Paper Citation Record · LEDGER

Improved upper limits on the 21-cm signal power spectrum at $z=17.0$ and $z=20.3$ from an optimal field observed with NenuFAR

As of 19 August 2026, this Paper Citation Record lists 100 of 116 outbound references and 7 inbound Pith citation observations for arXiv:2507.10533.

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

pith.paper-citation-record.v1
2507.10533 v2

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measured 100 of 116 reference resolution

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Outbound references

Observation ce3df4c0-e4c7-4397-95c1-730d0e63c2c0 · outbound

This paper cites an unresolved cited work.

Improved upper limits on the 21-cm signal power spectrum at $z=17.0$ and $z=20.3$ from an optimal field observed with NenuFAR Unresolved cited work

Reference 1

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Observation 200bdf13-6dc0-4693-89a9-4b5c0af0f631 · outbound

This paper cites an unresolved cited work.

Improved upper limits on the 21-cm signal power spectrum at $z=17.0$ and $z=20.3$ from an optimal field observed with NenuFAR Unresolved cited work

Reference 2

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Improved upper limits on the 21-cm signal power spectrum at $z=17.0$ and $z=20.3$ from an optimal field observed with NenuFAR Unresolved cited work

Reference 3

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Improved upper limits on the 21-cm signal power spectrum at $z=17.0$ and $z=20.3$ from an optimal field observed with NenuFAR Unresolved cited work

Reference 4

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Improved upper limits on the 21-cm signal power spectrum at $z=17.0$ and $z=20.3$ from an optimal field observed with NenuFAR Unresolved cited work

Reference 5

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Improved upper limits on the 21-cm signal power spectrum at $z=17.0$ and $z=20.3$ from an optimal field observed with NenuFAR Unresolved cited work

Reference 6

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Improved upper limits on the 21-cm signal power spectrum at $z=17.0$ and $z=20.3$ from an optimal field observed with NenuFAR Unresolved cited work

Reference 7

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This paper cites D., 2018, Physical review letters, 121, 011102.

Improved upper limits on the 21-cm signal power spectrum at $z=17.0$ and $z=20.3$ from an optimal field observed with NenuFAR D., 2018, Physical review letters, 121, 011102

Reference 8

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Improved upper limits on the 21-cm signal power spectrum at $z=17.0$ and $z=20.3$ from an optimal field observed with NenuFAR Unresolved cited work

Reference 9

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Observation 80debf19-f8d4-4fed-a4cb-5ff292ff3e91 · outbound

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Improved upper limits on the 21-cm signal power spectrum at $z=17.0$ and $z=20.3$ from an optimal field observed with NenuFAR D., Rogers A

Reference 10

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Improved upper limits on the 21-cm signal power spectrum at $z=17.0$ and $z=20.3$ from an optimal field observed with NenuFAR Unresolved cited work

Reference 11

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Observation 4d3a91d8-dfa5-477b-bf5f-32dc33bd4266 · outbound

This paper cites Robust direction-dependent gain-calibration of beam-modelling errors far from the target field.

Improved upper limits on the 21-cm signal power spectrum at $z=17.0$ and $z=20.3$ from an optimal field observed with NenuFAR Robust direction-dependent gain-calibration of beam-modelling errors far from the target field

Reference 12

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Improved upper limits on the 21-cm signal power spectrum at $z=17.0$ and $z=20.3$ from an optimal field observed with NenuFAR Unresolved cited work

Reference 13

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This paper cites The EDGES measurement disfavors an excess radio background during the cosmic dawn.

Improved upper limits on the 21-cm signal power spectrum at $z=17.0$ and $z=20.3$ from an optimal field observed with NenuFAR The EDGES measurement disfavors an excess radio background during the cosmic dawn

Reference 14

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Improved upper limits on the 21-cm signal power spectrum at $z=17.0$ and $z=20.3$ from an optimal field observed with NenuFAR Unresolved cited work

Reference 15

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This paper cites Spectral modelling of Cygnus A between 110 and 250 MHz. Impact on the LOFAR 21-cm signal power spectrum.

Improved upper limits on the 21-cm signal power spectrum at $z=17.0$ and $z=20.3$ from an optimal field observed with NenuFAR Spectral modelling of Cygnus A between 110 and 250 MHz. Impact on the LOFAR 21-cm signal power spectrum

Reference 16

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Improved upper limits on the 21-cm signal power spectrum at $z=17.0$ and $z=20.3$ from an optimal field observed with NenuFAR Unresolved cited work

Reference 17

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Improved upper limits on the 21-cm signal power spectrum at $z=17.0$ and $z=20.3$ from an optimal field observed with NenuFAR Unresolved cited work

Reference 18

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Improved upper limits on the 21-cm signal power spectrum at $z=17.0$ and $z=20.3$ from an optimal field observed with NenuFAR Unresolved cited work

Reference 19

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Improved upper limits on the 21-cm signal power spectrum at $z=17.0$ and $z=20.3$ from an optimal field observed with NenuFAR Unresolved cited work

Reference 20

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Observation dc66bc97-cb50-4dd6-9fdb-216d8dcee7ef · outbound

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Improved upper limits on the 21-cm signal power spectrum at $z=17.0$ and $z=20.3$ from an optimal field observed with NenuFAR K., Mellema G., Mao Y., Iliev I

Reference 21

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Improved upper limits on the 21-cm signal power spectrum at $z=17.0$ and $z=20.3$ from an optimal field observed with NenuFAR K., Jensen H., Majumdar S., Mellema G., Iliev I

Reference 22

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Observation 90740240-e171-470c-bd05-8c96fd3b4ff3 · outbound

This paper cites Exploiting synergies between JWST and cosmic 21-cm observations to uncover star formation in the early Universe.

Improved upper limits on the 21-cm signal power spectrum at $z=17.0$ and $z=20.3$ from an optimal field observed with NenuFAR Exploiting synergies between JWST and cosmic 21-cm observations to uncover star formation in the early Universe

Reference 23

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Improved upper limits on the 21-cm signal power spectrum at $z=17.0$ and $z=20.3$ from an optimal field observed with NenuFAR W., Barja P

Reference 24

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Improved upper limits on the 21-cm signal power spectrum at $z=17.0$ and $z=20.3$ from an optimal field observed with NenuFAR B., 2018a, The Astrophysical Journal Letters, 858, L9

Reference 25

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This paper cites B., 2018b, @doi [ ] 10.3847/2041-8213/aabf86 , https://ui.adsabs.harvard.edu/abs/2018ApJ...858L...9D 858, L9.

Improved upper limits on the 21-cm signal power spectrum at $z=17.0$ and $z=20.3$ from an optimal field observed with NenuFAR B., 2018b, @doi [ ] 10.3847/2041-8213/aabf86 , https://ui.adsabs.harvard.edu/abs/2018ApJ...858L...9D 858, L9

Reference 26

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Improved upper limits on the 21-cm signal power spectrum at $z=17.0$ and $z=20.3$ from an optimal field observed with NenuFAR W., et al., 2019, AJ, 158, 84

Reference 27

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Improved upper limits on the 21-cm signal power spectrum at $z=17.0$ and $z=20.3$ from an optimal field observed with NenuFAR Unresolved cited work

Reference 28

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Improved upper limits on the 21-cm signal power spectrum at $z=17.0$ and $z=20.3$ from an optimal field observed with NenuFAR Unresolved cited work

Reference 29

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Improved upper limits on the 21-cm signal power spectrum at $z=17.0$ and $z=20.3$ from an optimal field observed with NenuFAR Unresolved cited work

Reference 30

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Improved upper limits on the 21-cm signal power spectrum at $z=17.0$ and $z=20.3$ from an optimal field observed with NenuFAR Unresolved cited work

Reference 31

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Improved upper limits on the 21-cm signal power spectrum at $z=17.0$ and $z=20.3$ from an optimal field observed with NenuFAR Unresolved cited work

Reference 32

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This paper cites M., 2012, @doi [ ] 10.1111/j.1365-2966.2012.21318.x , https://ui.adsabs.harvard.edu/abs/2012MNRAS.424.1335F 424, 1335.

Improved upper limits on the 21-cm signal power spectrum at $z=17.0$ and $z=20.3$ from an optimal field observed with NenuFAR M., 2012, @doi [ ] 10.1111/j.1365-2966.2012.21318.x , https://ui.adsabs.harvard.edu/abs/2012MNRAS.424.1335F 424, 1335

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This paper cites M., 2013, @doi [ ] 10.1093/mnras/stt650 , https://ui.adsabs.harvard.edu/abs/2013MNRAS.432.2909F 432, 2909.

Improved upper limits on the 21-cm signal power spectrum at $z=17.0$ and $z=20.3$ from an optimal field observed with NenuFAR M., 2013, @doi [ ] 10.1093/mnras/stt650 , https://ui.adsabs.harvard.edu/abs/2013MNRAS.432.2909F 432, 2909

Reference 34

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Improved upper limits on the 21-cm signal power spectrum at $z=17.0$ and $z=20.3$ from an optimal field observed with NenuFAR Unresolved cited work

Reference 35

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Improved upper limits on the 21-cm signal power spectrum at $z=17.0$ and $z=20.3$ from an optimal field observed with NenuFAR Unresolved cited work

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Improved upper limits on the 21-cm signal power spectrum at $z=17.0$ and $z=20.3$ from an optimal field observed with NenuFAR J., et al., 2011, @doi [ ] 10.1088/0004-637X/734/1/5 , https://ui.adsabs.harvard.edu/abs/2011ApJ...734....5F 734, 5

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Improved upper limits on the 21-cm signal power spectrum at $z=17.0$ and $z=20.3$ from an optimal field observed with NenuFAR Unresolved cited work

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Improved upper limits on the 21-cm signal power spectrum at $z=17.0$ and $z=20.3$ from an optimal field observed with NenuFAR D., Naoz S., Zezas A., Basu-Zych A., 2013b, @doi [ ] 10.1088/2041-8205/776/2/L31 , https://ui.adsabs.harvard.edu/abs/2013ApJ...776L..31F 776, L31

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Improved upper limits on the 21-cm signal power spectrum at $z=17.0$ and $z=20.3$ from an optimal field observed with NenuFAR R., Oh S

Reference 40

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This paper cites Assessing the impact of two independent direction-dependent calibration algorithms on the LOFAR 21-cm signal power spectrum.

Improved upper limits on the 21-cm signal power spectrum at $z=17.0$ and $z=20.3$ from an optimal field observed with NenuFAR Assessing the impact of two independent direction-dependent calibration algorithms on the LOFAR 21-cm signal power spectrum

Reference 41

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Improved upper limits on the 21-cm signal power spectrum at $z=17.0$ and $z=20.3$ from an optimal field observed with NenuFAR Unresolved cited work

Reference 42

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Improved upper limits on the 21-cm signal power spectrum at $z=17.0$ and $z=20.3$ from an optimal field observed with NenuFAR Unresolved cited work

Reference 43

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Improved upper limits on the 21-cm signal power spectrum at $z=17.0$ and $z=20.3$ from an optimal field observed with NenuFAR Unresolved cited work

Reference 44

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Improved upper limits on the 21-cm signal power spectrum at $z=17.0$ and $z=20.3$ from an optimal field observed with NenuFAR Unresolved cited work

Reference 45

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Improved upper limits on the 21-cm signal power spectrum at $z=17.0$ and $z=20.3$ from an optimal field observed with NenuFAR Unresolved cited work

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Improved upper limits on the 21-cm signal power spectrum at $z=17.0$ and $z=20.3$ from an optimal field observed with NenuFAR Unresolved cited work

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Improved upper limits on the 21-cm signal power spectrum at $z=17.0$ and $z=20.3$ from an optimal field observed with NenuFAR Unresolved cited work

Reference 48

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Improved upper limits on the 21-cm signal power spectrum at $z=17.0$ and $z=20.3$ from an optimal field observed with NenuFAR Unresolved cited work

Reference 49

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Observation f12d9b75-0afe-465c-8447-5548e4a1cc67 · outbound

This paper cites Constraints on the state of the IGM at $z\sim 8-10$ using redshifted 21-cm observations with LOFAR.

Improved upper limits on the 21-cm signal power spectrum at $z=17.0$ and $z=20.3$ from an optimal field observed with NenuFAR Constraints on the state of the IGM at $z\sim 8-10$ using redshifted 21-cm observations with LOFAR

Reference 50

Resolution: unresolved; no resolver link, observed 2026-08-06T17:35:29.464923Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 352d3737-82d6-44ac-bcd7-147ef80c160c · outbound

This paper cites M., Barry N., Mutch S.

Improved upper limits on the 21-cm signal power spectrum at $z=17.0$ and $z=20.3$ from an optimal field observed with NenuFAR M., Barry N., Mutch S

Reference 51

Resolution: unresolved; no resolver link, observed 2026-08-06T17:35:29.476226Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation fd67efb8-7ed9-41cb-b7eb-53c373ea23b7 · outbound

This paper cites an unresolved cited work.

Improved upper limits on the 21-cm signal power spectrum at $z=17.0$ and $z=20.3$ from an optimal field observed with NenuFAR Unresolved cited work

Reference 52

Resolution: unresolved; no resolver link, observed 2026-08-06T17:35:29.486550Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d17ec51d-825a-40a5-befe-e7f5f6e30b5b · outbound

This paper cites J., et al., 2016, @doi [ ] 10.1093/mnras/stw1763 , https://ui.adsabs.harvard.edu/abs/2016MNRAS.462.1910H 462, 1910.

Improved upper limits on the 21-cm signal power spectrum at $z=17.0$ and $z=20.3$ from an optimal field observed with NenuFAR J., et al., 2016, @doi [ ] 10.1093/mnras/stw1763 , https://ui.adsabs.harvard.edu/abs/2016MNRAS.462.1910H 462, 1910

Reference 53

Resolution: unresolved; no resolver link, observed 2026-08-06T17:35:29.498642Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ea020ef4-3ae9-494e-881d-f3746723bb0e · outbound

This paper cites an unresolved cited work.

Improved upper limits on the 21-cm signal power spectrum at $z=17.0$ and $z=20.3$ from an optimal field observed with NenuFAR Unresolved cited work

Reference 54

Resolution: verified exact; raw_fallback, observed 2026-08-06T17:35:32.317336Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation bb0650bc-0809-4596-b8bf-1c9c0dbe4e4e · outbound

This paper cites an unresolved cited work.

Improved upper limits on the 21-cm signal power spectrum at $z=17.0$ and $z=20.3$ from an optimal field observed with NenuFAR Unresolved cited work

Reference 55

Resolution: unresolved; no resolver link, observed 2026-08-06T17:35:29.515903Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 9482453a-5d9f-43e9-a6a1-ddcafb7b6f55 · outbound

This paper cites S., Parsons A.

Improved upper limits on the 21-cm signal power spectrum at $z=17.0$ and $z=20.3$ from an optimal field observed with NenuFAR S., Parsons A

Reference 56

Resolution: unresolved; no resolver link, observed 2026-08-06T17:35:29.523094Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7a0182f3-9672-4738-80e8-f8256dd285b8 · outbound

This paper cites S., et al., 2020, ApJ, 888, 70.

Improved upper limits on the 21-cm signal power spectrum at $z=17.0$ and $z=20.3$ from an optimal field observed with NenuFAR S., et al., 2020, ApJ, 888, 70

Reference 57

Resolution: unresolved; no resolver link, observed 2026-08-06T17:35:29.531455Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c950119e-664b-4d9e-a30c-cbefaedccce1 · outbound

This paper cites an unresolved cited work.

Improved upper limits on the 21-cm signal power spectrum at $z=17.0$ and $z=20.3$ from an optimal field observed with NenuFAR Unresolved cited work

Reference 58

Resolution: unresolved; raw_fallback, observed 2026-08-06T17:35:33.429958Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation 027cad3a-eda2-4386-904f-645bf645ccfb · outbound

This paper cites The Cosmic Dawn and Epoch of Reionization with the Square Kilometre Array.

Improved upper limits on the 21-cm signal power spectrum at $z=17.0$ and $z=20.3$ from an optimal field observed with NenuFAR The Cosmic Dawn and Epoch of Reionization with the Square Kilometre Array

Reference 59

Resolution: unresolved; no resolver link, observed 2026-08-06T17:35:29.546176Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 4a28ceeb-f094-4b80-9ee8-416836a3ab96 · outbound

This paper cites an unresolved cited work.

Improved upper limits on the 21-cm signal power spectrum at $z=17.0$ and $z=20.3$ from an optimal field observed with NenuFAR Unresolved cited work

Reference 60

Resolution: unresolved; raw_fallback, observed 2026-08-06T17:35:33.411710Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation d8c95fee-392d-4233-9cc8-9c9250f83e3a · outbound

This paper cites J., Redigolo D., Volansky T., 2019, Physical Review D, 100, 123011.

Improved upper limits on the 21-cm signal power spectrum at $z=17.0$ and $z=20.3$ from an optimal field observed with NenuFAR J., Redigolo D., Volansky T., 2019, Physical Review D, 100, 123011

Reference 61

Resolution: verified fuzzy; raw_fallback, observed 2026-08-06T17:35:33.396069Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation 6eba5849-89f2-4f5f-853f-03700610f11b · outbound

This paper cites Effects of chemically homogeneous evolution of the first stars on the 21-cm signal and reionization.

Improved upper limits on the 21-cm signal power spectrum at $z=17.0$ and $z=20.3$ from an optimal field observed with NenuFAR Effects of chemically homogeneous evolution of the first stars on the 21-cm signal and reionization

Reference 62

Resolution: unresolved; no resolver link, observed 2026-08-06T17:35:29.580339Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 9a7ba095-6642-4c91-a5ce-226cecd71e56 · outbound

This paper cites an unresolved cited work.

Improved upper limits on the 21-cm signal power spectrum at $z=17.0$ and $z=20.3$ from an optimal field observed with NenuFAR Unresolved cited work

Reference 63

Resolution: unresolved; no resolver link, observed 2026-08-06T17:35:29.591701Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 8a68ab0c-3773-4264-a5dc-1969455b61f9 · outbound

This paper cites pp 281--298.

Improved upper limits on the 21-cm signal power spectrum at $z=17.0$ and $z=20.3$ from an optimal field observed with NenuFAR pp 281--298

Reference 64

Resolution: unresolved; no resolver link, observed 2026-08-06T17:35:29.642425Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 6620d9af-b60d-471d-91dd-cb2f889357a1 · outbound

This paper cites an unresolved cited work.

Improved upper limits on the 21-cm signal power spectrum at $z=17.0$ and $z=20.3$ from an optimal field observed with NenuFAR Unresolved cited work

Reference 65

Resolution: unresolved; no resolver link, observed 2026-08-06T17:35:29.718015Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 14f638c4-4478-4b20-8a38-aeb6c431f059 · outbound

This paper cites Comparison of Bayesian inference methods using the Loreli II database of hydro-radiative simulations of the 21-cm signal.

Improved upper limits on the 21-cm signal power spectrum at $z=17.0$ and $z=20.3$ from an optimal field observed with NenuFAR Comparison of Bayesian inference methods using the Loreli II database of hydro-radiative simulations of the 21-cm signal

Reference 66

Resolution: unresolved; no resolver link, observed 2026-08-06T17:35:29.830160Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 023f5fc7-c9be-4b3e-8613-397853ff1a9c · outbound

This paper cites an unresolved cited work.

Improved upper limits on the 21-cm signal power spectrum at $z=17.0$ and $z=20.3$ from an optimal field observed with NenuFAR Unresolved cited work

Reference 67

Resolution: unresolved; raw_fallback, observed 2026-08-06T17:35:33.354750Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation 2ae5feee-0f6f-4560-b1f2-5fdd622f9ca0 · outbound

This paper cites G., et al., 2020, MNRAS, 493, 1662.

Improved upper limits on the 21-cm signal power spectrum at $z=17.0$ and $z=20.3$ from an optimal field observed with NenuFAR G., et al., 2020, MNRAS, 493, 1662

Reference 68

Resolution: verified fuzzy; raw_fallback, observed 2026-08-06T17:35:33.339101Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation b7ca66e4-197c-449f-87c2-8c0aea76205f · outbound

This paper cites Exploring the Cosmic Dawn with NenuFAR.

Improved upper limits on the 21-cm signal power spectrum at $z=17.0$ and $z=20.3$ from an optimal field observed with NenuFAR Exploring the Cosmic Dawn with NenuFAR

Reference 69

Resolution: unresolved; no resolver link, observed 2026-08-06T17:35:30.199177Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 8d4739d3-b96d-4486-9317-8288942d9dc1 · outbound

This paper cites G., Bobin J., Carucci I.

Improved upper limits on the 21-cm signal power spectrum at $z=17.0$ and $z=20.3$ from an optimal field observed with NenuFAR G., Bobin J., Carucci I

Reference 70

Resolution: verified fuzzy; raw_fallback, observed 2026-08-06T17:35:33.321464Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation c2056b58-9e25-4633-aa68-ad907b7c3c38 · outbound

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

Improved upper limits on the 21-cm signal power spectrum at $z=17.0$ and $z=20.3$ from an optimal field observed with NenuFAR Deeper multi-redshift upper limits on the Epoch of Reionization 21-cm signal power spectrum from LOFAR between z=8.3 and z=10.1

Reference 71

Resolution: unresolved; no resolver link, observed 2026-08-06T17:35:30.482021Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c49fc1b6-fecf-45aa-94dd-c710822b49a9 · outbound

This paper cites an unresolved cited work.

Improved upper limits on the 21-cm signal power spectrum at $z=17.0$ and $z=20.3$ from an optimal field observed with NenuFAR Unresolved cited work

Reference 72

Resolution: unresolved; raw_fallback, observed 2026-08-06T17:35:33.304415Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation d2b5fd77-400e-42fa-b91d-a245cba90681 · outbound

This paper cites an unresolved cited work.

Improved upper limits on the 21-cm signal power spectrum at $z=17.0$ and $z=20.3$ from an optimal field observed with NenuFAR Unresolved cited work

Reference 73

Resolution: unresolved; raw_fallback, observed 2026-08-06T17:35:33.287575Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation e1f0ee44-a1b1-4322-a3d6-c365138f691b · outbound

This paper cites an unresolved cited work.

Improved upper limits on the 21-cm signal power spectrum at $z=17.0$ and $z=20.3$ from an optimal field observed with NenuFAR Unresolved cited work

Reference 74

Resolution: unresolved; raw_fallback, observed 2026-08-06T17:35:33.271237Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation 6af89e07-5fc1-4b85-96e9-cb44fa02ae3c · outbound

This paper cites R., 2019, @doi [ ] 10.1093/mnras/sty3260 , https://ui.adsabs.harvard.edu/abs/2019MNRAS.483.1980M 483, 1980.

Improved upper limits on the 21-cm signal power spectrum at $z=17.0$ and $z=20.3$ from an optimal field observed with NenuFAR R., 2019, @doi [ ] 10.1093/mnras/sty3260 , https://ui.adsabs.harvard.edu/abs/2019MNRAS.483.1980M 483, 1980

Reference 75

Resolution: unresolved; no resolver link, observed 2026-08-06T17:35:30.981996Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation beba0fe5-7584-4b84-a956-ec246b4b643c · outbound

This paper cites an unresolved cited work.

Improved upper limits on the 21-cm signal power spectrum at $z=17.0$ and $z=20.3$ from an optimal field observed with NenuFAR Unresolved cited work

Reference 76

Resolution: unresolved; raw_fallback, observed 2026-08-06T17:35:33.255005Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation 34d78326-3bd4-4ee7-9e4c-3e0d64d097ff · outbound

This paper cites F., Hazelton B., Sullivan I., Beardsley A., 2012, ApJ, 752, 137.

Improved upper limits on the 21-cm signal power spectrum at $z=17.0$ and $z=20.3$ from an optimal field observed with NenuFAR F., Hazelton B., Sullivan I., Beardsley A., 2012, ApJ, 752, 137

Reference 77

Resolution: verified fuzzy; raw_fallback, observed 2026-08-06T17:35:33.238606Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation 49e64d83-9d02-4edd-810f-69dc628e3fb4 · outbound

This paper cites an unresolved cited work.

Improved upper limits on the 21-cm signal power spectrum at $z=17.0$ and $z=20.3$ from an optimal field observed with NenuFAR Unresolved cited work

Reference 78

Resolution: unresolved; raw_fallback, observed 2026-08-06T17:35:33.223502Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation 3b8e242b-6045-480e-82bd-d98ad0b9f459 · outbound

This paper cites B., Loeb A., 2018, Nature, 557, 684.

Improved upper limits on the 21-cm signal power spectrum at $z=17.0$ and $z=20.3$ from an optimal field observed with NenuFAR B., Loeb A., 2018, Nature, 557, 684

Reference 79

Resolution: verified fuzzy; raw_fallback, observed 2026-08-06T17:35:33.208859Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation 7060d2f3-1ede-4eac-8663-e709b1d1f066 · outbound

This paper cites an unresolved cited work.

Improved upper limits on the 21-cm signal power spectrum at $z=17.0$ and $z=20.3$ from an optimal field observed with NenuFAR Unresolved cited work

Reference 80

Resolution: unresolved; raw_fallback, observed 2026-08-06T17:35:33.192957Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation 6267c2ec-6ef7-4c21-a911-ecde141f8ca0 · outbound

This paper cites an unresolved cited work.

Improved upper limits on the 21-cm signal power spectrum at $z=17.0$ and $z=20.3$ from an optimal field observed with NenuFAR Unresolved cited work

Reference 81

Resolution: unresolved; raw_fallback, observed 2026-08-06T17:35:33.176739Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation b4d61a9a-9ae7-45f8-aafa-b979f5dc3857 · outbound

This paper cites an unresolved cited work.

Improved upper limits on the 21-cm signal power spectrum at $z=17.0$ and $z=20.3$ from an optimal field observed with NenuFAR Unresolved cited work

Reference 82

Resolution: unresolved; raw_fallback, observed 2026-08-06T17:35:33.154008Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation 900f06c7-150f-469b-9d45-82e0a555ae46 · outbound

This paper cites an unresolved cited work.

Improved upper limits on the 21-cm signal power spectrum at $z=17.0$ and $z=20.3$ from an optimal field observed with NenuFAR Unresolved cited work

Reference 83

Resolution: unresolved; raw_fallback, observed 2026-08-06T17:35:33.137915Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation d44fe8ef-4291-4bb6-a9b2-808323e7b86c · outbound

This paper cites Limits on the 21 cm power spectrum at z=6.5-7.0 from MWA observations.

Improved upper limits on the 21-cm signal power spectrum at $z=17.0$ and $z=20.3$ from an optimal field observed with NenuFAR Limits on the 21 cm power spectrum at z=6.5-7.0 from MWA observations

Reference 84

Resolution: unresolved; no resolver link, observed 2026-08-06T17:35:31.371736Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 52f9a48d-15ad-4320-a161-48326b0479be · outbound

This paper cites an unresolved cited work.

Improved upper limits on the 21-cm signal power spectrum at $z=17.0$ and $z=20.3$ from an optimal field observed with NenuFAR Unresolved cited work

Reference 85

Resolution: unresolved; raw_fallback, observed 2026-08-06T17:35:33.121353Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation 703014b8-f58f-46fe-bdea-8a793b95856a · outbound

This paper cites an unresolved cited work.

Improved upper limits on the 21-cm signal power spectrum at $z=17.0$ and $z=20.3$ from an optimal field observed with NenuFAR Unresolved cited work

Reference 86

Resolution: unresolved; raw_fallback, observed 2026-08-06T17:35:33.103717Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation 666647f3-cac8-49ed-b176-5eb2a16777a8 · outbound

This paper cites an unresolved cited work.

Improved upper limits on the 21-cm signal power spectrum at $z=17.0$ and $z=20.3$ from an optimal field observed with NenuFAR Unresolved cited work

Reference 87

Resolution: unresolved; raw_fallback, observed 2026-08-06T17:35:33.080795Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation 7eaebc4c-ce45-4a63-92de-1322a93b2f10 · outbound

This paper cites an unresolved cited work.

Improved upper limits on the 21-cm signal power spectrum at $z=17.0$ and $z=20.3$ from an optimal field observed with NenuFAR Unresolved cited work

Reference 88

Resolution: unresolved; raw_fallback, observed 2026-08-06T17:35:33.058451Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation a46cad0c-66a9-4911-bd2b-a0307978cf2b · outbound

This paper cites an unresolved cited work.

Improved upper limits on the 21-cm signal power spectrum at $z=17.0$ and $z=20.3$ from an optimal field observed with NenuFAR Unresolved cited work

Reference 89

Resolution: unresolved; raw_fallback, observed 2026-08-06T17:35:33.039269Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation 106a5dd3-a5a3-44f3-a2be-f6f38b4bac96 · outbound

This paper cites an unresolved cited work.

Improved upper limits on the 21-cm signal power spectrum at $z=17.0$ and $z=20.3$ from an optimal field observed with NenuFAR Unresolved cited work

Reference 90

Resolution: unresolved; raw_fallback, observed 2026-08-06T17:35:33.014931Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation be5f62fe-9e6d-4225-81e6-7906fd0f0320 · outbound

This paper cites H., et al., 2016, MNRAS, 463, 4317.

Improved upper limits on the 21-cm signal power spectrum at $z=17.0$ and $z=20.3$ from an optimal field observed with NenuFAR H., et al., 2016, MNRAS, 463, 4317

Reference 91

Resolution: verified fuzzy; raw_fallback, observed 2026-08-06T17:35:32.995822Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation 32a41106-ba40-4e00-b5c5-7aa934ea4efe · outbound

This paper cites an unresolved cited work.

Improved upper limits on the 21-cm signal power spectrum at $z=17.0$ and $z=20.3$ from an optimal field observed with NenuFAR Unresolved cited work

Reference 92

Resolution: unresolved; raw_fallback, observed 2026-08-06T17:35:32.978140Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation be831887-7172-4e30-a043-690fcaedb06b · outbound

This paper cites an unresolved cited work.

Improved upper limits on the 21-cm signal power spectrum at $z=17.0$ and $z=20.3$ from an optimal field observed with NenuFAR Unresolved cited work

Reference 93

Resolution: unresolved; raw_fallback, observed 2026-08-06T17:35:32.960904Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation 2c886a6f-fb4a-45f5-a8e7-a1c9f76cf780 · outbound

This paper cites an unresolved cited work.

Improved upper limits on the 21-cm signal power spectrum at $z=17.0$ and $z=20.3$ from an optimal field observed with NenuFAR Unresolved cited work

Reference 94

Resolution: unresolved; no resolver link, observed 2026-08-06T17:35:31.424722Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation cf77f291-974b-4018-af30-ecceaba0f85c · outbound

This paper cites an unresolved cited work.

Improved upper limits on the 21-cm signal power spectrum at $z=17.0$ and $z=20.3$ from an optimal field observed with NenuFAR Unresolved cited work

Reference 95

Resolution: unresolved; raw_fallback, observed 2026-08-06T17:35:32.945137Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation 02fe2302-8142-4057-bac3-d9229906409b · outbound

This paper cites R., Loeb A., 2012, Reports on Progress in Physics, 75, 086901.

Improved upper limits on the 21-cm signal power spectrum at $z=17.0$ and $z=20.3$ from an optimal field observed with NenuFAR R., Loeb A., 2012, Reports on Progress in Physics, 75, 086901

Reference 96

Resolution: unresolved; no resolver link, observed 2026-08-06T17:35:31.437409Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 2dd8ab28-2685-4cc9-9b2c-ad6d57acf69c · outbound

This paper cites an unresolved cited work.

Improved upper limits on the 21-cm signal power spectrum at $z=17.0$ and $z=20.3$ from an optimal field observed with NenuFAR Unresolved cited work

Reference 97

Resolution: unresolved; no resolver link, observed 2026-08-06T17:35:31.442109Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 86587836-a150-4d97-9908-82a1b01734d3 · outbound

This paper cites an unresolved cited work.

Improved upper limits on the 21-cm signal power spectrum at $z=17.0$ and $z=20.3$ from an optimal field observed with NenuFAR Unresolved cited work

Reference 98

Resolution: unresolved; no resolver link, observed 2026-08-06T17:35:31.447034Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ca4abaef-3360-4c54-8cb8-3ea0f83da225 · outbound

This paper cites an unresolved cited work.

Improved upper limits on the 21-cm signal power spectrum at $z=17.0$ and $z=20.3$ from an optimal field observed with NenuFAR Unresolved cited work

Reference 99

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Improved upper limits on the 21-cm signal power spectrum at $z=17.0$ and $z=20.3$ from an optimal field observed with NenuFAR Unresolved cited work

Reference 100

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Flash Ionization of the Early Universe by Pop III.1 Supermassive Stars cites this paper.

Flash Ionization of the Early Universe by Pop III.1 Supermassive Stars Improved upper limits on the 21-cm signal power spectrum at $z=17.0$ and $z=20.3$ from an optimal field observed with NenuFAR

Reference 35

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Observation 223cf99e-c3f5-4e9b-8889-a11d140c90b8 · inbound

A New Boundary Condition on Reionization cites this paper.

A New Boundary Condition on Reionization Improved upper limits on the 21-cm signal power spectrum at $z=17.0$ and $z=20.3$ from an optimal field observed with NenuFAR

Reference 70

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Into the Gompverse: A robust Gompertzian reionization model for CMB analyses cites this paper.

Into the Gompverse: A robust Gompertzian reionization model for CMB analyses Improved upper limits on the 21-cm signal power spectrum at $z=17.0$ and $z=20.3$ from an optimal field observed with NenuFAR

Reference 72

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Mitigating residual foregrounds and systematic errors in SKA1-Low AA* EoR observations via Bayesian Gaussian Process Regression cites this paper.

Mitigating residual foregrounds and systematic errors in SKA1-Low AA* EoR observations via Bayesian Gaussian Process Regression Improved upper limits on the 21-cm signal power spectrum at $z=17.0$ and $z=20.3$ from an optimal field observed with NenuFAR

Reference 14

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Late-time Quantum Vacuum Decay and its Cosmological Implications cites this paper.

Late-time Quantum Vacuum Decay and its Cosmological Implications Improved upper limits on the 21-cm signal power spectrum at $z=17.0$ and $z=20.3$ from an optimal field observed with NenuFAR

Reference 93

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Observation 79730c24-392f-47c0-b00c-acf07fa1cf3d · inbound

Machine Learning and the SKA for Cosmic Dawn and the Epoch of Reionization cites this paper.

Machine Learning and the SKA for Cosmic Dawn and the Epoch of Reionization Improved upper limits on the 21-cm signal power spectrum at $z=17.0$ and $z=20.3$ from an optimal field observed with NenuFAR

Reference 157

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Observation 4dfd5724-e894-4d46-8fd2-ee2fdb695acb · inbound

Impact of numerical stability in Bayesian noise wave calibration on global 21-cm experiments cites this paper.

Impact of numerical stability in Bayesian noise wave calibration on global 21-cm experiments Improved upper limits on the 21-cm signal power spectrum at $z=17.0$ and $z=20.3$ from an optimal field observed with NenuFAR

Reference 55

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