When galaxies burst II. Implications of enhanced burstiness for the 21-cm Cosmic Dawn signal | Paper Citation Record

Observation ffd8a46c-c627-45dc-b8e3-b7e9fa4a0812 · outbound

This paper cites The brightest galaxies at Cosmic Dawn.

When galaxies burst II. Implications of enhanced burstiness for the 21-cm Cosmic Dawn signal The brightest galaxies at Cosmic Dawn

Reference 1

Resolution: unresolved; no resolver link, observed 2026-08-01T09:49:16.895754Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 2b592bdc-feed-4bf3-905e-2701781038de · outbound

This paper cites an unresolved cited work.

When galaxies burst II. Implications of enhanced burstiness for the 21-cm Cosmic Dawn signal Unresolved cited work

Reference 2

Resolution: unresolved; no resolver link, observed 2026-08-01T09:49:16.601276Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7ce561d5-97a3-458d-b5ce-c1934e887ef0 · outbound

This paper cites (17), but with two emission red- shifts per shell-pair rather than one.

When galaxies burst II. Implications of enhanced burstiness for the 21-cm Cosmic Dawn signal (17), but with two emission red- shifts per shell-pair rather than one

Reference 3

Resolution: malformed identifier; no resolver link, observed 2026-08-01T09:49:16.763274Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 3b2e8fcf-ece5-4178-b2b0-e5af6eb3923e · outbound

This paper cites A Comprehensive Study on Galaxies at z~9-16 Found in the Early JWST Data: UV Luminosity Functions and Cosmic Star-Formation History at the Pre-Reionization Epoch.

When galaxies burst II. Implications of enhanced burstiness for the 21-cm Cosmic Dawn signal A Comprehensive Study on Galaxies at z~9-16 Found in the Early JWST Data: UV Luminosity Functions and Cosmic Star-Formation History at the Pre-Reionization Epoch

Reference 4

Resolution: unresolved; no resolver link, observed 2026-08-01T09:49:17.077173Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 89e244f3-482a-489f-a6c3-1d64c2b646ee · 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.

When galaxies burst II. Implications of enhanced burstiness for the 21-cm Cosmic Dawn signal 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 5

Resolution: unresolved; no resolver link, observed 2026-08-01T09:49:17.240501Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 64e3964a-000c-4f0b-ba01-a7aa18c29a0d · outbound

This paper cites JWST PRIMER: A new multi-field determination of the evolving galaxy UV luminosity function at redshifts $\mathbf{z \simeq 9-15}$.

When galaxies burst II. Implications of enhanced burstiness for the 21-cm Cosmic Dawn signal JWST PRIMER: A new multi-field determination of the evolving galaxy UV luminosity function at redshifts $\mathbf{z \simeq 9-15}$

Reference 6

Resolution: unresolved; no resolver link, observed 2026-08-01T09:49:17.418307Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 547135a9-6166-48cc-bc90-d7d11cf536d8 · outbound

This paper cites Earliest Galax- ies in the JADES Origins Field: Luminosity Function and Cosmic Star Formation Rate Density 300 Myr af- ter the Big Bang,.

When galaxies burst II. Implications of enhanced burstiness for the 21-cm Cosmic Dawn signal Earliest Galax- ies in the JADES Origins Field: Luminosity Function and Cosmic Star Formation Rate Density 300 Myr af- ter the Big Bang,

Reference 7

Resolution: unresolved; no resolver link, observed 2026-08-01T09:49:17.589608Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a6505374-d424-456a-823f-a656d9bfbe9b · outbound

This paper cites Bursty Star Formation Naturally Explains the Abundance of Bright Galaxies at Cosmic Dawn.

When galaxies burst II. Implications of enhanced burstiness for the 21-cm Cosmic Dawn signal Bursty Star Formation Naturally Explains the Abundance of Bright Galaxies at Cosmic Dawn

Reference 8

Resolution: unresolved; no resolver link, observed 2026-08-01T09:49:17.727889Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 662bd127-3b07-4ee3-9945-d45957c9be2b · outbound

This paper cites Identification and properties of intense star-forming galaxies at red- shifts z>10,.

When galaxies burst II. Implications of enhanced burstiness for the 21-cm Cosmic Dawn signal Identification and properties of intense star-forming galaxies at red- shifts z>10,

Reference 9

Resolution: unresolved; no resolver link, observed 2026-08-01T09:49:17.902678Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 716eb9ff-5ce8-4120-8e5d-df47e412a33f · outbound

This paper cites Stochastic star formation in early galaxies: JWST implications.

When galaxies burst II. Implications of enhanced burstiness for the 21-cm Cosmic Dawn signal Stochastic star formation in early galaxies: JWST implications

Reference 10

Resolution: unresolved; no resolver link, observed 2026-08-01T09:49:18.038993Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f9af0c5b-e50c-4d57-8b87-f9773447249c · outbound

This paper cites Balancing the efficiency and stochasticity of star formation with dust extinction in z > 10 galaxies observed by JWST.

When galaxies burst II. Implications of enhanced burstiness for the 21-cm Cosmic Dawn signal Balancing the efficiency and stochasticity of star formation with dust extinction in z > 10 galaxies observed by JWST

Reference 11

Resolution: unresolved; no resolver link, observed 2026-08-01T09:49:18.216939Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c04f10ae-a47a-4f5c-8b2e-ba1d5ec007f6 · outbound

This paper cites (Star)bursts of FIRE: observational signatures of bursty star formation in galaxies.

When galaxies burst II. Implications of enhanced burstiness for the 21-cm Cosmic Dawn signal (Star)bursts of FIRE: observational signatures of bursty star formation in galaxies

Reference 12

Resolution: unresolved; no resolver link, observed 2026-08-01T09:49:18.327493Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7573fbcf-d433-46b9-9139-07df1b27488b · outbound

This paper cites A Model for the Origin of Bursty Star Formation in Galaxies.

When galaxies burst II. Implications of enhanced burstiness for the 21-cm Cosmic Dawn signal A Model for the Origin of Bursty Star Formation in Galaxies

Reference 13

Resolution: unresolved; no resolver link, observed 2026-08-01T09:49:18.460981Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 78ae9a1d-2524-4d98-b006-b6aea298c5e4 · outbound

This paper cites Bursty star formation during the Cosmic Dawn driven by delayed stellar feedback.

When galaxies burst II. Implications of enhanced burstiness for the 21-cm Cosmic Dawn signal Bursty star formation during the Cosmic Dawn driven by delayed stellar feedback

Reference 14

Resolution: unresolved; no resolver link, observed 2026-08-01T09:49:18.572324Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 896727e3-bf3d-4c34-ab49-a2003a770ad2 · outbound

This paper cites Seen and unseen: bursty star formation and its implications for observations of high-redshift galaxies with JWST.

When galaxies burst II. Implications of enhanced burstiness for the 21-cm Cosmic Dawn signal Seen and unseen: bursty star formation and its implications for observations of high-redshift galaxies with JWST

Reference 15

Resolution: unresolved; no resolver link, observed 2026-08-01T09:49:18.731092Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 6aabd3cc-54c0-4141-8580-258e3078942d · outbound

This paper cites The Star-Forming Main Sequence in JADES and CEERS at $z>1.4$: Investigating the Burstiness of Star Formation.

When galaxies burst II. Implications of enhanced burstiness for the 21-cm Cosmic Dawn signal The Star-Forming Main Sequence in JADES and CEERS at $z>1.4$: Investigating the Burstiness of Star Formation

Reference 16

Resolution: unresolved; no resolver link, observed 2026-08-01T09:49:18.850901Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 5e98571f-19a5-43c0-8f27-3ac020ebba18 · outbound

This paper cites The Star-forming and Ionizing Properties of Dwarf z~6-9 Galaxies in JADES: Insights on Bursty Star Formation and Ionized Bubble Growth.

When galaxies burst II. Implications of enhanced burstiness for the 21-cm Cosmic Dawn signal The Star-forming and Ionizing Properties of Dwarf z~6-9 Galaxies in JADES: Insights on Bursty Star Formation and Ionized Bubble Growth

Reference 17

Resolution: unresolved; no resolver link, observed 2026-08-01T09:49:19.021108Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation bf030f07-8e6c-4ec6-ad26-cb31630d4af2 · outbound

This paper cites Constraining bursty star formation histories with galaxy UV and Hαluminosity functions and clus- tering,.

When galaxies burst II. Implications of enhanced burstiness for the 21-cm Cosmic Dawn signal Constraining bursty star formation histories with galaxy UV and Hαluminosity functions and clus- tering,

Reference 18

Resolution: unresolved; no resolver link, observed 2026-08-01T09:49:19.137970Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7cdc84fd-a17c-4c5d-913e-b36c9cf67a7b · outbound

This paper cites Relatively Fast and Reasonably Furious: Evidence for Increased Burstiness in Smaller Halos at Cosmic Dawn.

When galaxies burst II. Implications of enhanced burstiness for the 21-cm Cosmic Dawn signal Relatively Fast and Reasonably Furious: Evidence for Increased Burstiness in Smaller Halos at Cosmic Dawn

Reference 19

Resolution: unresolved; no resolver link, observed 2026-08-01T09:49:19.269279Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation eba75b5a-f97a-46ae-92d9-67e957574649 · outbound

This paper cites When galaxies burst: enhanced shot-noise for line-intensity mapping in the JWST era.

When galaxies burst II. Implications of enhanced burstiness for the 21-cm Cosmic Dawn signal When galaxies burst: enhanced shot-noise for line-intensity mapping in the JWST era

Reference 20

Resolution: unresolved; no resolver link, observed 2026-08-01T09:49:19.420307Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c174a541-5122-4470-a050-defff10520f7 · outbound

This paper cites Line-Intensity Mapping: 2017 Status Report.

When galaxies burst II. Implications of enhanced burstiness for the 21-cm Cosmic Dawn signal Line-Intensity Mapping: 2017 Status Report

Reference 21

Resolution: unresolved; no resolver link, observed 2026-08-01T09:49:19.579730Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 595f0ad7-5f1e-4a19-9f2d-6db30c8433c9 · outbound

This paper cites Line-Intensity Mapping: Theory Review.

When galaxies burst II. Implications of enhanced burstiness for the 21-cm Cosmic Dawn signal Line-Intensity Mapping: Theory Review

Reference 22

Resolution: unresolved; no resolver link, observed 2026-08-01T09:49:19.698291Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a76f46d1-bd45-495c-b0ce-b22ad0233c55 · outbound

This paper cites Line-Intensity Mapping,.

When galaxies burst II. Implications of enhanced burstiness for the 21-cm Cosmic Dawn signal Line-Intensity Mapping,

Reference 23

Resolution: unresolved; no resolver link, observed 2026-08-01T09:49:19.763070Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation de94e510-d89d-4008-9bb6-4ee667f6e038 · outbound

This paper cites Effects of Bursty Star Formation on [CII] Line Intensity Mapping of High-redshift Galaxies.

When galaxies burst II. Implications of enhanced burstiness for the 21-cm Cosmic Dawn signal Effects of Bursty Star Formation on [CII] Line Intensity Mapping of High-redshift Galaxies

Reference 24

Resolution: unresolved; no resolver link, observed 2026-08-01T09:49:19.839225Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 83ccf117-84e6-45b7-86f8-fbc902d6b6cd · outbound

This paper cites The First Galaxies in the Universe.

When galaxies burst II. Implications of enhanced burstiness for the 21-cm Cosmic Dawn signal The First Galaxies in the Universe

Reference 25

Resolution: unresolved; no resolver link, observed 2026-08-01T09:49:19.924539Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation b96cefb4-990b-4052-b99d-3f607b98cb75 · outbound

This paper cites 21-cm cosmology.

When galaxies burst II. Implications of enhanced burstiness for the 21-cm Cosmic Dawn signal 21-cm cosmology

Reference 26

Resolution: unresolved; no resolver link, observed 2026-08-01T09:49:19.987180Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d18ee576-14fc-4dd7-90a1-6a9d0b73634f · outbound

This paper cites 21-cm Tomography of the Intergalactic Medium at High Redshift.

When galaxies burst II. Implications of enhanced burstiness for the 21-cm Cosmic Dawn signal 21-cm Tomography of the Intergalactic Medium at High Redshift

Reference 27

Resolution: unresolved; no resolver link, observed 2026-08-01T09:49:20.051652Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0c526e8d-21e0-46ed-b20f-f27b4754b582 · outbound

This paper cites Measuring the small - scale power spectrum of cosmic density fluctuations through 21 cm tomography prior to the epoch of structure forma- tion,.

When galaxies burst II. Implications of enhanced burstiness for the 21-cm Cosmic Dawn signal Measuring the small - scale power spectrum of cosmic density fluctuations through 21 cm tomography prior to the epoch of structure forma- tion,

Reference 28

Resolution: unresolved; no resolver link, observed 2026-08-01T09:49:20.123110Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 2018076f-a31e-48ff-9168-a915b2a7a1ce · outbound

This paper cites What Next-Generation 21 cm Power Spectrum Measurements Can Teach Us About the Epoch of Reionization.

When galaxies burst II. Implications of enhanced burstiness for the 21-cm Cosmic Dawn signal What Next-Generation 21 cm Power Spectrum Measurements Can Teach Us About the Epoch of Reionization

Reference 29

Resolution: unresolved; no resolver link, observed 2026-08-01T09:49:20.238008Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 17452115-2835-4a14-976c-4768d801a3f3 · outbound

This paper cites Snowmass2021 Cosmic Frontier White Paper: 21cm Radiation as a Probe of Physics Across Cosmic Ages.

When galaxies burst II. Implications of enhanced burstiness for the 21-cm Cosmic Dawn signal Snowmass2021 Cosmic Frontier White Paper: 21cm Radiation as a Probe of Physics Across Cosmic Ages

Reference 30

Resolution: unresolved; no resolver link, observed 2026-08-01T09:49:20.339272Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 9736fc86-1e51-4922-a988-75ead339dd22 · outbound

This paper cites Cosmology at Low Frequencies: The 21 cm Transition and the High-Redshift Universe,.

When galaxies burst II. Implications of enhanced burstiness for the 21-cm Cosmic Dawn signal Cosmology at Low Frequencies: The 21 cm Transition and the High-Redshift Universe,

Reference 31

Resolution: unresolved; no resolver link, observed 2026-08-01T09:49:20.465012Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 65aff407-20d2-4cb1-a948-5b8a3eda490b · outbound

This paper cites Effects of feedback-free starburst galaxies on the 21-cm signal and reionization history.

When galaxies burst II. Implications of enhanced burstiness for the 21-cm Cosmic Dawn signal Effects of feedback-free starburst galaxies on the 21-cm signal and reionization history

Reference 32

Resolution: unresolved; no resolver link, observed 2026-08-01T09:49:20.553980Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 6412b1f6-b766-4ccd-99f2-1d68b2caf757 · outbound

This paper cites JWST constraints on the UV luminosity density at cosmic dawn: implications for 21-cm cosmology.

When galaxies burst II. Implications of enhanced burstiness for the 21-cm Cosmic Dawn signal JWST constraints on the UV luminosity density at cosmic dawn: implications for 21-cm cosmology

Reference 33

Resolution: unresolved; no resolver link, observed 2026-08-01T09:49:20.653094Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 65075249-0c48-4a59-8878-10b5479dc1c4 · outbound

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

When galaxies burst II. Implications of enhanced burstiness for the 21-cm Cosmic Dawn signal Exploiting synergies between JWST and cosmic 21-cm observations to uncover star formation in the early Universe

Reference 34

Resolution: unresolved; no resolver link, observed 2026-08-01T09:49:20.735261Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 6a952dfa-fcdf-40e3-a8a6-50603be458a9 · outbound

This paper cites On the excitation mechanism of the 21-cm (radio-frequency) interstellar hydrogen emission line.,.

When galaxies burst II. Implications of enhanced burstiness for the 21-cm Cosmic Dawn signal On the excitation mechanism of the 21-cm (radio-frequency) interstellar hydrogen emission line.,

Reference 35

Resolution: unresolved; no resolver link, observed 2026-08-01T09:49:20.817799Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 2535b08c-3c05-421b-93b3-36896406632c · outbound

This paper cites The Spin Temperature of Intergalactic Neu- tral Hydrogen.,.

When galaxies burst II. Implications of enhanced burstiness for the 21-cm Cosmic Dawn signal The Spin Temperature of Intergalactic Neu- tral Hydrogen.,

Reference 36

Resolution: unresolved; no resolver link, observed 2026-08-01T09:49:20.893558Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation cc5521b7-05f0-463a-995a-3909fbb23f4e · outbound

This paper cites Wouthuysen-Field coupling strength and 18 application to high-redshift 21 cm radiation,.

When galaxies burst II. Implications of enhanced burstiness for the 21-cm Cosmic Dawn signal Wouthuysen-Field coupling strength and 18 application to high-redshift 21 cm radiation,

Reference 37

Resolution: unresolved; no resolver link, observed 2026-08-01T09:49:20.981569Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 22444a4b-b216-4003-a62e-2a0e3d2b4ca3 · outbound

This paper cites Descending from on high: lyman series cascades and spin-kinetic temperature coupling in the 21 cm line,.

When galaxies burst II. Implications of enhanced burstiness for the 21-cm Cosmic Dawn signal Descending from on high: lyman series cascades and spin-kinetic temperature coupling in the 21 cm line,

Reference 38

Resolution: unresolved; no resolver link, observed 2026-08-01T09:49:21.049534Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 276e9464-57a3-4798-bebd-87c1c488bf51 · outbound

This paper cites Radiation Backgrounds at Cosmic Dawn: X-Rays from Compact Binaries.

When galaxies burst II. Implications of enhanced burstiness for the 21-cm Cosmic Dawn signal Radiation Backgrounds at Cosmic Dawn: X-Rays from Compact Binaries

Reference 39

Resolution: unresolved; no resolver link, observed 2026-08-01T09:49:21.123981Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f7ee4fde-eaa4-4064-80fd-78ec1dfe1ae4 · outbound

This paper cites 21 cm fluctuations from inhomogeneous X-ray heating before reionization.

When galaxies burst II. Implications of enhanced burstiness for the 21-cm Cosmic Dawn signal 21 cm fluctuations from inhomogeneous X-ray heating before reionization

Reference 40

Resolution: unresolved; no resolver link, observed 2026-08-01T09:49:21.196455Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation eb583b66-0e81-43bd-a3bd-cd4f0051e92b · outbound

This paper cites Signatures of X-rays in the early Universe.

When galaxies burst II. Implications of enhanced burstiness for the 21-cm Cosmic Dawn signal Signatures of X-rays in the early Universe

Reference 41

Resolution: unresolved; no resolver link, observed 2026-08-01T09:49:21.265662Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f29f1956-a41d-427d-9f09-2fdb7dbb7586 · outbound

This paper cites The X-ray spectra of the first galaxies: 21cm signatures.

When galaxies burst II. Implications of enhanced burstiness for the 21-cm Cosmic Dawn signal The X-ray spectra of the first galaxies: 21cm signatures

Reference 42

Resolution: unresolved; no resolver link, observed 2026-08-01T09:49:21.371317Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 906460ae-0bd6-42a0-92d1-73f102ec7e53 · outbound

This paper cites The observable signature of late heating of the Universe during cosmic reionization.

When galaxies burst II. Implications of enhanced burstiness for the 21-cm Cosmic Dawn signal The observable signature of late heating of the Universe during cosmic reionization

Reference 43

Resolution: unresolved; no resolver link, observed 2026-08-01T09:49:21.442289Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 2c21095e-3e23-477c-8ca8-977b0454ee9a · outbound

This paper cites Unequal-Time Correlators for Cosmology.

When galaxies burst II. Implications of enhanced burstiness for the 21-cm Cosmic Dawn signal Unequal-Time Correlators for Cosmology

Reference 44

Resolution: unresolved; no resolver link, observed 2026-08-01T09:49:21.489771Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation bca2a60f-4996-4a10-be0a-4faa2f1d0853 · outbound

This paper cites Power spectrum in the cave.

When galaxies burst II. Implications of enhanced burstiness for the 21-cm Cosmic Dawn signal Power spectrum in the cave

Reference 45

Resolution: unresolved; no resolver link, observed 2026-08-01T09:49:21.563917Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 48d5c928-a34e-470d-9b61-6d90548b843e · outbound

This paper cites Observed unequal-time power spectrum.

When galaxies burst II. Implications of enhanced burstiness for the 21-cm Cosmic Dawn signal Observed unequal-time power spectrum

Reference 46

Resolution: unresolved; no resolver link, observed 2026-08-01T09:49:21.642053Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 639fa6ab-9911-41d8-a980-ac9c2a11f31e · outbound

This paper cites The unequal-time matter power spectrum: impact on weak lensing observables.

When galaxies burst II. Implications of enhanced burstiness for the 21-cm Cosmic Dawn signal The unequal-time matter power spectrum: impact on weak lensing observables

Reference 47

Resolution: unresolved; no resolver link, observed 2026-08-01T09:49:21.728587Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f5499007-2a51-4bfc-8251-e6d657bb74fa · outbound

This paper cites Unequal time correlators and the Zeldovich approximation.

When galaxies burst II. Implications of enhanced burstiness for the 21-cm Cosmic Dawn signal Unequal time correlators and the Zeldovich approximation

Reference 48

Resolution: unresolved; no resolver link, observed 2026-08-01T09:49:21.872868Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation abe748da-acb6-43dc-9c5a-1a7f2c965f77 · outbound

This paper cites The multi-frequency angular power spectrum of the epoch of reionization 21 cm signal.

When galaxies burst II. Implications of enhanced burstiness for the 21-cm Cosmic Dawn signal The multi-frequency angular power spectrum of the epoch of reionization 21 cm signal

Reference 49

Resolution: unresolved; no resolver link, observed 2026-08-01T09:49:22.012153Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation eddd9ee4-4c5a-4718-a424-7f596028947c · outbound

This paper cites The Evolving Power Spectrum for the light cone Epoch of Reionization (EoR) 21-cm signal.

When galaxies burst II. Implications of enhanced burstiness for the 21-cm Cosmic Dawn signal The Evolving Power Spectrum for the light cone Epoch of Reionization (EoR) 21-cm signal

Reference 50

Resolution: unresolved; no resolver link, observed 2026-08-01T09:49:22.153970Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 20b178e6-3f30-4688-8ac1-e59b62d88be7 · outbound

This paper cites Beyond the Power Spectrum: A New Framework for Non-Stationary Fields with Applications to Light-Cone Effects in Line Intensity Mapping.

When galaxies burst II. Implications of enhanced burstiness for the 21-cm Cosmic Dawn signal Beyond the Power Spectrum: A New Framework for Non-Stationary Fields with Applications to Light-Cone Effects in Line Intensity Mapping

Reference 51

Resolution: unresolved; no resolver link, observed 2026-08-01T09:49:22.352331Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ab2166fb-8eca-4e58-8d3b-f8a153b8df25 · outbound

This paper cites Time-dependent fluctuations in the metagalactic photoionization background.

When galaxies burst II. Implications of enhanced burstiness for the 21-cm Cosmic Dawn signal Time-dependent fluctuations in the metagalactic photoionization background

Reference 52

Resolution: unresolved; no resolver link, observed 2026-08-01T09:49:22.548803Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation b5f93565-6986-43ee-94c9-0c54bd71b537 · outbound

This paper cites Shot noise and scatter in the star formation efficiency as a source of 21-cm fluctuations.

When galaxies burst II. Implications of enhanced burstiness for the 21-cm Cosmic Dawn signal Shot noise and scatter in the star formation efficiency as a source of 21-cm fluctuations

Reference 53

Resolution: unresolved; no resolver link, observed 2026-08-01T09:49:22.681757Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 228a5d56-52fe-444a-9010-bd2944a7a2ad · outbound

This paper cites Efficient simulation of discrete galaxy populations and associated radiation fields over the first billion years,.

When galaxies burst II. Implications of enhanced burstiness for the 21-cm Cosmic Dawn signal Efficient simulation of discrete galaxy populations and associated radiation fields over the first billion years,

Reference 54

Resolution: unresolved; no resolver link, observed 2026-08-01T09:49:22.878686Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c4a15c68-ff19-4e95-ac8e-1ea834d830b4 · outbound

This paper cites 21cmFAST: A Fast, Semi-Numerical Simulation of the High-Redshift 21-cm Signal.

When galaxies burst II. Implications of enhanced burstiness for the 21-cm Cosmic Dawn signal 21cmFAST: A Fast, Semi-Numerical Simulation of the High-Redshift 21-cm Signal

Reference 55

Resolution: unresolved; no resolver link, observed 2026-08-01T09:49:23.081841Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 3807ea1c-0a7a-467a-b053-28b813981881 · outbound

This paper cites 21cmFAST v3: A Python-integrated C code forgenerating 3D realizations of the cosmic 21cm signal.

When galaxies burst II. Implications of enhanced burstiness for the 21-cm Cosmic Dawn signal 21cmFAST v3: A Python-integrated C code forgenerating 3D realizations of the cosmic 21cm signal

Reference 56

Resolution: unresolved; no resolver link, observed 2026-08-01T09:49:23.178093Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 96d20f02-9e0e-41d2-8fa4-20d14593f25a · outbound

This paper cites The Impact of the First Galaxies on Cosmic Dawn and Reionization.

When galaxies burst II. Implications of enhanced burstiness for the 21-cm Cosmic Dawn signal The Impact of the First Galaxies on Cosmic Dawn and Reionization

Reference 57

Resolution: unresolved; no resolver link, observed 2026-08-01T09:49:23.266783Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c04b8c23-5dfb-4d53-a76b-267df952231a · outbound

This paper cites Dark-ages Reionization & Galaxy Formation Simulation I: The dynamical lives of high redshift galaxies.

When galaxies burst II. Implications of enhanced burstiness for the 21-cm Cosmic Dawn signal Dark-ages Reionization & Galaxy Formation Simulation I: The dynamical lives of high redshift galaxies

Reference 58

Resolution: unresolved; no resolver link, observed 2026-08-01T09:49:23.343043Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 1e5bfc3e-9c92-4eed-96d2-30b561d2febc · outbound

This paper cites Piezoelectric Tunable Microwave Superconducting Cavity.

When galaxies burst II. Implications of enhanced burstiness for the 21-cm Cosmic Dawn signal Piezoelectric Tunable Microwave Superconducting Cavity

Reference 59

Resolution: unresolved; no resolver link, observed 2026-08-01T09:49:23.421239Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7e6010b2-2e31-4441-84eb-426cd123c8af · outbound

This paper cites Thermal and Reionisation History within a Large-Volume Semi-Analytic Galaxy Formation Simulation.

When galaxies burst II. Implications of enhanced burstiness for the 21-cm Cosmic Dawn signal Thermal and Reionisation History within a Large-Volume Semi-Analytic Galaxy Formation Simulation

Reference 60

Resolution: unresolved; no resolver link, observed 2026-08-01T09:49:23.586224Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 38e8bc90-5691-40ba-bcdb-8c40b25e7408 · outbound

This paper cites An Effective Model for the Cosmic-Dawn 21-cm Signal.

When galaxies burst II. Implications of enhanced burstiness for the 21-cm Cosmic Dawn signal An Effective Model for the Cosmic-Dawn 21-cm Signal

Reference 61

Resolution: unresolved; no resolver link, observed 2026-08-01T09:49:23.783028Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 36969814-a075-405e-9b1b-75f0759fa0f0 · outbound

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

When galaxies burst II. Implications of enhanced burstiness for the 21-cm Cosmic Dawn signal The First Billion Years in Seconds: An Effective Model for the 21-cm Signal with Population III Stars

Reference 62

Resolution: unresolved; no resolver link, observed 2026-08-01T09:49:24.001629Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation fc22dc5e-66a6-4305-9848-544a9179e74e · outbound

This paper cites Bursty or Heavy? The Surprise of Bright Population III Systems in the Reionization Era,.

When galaxies burst II. Implications of enhanced burstiness for the 21-cm Cosmic Dawn signal Bursty or Heavy? The Surprise of Bright Population III Systems in the Reionization Era,

Reference 63

Resolution: unresolved; no resolver link, observed 2026-08-01T09:49:24.177023Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 242dff1c-e9f0-46de-9686-640e96bbeb5e · outbound

This paper cites Hydrogen Epoch of Reionization Array (HERA).

When galaxies burst II. Implications of enhanced burstiness for the 21-cm Cosmic Dawn signal Hydrogen Epoch of Reionization Array (HERA)

Reference 64

Resolution: unresolved; no resolver link, observed 2026-08-01T09:49:24.350443Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 5aeb9271-72ed-48e5-b83b-562c6fef9c72 · outbound

This paper cites First Results from HERA Phase I: Upper Limits on the Epoch of Reionization 21 cm Power Spectrum.

When galaxies burst II. Implications of enhanced burstiness for the 21-cm Cosmic Dawn signal First Results from HERA Phase I: Upper Limits on the Epoch of Reionization 21 cm Power Spectrum

Reference 65

Resolution: unresolved; no resolver link, observed 2026-08-01T09:49:24.567728Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation eca1c980-a4aa-443b-bdc1-884ea4d5ec8d · outbound

This paper cites Improved Constraints on the 21 cm EoR Power Spectrum and the X-Ray Heating of the IGM with HERA Phase I Observations.

When galaxies burst II. Implications of enhanced burstiness for the 21-cm Cosmic Dawn signal Improved Constraints on the 21 cm EoR Power Spectrum and the X-Ray Heating of the IGM with HERA Phase I Observations

Reference 66

Resolution: unresolved; no resolver link, observed 2026-08-01T09:49:24.744160Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 80ff0822-167c-403d-8d6c-c364f16b4c2e · outbound

This paper cites LOFAR: The LOw-Frequency ARray.

When galaxies burst II. Implications of enhanced burstiness for the 21-cm Cosmic Dawn signal LOFAR: The LOw-Frequency ARray

Reference 67

Resolution: unresolved; no resolver link, observed 2026-08-01T09:49:24.880212Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 16415c97-0853-45c8-9a0d-71e5b5885b29 · outbound

This paper cites Improved upper limits on the 21-cm signal power spectrum of neutral hydrogen at $\boldsymbol{z \approx 9.1}$ from LOFAR.

When galaxies burst II. Implications of enhanced burstiness for the 21-cm Cosmic Dawn signal Improved upper limits on the 21-cm signal power spectrum of neutral hydrogen at $\boldsymbol{z \approx 9.1}$ from LOFAR

Reference 68

Resolution: unresolved; no resolver link, observed 2026-08-01T09:49:25.032083Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e8ef9fa9-a3e1-4752-811a-a98747c71dee · outbound

This paper cites First upper limits on the 21-cm signal power spectrum of neutral hydrogen atz= 9.16 from the LOF AR 3C196 field,.

When galaxies burst II. Implications of enhanced burstiness for the 21-cm Cosmic Dawn signal First upper limits on the 21-cm signal power spectrum of neutral hydrogen atz= 9.16 from the LOF AR 3C196 field,

Reference 69

Resolution: unresolved; no resolver link, observed 2026-08-01T09:49:25.203171Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 49a0621b-4503-45c2-be1a-6ee73e116b8f · outbound

This paper cites An absorption profile centred at 78 megahertz in the sky-averaged spectrum.

When galaxies burst II. Implications of enhanced burstiness for the 21-cm Cosmic Dawn signal An absorption profile centred at 78 megahertz in the sky-averaged spectrum

Reference 70

Resolution: unresolved; no resolver link, observed 2026-08-01T09:49:25.372928Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c5ea860f-b6ae-4410-b408-e1ac45ef7284 · outbound

This paper cites On the detection of a cosmic dawn signal in the radio background.

When galaxies burst II. Implications of enhanced burstiness for the 21-cm Cosmic Dawn signal On the detection of a cosmic dawn signal in the radio background

Reference 71

Resolution: unresolved; no resolver link, observed 2026-08-01T09:49:25.514618Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 5b591bdf-5f80-4c0e-929d-38a0a4805372 · outbound

This paper cites On the Theory of the Brownian Motion,.

When galaxies burst II. Implications of enhanced burstiness for the 21-cm Cosmic Dawn signal On the Theory of the Brownian Motion,

Reference 72

Resolution: unresolved; no resolver link, observed 2026-08-01T09:49:25.662950Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 988d78f9-e4f8-4a6a-bc47-5ed630a78254 · outbound

This paper cites Stochastic modelling of star- formation histories I: the scatter of the star-forming main sequence,.

When galaxies burst II. Implications of enhanced burstiness for the 21-cm Cosmic Dawn signal Stochastic modelling of star- formation histories I: the scatter of the star-forming main sequence,

Reference 73

Resolution: unresolved; no resolver link, observed 2026-08-01T09:49:25.853860Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation aca680de-2dae-422e-a2ca-37a658057361 · outbound

This paper cites The Impact of cold gas accretion above a mass floor on galaxy scaling relations.

When galaxies burst II. Implications of enhanced burstiness for the 21-cm Cosmic Dawn signal The Impact of cold gas accretion above a mass floor on galaxy scaling relations

Reference 74

Resolution: unresolved; no resolver link, observed 2026-08-01T09:49:26.034719Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 3e88c669-12f5-4577-afbe-cdb4513d7c7e · outbound

This paper cites An Analytic Model for the Evolution of the Stellar, Gas, and Metal Content of Galaxies.

When galaxies burst II. Implications of enhanced burstiness for the 21-cm Cosmic Dawn signal An Analytic Model for the Evolution of the Stellar, Gas, and Metal Content of Galaxies

Reference 75

Resolution: unresolved; no resolver link, observed 2026-08-01T09:49:26.213997Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d81fabd1-e689-4a0e-a5fd-96c0a886152c · outbound

This paper cites Halo Models of Large Scale Structure,.

When galaxies burst II. Implications of enhanced burstiness for the 21-cm Cosmic Dawn signal Halo Models of Large Scale Structure,

Reference 76

Resolution: unresolved; no resolver link, observed 2026-08-01T09:49:26.410411Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c15909cb-f01f-44ef-885d-ba72ef79bb3a · outbound

This paper cites Multi-tracer intensity mapping: Cross-correlations, Line noise & Decorrelation.

When galaxies burst II. Implications of enhanced burstiness for the 21-cm Cosmic Dawn signal Multi-tracer intensity mapping: Cross-correlations, Line noise & Decorrelation

Reference 77

Resolution: unresolved; no resolver link, observed 2026-08-01T09:49:26.558344Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c53dbfb1-15f0-441c-b5c6-2af5c72c9ac6 · outbound

This paper cites A halo model approach for the 21-cm power spectrum at cosmic dawn.

When galaxies burst II. Implications of enhanced burstiness for the 21-cm Cosmic Dawn signal A halo model approach for the 21-cm power spectrum at cosmic dawn

Reference 78

Resolution: unresolved; no resolver link, observed 2026-08-01T09:49:26.720228Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 4c7b293f-b79a-4dbf-825a-3de1d73d0753 · outbound

This paper cites Toy Models for Galaxy Formation versus Simulations.

When galaxies burst II. Implications of enhanced burstiness for the 21-cm Cosmic Dawn signal Toy Models for Galaxy Formation versus Simulations

Reference 79

Resolution: unresolved; no resolver link, observed 2026-08-01T09:49:26.893767Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 9538cf3b-4fbd-4d39-91c5-1cd365cc58ae · outbound

This paper cites Detecting the Earliest Galaxies Through Two New Sources of 21cm Fluctuations.

When galaxies burst II. Implications of enhanced burstiness for the 21-cm Cosmic Dawn signal Detecting the Earliest Galaxies Through Two New Sources of 21cm Fluctuations

Reference 80

Resolution: unresolved; no resolver link, observed 2026-08-01T09:49:27.067745Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation cfc57107-d858-41d9-97ad-fecfe969f0fe · outbound

This paper cites Mapping discrete galaxies at cosmic dawn with 21-centimeter observations.

When galaxies burst II. Implications of enhanced burstiness for the 21-cm Cosmic Dawn signal Mapping discrete galaxies at cosmic dawn with 21-centimeter observations

Reference 81

Resolution: unresolved; no resolver link, observed 2026-08-01T09:49:27.236883Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f3953a1d-96cb-424b-8772-71f7fe57644a · outbound

This paper cites Semi-analytical approach to Ly$\alpha$ multiple-scattering in 21-cm signal simulations.

When galaxies burst II. Implications of enhanced burstiness for the 21-cm Cosmic Dawn signal Semi-analytical approach to Ly$\alpha$ multiple-scattering in 21-cm signal simulations

Reference 82

Resolution: unresolved; no resolver link, observed 2026-08-01T09:49:27.330011Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0f7b582d-86b2-473d-a242-f6b7cd37e2b1 · outbound

This paper cites Planck 2018 results. VI. Cosmological parameters.

When galaxies burst II. Implications of enhanced burstiness for the 21-cm Cosmic Dawn signal Planck 2018 results. VI. Cosmological parameters

Reference 83

Resolution: unresolved; no resolver link, observed 2026-08-01T09:49:27.405977Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d4bba268-9e8b-416e-9b9d-2a13b48f823a · outbound

This paper cites New Roads to the Small-Scale Universe: Measurements of the Clustering of Matter with the High-Redshift UV Galaxy Luminosity Function.

When galaxies burst II. Implications of enhanced burstiness for the 21-cm Cosmic Dawn signal New Roads to the Small-Scale Universe: Measurements of the Clustering of Matter with the High-Redshift UV Galaxy Luminosity Function

Reference 84

Resolution: unresolved; no resolver link, observed 2026-08-01T09:49:27.488311Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 59bcbfdd-f9ee-49c9-b804-0ec114e7745a · outbound

This paper cites GALLUMI: A Galaxy Luminosity Function Pipeline for Cosmology and Astrophysics.

When galaxies burst II. Implications of enhanced burstiness for the 21-cm Cosmic Dawn signal GALLUMI: A Galaxy Luminosity Function Pipeline for Cosmology and Astrophysics

Reference 85

Resolution: unresolved; no resolver link, observed 2026-08-01T09:49:27.545619Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation fa7388a4-19f4-4d77-97fe-dc1ffaf1172b · outbound

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

When galaxies burst II. Implications of enhanced burstiness for the 21-cm Cosmic Dawn signal Reionization and the Cosmic Dawn with the Square Kilometre Array

Reference 86

Resolution: unresolved; no resolver link, observed 2026-08-01T09:49:27.618556Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 385021c2-add1-4507-bdbd-578a80313f00 · outbound

This paper cites Square Kilometre Array: a concept design for Phase 1.

When galaxies burst II. Implications of enhanced burstiness for the 21-cm Cosmic Dawn signal Square Kilometre Array: a concept design for Phase 1

Reference 87

Resolution: unresolved; no resolver link, observed 2026-08-01T09:49:27.698932Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f4aa5175-87c5-4bb3-8647-13354d942e3e · outbound

This paper cites HERA bound on x-ray luminosity when accounting for population III stars.

When galaxies burst II. Implications of enhanced burstiness for the 21-cm Cosmic Dawn signal HERA bound on x-ray luminosity when accounting for population III stars

Reference 88

Resolution: unresolved; no resolver link, observed 2026-08-01T09:49:27.757036Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 674fd1ab-4c6d-4115-852e-e2bc3c3444a4 · outbound

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

When galaxies burst II. Implications of enhanced burstiness for the 21-cm Cosmic Dawn signal Constraints on the state of the IGM at $z\sim 8-10$ using redshifted 21-cm observations with LOFAR

Reference 89

Resolution: unresolved; no resolver link, observed 2026-08-01T09:49:27.833856Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 2b971a31-b9d8-4cf0-a770-826ae08310fa · outbound

This paper cites Hydrogen Epoch of Reionization Array (HERA) Phase II Deployment and Commissioning.

When galaxies burst II. Implications of enhanced burstiness for the 21-cm Cosmic Dawn signal Hydrogen Epoch of Reionization Array (HERA) Phase II Deployment and Commissioning

Reference 90

Resolution: unresolved; no resolver link, observed 2026-08-01T09:49:27.914756Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 95d34c13-5750-4c72-a598-0502df0ebbd3 · outbound

This paper cites First Results from HERA Phase II,.

When galaxies burst II. Implications of enhanced burstiness for the 21-cm Cosmic Dawn signal First Results from HERA Phase II,

Reference 91

Resolution: unresolved; no resolver link, observed 2026-08-01T09:49:27.992090Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 6f83ea88-a2bf-4d76-a070-172a7c0e44b0 · outbound

This paper cites Semi-analytic forecasts for Roman -- the beginning of a new era of deep-wide galaxy surveys.

When galaxies burst II. Implications of enhanced burstiness for the 21-cm Cosmic Dawn signal Semi-analytic forecasts for Roman -- the beginning of a new era of deep-wide galaxy surveys

Reference 92

Resolution: unresolved; no resolver link, observed 2026-08-01T09:49:28.098505Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 5f9bee35-7716-4273-a494-8f45e6be762d · outbound

This paper cites 21cmEMUv3: a hybrid diffusion-LSTM emulator of 21cmFAST summary observables.

When galaxies burst II. Implications of enhanced burstiness for the 21-cm Cosmic Dawn signal 21cmEMUv3: a hybrid diffusion-LSTM emulator of 21cmFAST summary observables

Reference 93

Resolution: unresolved; no resolver link, observed 2026-08-01T09:49:28.179145Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation b8267d62-9cce-489d-8b52-b5366a678d96 · outbound

This paper cites Probing bursty star formation by cross-correlating extragalactic background light and galaxy surveys.

When galaxies burst II. Implications of enhanced burstiness for the 21-cm Cosmic Dawn signal Probing bursty star formation by cross-correlating extragalactic background light and galaxy surveys

Reference 94

Resolution: unresolved; no resolver link, observed 2026-08-01T09:49:28.257478Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c1313913-28d5-4860-9099-d912d3369370 · outbound

This paper cites Effective model for line intensity mapping: Auto- and cross-power spectra in the cosmic dawn and reionization,.

When galaxies burst II. Implications of enhanced burstiness for the 21-cm Cosmic Dawn signal Effective model for line intensity mapping: Auto- and cross-power spectra in the cosmic dawn and reionization,

Reference 95

Resolution: unresolved; no resolver link, observed 2026-08-01T09:49:28.339311Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 3f279213-5c34-404a-9c47-27930692e9fe · outbound

This paper cites Sklansky, et al., in preparation.

When galaxies burst II. Implications of enhanced burstiness for the 21-cm Cosmic Dawn signal Sklansky, et al., in preparation

Reference 96

Resolution: unresolved; no resolver link, observed 2026-08-01T09:49:28.424147Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 8aa2102d-08ad-4eb0-8af1-a563582415f3 · outbound

This paper cites A Lognormal model for the cos- mological mass distribution,.

When galaxies burst II. Implications of enhanced burstiness for the 21-cm Cosmic Dawn signal A Lognormal model for the cos- mological mass distribution,

Reference 97

Resolution: unresolved; no resolver link, observed 2026-08-01T09:49:28.504825Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e557c036-d0c9-4827-87c2-a3fb0dcf16da · outbound

This paper cites Improving lognormal models for cosmological fields.

When galaxies burst II. Implications of enhanced burstiness for the 21-cm Cosmic Dawn signal Improving lognormal models for cosmological fields

Reference 98

Resolution: unresolved; no resolver link, observed 2026-08-01T09:49:28.586778Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 731e0d40-b6ad-4e8b-8c9b-d1af74a5f3aa · outbound

This paper cites an unresolved cited work.

When galaxies burst II. Implications of enhanced burstiness for the 21-cm Cosmic Dawn signal Unresolved cited work

Reference 99

Resolution: unresolved; no resolver link, observed 2026-08-01T09:49:28.665811Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Coverage vector

Reference resolution

Outbound references

Pith citing papers