evidence (yet) for increased star-formation efficiency at early times Unresolved cited work

Reference 8

Resolution: unresolved; no resolver link, observed 2026-08-10T21:58:21.625055Z

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Observation 13b1364e-6e92-4ae2-8ec0-e557383b2c34 · outbound

This paper cites The evolution of [OIII]$+\rm{H}\beta$ equivalent width from $\mathbf{z\simeq3-8}$: implications for the production and escape of ionizing photons during reionization.

No evidence (yet) for increased star-formation efficiency at early times The evolution of [OIII]$+\rm{H}\beta$ equivalent width from $\mathbf{z\simeq3-8}$: implications for the production and escape of ionizing photons during reionization

Reference 9

Resolution: unresolved; no resolver link, observed 2026-08-10T21:58:21.630770Z

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Observation b24e4de7-41af-4dd6-a0ec-f82adbf4bb2d · outbound

This paper cites S., Conroy C., Wechsler R.

No evidence (yet) for increased star-formation efficiency at early times S., Conroy C., Wechsler R

Reference 10

Resolution: unresolved; no resolver link, observed 2026-08-10T21:58:21.639438Z

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Observation c336aafd-204b-4723-a9ae-7dcf218a69ea · outbound

This paper cites S., Wechsler R.

No evidence (yet) for increased star-formation efficiency at early times S., Wechsler R

Reference 11

Resolution: unresolved; no resolver link, observed 2026-08-10T21:58:21.646058Z

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Observation f5750445-a16a-4a0f-9b38-bfa8e92e9810 · outbound

This paper cites an unresolved cited work.

No evidence (yet) for increased star-formation efficiency at early times Unresolved cited work

Reference 12

Resolution: unresolved; no resolver link, observed 2026-08-10T21:58:21.655624Z

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Observation 224b5e53-0942-4850-af7d-fe01d886cfa5 · outbound

This paper cites J., Illingworth G.

No evidence (yet) for increased star-formation efficiency at early times J., Illingworth G

Reference 13

Resolution: unresolved; no resolver link, observed 2026-08-10T21:58:21.661470Z

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Observation 7bb1c584-2906-415f-a8b6-fd2ef3b3a9e3 · outbound

This paper cites an unresolved cited work.

No evidence (yet) for increased star-formation efficiency at early times Unresolved cited work

Reference 14

Resolution: unresolved; no resolver link, observed 2026-08-10T21:58:21.667340Z

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Observation 3878cc2e-d6d1-4ea1-92bd-3bf7a244bac2 · outbound

This paper cites J., et al., 2021, @doi [ ] 10.3847/1538-3881/abf83e , https://ui.adsabs.harvard.edu/abs/2021AJ....162...47B 162, 47.

No evidence (yet) for increased star-formation efficiency at early times J., et al., 2021, @doi [ ] 10.3847/1538-3881/abf83e , https://ui.adsabs.harvard.edu/abs/2021AJ....162...47B 162, 47

Reference 15

Resolution: unresolved; no resolver link, observed 2026-08-10T21:58:21.674981Z

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Observation 019a1faf-51d8-428a-ada1-ce78209b409c · outbound

This paper cites J., et al., 2023, @doi [ ] 10.1093/mnras/stad1145 , https://ui.adsabs.harvard.edu/abs/2023MNRAS.523.1036B 523, 1036.

No evidence (yet) for increased star-formation efficiency at early times J., et al., 2023, @doi [ ] 10.1093/mnras/stad1145 , https://ui.adsabs.harvard.edu/abs/2023MNRAS.523.1036B 523, 1036

Reference 16

Resolution: unresolved; no resolver link, observed 2026-08-10T21:58:21.685157Z

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Observation 7dd05065-4ae1-4114-92ce-3522cd834fd2 · outbound

This paper cites an unresolved cited work.

No evidence (yet) for increased star-formation efficiency at early times Unresolved cited work

Reference 17

Resolution: unresolved; no resolver link, observed 2026-08-10T21:58:21.690168Z

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Observation 939ff4c3-2eed-40df-8c72-cc67e68c6f08 · outbound

This paper cites an unresolved cited work.

No evidence (yet) for increased star-formation efficiency at early times Unresolved cited work

Reference 18

Resolution: unresolved; no resolver link, observed 2026-08-10T21:58:21.706035Z

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Observation a3f1f1ba-a4b5-45b4-bd39-94ee58bbde53 · outbound

This paper cites an unresolved cited work.

No evidence (yet) for increased star-formation efficiency at early times Unresolved cited work

Reference 19

Resolution: unresolved; no resolver link, observed 2026-08-10T21:58:21.715990Z

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Observation 627e006e-1006-4a1c-b9aa-c8611a51c2a4 · outbound

This paper cites an unresolved cited work.

No evidence (yet) for increased star-formation efficiency at early times Unresolved cited work

Reference 20

Resolution: unresolved; no resolver link, observed 2026-08-10T21:58:21.730272Z

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Unavailable: canonical work link unavailable.

Observation 07113a21-f4b2-4396-b439-dddb993c01d1 · outbound

This paper cites an unresolved cited work.

No evidence (yet) for increased star-formation efficiency at early times Unresolved cited work

Reference 21

Resolution: unresolved; no resolver link, observed 2026-08-10T21:58:21.735846Z

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Observation 76833672-0d09-4326-a1c6-3ce80558c723 · outbound

This paper cites an unresolved cited work.

No evidence (yet) for increased star-formation efficiency at early times Unresolved cited work

Reference 22

Resolution: unresolved; no resolver link, observed 2026-08-10T21:58:21.742944Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 9e740178-00dd-4ac8-ac99-d33472b9ae67 · outbound

This paper cites JADES NIRSpec Initial Data Release for the Hubble Ultra Deep Field: Redshifts and Line Fluxes of Distant Galaxies from the Deepest JWST Cycle 1 NIRSpec Multi-Object Spectroscopy.

No evidence (yet) for increased star-formation efficiency at early times JADES NIRSpec Initial Data Release for the Hubble Ultra Deep Field: Redshifts and Line Fluxes of Distant Galaxies from the Deepest JWST Cycle 1 NIRSpec Multi-Object Spectroscopy

Reference 23

Resolution: unresolved; no resolver link, observed 2026-08-10T21:58:21.748226Z

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Unavailable: canonical work link unavailable.

Observation bf2df1e3-edc7-4487-815f-7b0fa547e537 · outbound

This paper cites Spectroscopic confirmation of two luminous galaxies at $z\sim14$.

No evidence (yet) for increased star-formation efficiency at early times Spectroscopic confirmation of two luminous galaxies at $z\sim14$

Reference 24

Resolution: unresolved; no resolver link, observed 2026-08-10T21:58:21.756934Z

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Observation 1f7a77d2-cfbd-4db8-8ec8-dc059bf4c74e · outbound

This paper cites The eventful life of a luminous galaxy at z = 14: metal enrichment, feedback, and low gas fraction?.

No evidence (yet) for increased star-formation efficiency at early times The eventful life of a luminous galaxy at z = 14: metal enrichment, feedback, and low gas fraction?

Reference 25

Resolution: unresolved; no resolver link, observed 2026-08-10T21:58:21.765282Z

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Observation 0925e341-8fd4-4222-b4e2-7eff221d531e · outbound

This paper cites M., et al., 2019, @doi [ ] 10.3847/1538-4357/ab52ff , https://ui.adsabs.harvard.edu/abs/2019ApJ...887...55C 887, 55.

No evidence (yet) for increased star-formation efficiency at early times M., et al., 2019, @doi [ ] 10.3847/1538-4357/ab52ff , https://ui.adsabs.harvard.edu/abs/2019ApJ...887...55C 887, 55

Reference 26

Resolution: unresolved; no resolver link, observed 2026-08-10T21:58:21.771651Z

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Unavailable: canonical work link unavailable.

Observation cded0e78-f542-40be-98fc-060a7b7a8114 · outbound

This paper cites M., et al., 2023, @doi [ ] 10.3847/1538-4357/acc2bc , https://ui.adsabs.harvard.edu/abs/2023ApJ...954...31C 954, 31.

No evidence (yet) for increased star-formation efficiency at early times M., et al., 2023, @doi [ ] 10.3847/1538-4357/acc2bc , https://ui.adsabs.harvard.edu/abs/2023ApJ...954...31C 954, 31

Reference 27

Resolution: unresolved; no resolver link, observed 2026-08-10T21:58:21.784889Z

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Observation 92fb9ece-9df7-463f-8eb3-5c9d1535e732 · outbound

This paper cites an unresolved cited work.

No evidence (yet) for increased star-formation efficiency at early times Unresolved cited work

Reference 28

Resolution: unresolved; no resolver link, observed 2026-08-10T21:58:21.789070Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 45129d78-abc1-4952-9a3b-249f98cc3ee8 · outbound

This paper cites JWST NIRSpec Spectroscopy of the Remarkable Bright Galaxy GHZ2/GLASS-z12 at Redshift 12.34.

No evidence (yet) for increased star-formation efficiency at early times JWST NIRSpec Spectroscopy of the Remarkable Bright Galaxy GHZ2/GLASS-z12 at Redshift 12.34

Reference 29

Resolution: unresolved; no resolver link, observed 2026-08-10T21:58:21.794453Z

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Unavailable: canonical work link unavailable.

Observation 6f779c62-e2d6-49a9-ba15-56cf95a2954e · outbound

This paper cites S., Glover S.

No evidence (yet) for increased star-formation efficiency at early times S., Glover S

Reference 30

Resolution: unresolved; no resolver link, observed 2026-08-10T21:58:21.799493Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 07afa8f4-35b6-4f04-abc9-2921b7a392bd · outbound

This paper cites an unresolved cited work.

No evidence (yet) for increased star-formation efficiency at early times Unresolved cited work

Reference 31

Resolution: unresolved; no resolver link, observed 2026-08-10T21:58:21.803603Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 1ff949ee-2a66-44a9-8492-90c8c966e939 · outbound

This paper cites an unresolved cited work.

No evidence (yet) for increased star-formation efficiency at early times Unresolved cited work

Reference 32

Resolution: unresolved; no resolver link, observed 2026-08-10T21:58:21.808816Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 85afb4e1-2c61-4327-8dba-407fef9a61cf · outbound

This paper cites an unresolved cited work.

No evidence (yet) for increased star-formation efficiency at early times Unresolved cited work

Reference 33

Resolution: unresolved; no resolver link, observed 2026-08-10T21:58:21.813714Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 6a75e44c-031b-4fb6-bf50-3e638b4a2042 · outbound

This paper cites an unresolved cited work.

No evidence (yet) for increased star-formation efficiency at early times Unresolved cited work

Reference 34

Resolution: unresolved; no resolver link, observed 2026-08-10T21:58:21.818566Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7291caef-73ef-4296-bbe3-8271b33710fd · outbound

This paper cites an unresolved cited work.

No evidence (yet) for increased star-formation efficiency at early times Unresolved cited work

Reference 35

Resolution: unresolved; no resolver link, observed 2026-08-10T21:58:21.828054Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 52b1ed79-a4db-4367-978a-dc32cb3641a4 · outbound

This paper cites C., Birnboim Y., Mandelker N., Li Z., 2023, @doi [ ] 10.1093/mnras/stad1557 , https://ui.adsabs.harvard.edu/abs/2023MNRAS.523.3201D 523, 3201.

No evidence (yet) for increased star-formation efficiency at early times C., Birnboim Y., Mandelker N., Li Z., 2023, @doi [ ] 10.1093/mnras/stad1557 , https://ui.adsabs.harvard.edu/abs/2023MNRAS.523.3201D 523, 3201

Reference 36

Resolution: unresolved; no resolver link, observed 2026-08-10T21:58:21.833341Z

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Unavailable: canonical work link unavailable.

Observation ca86a809-30c7-4828-9a85-93e5fd6c2a14 · outbound

This paper cites T., et al., 2023a, @doi [ ] 10.1093/mnras/stac3472 , https://ui.adsabs.harvard.edu/abs/2023MNRAS.518.6011D 518, 6011.

No evidence (yet) for increased star-formation efficiency at early times T., et al., 2023a, @doi [ ] 10.1093/mnras/stac3472 , https://ui.adsabs.harvard.edu/abs/2023MNRAS.518.6011D 518, 6011

Reference 37

Resolution: unresolved; no resolver link, observed 2026-08-10T21:58:21.840171Z

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Unavailable: canonical work link unavailable.

Observation eb3b577c-ca3f-45d2-8c15-2028e9fe4734 · outbound

This paper cites T., McLeod D.

No evidence (yet) for increased star-formation efficiency at early times T., McLeod D

Reference 38

Resolution: unresolved; no resolver link, observed 2026-08-10T21:58:21.845145Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 8b6010d7-34ab-4a5a-87f9-988acf4d1d7f · outbound

This paper cites T., et al., 2024, @doi [ ] 10.1093/mnras/stae2037 , https://ui.adsabs.harvard.edu/abs/2024MNRAS.533.3222D 533, 3222.

No evidence (yet) for increased star-formation efficiency at early times T., et al., 2024, @doi [ ] 10.1093/mnras/stae2037 , https://ui.adsabs.harvard.edu/abs/2024MNRAS.533.3222D 533, 3222

Reference 39

Resolution: unresolved; no resolver link, observed 2026-08-10T21:58:21.853406Z

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Unavailable: canonical work link unavailable.

Observation 42dc52bf-fec0-4d44-bfb4-3efb62c92403 · outbound

This paper cites e U., et al., 2020, @doi [ ] 10.1093/mnras/staa769 , https://ui.adsabs.harvard.edu/abs/2020MNRAS.494.3828D 494, 3828.

No evidence (yet) for increased star-formation efficiency at early times e U., et al., 2020, @doi [ ] 10.1093/mnras/staa769 , https://ui.adsabs.harvard.edu/abs/2020MNRAS.494.3828D 494, 3828

Reference 40

Resolution: unresolved; no resolver link, observed 2026-08-10T21:58:21.859492Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0f2d5ae4-ce4e-4c4a-8210-e5a414570d3d · outbound

This paper cites an unresolved cited work.

No evidence (yet) for increased star-formation efficiency at early times Unresolved cited work

Reference 41

Resolution: unresolved; no resolver link, observed 2026-08-10T21:58:21.873039Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 986221fd-fa17-4c66-bfe6-2d3fb8bfe23b · outbound

This paper cites S., et al., 2017, @doi [ ] 10.1093/mnras/stw3088 , https://ui.adsabs.harvard.edu/abs/2017MNRAS.466..861D 466, 861.

No evidence (yet) for increased star-formation efficiency at early times S., et al., 2017, @doi [ ] 10.1093/mnras/stw3088 , https://ui.adsabs.harvard.edu/abs/2017MNRAS.466..861D 466, 861

Reference 42

Resolution: unresolved; no resolver link, observed 2026-08-10T21:58:21.878035Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 16a09ee8-c185-47a4-a1b7-d0133d001d25 · outbound

This paper cites S., et al., 2021, PRIMER: Public Release IMaging for Extragalactic Research , JWST Proposal.

No evidence (yet) for increased star-formation efficiency at early times S., et al., 2021, PRIMER: Public Release IMaging for Extragalactic Research , JWST Proposal

Reference 43

Resolution: unresolved; no resolver link, observed 2026-08-10T21:58:21.883043Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0d19de11-8fcb-4e43-a490-f0cc5b08a896 · outbound

This paper cites S., 1913, @doi [ ] 10.1093/mnras/73.5.359 , https://ui.adsabs.harvard.edu/abs/1913MNRAS..73..359E 73, 359.

No evidence (yet) for increased star-formation efficiency at early times S., 1913, @doi [ ] 10.1093/mnras/73.5.359 , https://ui.adsabs.harvard.edu/abs/1913MNRAS..73..359E 73, 359

Reference 44

Resolution: unresolved; no resolver link, observed 2026-08-10T21:58:21.900100Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation bd9b8f49-8ddf-450e-a05b-b847137525c6 · outbound

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

No evidence (yet) for increased star-formation efficiency at early times Overview of the JWST Advanced Deep Extragalactic Survey (JADES)

Reference 45

Resolution: unresolved; no resolver link, observed 2026-08-10T21:58:21.905538Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 1fad3c85-31fb-428a-956b-b6bcc5b42ecb · outbound

This paper cites J., Stanway E.

No evidence (yet) for increased star-formation efficiency at early times J., Stanway E

Reference 46

Resolution: unresolved; no resolver link, observed 2026-08-10T21:58:21.911263Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c26be6ff-f8ce-4970-8620-4c1f1a7109f1 · outbound

This paper cites Elevated UV luminosity density at Cosmic Dawn explained by non-evolving, weakly mass-dependent star formation efficiency.

No evidence (yet) for increased star-formation efficiency at early times Elevated UV luminosity density at Cosmic Dawn explained by non-evolving, weakly mass-dependent star formation efficiency

Reference 47

Resolution: unresolved; no resolver link, observed 2026-08-10T21:58:21.917910Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 673f72e5-3c5f-406d-b3cb-cb49d9d96351 · outbound

This paper cites an unresolved cited work.

No evidence (yet) for increased star-formation efficiency at early times Unresolved cited work

Reference 48

Resolution: unresolved; no resolver link, observed 2026-08-10T21:58:21.923207Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 418afea9-463b-4d0b-88e4-c5027839ead7 · outbound

This paper cites Blue Monsters at $z>10$. Where has all their dust gone?.

No evidence (yet) for increased star-formation efficiency at early times Blue Monsters at $z>10$. Where has all their dust gone?

Reference 49

Resolution: unresolved; no resolver link, observed 2026-08-10T21:58:21.933430Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 80a40812-3658-4293-b586-82145a248deb · outbound

This paper cites The Complete CEERS Early Universe Galaxy Sample: A Surprisingly Slow Evolution of the Space Density of Bright Galaxies at z ~ 8.5-14.5.

No evidence (yet) for increased star-formation efficiency at early times The Complete CEERS Early Universe Galaxy Sample: A Surprisingly Slow Evolution of the Space Density of Bright Galaxies at z ~ 8.5-14.5

Reference 50

Resolution: unresolved; no resolver link, observed 2026-08-10T21:58:21.938747Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 8429b6e9-f908-42f4-a5a6-8c899480d31f · outbound

This paper cites L., et al., 2023b, @doi [ ] 10.3847/2041-8213/acade4 , https://ui.adsabs.harvard.edu/abs/2023ApJ...946L..13F 946, L13.

No evidence (yet) for increased star-formation efficiency at early times L., et al., 2023b, @doi [ ] 10.3847/2041-8213/acade4 , https://ui.adsabs.harvard.edu/abs/2023ApJ...946L..13F 946, L13

Reference 51

Resolution: unresolved; no resolver link, observed 2026-08-10T21:58:21.945168Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 2a559d35-ec72-4f5c-a594-ee83d65f271c · outbound

This paper cites L., et al., 2024, @doi [ ] 10.3847/2041-8213/ad4495 , https://ui.adsabs.harvard.edu/abs/2024ApJ...969L...2F 969, L2.

No evidence (yet) for increased star-formation efficiency at early times L., et al., 2024, @doi [ ] 10.3847/2041-8213/ad4495 , https://ui.adsabs.harvard.edu/abs/2024ApJ...969L...2F 969, L2

Reference 52

Resolution: unresolved; no resolver link, observed 2026-08-10T21:58:21.950886Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e3889ff8-eb64-4fe5-a701-4d542b892510 · outbound

This paper cites an unresolved cited work.

No evidence (yet) for increased star-formation efficiency at early times Unresolved cited work

Reference 53

Resolution: unresolved; no resolver link, observed 2026-08-10T21:58:21.954975Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 9a8469d9-dc0f-45eb-8421-5f7af75e6e6b · outbound

This paper cites M., Dav \'e R., 2015, @doi [ ] 10.1093/mnras/stu2399 , https://ui.adsabs.harvard.edu/abs/2015MNRAS.447..374G 447, 374.

No evidence (yet) for increased star-formation efficiency at early times M., Dav \'e R., 2015, @doi [ ] 10.1093/mnras/stu2399 , https://ui.adsabs.harvard.edu/abs/2015MNRAS.447..374G 447, 374

Reference 54

Resolution: unresolved; no resolver link, observed 2026-08-10T21:58:21.959998Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 65189098-eef1-454c-aa04-38874e9510ce · outbound

This paper cites an unresolved cited work.

No evidence (yet) for increased star-formation efficiency at early times Unresolved cited work

Reference 55

Resolution: unresolved; no resolver link, observed 2026-08-10T21:58:21.969250Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 97568ebc-0063-47fd-be86-a714797a2254 · outbound

This paper cites an unresolved cited work.

No evidence (yet) for increased star-formation efficiency at early times Unresolved cited work

Reference 56

Resolution: unresolved; no resolver link, observed 2026-08-10T21:58:21.974858Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 01f5d2c0-6a53-49b4-97fa-1b9886b13701 · outbound

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

No evidence (yet) for increased star-formation efficiency at early times B., Wang F., Yang J., Hennawi J

Reference 57

Resolution: unresolved; no resolver link, observed 2026-08-10T21:58:21.981805Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7fe51297-cd6d-404e-9922-284e92497cc6 · outbound

This paper cites an unresolved cited work.

No evidence (yet) for increased star-formation efficiency at early times Unresolved cited work

Reference 58

Resolution: unresolved; no resolver link, observed 2026-08-10T21:58:21.986397Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 23c00bb7-4df0-4d46-8a2e-db065e8430f2 · outbound

This paper cites an unresolved cited work.

No evidence (yet) for increased star-formation efficiency at early times Unresolved cited work

Reference 59

Resolution: unresolved; no resolver link, observed 2026-08-10T21:58:21.993056Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation db9e4fe3-9c3d-4a32-88af-863297a4de81 · outbound

This paper cites EPOCHS IV: SED Modelling Assumptions and their impact on the Stellar Mass Function at 6.5 < z < 13.5 using PEARLS and public JWST observations.

No evidence (yet) for increased star-formation efficiency at early times EPOCHS IV: SED Modelling Assumptions and their impact on the Stellar Mass Function at 6.5 < z < 13.5 using PEARLS and public JWST observations

Reference 60

Resolution: unresolved; no resolver link, observed 2026-08-10T21:58:21.999666Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 5256b7f9-4d21-40be-924a-838ae0d7f9ce · outbound

This paper cites F., Hernquist L., Cox T.

No evidence (yet) for increased star-formation efficiency at early times F., Hernquist L., Cox T

Reference 61

Resolution: unresolved; no resolver link, observed 2026-08-10T21:58:22.009583Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a6d98612-16cd-4ef5-b895-9b6b9cf371ac · outbound

This paper cites Census of Ly$\alpha$ Emission from $\sim 600$ Galaxies at $z=5-14$: Evolution of the Ly$\alpha$ Luminosity Function and a Late Sharp Cosmic Reionization.

No evidence (yet) for increased star-formation efficiency at early times Census of Ly$\alpha$ Emission from $\sim 600$ Galaxies at $z=5-14$: Evolution of the Ly$\alpha$ Luminosity Function and a Late Sharp Cosmic Reionization

Reference 62

Resolution: unresolved; no resolver link, observed 2026-08-10T21:58:22.017327Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 681849a4-65dc-497f-9997-5e218002cc22 · outbound

This paper cites an unresolved cited work.

No evidence (yet) for increased star-formation efficiency at early times Unresolved cited work

Reference 63

Resolution: unresolved; no resolver link, observed 2026-08-10T21:58:22.027950Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a25d615d-901c-4ec8-9a79-18e65f3d503d · outbound

This paper cites an unresolved cited work.

No evidence (yet) for increased star-formation efficiency at early times Unresolved cited work

Reference 64

Resolution: unresolved; no resolver link, observed 2026-08-10T21:58:22.032819Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 5c6f2042-9151-4185-9413-7cf2eaa92a0a · outbound

This paper cites an unresolved cited work.

No evidence (yet) for increased star-formation efficiency at early times Unresolved cited work

Reference 65

Resolution: unresolved; no resolver link, observed 2026-08-10T21:58:22.040377Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 5fc17a45-a717-4fb0-9770-74456192526c · outbound

This paper cites J., 1999, @doi [ ] 10.1086/306975 , https://ui.adsabs.harvard.edu/abs/1999ApJ...514..648M 514, 648.

No evidence (yet) for increased star-formation efficiency at early times J., 1999, @doi [ ] 10.1086/306975 , https://ui.adsabs.harvard.edu/abs/1999ApJ...514..648M 514, 648

Reference 66

Resolution: unresolved; no resolver link, observed 2026-08-10T21:58:22.045859Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 5e675b5a-ed7f-4856-b102-d7dbb33ddbf2 · outbound

This paper cites A., Trenti M., Treu T., 2015, @doi [ ] 10.1088/0004-637X/813/1/21 , https://ui.adsabs.harvard.edu/abs/2015ApJ...813...21M 813, 21.

No evidence (yet) for increased star-formation efficiency at early times A., Trenti M., Treu T., 2015, @doi [ ] 10.1088/0004-637X/813/1/21 , https://ui.adsabs.harvard.edu/abs/2015ApJ...813...21M 813, 21

Reference 67

Resolution: unresolved; no resolver link, observed 2026-08-10T21:58:22.052113Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 1b6ddd92-0b07-4afa-90d0-f449ae50258d · outbound

This paper cites A., Naidu R.

No evidence (yet) for increased star-formation efficiency at early times A., Naidu R

Reference 68

Resolution: unresolved; no resolver link, observed 2026-08-10T21:58:22.059742Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c541f69c-baa9-4c04-ac2c-eb5e7118bf20 · outbound

This paper cites A., Oteo I., Bouwens R., R \"o ttgering H., 2017, @doi [ ] 10.1093/mnras/stw2973 , https://ui.adsabs.harvard.edu/abs/2017MNRAS.465.3637M 465, 3637.

No evidence (yet) for increased star-formation efficiency at early times A., Oteo I., Bouwens R., R \"o ttgering H., 2017, @doi [ ] 10.1093/mnras/stw2973 , https://ui.adsabs.harvard.edu/abs/2017MNRAS.465.3637M 465, 3637

Reference 69

Resolution: unresolved; no resolver link, observed 2026-08-10T21:58:22.066015Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f3ddde6f-4304-41ac-b05b-d3568cc478fc · outbound

This paper cites an unresolved cited work.

No evidence (yet) for increased star-formation efficiency at early times Unresolved cited work

Reference 70

Resolution: unresolved; no resolver link, observed 2026-08-10T21:58:22.071801Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 5e627926-edca-4f35-86e6-33745dc17f01 · outbound

This paper cites SCUBADive I: JWST+ALMA Analysis of 289 sub-millimeter galaxies in COSMOS-Web.

No evidence (yet) for increased star-formation efficiency at early times SCUBADive I: JWST+ALMA Analysis of 289 sub-millimeter galaxies in COSMOS-Web

Reference 71

Resolution: unresolved; no resolver link, observed 2026-08-10T21:58:22.076136Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 3196bc32-68ad-430c-a808-6d5563b2f1b5 · outbound

This paper cites J., McLure R.

No evidence (yet) for increased star-formation efficiency at early times J., McLure R

Reference 72

Resolution: unresolved; no resolver link, observed 2026-08-10T21:58:22.082543Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a5b3ab6c-cd28-4a3b-92de-37894d926d63 · outbound

This paper cites J., McLure R.

No evidence (yet) for increased star-formation efficiency at early times J., McLure R

Reference 73

Resolution: unresolved; no resolver link, observed 2026-08-10T21:58:22.088403Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7e07a333-66bb-43b2-b0c7-63e5fd254823 · outbound

This paper cites J., et al., 2024, @doi [ ] 10.1093/mnras/stad3471 , https://ui.adsabs.harvard.edu/abs/2024MNRAS.527.5004M 527, 5004.

No evidence (yet) for increased star-formation efficiency at early times J., et al., 2024, @doi [ ] 10.1093/mnras/stad3471 , https://ui.adsabs.harvard.edu/abs/2024MNRAS.527.5004M 527, 5004

Reference 74

Resolution: unresolved; no resolver link, observed 2026-08-10T21:58:22.093811Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 9a37b590-3a80-4d09-acc0-b80bff889e41 · outbound

This paper cites J., Dunlop J.

No evidence (yet) for increased star-formation efficiency at early times J., Dunlop J

Reference 76

Resolution: unresolved; no resolver link, observed 2026-08-10T21:58:22.105963Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d091abc3-93c9-4e1b-921a-cfe75ed172cf · outbound

This paper cites J., et al., 2013, @doi [ ] 10.1093/mnras/stt627 , https://ui.adsabs.harvard.edu/abs/2013MNRAS.432.2696M 432, 2696.

No evidence (yet) for increased star-formation efficiency at early times J., et al., 2013, @doi [ ] 10.1093/mnras/stt627 , https://ui.adsabs.harvard.edu/abs/2013MNRAS.432.2696M 432, 2696

Reference 77

Resolution: unresolved; no resolver link, observed 2026-08-10T21:58:22.112270Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 2ca4b106-0573-4269-8988-0f611c09a9c7 · outbound

This paper cites J., et al., 2018, @doi [ ] 10.1093/mnras/sty522 , https://ui.adsabs.harvard.edu/abs/2018MNRAS.476.3991M 476, 3991.

No evidence (yet) for increased star-formation efficiency at early times J., et al., 2018, @doi [ ] 10.1093/mnras/sty522 , https://ui.adsabs.harvard.edu/abs/2018MNRAS.476.3991M 476, 3991

Reference 78

Resolution: unresolved; no resolver link, observed 2026-08-10T21:58:22.117836Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ebc9e94b-3269-419d-9242-a96568681a48 · outbound

This paper cites Rest-Frame UV Colors for Faint Galaxies at $z \sim 9-16$ with the \textit{JWST} NGDEEP Survey.

No evidence (yet) for increased star-formation efficiency at early times Rest-Frame UV Colors for Faint Galaxies at $z \sim 9-16$ with the \textit{JWST} NGDEEP Survey

Reference 79

Resolution: metadata mismatch; local_arxiv, observed 2026-08-10T21:58:23.261136Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation 34af197e-b97a-4ee7-bb80-f064e9716dbe · outbound

This paper cites an unresolved cited work.

No evidence (yet) for increased star-formation efficiency at early times Unresolved cited work

Reference 80

Resolution: unresolved; no resolver link, observed 2026-08-10T21:58:22.129844Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 8e1cc7e4-febf-48d2-9f1c-26dd807c90aa · outbound

This paper cites an unresolved cited work.

No evidence (yet) for increased star-formation efficiency at early times Unresolved cited work

Reference 81

Resolution: verified exact; doi, observed 2026-08-10T21:58:23.221170Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation 2569eeb1-7459-475a-b0dd-57ea1ba68e00 · outbound

This paper cites B., Mirocha J., Chisholm J., Furlanetto S.

No evidence (yet) for increased star-formation efficiency at early times B., Mirocha J., Chisholm J., Furlanetto S

Reference 82

Resolution: unresolved; no resolver link, observed 2026-08-10T21:58:22.142323Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d1623f36-15b5-4cb5-b01e-972b8c10f6aa · outbound

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

No evidence (yet) for increased star-formation efficiency at early times G., Power C., Robotham A

Reference 83

Resolution: unresolved; no resolver link, observed 2026-08-10T21:58:22.147949Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f3904e00-c339-48f4-a66f-9c947c398a28 · outbound

This paper cites an unresolved cited work.

No evidence (yet) for increased star-formation efficiency at early times Unresolved cited work

Reference 84

Resolution: unresolved; no resolver link, observed 2026-08-10T21:58:22.159884Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 1e5d5a51-0c04-4756-8f51-881d24838d55 · outbound

This paper cites P., et al., 2022, @doi [ ] 10.3847/2041-8213/ac9b22 , https://ui.adsabs.harvard.edu/abs/2022ApJ...940L..14N 940, L14.

No evidence (yet) for increased star-formation efficiency at early times P., et al., 2022, @doi [ ] 10.3847/2041-8213/ac9b22 , https://ui.adsabs.harvard.edu/abs/2022ApJ...940L..14N 940, L14

Reference 85

Resolution: unresolved; no resolver link, observed 2026-08-10T21:58:22.164054Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d0e45f4a-ce8b-41e9-a9ec-625f91d27588 · outbound

This paper cites an unresolved cited work.

No evidence (yet) for increased star-formation efficiency at early times Unresolved cited work

Reference 86

Resolution: unresolved; no resolver link, observed 2026-08-10T21:58:22.168450Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 32410d26-d682-454e-99a9-4984d7a77ed1 · outbound

This paper cites B., 1974, @doi [ ] 10.1086/190287 , https://ui.adsabs.harvard.edu/abs/1974ApJS...27...21O 27, 21.

No evidence (yet) for increased star-formation efficiency at early times B., 1974, @doi [ ] 10.1086/190287 , https://ui.adsabs.harvard.edu/abs/1974ApJS...27...21O 27, 21

Reference 87

Resolution: unresolved; no resolver link, observed 2026-08-10T21:58:22.174674Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 72faefca-fa0f-40c2-9dd1-d6d743303188 · outbound

This paper cites B., Gunn J.

No evidence (yet) for increased star-formation efficiency at early times B., Gunn J

Reference 88

Resolution: unresolved; no resolver link, observed 2026-08-10T21:58:22.180159Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 4e1b4142-19cc-41d9-8cfc-1755e29d7f0f · outbound

This paper cites J., Shapley A., Steidel C.

No evidence (yet) for increased star-formation efficiency at early times J., Shapley A., Steidel C

Reference 89

Resolution: unresolved; no resolver link, observed 2026-08-10T21:58:22.186406Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation af1bb434-c37d-447e-9740-b10529b78095 · outbound

This paper cites A spectroscopic analysis of the ionizing photon production efficiency in JADES and CEERS: implications for the ionizing photon budget.

No evidence (yet) for increased star-formation efficiency at early times A spectroscopic analysis of the ionizing photon production efficiency in JADES and CEERS: implications for the ionizing photon budget

Reference 90

Resolution: unresolved; no resolver link, observed 2026-08-10T21:58:22.193451Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7ecc3caf-f4cc-4b6d-b91d-7a85f0839b87 · outbound

This paper cites S., McLure R.

No evidence (yet) for increased star-formation efficiency at early times S., McLure R

Reference 91

Resolution: unresolved; no resolver link, observed 2026-08-10T21:58:22.201417Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d6650e8c-6e0b-4524-baf4-4ddc2a3961b5 · outbound

This paper cites G., et al., 2023, @doi [ ] 10.3847/2041-8213/acd9d0 , https://ui.adsabs.harvard.edu/abs/2023ApJ...951L...1P 951, L1.

No evidence (yet) for increased star-formation efficiency at early times G., et al., 2023, @doi [ ] 10.3847/2041-8213/acd9d0 , https://ui.adsabs.harvard.edu/abs/2023ApJ...951L...1P 951, L1

Reference 92

Resolution: unresolved; no resolver link, observed 2026-08-10T21:58:22.207752Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e5ff349f-2026-4020-94f3-db609a739aa5 · outbound

This paper cites an unresolved cited work.

No evidence (yet) for increased star-formation efficiency at early times Unresolved cited work

Reference 93

Resolution: unresolved; no resolver link, observed 2026-08-10T21:58:22.213103Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 08bb3f11-1457-486e-8cf3-f104c1216971 · outbound

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

No evidence (yet) for increased star-formation efficiency at early times S., Bower R., Frenk C

Reference 94

Resolution: unresolved; no resolver link, observed 2026-08-10T21:58:22.221073Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e3ba9b22-95bd-41cc-9ed0-fa0f24a8c4a2 · outbound

This paper cites E., Ellis R.

No evidence (yet) for increased star-formation efficiency at early times E., Ellis R

Reference 95

Resolution: unresolved; no resolver link, observed 2026-08-10T21:58:22.226119Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d21e07c8-6d7f-4d8e-ac83-48db7bba9f55 · outbound

This paper cites an unresolved cited work.

No evidence (yet) for increased star-formation efficiency at early times Unresolved cited work

Reference 96

Resolution: unresolved; no resolver link, observed 2026-08-10T21:58:22.230123Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0562d3cd-28a7-4c56-95b0-34b3a46d858b · outbound

This paper cites Detection of [OIII]88$\mu$m in JADES-GS-z14-0 at z=14.1793.

No evidence (yet) for increased star-formation efficiency at early times Detection of [OIII]88$\mu$m in JADES-GS-z14-0 at z=14.1793

Reference 97

Resolution: unresolved; no resolver link, observed 2026-08-10T21:58:22.236680Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0f74a10b-48bf-4d51-a9cf-dd3ced7727f9 · outbound

This paper cites M., Smith B.

No evidence (yet) for increased star-formation efficiency at early times M., Smith B

Reference 98

Resolution: unresolved; no resolver link, observed 2026-08-10T21:58:22.241296Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 135825e4-761b-4ac2-91a4-ff3e4e5cfac3 · outbound

This paper cites COSMOS-Web: stellar mass assembly in relation to dark matter halos across $0.2<z<12$ of cosmic history.

No evidence (yet) for increased star-formation efficiency at early times COSMOS-Web: stellar mass assembly in relation to dark matter halos across $0.2<z<12$ of cosmic history

Reference 99

Resolution: unresolved; no resolver link, observed 2026-08-10T21:58:22.245811Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation fd94e96f-7652-4cdb-b455-f2c1db524052 · outbound

This paper cites Ionising properties of galaxies in JADES for a stellar mass complete sample: resolving the cosmic ionising photon budget crisis at the Epoch of Reionisation.

No evidence (yet) for increased star-formation efficiency at early times Ionising properties of galaxies in JADES for a stellar mass complete sample: resolving the cosmic ionising photon budget crisis at the Epoch of Reionisation

Reference 100

Resolution: unresolved; no resolver link, observed 2026-08-10T21:58:22.251733Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 4c7b4f12-9823-4cc3-bf39-8c3c6320a195 · outbound

This paper cites an unresolved cited work.

No evidence (yet) for increased star-formation efficiency at early times Unresolved cited work

Reference 101

Resolution: unresolved; no resolver link, observed 2026-08-10T21:58:22.257434Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Pith citing papers

Observation 06efd81a-70da-4b63-94ce-93be26b1cecb · inbound

Signatures of Rapidly Rotating Stars with Chemically Homogeneous Evolution in the First Galaxies cites this paper.

Signatures of Rapidly Rotating Stars with Chemically Homogeneous Evolution in the First Galaxies No evidence (yet) for increased star-formation efficiency at early times

Reference 25

Resolution: unresolved; no resolver link, observed 2026-08-12T00:06:12.089404Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 53de2acf-5ab2-4567-bae8-706c8389233c · inbound

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GLIMPSE: An ultra-faint $\simeq$ 10$^{5}$ $M_{\odot}$ Pop III Galaxy Candidate and First Constraints on the Pop III UV Luminosity Function at $z\simeq6-7$ No evidence (yet) for increased star-formation efficiency at early times

Reference 29

Resolution: unresolved; no resolver link, observed 2026-08-10T18:06:28.949401Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation acd8d3c8-3e6c-46e0-9e07-bb0a6a5dba70 · inbound

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The impact of medium-width bands on the selection, and subsequent luminosity function measurements, of high-z galaxies No evidence (yet) for increased star-formation efficiency at early times

Reference 35

Resolution: unresolved; no resolver link, observed 2026-08-07T18:45:27.254495Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a86bd545-e52e-487c-9193-d8f93b44ce0f · inbound

Exploring Cosmic Dawn with PANORAMIC I: The Bright End of the UVLF at $z\sim9 -17$ cites this paper.

Exploring Cosmic Dawn with PANORAMIC I: The Bright End of the UVLF at $z\sim9 -17$ No evidence (yet) for increased star-formation efficiency at early times

Reference 49

Resolution: unresolved; no resolver link, observed 2026-08-06T19:14:38.159767Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 20a7a166-e314-45eb-8187-7c09bd43345a · inbound

Physical properties of galaxies and the UV Luminosity Function from $z\sim6$ to $z\sim14$ in COSMOS-Web cites this paper.

Physical properties of galaxies and the UV Luminosity Function from $z\sim6$ to $z\sim14$ in COSMOS-Web No evidence (yet) for increased star-formation efficiency at early times

Reference 68

Resolution: unresolved; no resolver link, observed 2026-08-05T23:52:39.394879Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f06d41a9-dc48-4c99-a868-754bfc8ca3e9 · inbound

Exploring Cosmic Dawn with PANORAMIC II: Cosmic Variance and Galaxy Clustering at $z\sim10$ cites this paper.

Exploring Cosmic Dawn with PANORAMIC II: Cosmic Variance and Galaxy Clustering at $z\sim10$ No evidence (yet) for increased star-formation efficiency at early times

Reference 30

Resolution: unresolved; no resolver link, observed 2026-08-03T16:19:30.887267Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation bcb689f8-933f-4cf3-8a72-c24cb616ce6f · inbound

Grain-size evolution and rapid dust growth in high-redshift galaxies cites this paper.

Grain-size evolution and rapid dust growth in high-redshift galaxies No evidence (yet) for increased star-formation efficiency at early times

Reference 188

Resolution: metadata mismatch; arxiv_id, observed 2026-06-28T00:51:27.057892Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation e1c8de1f-f7d0-4cd3-a36f-60bc899fdff8 · inbound

Gamma-ray bursts reveal the history and faint contributors of cosmic reionization cites this paper.

Gamma-ray bursts reveal the history and faint contributors of cosmic reionization No evidence (yet) for increased star-formation efficiency at early times

Reference 247

Resolution: metadata mismatch; local_arxiv, observed 2026-07-09T05:26:01.856097Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.