SCRIPT in the Cosmic Dawn: Distinguishing Redshift-Evolving Galaxy Populations with 21-cm Fluctuations | Paper Citation Record

Observation 03742c7d-d517-44b3-9ec9-5f869c079d71 · outbound

This paper cites Two Remarkably Luminous Galaxy Candidates at $z\approx10-12$ Revealed by JWST.

SCRIPT in the Cosmic Dawn: Distinguishing Redshift-Evolving Galaxy Populations with 21-cm Fluctuations Two Remarkably Luminous Galaxy Candidates at $z\approx10-12$ Revealed by JWST

Reference 1

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Observation 3a5d7942-4ca6-445c-9485-6cd2197ef6a7 · outbound

This paper cites Early results from GLASS-JWST. III: Galaxy candidates at z$\sim$9-15.

SCRIPT in the Cosmic Dawn: Distinguishing Redshift-Evolving Galaxy Populations with 21-cm Fluctuations Early results from GLASS-JWST. III: Galaxy candidates at z$\sim$9-15

Reference 2

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Observation 34e05893-98f8-4e90-a9ea-2a0c04a09b6a · outbound

This paper cites A Long Time Ago in a Galaxy Far, Far Away: A Candidate z ~ 12 Galaxy in Early JWST CEERS Imaging.

SCRIPT in the Cosmic Dawn: Distinguishing Redshift-Evolving Galaxy Populations with 21-cm Fluctuations A Long Time Ago in a Galaxy Far, Far Away: A Candidate z ~ 12 Galaxy in Early JWST CEERS Imaging

Reference 3

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Observation 5b8f6f8e-ff54-4ac0-abbc-40c281349b27 · outbound

This paper cites A population of red candidate massive galaxies ~600 Myr after the Big Bang.

SCRIPT in the Cosmic Dawn: Distinguishing Redshift-Evolving Galaxy Populations with 21-cm Fluctuations A population of red candidate massive galaxies ~600 Myr after the Big Bang

Reference 4

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Observation 2305118d-c3fd-408b-b8e9-bf71f2c1ffa1 · outbound

This paper cites Revealing Galaxy Candidates out to $z \sim 16$ with JWST Observations of the Lensing Cluster SMACS0723.

SCRIPT in the Cosmic Dawn: Distinguishing Redshift-Evolving Galaxy Populations with 21-cm Fluctuations Revealing Galaxy Candidates out to $z \sim 16$ with JWST Observations of the Lensing Cluster SMACS0723

Reference 5

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Observation 8d6b049a-34c9-417c-9f6a-8897872c90b5 · outbound

This paper cites Discovery and properties of ultra-high redshift galaxies ($9<z<12$) in the JWST ERO SMACS 0723 Field.

SCRIPT in the Cosmic Dawn: Distinguishing Redshift-Evolving Galaxy Populations with 21-cm Fluctuations Discovery and properties of ultra-high redshift galaxies ($9<z<12$) in the JWST ERO SMACS 0723 Field

Reference 6

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Observation 7d984f13-445d-41b4-bbbc-c5792594aebc · outbound

This paper cites High-Redshift Galaxy Candidates at $z = 9-10$ as Revealed by JWST Observations of WHL0137-08.

SCRIPT in the Cosmic Dawn: Distinguishing Redshift-Evolving Galaxy Populations with 21-cm Fluctuations High-Redshift Galaxy Candidates at $z = 9-10$ as Revealed by JWST Observations of WHL0137-08

Reference 7

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Observation e35f837e-fa9e-4472-b8b3-b13eb2b2e8e3 · outbound

This paper cites On the ages of bright galaxies $\sim 500$ Myr after the Big Bang: insights into star formation activity at $z \gtrsim 15$ with JWST.

SCRIPT in the Cosmic Dawn: Distinguishing Redshift-Evolving Galaxy Populations with 21-cm Fluctuations On the ages of bright galaxies $\sim 500$ Myr after the Big Bang: insights into star formation activity at $z \gtrsim 15$ with JWST

Reference 8

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Observation 4b683a22-db2f-4169-9648-84da4e438117 · outbound

This paper cites Robertson, B.D.

SCRIPT in the Cosmic Dawn: Distinguishing Redshift-Evolving Galaxy Populations with 21-cm Fluctuations Robertson, B.D

Reference 9

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Observation 2fc5cb38-cfb8-48e6-b357-0135e91cab48 · outbound

This paper cites Early Results from GLASS-JWST. XIX: A High Density of Bright Galaxies at $z\approx10$ in the Abell 2744 Region.

SCRIPT in the Cosmic Dawn: Distinguishing Redshift-Evolving Galaxy Populations with 21-cm Fluctuations Early Results from GLASS-JWST. XIX: A High Density of Bright Galaxies at $z\approx10$ in the Abell 2744 Region

Reference 10

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Observation c7800805-f123-480d-8afb-e8bd83b2b10a · outbound

This paper cites CEERS Key Paper I: An Early Look into the First 500 Myr of Galaxy Formation with JWST.

SCRIPT in the Cosmic Dawn: Distinguishing Redshift-Evolving Galaxy Populations with 21-cm Fluctuations CEERS Key Paper I: An Early Look into the First 500 Myr of Galaxy Formation with JWST

Reference 11

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Observation 7a056626-02ac-4618-bdba-8184093794d0 · outbound

This paper cites Life beyond 30: probing the -20<M_UV<-17 luminosity function at 8<z<13 with the NIRCam parallel field of the MIRI Deep Survey.

SCRIPT in the Cosmic Dawn: Distinguishing Redshift-Evolving Galaxy Populations with 21-cm Fluctuations Life beyond 30: probing the -20<M_UV<-17 luminosity function at 8<z<13 with the NIRCam parallel field of the MIRI Deep Survey

Reference 12

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Observation 1657f687-ab8e-4146-806c-88b01969a455 · outbound

This paper cites The evolution of the galaxy UV luminosity function at redshifts z ~ 8-15 from deep JWST and ground-based near-infrared imaging.

SCRIPT in the Cosmic Dawn: Distinguishing Redshift-Evolving Galaxy Populations with 21-cm Fluctuations The evolution of the galaxy UV luminosity function at redshifts z ~ 8-15 from deep JWST and ground-based near-infrared imaging

Reference 13

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Observation 21456d01-03f0-4651-abd8-c6f9afe2b8f1 · 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.

SCRIPT in the Cosmic Dawn: Distinguishing Redshift-Evolving Galaxy Populations with 21-cm Fluctuations 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 14

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Observation 5bb7fac6-0062-483c-9b5d-17551a95991d · outbound

This paper cites UV Luminosity Density Results at z>8 from the First JWST/NIRCam Fields: Limitations of Early Data Sets and the Need for Spectroscopy.

SCRIPT in the Cosmic Dawn: Distinguishing Redshift-Evolving Galaxy Populations with 21-cm Fluctuations UV Luminosity Density Results at z>8 from the First JWST/NIRCam Fields: Limitations of Early Data Sets and the Need for Spectroscopy

Reference 15

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Observation 68f56f09-5313-4d12-b799-9134c58551a9 · outbound

This paper cites The galaxy UV luminosity function at $\mathbf{z \simeq 11}$ from a suite of public JWST ERS, ERO and Cycle-1 programs.

SCRIPT in the Cosmic Dawn: Distinguishing Redshift-Evolving Galaxy Populations with 21-cm Fluctuations The galaxy UV luminosity function at $\mathbf{z \simeq 11}$ from a suite of public JWST ERS, ERO and Cycle-1 programs

Reference 16

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Observation 403a7580-7d43-4807-8498-d4aa309491bc · outbound

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

SCRIPT in the Cosmic Dawn: Distinguishing Redshift-Evolving Galaxy Populations with 21-cm Fluctuations EPOCHS Paper II: The Ultraviolet Luminosity Function from $7.5<z<13.5$ using 180 square arcminutes of deep, blank-fields from the PEARLS Survey and Public JWST data

Reference 17

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Observation 420fbcb1-f8f3-4ff3-abec-006d05844109 · 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.

SCRIPT in the Cosmic Dawn: Distinguishing Redshift-Evolving Galaxy Populations with 21-cm Fluctuations 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 18

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Observation f59f8f01-ad9a-4bbc-b614-b52fa3e8eadc · outbound

This paper cites Whitler, D.P.

SCRIPT in the Cosmic Dawn: Distinguishing Redshift-Evolving Galaxy Populations with 21-cm Fluctuations Whitler, D.P

Reference 19

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Observation ad53ff43-fc2f-42dc-9f1a-6acd01381af2 · outbound

This paper cites Pérez-González, G.

SCRIPT in the Cosmic Dawn: Distinguishing Redshift-Evolving Galaxy Populations with 21-cm Fluctuations Pérez-González, G

Reference 20

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Observation 26aef602-9dbd-40cb-8f11-897a253f05b6 · outbound

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

SCRIPT in the Cosmic Dawn: Distinguishing Redshift-Evolving Galaxy Populations with 21-cm Fluctuations Exploring Cosmic Dawn with PANORAMIC I: The Bright End of the UVLF at $z\sim9 -17$

Reference 21

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Observation 3a737b98-2927-4a14-a323-bfa5dcaa32a4 · outbound

This paper cites Efficient Formation of Massive Galaxies at Cosmic Dawn by Feedback-Free Starbursts.

SCRIPT in the Cosmic Dawn: Distinguishing Redshift-Evolving Galaxy Populations with 21-cm Fluctuations Efficient Formation of Massive Galaxies at Cosmic Dawn by Feedback-Free Starbursts

Reference 22

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Observation 346702d3-f049-4a80-be15-7425f4a041ce · outbound

This paper cites Feedback-Free Starbursts at Cosmic Dawn: Observable Predictions for JWST.

SCRIPT in the Cosmic Dawn: Distinguishing Redshift-Evolving Galaxy Populations with 21-cm Fluctuations Feedback-Free Starbursts at Cosmic Dawn: Observable Predictions for JWST

Reference 23

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Observation 6042203a-fa60-4179-9257-9c9a218f3c0d · outbound

This paper cites Implications of $z>{\sim}12$ JWST galaxies for galaxy formation at high redshift.

SCRIPT in the Cosmic Dawn: Distinguishing Redshift-Evolving Galaxy Populations with 21-cm Fluctuations Implications of $z>{\sim}12$ JWST galaxies for galaxy formation at high redshift

Reference 24

Resolution: verified exact; local_arxiv, observed 2026-08-15T14:54:43.156466Z

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Observation 891982c5-fda1-44d0-826d-74cb856e88ba · outbound

This paper cites Modelling the star-formation activity and ionizing properties of high-redshift galaxies.

SCRIPT in the Cosmic Dawn: Distinguishing Redshift-Evolving Galaxy Populations with 21-cm Fluctuations Modelling the star-formation activity and ionizing properties of high-redshift galaxies

Reference 25

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Observation 16666b8e-2f88-4156-8ddb-ef1cc8c8f823 · outbound

This paper cites Chakraborty and T.R.

SCRIPT in the Cosmic Dawn: Distinguishing Redshift-Evolving Galaxy Populations with 21-cm Fluctuations Chakraborty and T.R

Reference 26

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Observation ba893c66-401f-4e6e-a04a-4437c64a8ee8 · outbound

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

SCRIPT in the Cosmic Dawn: Distinguishing Redshift-Evolving Galaxy Populations with 21-cm Fluctuations Balancing the efficiency and stochasticity of star formation with dust extinction in z > 10 galaxies observed by JWST

Reference 27

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Observation 22280c8c-8efa-48d3-9bc3-d1ef4ecd9100 · outbound

This paper cites The brightest galaxies at Cosmic Dawn.

SCRIPT in the Cosmic Dawn: Distinguishing Redshift-Evolving Galaxy Populations with 21-cm Fluctuations The brightest galaxies at Cosmic Dawn

Reference 28

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Observation ecd330b1-3299-4f54-957b-1eb8f9eae0f4 · outbound

This paper cites The impact of UV variability on the abundance of bright galaxies at $z \geq 9$.

SCRIPT in the Cosmic Dawn: Distinguishing Redshift-Evolving Galaxy Populations with 21-cm Fluctuations The impact of UV variability on the abundance of bright galaxies at $z \geq 9$

Reference 29

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Observation 9d440f50-c2e3-434d-abbe-c75fb599a2c1 · outbound

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

SCRIPT in the Cosmic Dawn: Distinguishing Redshift-Evolving Galaxy Populations with 21-cm Fluctuations Bursty Star Formation Naturally Explains the Abundance of Bright Galaxies at Cosmic Dawn

Reference 30

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Observation 971ca333-e624-47db-b53e-bb5c72060feb · outbound

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

SCRIPT in the Cosmic Dawn: Distinguishing Redshift-Evolving Galaxy Populations with 21-cm Fluctuations Stochastic star formation in early galaxies: JWST implications

Reference 31

Resolution: verified exact; local_arxiv, observed 2026-08-15T14:54:43.025727Z

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Observation 89450011-88c0-48c7-82d6-cce28850a6f4 · outbound

This paper cites The impact of mass-dependent stochasticity at cosmic dawn.

SCRIPT in the Cosmic Dawn: Distinguishing Redshift-Evolving Galaxy Populations with 21-cm Fluctuations The impact of mass-dependent stochasticity at cosmic dawn

Reference 32

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Observation a8a7fe0b-6a22-4ecf-bf02-b62eed41c61e · outbound

This paper cites Stochastic star formation and the abundance of $z>10$ UV-bright galaxies.

SCRIPT in the Cosmic Dawn: Distinguishing Redshift-Evolving Galaxy Populations with 21-cm Fluctuations Stochastic star formation and the abundance of $z>10$ UV-bright galaxies

Reference 33

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Observation 881dad37-6502-4d0c-858a-7d14b587aa25 · outbound

This paper cites A Lower Bound of Star Formation Activity in Ultra-high Redshift Galaxies Detected with JWST: Implications for Stellar Populations and Radiation Sources.

SCRIPT in the Cosmic Dawn: Distinguishing Redshift-Evolving Galaxy Populations with 21-cm Fluctuations A Lower Bound of Star Formation Activity in Ultra-high Redshift Galaxies Detected with JWST: Implications for Stellar Populations and Radiation Sources

Reference 34

Resolution: verified exact; local_arxiv, observed 2026-08-15T14:54:42.987112Z

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Observation f7e022f7-3064-4f57-93a4-cb72447318bf · outbound

This paper cites Exploring the nature of UV-bright $z \gtrsim 10$ galaxies detected by JWST: star formation, black hole accretion, or a non-universal IMF?.

SCRIPT in the Cosmic Dawn: Distinguishing Redshift-Evolving Galaxy Populations with 21-cm Fluctuations Exploring the nature of UV-bright $z \gtrsim 10$ galaxies detected by JWST: star formation, black hole accretion, or a non-universal IMF?

Reference 35

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Observation 73c224a9-2569-4a03-9ee4-f19fd9e1c25c · outbound

This paper cites Semi-analytic modelling of Pop. III star formation and metallicity evolution -- I. Impact on the UV luminosity functions at z = 9-16.

SCRIPT in the Cosmic Dawn: Distinguishing Redshift-Evolving Galaxy Populations with 21-cm Fluctuations Semi-analytic modelling of Pop. III star formation and metallicity evolution -- I. Impact on the UV luminosity functions at z = 9-16

Reference 36

Resolution: verified exact; local_arxiv, observed 2026-08-15T14:54:42.962528Z

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Observation 81ce6a94-d6ba-47da-9e47-bff7a0ce85ba · outbound

This paper cites Are the ultra-high-redshift galaxies at z > 10 surprising in the context of standard galaxy formation models?.

SCRIPT in the Cosmic Dawn: Distinguishing Redshift-Evolving Galaxy Populations with 21-cm Fluctuations Are the ultra-high-redshift galaxies at z > 10 surprising in the context of standard galaxy formation models?

Reference 37

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Observation 8c1615fb-5304-476f-b076-7386caab667c · outbound

This paper cites Astraeus X: Indications of a top-heavy initial mass function in highly star-forming galaxies from JWST observations at z>10.

SCRIPT in the Cosmic Dawn: Distinguishing Redshift-Evolving Galaxy Populations with 21-cm Fluctuations Astraeus X: Indications of a top-heavy initial mass function in highly star-forming galaxies from JWST observations at z>10

Reference 38

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Observation 3e88b09c-33bb-47f7-96a2-b57ccbafd1ad · outbound

This paper cites A comparison of pre-existing $\Lambda$CDM predictions with the abundance of {\it JWST} galaxies at high redshift.

SCRIPT in the Cosmic Dawn: Distinguishing Redshift-Evolving Galaxy Populations with 21-cm Fluctuations A comparison of pre-existing $\Lambda$CDM predictions with the abundance of {\it JWST} galaxies at high redshift

Reference 39

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Observation f3d3413a-0b30-4f9b-b488-1913b76e6c0b · outbound

This paper cites On the stunning abundance of super-early, massive galaxies revealed by JWST.

SCRIPT in the Cosmic Dawn: Distinguishing Redshift-Evolving Galaxy Populations with 21-cm Fluctuations On the stunning abundance of super-early, massive galaxies revealed by JWST

Reference 40

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Observation 5b740fa6-924e-4998-9601-f13c1d596cb0 · outbound

This paper cites Blue Monsters. Why are JWST super-early, massive galaxies so blue?.

SCRIPT in the Cosmic Dawn: Distinguishing Redshift-Evolving Galaxy Populations with 21-cm Fluctuations Blue Monsters. Why are JWST super-early, massive galaxies so blue?

Reference 41

Resolution: verified exact; local_arxiv, observed 2026-08-15T14:54:42.909553Z

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Observation 060fab36-534f-4ebd-a42d-be4e929b0e1b · outbound

This paper cites Super-early JWST galaxies, outflows and Lyman alpha visibility in the EoR.

SCRIPT in the Cosmic Dawn: Distinguishing Redshift-Evolving Galaxy Populations with 21-cm Fluctuations Super-early JWST galaxies, outflows and Lyman alpha visibility in the EoR

Reference 42

Resolution: unresolved; no resolver link, observed 2026-08-15T14:54:41.590582Z

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Observation a33a0167-ce0e-4cdc-ae87-4e26780b78d3 · outbound

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

SCRIPT in the Cosmic Dawn: Distinguishing Redshift-Evolving Galaxy Populations with 21-cm Fluctuations Blue Monsters at $z>10$. Where has all their dust gone?

Reference 43

Resolution: unresolved; no resolver link, observed 2026-08-15T14:54:41.594299Z

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Observation 7730a5ff-559e-489d-8db0-02d13d7f856e · outbound

This paper cites Are the Newly-Discovered $z \sim 13$ Drop-out Sources Starburst Galaxies or Quasars?.

SCRIPT in the Cosmic Dawn: Distinguishing Redshift-Evolving Galaxy Populations with 21-cm Fluctuations Are the Newly-Discovered $z \sim 13$ Drop-out Sources Starburst Galaxies or Quasars?

Reference 44

Resolution: verified exact; local_arxiv, observed 2026-08-15T14:54:42.875304Z

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Observation 888ead0a-c554-4942-b71c-f0edbbe17c5b · outbound

This paper cites A hidden population of active galactic nuclei can explain the overabundance of luminous $z>10$ objects observed by JWST.

SCRIPT in the Cosmic Dawn: Distinguishing Redshift-Evolving Galaxy Populations with 21-cm Fluctuations A hidden population of active galactic nuclei can explain the overabundance of luminous $z>10$ objects observed by JWST

Reference 45

Resolution: verified exact; local_arxiv, observed 2026-08-15T14:54:42.859387Z

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Observation 69ab9427-ff0c-4c27-8724-6fbda74ad708 · outbound

This paper cites UNCOVER: A NIRSpec Census of Lensed Galaxies at z=8.50-13.08 Probing a High AGN Fraction and Ionized Bubbles in the Shadow.

SCRIPT in the Cosmic Dawn: Distinguishing Redshift-Evolving Galaxy Populations with 21-cm Fluctuations UNCOVER: A NIRSpec Census of Lensed Galaxies at z=8.50-13.08 Probing a High AGN Fraction and Ionized Bubbles in the Shadow

Reference 46

Resolution: unresolved; no resolver link, observed 2026-08-15T14:54:41.604921Z

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Observation 289b663e-16f8-4a5c-b56a-5c3636b55a06 · outbound

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

SCRIPT in the Cosmic Dawn: Distinguishing Redshift-Evolving Galaxy Populations with 21-cm Fluctuations An absorption profile centred at 78 megahertz in the sky-averaged spectrum

Reference 47

Resolution: unresolved; no resolver link, observed 2026-08-15T14:54:41.609236Z

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Observation 180253f0-df70-4404-a05b-d56ebe49f002 · outbound

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

SCRIPT in the Cosmic Dawn: Distinguishing Redshift-Evolving Galaxy Populations with 21-cm Fluctuations On the detection of a cosmic dawn signal in the radio background

Reference 48

Resolution: unresolved; no resolver link, observed 2026-08-15T14:54:41.613400Z

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Observation b22c16e1-b429-49bc-b6ab-ec58f352019c · outbound

This paper cites The REACH radiometer for detecting the 21-cm hydrogen signal from redshift 7.5 to 28.

SCRIPT in the Cosmic Dawn: Distinguishing Redshift-Evolving Galaxy Populations with 21-cm Fluctuations The REACH radiometer for detecting the 21-cm hydrogen signal from redshift 7.5 to 28

Reference 49

Resolution: unresolved; no resolver link, observed 2026-08-15T14:54:41.617358Z

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Observation 0ffae8d7-05ba-45fc-9750-ee2767df7724 · outbound

This paper cites Mapper of the IGM spin temperature: instrument overview.

SCRIPT in the Cosmic Dawn: Distinguishing Redshift-Evolving Galaxy Populations with 21-cm Fluctuations Mapper of the IGM spin temperature: instrument overview

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Resolution: unresolved; no resolver link, observed 2026-08-15T14:54:41.620861Z

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Observation d3635dd4-8771-43e1-a1c3-0eb2cdab69e8 · outbound

This paper cites an unresolved cited work.

SCRIPT in the Cosmic Dawn: Distinguishing Redshift-Evolving Galaxy Populations with 21-cm Fluctuations Unresolved cited work

Reference 51

Resolution: unresolved; no resolver link, observed 2026-08-15T14:54:41.624596Z

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Observation b37a19bf-e527-4c54-a9f4-2f0784034a7b · outbound

This paper cites Probing Radio Intensity at high-Z from Marion: 2017 Instrument.

SCRIPT in the Cosmic Dawn: Distinguishing Redshift-Evolving Galaxy Populations with 21-cm Fluctuations Probing Radio Intensity at high-Z from Marion: 2017 Instrument

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Resolution: unresolved; no resolver link, observed 2026-08-15T14:54:41.628030Z

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Observation 17e928d8-72c3-4900-825d-323e1535d61a · outbound

This paper cites A simulation calibrated limit on the HI power spectrum from the GMRT Epoch of Reionization experiment.

SCRIPT in the Cosmic Dawn: Distinguishing Redshift-Evolving Galaxy Populations with 21-cm Fluctuations A simulation calibrated limit on the HI power spectrum from the GMRT Epoch of Reionization experiment

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Resolution: unresolved; no resolver link, observed 2026-08-15T14:54:41.631793Z

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Observation 97370fe2-2c29-4143-aa09-6209e660b523 · outbound

This paper cites The Murchison Widefield Array: the Square Kilometre Array Precursor at low radio frequencies.

SCRIPT in the Cosmic Dawn: Distinguishing Redshift-Evolving Galaxy Populations with 21-cm Fluctuations The Murchison Widefield Array: the Square Kilometre Array Precursor at low radio frequencies

Reference 54

Resolution: unresolved; no resolver link, observed 2026-08-15T14:54:41.635237Z

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Observation 1894ac2e-999e-4cef-bd6f-57137737f866 · outbound

This paper cites LOFAR: The LOw-Frequency ARray.

SCRIPT in the Cosmic Dawn: Distinguishing Redshift-Evolving Galaxy Populations with 21-cm Fluctuations LOFAR: The LOw-Frequency ARray

Reference 55

Resolution: unresolved; no resolver link, observed 2026-08-15T14:54:41.638898Z

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Observation 7782c4b1-b19c-4ed3-8594-4d6b2d3bee49 · outbound

This paper cites DeBoer, A.R.

SCRIPT in the Cosmic Dawn: Distinguishing Redshift-Evolving Galaxy Populations with 21-cm Fluctuations DeBoer, A.R

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Resolution: unresolved; no resolver link, observed 2026-08-15T14:54:41.642597Z

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Observation b6b056b3-4087-44a8-884e-658bc3ed1c6c · outbound

This paper cites Overview of 21cm Experiments at high redshift with SKAO.

SCRIPT in the Cosmic Dawn: Distinguishing Redshift-Evolving Galaxy Populations with 21-cm Fluctuations Overview of 21cm Experiments at high redshift with SKAO

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Resolution: verified exact; local_arxiv, observed 2026-08-15T14:54:42.698704Z

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No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation c1c6d3cd-1df7-455d-8884-56be6f4c12c1 · outbound

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

SCRIPT in the Cosmic Dawn: Distinguishing Redshift-Evolving Galaxy Populations with 21-cm Fluctuations Cosmology at Low Frequencies: The 21 cm Transition and the High-Redshift Universe

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Resolution: unresolved; no resolver link, observed 2026-08-15T14:54:41.649659Z

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Observation f50081fc-6cb8-45ba-a15f-9bb99e60cf3c · outbound

This paper cites 21-cm cosmology.

SCRIPT in the Cosmic Dawn: Distinguishing Redshift-Evolving Galaxy Populations with 21-cm Fluctuations 21-cm cosmology

Reference 59

Resolution: unresolved; no resolver link, observed 2026-08-15T14:54:41.653175Z

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Observation ad49ea20-11bd-492d-b382-0628187a6db7 · outbound

This paper cites Inferring the astrophysics of reionization and cosmic dawn from galaxy luminosity functions and the 21-cm signal.

SCRIPT in the Cosmic Dawn: Distinguishing Redshift-Evolving Galaxy Populations with 21-cm Fluctuations Inferring the astrophysics of reionization and cosmic dawn from galaxy luminosity functions and the 21-cm signal

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Resolution: unresolved; no resolver link, observed 2026-08-15T14:54:41.656625Z

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Observation d3431f11-98be-49e3-885f-47447d1d5dec · outbound

This paper cites A tale of two sites -- I: Inferring the properties of minihalo-hosted galaxies from current observations.

SCRIPT in the Cosmic Dawn: Distinguishing Redshift-Evolving Galaxy Populations with 21-cm Fluctuations A tale of two sites -- I: Inferring the properties of minihalo-hosted galaxies from current observations

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Resolution: unresolved; no resolver link, observed 2026-08-15T14:54:41.660234Z

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Observation 68aa5f7f-7e4e-4808-8848-c20e4ff9ad2d · outbound

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

SCRIPT in the Cosmic Dawn: Distinguishing Redshift-Evolving Galaxy Populations with 21-cm Fluctuations The Impact of the First Galaxies on Cosmic Dawn and Reionization

Reference 62

Resolution: unresolved; no resolver link, observed 2026-08-15T14:54:41.663651Z

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Observation 77019b1e-b28d-4f3c-a7c1-cd0fb6198fd8 · outbound

This paper cites The importance of stochasticity in determining galaxy emissivities and UV LFs during cosmic dawn and reionization.

SCRIPT in the Cosmic Dawn: Distinguishing Redshift-Evolving Galaxy Populations with 21-cm Fluctuations The importance of stochasticity in determining galaxy emissivities and UV LFs during cosmic dawn and reionization

Reference 63

Resolution: unresolved; no resolver link, observed 2026-08-15T14:54:41.667543Z

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Observation 12310b28-7d5e-471b-b99e-38f50765de13 · outbound

This paper cites Joint analysis constraints on the physics of the first galaxies with low frequency radio astronomy data.

SCRIPT in the Cosmic Dawn: Distinguishing Redshift-Evolving Galaxy Populations with 21-cm Fluctuations Joint analysis constraints on the physics of the first galaxies with low frequency radio astronomy data

Reference 64

Resolution: unresolved; no resolver link, observed 2026-08-15T14:54:41.670982Z

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Observation 2ca2b395-96d6-4942-bc1f-0449db2ed867 · outbound

This paper cites Constraining the properties of Population III galaxies with multi-wavelength observations.

SCRIPT in the Cosmic Dawn: Distinguishing Redshift-Evolving Galaxy Populations with 21-cm Fluctuations Constraining the properties of Population III galaxies with multi-wavelength observations

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Resolution: unresolved; no resolver link, observed 2026-08-15T14:54:41.675281Z

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Observation 6eb72417-5722-4388-8952-7f6b5b530623 · outbound

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

SCRIPT in the Cosmic Dawn: Distinguishing Redshift-Evolving Galaxy Populations with 21-cm Fluctuations Exploiting synergies between JWST and cosmic 21-cm observations to uncover star formation in the early Universe

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Resolution: unresolved; no resolver link, observed 2026-08-15T14:54:41.678893Z

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Observation e03e643f-281a-4acc-ace5-7f9474329807 · outbound

This paper cites Dhandha, A.

SCRIPT in the Cosmic Dawn: Distinguishing Redshift-Evolving Galaxy Populations with 21-cm Fluctuations Dhandha, A

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Resolution: unresolved; no resolver link, observed 2026-08-15T14:54:41.682583Z

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Observation fb08c2df-3f77-49c8-8e6b-0f63781aab7a · outbound

This paper cites Davies, A.

SCRIPT in the Cosmic Dawn: Distinguishing Redshift-Evolving Galaxy Populations with 21-cm Fluctuations Davies, A

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Resolution: unresolved; no resolver link, observed 2026-08-15T14:54:41.686207Z

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Observation e193e2c9-bfab-4569-83b7-8e93146f26ee · outbound

This paper cites Lyman-alpha radiative transfer during the Epoch of Reionization: contribution to 21-cm signal fluctuations.

SCRIPT in the Cosmic Dawn: Distinguishing Redshift-Evolving Galaxy Populations with 21-cm Fluctuations Lyman-alpha radiative transfer during the Epoch of Reionization: contribution to 21-cm signal fluctuations

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Resolution: unresolved; no resolver link, observed 2026-08-15T14:54:41.689765Z

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Observation 1372b876-d350-41ce-9393-44d8af3bcab0 · outbound

This paper cites The simulated 21 cm signal during the epoch of reionization : full modeling of the Ly-alpha pumping.

SCRIPT in the Cosmic Dawn: Distinguishing Redshift-Evolving Galaxy Populations with 21-cm Fluctuations The simulated 21 cm signal during the epoch of reionization : full modeling of the Ly-alpha pumping

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Resolution: unresolved; no resolver link, observed 2026-08-15T14:54:41.693413Z

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Observation 75a0c02a-cda7-4bb7-9f45-50175052a902 · outbound

This paper cites 21SSD: a public database of simulated 21-cm signals from the epoch of reionization.

SCRIPT in the Cosmic Dawn: Distinguishing Redshift-Evolving Galaxy Populations with 21-cm Fluctuations 21SSD: a public database of simulated 21-cm signals from the epoch of reionization

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Resolution: verified exact; local_arxiv, observed 2026-08-15T14:54:42.451192Z

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No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation dcc7f94a-b6e4-444f-be22-9ae5b43db6b1 · outbound

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

SCRIPT in the Cosmic Dawn: Distinguishing Redshift-Evolving Galaxy Populations with 21-cm Fluctuations 21cmFAST: A Fast, Semi-Numerical Simulation of the High-Redshift 21-cm Signal

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Resolution: unresolved; no resolver link, observed 2026-08-15T14:54:41.700972Z

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Observation 9aa287dc-08cd-4552-be19-549e61c0c3b7 · outbound

This paper cites Fast Large Volume Simulations of the 21 cm Signal from the Reionization and pre-Reionization Epochs.

SCRIPT in the Cosmic Dawn: Distinguishing Redshift-Evolving Galaxy Populations with 21-cm Fluctuations Fast Large Volume Simulations of the 21 cm Signal from the Reionization and pre-Reionization Epochs

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Resolution: verified exact; local_arxiv, observed 2026-08-15T14:54:42.425284Z

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No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation 029918a4-83f9-40ee-bf34-a11e03aff1a6 · outbound

This paper cites Impact of the Relative Motion between the Dark Matter and Baryons on the First Stars.

SCRIPT in the Cosmic Dawn: Distinguishing Redshift-Evolving Galaxy Populations with 21-cm Fluctuations Impact of the Relative Motion between the Dark Matter and Baryons on the First Stars

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Resolution: unresolved; no resolver link, observed 2026-08-15T14:54:41.708450Z

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Observation 20c594b2-79c7-4177-9338-a09f70a4349e · outbound

This paper cites The signature of the first stars in atomic hydrogen at redshift 20.

SCRIPT in the Cosmic Dawn: Distinguishing Redshift-Evolving Galaxy Populations with 21-cm Fluctuations The signature of the first stars in atomic hydrogen at redshift 20

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Resolution: unresolved; no resolver link, observed 2026-08-15T14:54:41.711962Z

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Observation e8607892-87e6-442d-a367-179be6348c44 · outbound

This paper cites Fast Large-Scale Reionization Simulations.

SCRIPT in the Cosmic Dawn: Distinguishing Redshift-Evolving Galaxy Populations with 21-cm Fluctuations Fast Large-Scale Reionization Simulations

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Resolution: verified exact; local_arxiv, observed 2026-08-15T14:54:42.390444Z

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No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation 7f619aa9-ed85-4b40-bc74-a6fe739d20b6 · outbound

This paper cites Prediction of the 21-cm signal from reionization: comparison between 3D and 1D radiative transfer schemes.

SCRIPT in the Cosmic Dawn: Distinguishing Redshift-Evolving Galaxy Populations with 21-cm Fluctuations Prediction of the 21-cm signal from reionization: comparison between 3D and 1D radiative transfer schemes

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Resolution: unresolved; no resolver link, observed 2026-08-15T14:54:41.719039Z

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Observation 238d14ec-2e30-4fc3-9b79-f1226949df43 · outbound

This paper cites BEoRN: A fast and flexible framework to simulate the epoch of reionisation and cosmic dawn.

SCRIPT in the Cosmic Dawn: Distinguishing Redshift-Evolving Galaxy Populations with 21-cm Fluctuations BEoRN: A fast and flexible framework to simulate the epoch of reionisation and cosmic dawn

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Resolution: unresolved; no resolver link, observed 2026-08-15T14:54:41.722745Z

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Observation 52f8f10f-2aab-42cb-9f9f-78234dd18aa8 · outbound

This paper cites Decoding the X-ray Properties of Pre-Reionization Era Sources.

SCRIPT in the Cosmic Dawn: Distinguishing Redshift-Evolving Galaxy Populations with 21-cm Fluctuations Decoding the X-ray Properties of Pre-Reionization Era Sources

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Resolution: unresolved; no resolver link, observed 2026-08-15T14:54:41.726567Z

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Observation 5d4f2ae4-c7ef-49e1-aa31-0c06cc3ca963 · outbound

This paper cites Mittal, G.

SCRIPT in the Cosmic Dawn: Distinguishing Redshift-Evolving Galaxy Populations with 21-cm Fluctuations Mittal, G

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Resolution: verified exact; raw_fallback, observed 2026-08-15T14:54:42.343826Z

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No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation 2f580a20-f330-4f58-ab7c-e5498ae2f183 · outbound

This paper cites Raste and S.

SCRIPT in the Cosmic Dawn: Distinguishing Redshift-Evolving Galaxy Populations with 21-cm Fluctuations Raste and S

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Resolution: unresolved; no resolver link, observed 2026-08-15T14:54:41.733765Z

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Observation cb0744d3-6dcb-4b90-ab2a-a4be257897bf · outbound

This paper cites Raste and S.

SCRIPT in the Cosmic Dawn: Distinguishing Redshift-Evolving Galaxy Populations with 21-cm Fluctuations Raste and S

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Resolution: unresolved; no resolver link, observed 2026-08-15T14:54:41.737182Z

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Observation 729d4ac7-14c0-4b2d-8bd1-7c321a5a3bda · outbound

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

SCRIPT in the Cosmic Dawn: Distinguishing Redshift-Evolving Galaxy Populations with 21-cm Fluctuations An Effective Model for the Cosmic-Dawn 21-cm Signal

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Resolution: unresolved; no resolver link, observed 2026-08-15T14:54:41.740447Z

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Observation 709c7040-2e32-4c13-9cfe-62d7a0451051 · outbound

This paper cites Photon number conservation and the large-scale 21 cm power spectrum in semi-numerical models of reionization.

SCRIPT in the Cosmic Dawn: Distinguishing Redshift-Evolving Galaxy Populations with 21-cm Fluctuations Photon number conservation and the large-scale 21 cm power spectrum in semi-numerical models of reionization

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Resolution: unresolved; no resolver link, observed 2026-08-15T14:54:41.743886Z

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Observation 1b72ed96-b53f-4c4b-8079-ac4813b8f0cd · outbound

This paper cites Choudhury and A.

SCRIPT in the Cosmic Dawn: Distinguishing Redshift-Evolving Galaxy Populations with 21-cm Fluctuations Choudhury and A

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Resolution: unresolved; no resolver link, observed 2026-08-15T14:54:41.747569Z

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Observation 34dc0123-6792-41ab-9358-e5af8b728d29 · outbound

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

SCRIPT in the Cosmic Dawn: Distinguishing Redshift-Evolving Galaxy Populations with 21-cm Fluctuations Planck 2018 results. VI. Cosmological parameters

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Resolution: unresolved; no resolver link, observed 2026-08-15T14:54:41.750758Z

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Observation 1877f58a-19ca-4814-a000-13ae6d949115 · outbound

This paper cites Multi-scale initial conditions for cosmological simulations.

SCRIPT in the Cosmic Dawn: Distinguishing Redshift-Evolving Galaxy Populations with 21-cm Fluctuations Multi-scale initial conditions for cosmological simulations

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Resolution: unresolved; no resolver link, observed 2026-08-15T14:54:41.754675Z

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Observation 396e0574-836a-4ece-bac4-d49c264e9ef5 · outbound

This paper cites An excursion set model of hierarchical clustering: Ellipsoidal collapse and the moving barrier.

SCRIPT in the Cosmic Dawn: Distinguishing Redshift-Evolving Galaxy Populations with 21-cm Fluctuations An excursion set model of hierarchical clustering: Ellipsoidal collapse and the moving barrier

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Resolution: unresolved; no resolver link, observed 2026-08-15T14:54:41.758254Z

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Observation a13f6445-2ed3-460e-8d86-90760b7a0dbd · outbound

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

SCRIPT in the Cosmic Dawn: Distinguishing Redshift-Evolving Galaxy Populations with 21-cm Fluctuations Descending from on high: Lyman series cascades and spin-kinetic temperature coupling in the 21 cm line

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Resolution: unresolved; no resolver link, observed 2026-08-15T14:54:41.761851Z

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Observation 3fbb5b33-8eb0-42c9-a05b-8b64a9070a43 · outbound

This paper cites The Spin-Kinetic Temperature Coupling and the Heating Rate due to Lyman Alpha Scattering before Reionization: Predictions for 21cm Emission and Absorption.

SCRIPT in the Cosmic Dawn: Distinguishing Redshift-Evolving Galaxy Populations with 21-cm Fluctuations The Spin-Kinetic Temperature Coupling and the Heating Rate due to Lyman Alpha Scattering before Reionization: Predictions for 21cm Emission and Absorption

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Resolution: unresolved; no resolver link, observed 2026-08-15T14:54:41.765288Z

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Observation 1eafa663-4a17-4eb6-959d-339c71ce46b2 · outbound

This paper cites Thermal Evolution of the IGM due to Lyman-{\alpha} photons during the Cosmic Dawn.

SCRIPT in the Cosmic Dawn: Distinguishing Redshift-Evolving Galaxy Populations with 21-cm Fluctuations Thermal Evolution of the IGM due to Lyman-{\alpha} photons during the Cosmic Dawn

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Resolution: verified exact; local_arxiv, observed 2026-08-15T14:54:42.124931Z

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No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation da25fcbb-575e-4fc1-a486-c2839204d369 · outbound

This paper cites Raste and S.K.

SCRIPT in the Cosmic Dawn: Distinguishing Redshift-Evolving Galaxy Populations with 21-cm Fluctuations Raste and S.K

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Resolution: verified exact; raw_fallback, observed 2026-08-15T14:54:42.107048Z

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No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation 6357224b-1653-4639-8815-99b69b16d8a9 · outbound

This paper cites Wouthuysen,On the excitation mechanism of the 21-cm (radio-frequency) interstellar hydrogen emission line., AJ57(1952) 31.

SCRIPT in the Cosmic Dawn: Distinguishing Redshift-Evolving Galaxy Populations with 21-cm Fluctuations Wouthuysen,On the excitation mechanism of the 21-cm (radio-frequency) interstellar hydrogen emission line., AJ57(1952) 31

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Resolution: unresolved; no resolver link, observed 2026-08-15T14:54:41.775590Z

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Observation 715ff4c4-397d-4194-b251-35f419ec7a5e · outbound

This paper cites Field,Excitation of the Hydrogen 21-CM Line,Proceedings of the IRE46(1958) 240.

SCRIPT in the Cosmic Dawn: Distinguishing Redshift-Evolving Galaxy Populations with 21-cm Fluctuations Field,Excitation of the Hydrogen 21-CM Line,Proceedings of the IRE46(1958) 240

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Resolution: unresolved; no resolver link, observed 2026-08-15T14:54:41.778985Z

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Observation 3675479f-8568-4bcb-8721-c8987b3f5c8a · outbound

This paper cites X-ray emission from star-forming galaxies - I. High-mass X-ray binaries.

SCRIPT in the Cosmic Dawn: Distinguishing Redshift-Evolving Galaxy Populations with 21-cm Fluctuations X-ray emission from star-forming galaxies - I. High-mass X-ray binaries

Reference 95

Resolution: unresolved; no resolver link, observed 2026-08-15T14:54:41.782838Z

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Observation d792feae-2244-4a0a-9755-f38e09ad22e4 · outbound

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

SCRIPT in the Cosmic Dawn: Distinguishing Redshift-Evolving Galaxy Populations with 21-cm Fluctuations 21 cm fluctuations from inhomogeneous X-ray heating before reionization

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Resolution: unresolved; no resolver link, observed 2026-08-15T14:54:41.786463Z

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Observation 629f806a-2c0b-447d-89e3-059b8a8621d6 · outbound

This paper cites Shull and M.E.

SCRIPT in the Cosmic Dawn: Distinguishing Redshift-Evolving Galaxy Populations with 21-cm Fluctuations Shull and M.E

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Resolution: unresolved; no resolver link, observed 2026-08-15T14:54:41.790321Z

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Observation 0fff7606-1041-4e89-87c9-f433c01e05b6 · outbound

This paper cites Heating and Ionization of the Intergalactic Medium by an Early X-Ray Background.

SCRIPT in the Cosmic Dawn: Distinguishing Redshift-Evolving Galaxy Populations with 21-cm Fluctuations Heating and Ionization of the Intergalactic Medium by an Early X-Ray Background

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Resolution: unresolved; no resolver link, observed 2026-08-15T14:54:41.793760Z

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Observation 014d0dfe-b6ae-417b-bd54-5a8b3b298d41 · outbound

This paper cites Secondary ionization and heating by fast electrons.

SCRIPT in the Cosmic Dawn: Distinguishing Redshift-Evolving Galaxy Populations with 21-cm Fluctuations Secondary ionization and heating by fast electrons

Reference 99

Resolution: unresolved; no resolver link, observed 2026-08-15T14:54:41.797342Z

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Observation 7671e3e3-14a9-434a-99ed-db17cdf54599 · outbound

This paper cites New Determinations of the UV Luminosity Functions from z~9 to z~2 show a remarkable consistency with halo growth and a constant star formation efficiency.

SCRIPT in the Cosmic Dawn: Distinguishing Redshift-Evolving Galaxy Populations with 21-cm Fluctuations New Determinations of the UV Luminosity Functions from z~9 to z~2 show a remarkable consistency with halo growth and a constant star formation efficiency

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Resolution: unresolved; no resolver link, observed 2026-08-15T14:54:41.800886Z

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