Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity | Paper Citation Record

Observation 14a9cf50-11f6-4fe6-8920-59a92bb76d8e · outbound

This paper cites Chemical evolution of the Large Magellanic Cloud.

Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity Chemical evolution of the Large Magellanic Cloud

Reference 1

Resolution: unresolved; no resolver link, observed 2026-08-01T14:10:48.682313Z

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Observation f8c93d5c-a243-4a37-a6e4-3bacb080c188 · outbound

This paper cites N-enhancement in GN-z11: First evidence for supermassive stars nucleosynthesis in proto-globular clusters-like conditions at high redshift ?.

Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity N-enhancement in GN-z11: First evidence for supermassive stars nucleosynthesis in proto-globular clusters-like conditions at high redshift ?

Reference 2

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Observation 4cd50040-3ec0-4794-b720-4069ff90f711 · outbound

This paper cites Gravitational fragmentation in turbulent primordial gas and the initial mass function of Population III stars.

Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity Gravitational fragmentation in turbulent primordial gas and the initial mass function of Population III stars

Reference 3

Resolution: unresolved; no resolver link, observed 2026-08-01T14:10:48.806496Z

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Observation a5018d8f-0ac1-478b-8a4c-54d772ce69f4 · outbound

This paper cites JADES: The star-formation and chemical enrichment history of a luminous galaxy at z~9.43 probed by ultra-deep JWST/NIRSpec spectroscopy.

Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity JADES: The star-formation and chemical enrichment history of a luminous galaxy at z~9.43 probed by ultra-deep JWST/NIRSpec spectroscopy

Reference 4

Resolution: unresolved; no resolver link, observed 2026-08-01T14:10:48.856156Z

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Observation b9fbdc50-be5c-4d3f-a4f6-b9f80378e23e · outbound

This paper cites Grids of stellar models with rotation VI: Models from 0.8 to 120 $M_\odot$ at a metallicity Z = 0.006.

Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity Grids of stellar models with rotation VI: Models from 0.8 to 120 $M_\odot$ at a metallicity Z = 0.006

Reference 5

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Observation 92c3c319-04dc-4e2c-8a1b-502538a4bbe0 · outbound

This paper cites Frontiers in Astronomy and Space Sciences , keywords =.

Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity Frontiers in Astronomy and Space Sciences , keywords =

Reference 6

Resolution: unresolved; no resolver link, observed 2026-08-01T14:10:48.925052Z

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Observation 8c3ca9ff-4bfc-49ff-ad1b-0c8888c64dd1 · outbound

This paper cites 2024 , eprint=.

Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity 2024 , eprint=

Reference 7

Resolution: unresolved; no resolver link, observed 2026-08-01T14:10:48.960933Z

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Observation 688da9ab-15b0-4c0e-b39d-a996e8793be5 · outbound

This paper cites Impacts of stellar wind and supernovae on the star cluster formation: origins of extremely high N/O ratios and multiple stellar populations.

Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity Impacts of stellar wind and supernovae on the star cluster formation: origins of extremely high N/O ratios and multiple stellar populations

Reference 8

Resolution: unresolved; no resolver link, observed 2026-08-01T14:10:48.976948Z

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Observation 754b7103-8873-40b6-9489-aca579dfb76a · outbound

This paper cites Massive star evolution : rotation, winds, and overshooting vectors in the Mass-Luminosity plane I. A calibrated grid of rotating single star models.

Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity Massive star evolution : rotation, winds, and overshooting vectors in the Mass-Luminosity plane I. A calibrated grid of rotating single star models

Reference 9

Resolution: unresolved; no resolver link, observed 2026-08-01T14:10:49.003753Z

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Observation 0191e0bc-9bd7-49f2-a1f5-c54581d6f4fe · outbound

This paper cites Stellar Wind Yields of Very Massive Stars.

Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity Stellar Wind Yields of Very Massive Stars

Reference 10

Resolution: unresolved; no resolver link, observed 2026-08-01T14:10:49.054408Z

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Observation 02d47851-ef16-465b-9d31-6531a0a24918 · outbound

This paper cites JWST Identification of Extremely Low C/N Galaxies with [N/O]$\gtrsim 0.5$ at $z\sim 6-10$ Evidencing the Early CNO-Cycle Enrichment and a Connection with Globular Cluster Formation.

Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity JWST Identification of Extremely Low C/N Galaxies with [N/O]$\gtrsim 0.5$ at $z\sim 6-10$ Evidencing the Early CNO-Cycle Enrichment and a Connection with Globular Cluster Formation

Reference 11

Resolution: unresolved; no resolver link, observed 2026-08-01T14:10:49.105851Z

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Observation 02a511e0-476f-4929-9a27-8824c5aa7e94 · outbound

This paper cites GA-NIFS: An extremely nitrogen-loud and chemically stratified galaxy at $z\sim 5.55$.

Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity GA-NIFS: An extremely nitrogen-loud and chemically stratified galaxy at $z\sim 5.55$

Reference 12

Resolution: metadata mismatch; local_arxiv, observed 2026-08-01T14:14:42.603374Z

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Observation adacd8d5-6971-4a73-95a5-f2c45055f07d · outbound

This paper cites Rapid Chemical Enrichment by Intermittent Star Formation in GN-z11.

Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity Rapid Chemical Enrichment by Intermittent Star Formation in GN-z11

Reference 13

Resolution: unresolved; no resolver link, observed 2026-08-01T14:10:49.287155Z

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Observation 170c5fdf-8c79-4d1b-9700-9e93dfe8df12 · outbound

This paper cites Presupernova evolution and explosive nucleosynthesis of rotating massive stars in the metallicity range -3 <=[Fe/H]<= 0.

Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity Presupernova evolution and explosive nucleosynthesis of rotating massive stars in the metallicity range -3 <=[Fe/H]<= 0

Reference 14

Resolution: unresolved; no resolver link, observed 2026-08-01T14:10:49.355984Z

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Observation 71412797-2ee6-4fac-abe3-b277b860fb4c · outbound

This paper cites Extreme N-emitters at high-redshift: signatures of supermassive stars and globular cluster or black hole formation in action?.

Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity Extreme N-emitters at high-redshift: signatures of supermassive stars and globular cluster or black hole formation in action?

Reference 15

Resolution: unresolved; no resolver link, observed 2026-08-01T14:10:49.478744Z

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Observation 9a663c38-7e4a-463a-b911-ceb4a8f1bc4d · outbound

This paper cites Multiple channels for nitrogen pollution by metal enriched supermassive stars and implications for GN-z11.

Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity Multiple channels for nitrogen pollution by metal enriched supermassive stars and implications for GN-z11

Reference 16

Resolution: unresolved; no resolver link, observed 2026-08-01T14:10:49.581764Z

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Observation a423ac5f-415c-4f72-b882-2de9c8e78f79 · outbound

This paper cites Low [O/Fe] Ratio in a Luminous Galaxy at the Early Cosmic Epoch ($z>10$): Signature of Short Delay Time or Bright Hypernovae/Pair-Instability Supernovae?.

Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity Low [O/Fe] Ratio in a Luminous Galaxy at the Early Cosmic Epoch ($z>10$): Signature of Short Delay Time or Bright Hypernovae/Pair-Instability Supernovae?

Reference 17

Resolution: metadata mismatch; local_arxiv, observed 2026-08-01T14:14:42.590946Z

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Observation 2ffef0b1-ceab-4a20-adf1-4d173b8e4fa7 · outbound

This paper cites Fast-rotating massive Population~III stars as possible sources of extreme N-enrichment in high-redshift galaxies.

Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity Fast-rotating massive Population~III stars as possible sources of extreme N-enrichment in high-redshift galaxies

Reference 18

Resolution: unresolved; no resolver link, observed 2026-08-01T14:10:49.708164Z

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Observation bbc88397-88e1-45f8-8dc9-86d9157fc1f8 · outbound

This paper cites High N/O ratio at high redshift as a result of a strong burst of star formation and differential galactic winds.

Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity High N/O ratio at high redshift as a result of a strong burst of star formation and differential galactic winds

Reference 19

Resolution: unresolved; no resolver link, observed 2026-08-01T14:10:49.797734Z

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Observation 69678f00-dfc0-4c9c-8d04-c4dfe80c828f · outbound

This paper cites , keywords =.

Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity , keywords =

Reference 20

Resolution: unresolved; no resolver link, observed 2026-08-01T14:10:49.885658Z

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Observation 364a0b65-f1f5-4060-b58c-663ab9887441 · outbound

This paper cites Building up the Population III initial mass function from cosmological initial conditions.

Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity Building up the Population III initial mass function from cosmological initial conditions

Reference 21

Resolution: unresolved; no resolver link, observed 2026-08-01T14:10:49.949020Z

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Observation f0c291f1-2fa5-4901-9c9d-ca011ef20a88 · outbound

This paper cites 2024 , eprint=.

Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity 2024 , eprint=

Reference 22

Resolution: unresolved; no resolver link, observed 2026-08-01T14:10:50.011384Z

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Observation 85c5448b-3beb-449a-9315-c4dc6183d549 · outbound

This paper cites Stellar Yields of Rotating First Stars. II. Pair Instability Supernovae and Comparison with Observations.

Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity Stellar Yields of Rotating First Stars. II. Pair Instability Supernovae and Comparison with Observations

Reference 23

Resolution: unresolved; no resolver link, observed 2026-08-01T14:10:50.153475Z

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Observation 39e3e50c-b33f-4ee8-b72f-a5419004bf33 · outbound

This paper cites Rapidly rotating Population III stellar models as a source of primary nitrogen.

Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity Rapidly rotating Population III stellar models as a source of primary nitrogen

Reference 24

Resolution: unresolved; no resolver link, observed 2026-08-01T14:10:50.235763Z

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Observation 76f139cf-b01b-487c-b74f-3c9e729845bd · outbound

This paper cites Deep rest-UV JWST/NIRSpec spectroscopy of early galaxies: the demographics of CIV and N-emitters in the reionization era.

Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity Deep rest-UV JWST/NIRSpec spectroscopy of early galaxies: the demographics of CIV and N-emitters in the reionization era

Reference 25

Resolution: unresolved; no resolver link, observed 2026-08-01T14:10:50.308794Z

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Observation 7b060fdd-77f8-4e2f-868a-5b9d5b984a30 · outbound

This paper cites Very massive stars and Nitrogen emitting galaxies.

Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity Very massive stars and Nitrogen emitting galaxies

Reference 26

Resolution: unresolved; no resolver link, observed 2026-08-01T14:10:50.423910Z

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Observation f6506c89-f8e1-4332-b376-3d50b0fa1543 · outbound

This paper cites A Study of Primordial Very Massive Star Evolution.

Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity A Study of Primordial Very Massive Star Evolution

Reference 27

Resolution: unresolved; no resolver link, observed 2026-08-01T14:10:50.489496Z

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Observation f024661f-a69c-4d08-8fdf-0a582c0535dd · outbound

This paper cites EMPRESS. XIII. Chemical Enrichments of Young Galaxies Near and Far at z ~ 0 and 4-10: Fe/O, Ar/O, S/O, and N/O Measurements with Chemical Evolution Model Comparisons.

Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity EMPRESS. XIII. Chemical Enrichments of Young Galaxies Near and Far at z ~ 0 and 4-10: Fe/O, Ar/O, S/O, and N/O Measurements with Chemical Evolution Model Comparisons

Reference 28

Resolution: unresolved; no resolver link, observed 2026-08-01T14:10:50.594286Z

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Observation ebc583f1-d28f-4855-afab-c57b6a535835 · outbound

This paper cites EAS2024 , year = 2024, month = jul, eid =.

Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity EAS2024 , year = 2024, month = jul, eid =

Reference 29

Resolution: unresolved; no resolver link, observed 2026-08-01T14:10:50.657859Z

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Observation 584f77ab-e2b8-46fe-8f0c-29931490ec28 · outbound

This paper cites Grids of stellar models with rotation VIII: Models from 1.7 to 500 $M_\odot$ at metallicity $Z = 10^{-5}$.

Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity Grids of stellar models with rotation VIII: Models from 1.7 to 500 $M_\odot$ at metallicity $Z = 10^{-5}$

Reference 30

Resolution: unresolved; no resolver link, observed 2026-08-01T14:10:50.745434Z

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Observation aa33dbd5-ac8e-4ceb-89b9-b68391217a2a · outbound

This paper cites Roll of the Dice: A Stochastically Sampled IMF Alters the Stellar Content of Simulated Dwarf Galaxies.

Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity Roll of the Dice: A Stochastically Sampled IMF Alters the Stellar Content of Simulated Dwarf Galaxies

Reference 31

Resolution: unresolved; no resolver link, observed 2026-08-01T14:10:50.854682Z

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Observation 1b2bbd5d-d451-42b6-9ee7-52ed274f769c · outbound

This paper cites Calibrated, cosmological hydrodynamical simulations with variable IMFs I: Method and effect on global galaxy scaling relations.

Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity Calibrated, cosmological hydrodynamical simulations with variable IMFs I: Method and effect on global galaxy scaling relations

Reference 32

Resolution: unresolved; no resolver link, observed 2026-08-01T14:10:50.928585Z

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Observation 451a42f9-41db-447a-95d4-913b4cf1cd3e · outbound

This paper cites Protostars and Planets V , year = 2007, editor =.

Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity Protostars and Planets V , year = 2007, editor =

Reference 33

Resolution: unresolved; no resolver link, observed 2026-08-01T14:10:51.002756Z

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Observation 30958f4f-c490-409c-8070-7aaa61c2e7ef · outbound

This paper cites The Atlas3D project - XX. Mass-size and mass-sigma distributions of early-type galaxies: bulge fraction drives kinematics, mass-to-light ratio, molecular gas fraction and stellar initial mass function.

Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity The Atlas3D project - XX. Mass-size and mass-sigma distributions of early-type galaxies: bulge fraction drives kinematics, mass-to-light ratio, molecular gas fraction and stellar initial mass function

Reference 34

Resolution: unresolved; no resolver link, observed 2026-08-01T14:10:51.080133Z

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Observation 4bc59a7d-f1a2-4d4b-a6d5-86702db433a4 · outbound

This paper cites Transition of the initial mass function in the metal-poor environments.

Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity Transition of the initial mass function in the metal-poor environments

Reference 35

Resolution: unresolved; no resolver link, observed 2026-08-01T14:10:51.186981Z

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Observation 4472f17a-6038-4947-9cf9-969fa52ffa95 · outbound

This paper cites Chemo-Archaeological Downsizing in a Hierarchical Universe: Impact of a Top Heavy IGIMF.

Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity Chemo-Archaeological Downsizing in a Hierarchical Universe: Impact of a Top Heavy IGIMF

Reference 36

Resolution: unresolved; no resolver link, observed 2026-08-01T14:10:51.234717Z

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Observation ea844453-6f62-4933-a896-cb22c180c390 · outbound

This paper cites Chemodynamics of a Simulated Disc Galaxy: Initial Mass Functions and SNIa Progenitors.

Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity Chemodynamics of a Simulated Disc Galaxy: Initial Mass Functions and SNIa Progenitors

Reference 37

Resolution: unresolved; no resolver link, observed 2026-08-01T14:10:51.335798Z

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Observation 48182e91-6d69-471a-83ef-fc7582bb2fa6 · outbound

This paper cites Mapping the core mass function to the initial mass function.

Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity Mapping the core mass function to the initial mass function

Reference 38

Resolution: unresolved; no resolver link, observed 2026-08-01T14:10:51.398049Z

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Observation 5e9c0626-514d-465e-8f9d-0f65081eb5b1 · outbound

This paper cites The Necessity of Feedback Physics in Setting the Peak of the Initial Mass Function.

Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity The Necessity of Feedback Physics in Setting the Peak of the Initial Mass Function

Reference 39

Resolution: unresolved; no resolver link, observed 2026-08-01T14:10:51.517690Z

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Observation ae1b4bb3-20b6-4928-a802-e75e18f85ce3 · outbound

This paper cites Protostellar Feedback in Turbulent Fragmentation: Consequences for Stellar Clustering and Multiplicity.

Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity Protostellar Feedback in Turbulent Fragmentation: Consequences for Stellar Clustering and Multiplicity

Reference 40

Resolution: unresolved; no resolver link, observed 2026-08-01T14:10:51.595634Z

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Observation 4009473c-16a9-4399-a22a-ce399460923c · outbound

This paper cites Universal Scaling Relations in Scale-Free Structure Formation.

Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity Universal Scaling Relations in Scale-Free Structure Formation

Reference 41

Resolution: unresolved; no resolver link, observed 2026-08-01T14:10:51.686383Z

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Observation f549c00a-d08c-4ecf-a6d9-2df9f5ad7434 · outbound

This paper cites Isothermal Fragmentation: Is there a low-mass cut-off?.

Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity Isothermal Fragmentation: Is there a low-mass cut-off?

Reference 42

Resolution: unresolved; no resolver link, observed 2026-08-01T14:10:51.753650Z

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Observation 9a2d14b5-a9ac-4925-89cc-a85ec05c1af8 · outbound

This paper cites Simulating a metallicity-dependent initial mass function: Consequences for feedback and chemical abundances.

Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity Simulating a metallicity-dependent initial mass function: Consequences for feedback and chemical abundances

Reference 43

Resolution: unresolved; no resolver link, observed 2026-08-01T14:10:51.838621Z

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Observation 1426f1dd-e0ae-402b-ae85-7d2ad9cd2c19 · outbound

This paper cites A Possible Solution for the $M/L-\mathrm{[Fe/H]}$ Relation of Globular Clusters in M31. II. the Age-Metallicity Relation.

Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity A Possible Solution for the $M/L-\mathrm{[Fe/H]}$ Relation of Globular Clusters in M31. II. the Age-Metallicity Relation

Reference 44

Resolution: unresolved; no resolver link, observed 2026-08-01T14:10:51.902276Z

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Observation 61ce316c-6992-4bcd-9d42-83f7783df216 · outbound

This paper cites Magnetic processes in a collapsing dense core. II Fragmentation. Is there a fragmentation crisis ?.

Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity Magnetic processes in a collapsing dense core. II Fragmentation. Is there a fragmentation crisis ?

Reference 45

Resolution: unresolved; no resolver link, observed 2026-08-01T14:10:51.991246Z

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Observation 7149e277-e1ac-43c8-9e21-920a74766f11 · outbound

This paper cites What is the role of stellar radiative feedback in setting the stellar mass spectrum?.

Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity What is the role of stellar radiative feedback in setting the stellar mass spectrum?

Reference 46

Resolution: unresolved; no resolver link, observed 2026-08-01T14:10:52.141000Z

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Observation 73c15af5-b400-41fb-95b0-19ef66cc561d · outbound

This paper cites The formation of UCDs and massive GCs: Quasar-like objects for testing for a variable stellar initial mass function (IMF).

Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity The formation of UCDs and massive GCs: Quasar-like objects for testing for a variable stellar initial mass function (IMF)

Reference 48

Resolution: unresolved; no resolver link, observed 2026-08-01T14:10:52.302397Z

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Observation 32752b2f-35c9-4717-9c93-08f137195429 · outbound

This paper cites The impact of the metallicity and star formation rate on the time-dependent galaxy-wide stellar initial mass function.

Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity The impact of the metallicity and star formation rate on the time-dependent galaxy-wide stellar initial mass function

Reference 49

Resolution: unresolved; no resolver link, observed 2026-08-01T14:10:52.374451Z

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Observation 21ee7fac-989b-4a54-9d8b-414142dcf7b7 · outbound

This paper cites The Cosmic Microwave Background and the Stellar Initial Mass Function.

Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity The Cosmic Microwave Background and the Stellar Initial Mass Function

Reference 50

Resolution: unresolved; no resolver link, observed 2026-08-01T14:10:52.469571Z

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Observation 823ab203-1f9b-41e3-9b15-877f3b612f96 · outbound

This paper cites The Magellanic Bridge cluster NGC 796: Deep optical AO imaging reveals the stellar content and initial mass function of a massive open cluster.

Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity The Magellanic Bridge cluster NGC 796: Deep optical AO imaging reveals the stellar content and initial mass function of a massive open cluster

Reference 51

Resolution: unresolved; no resolver link, observed 2026-08-01T14:10:52.557889Z

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Observation ca765dd0-c52c-479f-8414-68c53b3d02f3 · outbound

This paper cites The Big Problems in Star Formation: the Star Formation Rate, Stellar Clustering, and the Initial Mass Function.

Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity The Big Problems in Star Formation: the Star Formation Rate, Stellar Clustering, and the Initial Mass Function

Reference 52

Resolution: unresolved; no resolver link, observed 2026-08-01T14:10:52.625135Z

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Observation f80232ae-4a4b-4d74-b167-331ad07a1619 · outbound

This paper cites , keywords =.

Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity , keywords =

Reference 53

Resolution: unresolved; no resolver link, observed 2026-08-01T14:10:52.715410Z

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Observation 4ce078b0-686a-4759-bb10-44d2c5442752 · outbound

This paper cites , keywords =.

Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity , keywords =

Reference 54

Resolution: unresolved; no resolver link, observed 2026-08-01T14:10:52.801860Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 8718cac5-ccd3-4a1f-9ba0-edde7d693ed0 · outbound

This paper cites , keywords =.

Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity , keywords =

Reference 55

Resolution: verified exact; doi, observed 2026-08-01T14:14:42.572692Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

Observation 7f22ad11-f315-4cfb-b5fa-12764b0f1b6d · outbound

This paper cites IMF - metallicity: a tight local relation revealed by the CALIFA survey.

Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity IMF - metallicity: a tight local relation revealed by the CALIFA survey

Reference 57

Resolution: unresolved; no resolver link, observed 2026-08-01T14:10:52.997095Z

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Observation 381b4aa0-099f-4579-bf5a-c7c0dc2ce54d · outbound

This paper cites The Fornax 3D project: a two-dimensional view of the stellar initial mass function in the massive lenticular galaxy FCC 167.

Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity The Fornax 3D project: a two-dimensional view of the stellar initial mass function in the massive lenticular galaxy FCC 167

Reference 58

Resolution: unresolved; no resolver link, observed 2026-08-01T14:10:53.108135Z

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Observation 0bc7c074-50a2-4fe2-a76c-186027b2ea99 · outbound

This paper cites Fornax 3D project: assessing the diversity of IMF and stellar population maps within the Fornax Cluster.

Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity Fornax 3D project: assessing the diversity of IMF and stellar population maps within the Fornax Cluster

Reference 59

Resolution: unresolved; no resolver link, observed 2026-08-01T14:10:53.180983Z

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Observation 85bcdbfe-31f2-4c0c-9893-8addbca57226 · outbound

This paper cites The IMF and multiplicity of stars from gravity, turbulence, magnetic fields, radiation and outflow feedback.

Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity The IMF and multiplicity of stars from gravity, turbulence, magnetic fields, radiation and outflow feedback

Reference 60

Resolution: unresolved; no resolver link, observed 2026-08-01T14:10:53.267300Z

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Observation def1f7a7-0024-4aec-9d45-e43cf4cdb5fb · outbound

This paper cites Malicious User Experience Design Research for Cybersecurity.

Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity Malicious User Experience Design Research for Cybersecurity

Reference 61

Resolution: unresolved; no resolver link, observed 2026-08-01T14:10:53.350020Z

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Unavailable: canonical work link unavailable.

Observation cc4d16ec-1155-48c9-a162-45893611cba0 · outbound

This paper cites On the Origin of the Salpeter Slope for the Initial Mass Function.

Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity On the Origin of the Salpeter Slope for the Initial Mass Function

Reference 62

Resolution: unresolved; no resolver link, observed 2026-08-01T14:10:53.434254Z

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Unavailable: canonical work link unavailable.

Observation 36b70ddd-950e-4ebe-815c-318a79a1616e · outbound

This paper cites Low-Metallicity Star Formation : Prestellar Collapse and Protostellar Accretion in the Spherical Symmetry.

Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity Low-Metallicity Star Formation : Prestellar Collapse and Protostellar Accretion in the Spherical Symmetry

Reference 63

Resolution: unresolved; no resolver link, observed 2026-08-01T14:10:53.496628Z

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Observation 13958025-57a2-41f1-b5ed-7f04d287136f · outbound

This paper cites Commmunications of the Konkoly Observatory Hungary , year = 1997, month = jan, volume =.

Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity Commmunications of the Konkoly Observatory Hungary , year = 1997, month = jan, volume =

Reference 64

Resolution: unresolved; no resolver link, observed 2026-08-01T14:10:53.578146Z

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Observation c5570b75-2144-4be4-be36-bdaf920fd237 · outbound

This paper cites The Stellar IMF from Turbulent Fragmentation.

Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity The Stellar IMF from Turbulent Fragmentation

Reference 65

Resolution: unresolved; no resolver link, observed 2026-08-01T14:10:53.665153Z

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Unavailable: canonical work link unavailable.

Observation ed57a1d9-eaec-48e1-81f0-bb37c587cd4f · outbound

This paper cites The influence of a top-heavy integrated galactic IMF and dust on the chemical evolution of high-redshift starbursts.

Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity The influence of a top-heavy integrated galactic IMF and dust on the chemical evolution of high-redshift starbursts

Reference 66

Resolution: unresolved; no resolver link, observed 2026-08-01T14:10:53.748196Z

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Observation 83975088-995c-4551-bcca-526fbd3b840b · outbound

This paper cites SDSS-IV MaNGA: The Spatially Resolved Stellar Initial Mass Function in $\sim$400 Early-Type Galaxies.

Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity SDSS-IV MaNGA: The Spatially Resolved Stellar Initial Mass Function in $\sim$400 Early-Type Galaxies

Reference 67

Resolution: unresolved; no resolver link, observed 2026-08-01T14:10:53.812505Z

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Observation da481880-ffb2-4738-94ef-6083c99dae83 · outbound

This paper cites arXiv e-prints , keywords =.

Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity arXiv e-prints , keywords =

Reference 68

Resolution: unresolved; no resolver link, observed 2026-08-01T14:10:53.910185Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation cf6860c2-778a-4488-b5f9-7d1f47520b5d · outbound

This paper cites Do fragmentation and accretion affect the stellar Initial Mass Function?.

Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity Do fragmentation and accretion affect the stellar Initial Mass Function?

Reference 69

Resolution: unresolved; no resolver link, observed 2026-08-01T14:10:54.013141Z

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Unavailable: canonical work link unavailable.

Observation d6d3b58f-e794-4c84-8d70-674afa455c19 · outbound

This paper cites Stellar Initial Mass Function over a range of redshifts.

Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity Stellar Initial Mass Function over a range of redshifts

Reference 70

Resolution: unresolved; no resolver link, observed 2026-08-01T14:10:54.066598Z

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Observation 1272c38f-707a-4c74-9b79-22a037622ae5 · outbound

This paper cites MUSE observations of M87: radial gradients for the stellar initial-mass function and the abundance of Sodium.

Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity MUSE observations of M87: radial gradients for the stellar initial-mass function and the abundance of Sodium

Reference 71

Resolution: unresolved; no resolver link, observed 2026-08-01T14:10:54.157382Z

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Unavailable: canonical work link unavailable.

Observation 17eb4135-5568-4cdb-8d13-0648d668bad0 · outbound

This paper cites An excess of massive stars in the local 30 Doradus starburst.

Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity An excess of massive stars in the local 30 Doradus starburst

Reference 75

Resolution: unresolved; no resolver link, observed 2026-08-01T14:10:54.449688Z

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Unavailable: canonical work link unavailable.

Observation 9ab8f41b-dd05-4c1c-ae8c-fdb445b7d64b · outbound

This paper cites The importance of magnetic fields for the initial mass function of the first stars.

Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity The importance of magnetic fields for the initial mass function of the first stars

Reference 76

Resolution: unresolved; no resolver link, observed 2026-08-01T14:10:54.546944Z

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Unavailable: canonical work link unavailable.

Observation 309499dc-6b32-4569-bd23-daeee4654834 · outbound

This paper cites Magnetic field amplification in accretion discs around the first stars: implications for the primordial IMF.

Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity Magnetic field amplification in accretion discs around the first stars: implications for the primordial IMF

Reference 77

Resolution: unresolved; no resolver link, observed 2026-08-01T14:10:54.614011Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 8adb5579-9495-4999-b18c-5251fa8ccdca · outbound

This paper cites When did the initial mass function become bottom-heavy?.

Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity When did the initial mass function become bottom-heavy?

Reference 78

Resolution: unresolved; no resolver link, observed 2026-08-01T14:10:54.686369Z

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Unavailable: canonical work link unavailable.

Observation 558f8b54-2fb0-48ba-858f-c7c2c2404ca8 · outbound

This paper cites Thermal Regulation and the Star-Forming Main Sequence.

Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity Thermal Regulation and the Star-Forming Main Sequence

Reference 79

Resolution: unresolved; no resolver link, observed 2026-08-01T14:10:54.738483Z

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Observation aa211734-8125-42c7-ad34-db82f8437cb2 · outbound

This paper cites The Stellar Initial Mass Function in Early-Type Galaxies from Absorption Line Spectroscopy. III. Radial Gradients.

Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity The Stellar Initial Mass Function in Early-Type Galaxies from Absorption Line Spectroscopy. III. Radial Gradients

Reference 80

Resolution: unresolved; no resolver link, observed 2026-08-01T14:10:54.818265Z

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Unavailable: canonical work link unavailable.

Observation 6d7d91e8-fbc2-4ec5-a950-5e322823eccc · outbound

This paper cites The galaxy-wide IMF of dwarf late-type to massive early-type galaxies.

Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity The galaxy-wide IMF of dwarf late-type to massive early-type galaxies

Reference 81

Resolution: unresolved; no resolver link, observed 2026-08-01T14:10:54.892660Z

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Unavailable: canonical work link unavailable.

Observation 11c33930-276f-4909-8873-12e908bfc273 · outbound

This paper cites The optimally-sampled galaxy-wide stellar initial mass function - Observational tests and the publicly available GalIMF code.

Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity The optimally-sampled galaxy-wide stellar initial mass function - Observational tests and the publicly available GalIMF code

Reference 82

Resolution: unresolved; no resolver link, observed 2026-08-01T14:10:54.955667Z

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Unavailable: canonical work link unavailable.

Observation ba9a3171-43b7-4a84-aeab-bce0e097b03f · outbound

This paper cites SDSS-IV MaNGA: Stellar initial mass function variation inferred from Bayesian analysis of the integral field spectroscopy of early type galaxies.

Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity SDSS-IV MaNGA: Stellar initial mass function variation inferred from Bayesian analysis of the integral field spectroscopy of early type galaxies

Reference 83

Resolution: unresolved; no resolver link, observed 2026-08-01T14:10:55.028556Z

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Observation c1a4400c-91e1-4e7b-b3d5-264d75a53b23 · outbound

This paper cites A Possible Solution for the M/L-[Fe/H] Relation of Globular Clusters in M31: A metallicity and density dependent top-heavy IMF.

Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity A Possible Solution for the M/L-[Fe/H] Relation of Globular Clusters in M31: A metallicity and density dependent top-heavy IMF

Reference 84

Resolution: unresolved; no resolver link, observed 2026-08-01T14:10:55.082627Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation fee52052-d614-4755-938a-c19984eb3c06 · outbound

This paper cites Bound star clusters observed in a lensed galaxy 460 Myr after the Big Bang.

Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity Bound star clusters observed in a lensed galaxy 460 Myr after the Big Bang

Reference 85

Resolution: unresolved; no resolver link, observed 2026-08-01T14:10:55.157518Z

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Unavailable: canonical work link unavailable.

Observation c67524dc-7728-4436-9211-d23f19ddcac0 · outbound

This paper cites Radii of Young Star Clusters in Nearby Galaxies.

Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity Radii of Young Star Clusters in Nearby Galaxies

Reference 86

Resolution: unresolved; no resolver link, observed 2026-08-01T14:10:55.232700Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 87a8631c-a690-4cfd-bd30-bc8a74bcf5e7 · outbound

This paper cites A Comparative Study of Giant Molecular Clouds in M51, M33 and the Large Magellanic Cloud.

Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity A Comparative Study of Giant Molecular Clouds in M51, M33 and the Large Magellanic Cloud

Reference 87

Resolution: unresolved; no resolver link, observed 2026-08-01T14:10:55.312969Z

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Unavailable: canonical work link unavailable.

Observation 91ffd322-c4c9-4cf6-ae7f-64e9d8e8fdb2 · outbound

This paper cites Metal-poor star formation at $z>6$ with JWST: new insight into hard radiation fields and nitrogen enrichment on 20 pc scales.

Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity Metal-poor star formation at $z>6$ with JWST: new insight into hard radiation fields and nitrogen enrichment on 20 pc scales

Reference 88

Resolution: unresolved; no resolver link, observed 2026-08-01T14:10:55.426375Z

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Unavailable: canonical work link unavailable.

Observation 1f1624a9-6df6-471e-a69d-13dbb675f59d · outbound

This paper cites A unified model for the co-evolution of galaxies and their circumgalactic medium: the relative roles of turbulence and atomic cooling physics.

Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity A unified model for the co-evolution of galaxies and their circumgalactic medium: the relative roles of turbulence and atomic cooling physics

Reference 89

Resolution: unresolved; no resolver link, observed 2026-08-01T14:10:55.530172Z

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Unavailable: canonical work link unavailable.

Observation da82d14e-ae05-4ffe-ad35-4a2543a725cc · outbound

This paper cites Equilibrium States of Galactic Atmospheres I: The Flip Side of Mass Loading.

Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity Equilibrium States of Galactic Atmospheres I: The Flip Side of Mass Loading

Reference 90

Resolution: unresolved; no resolver link, observed 2026-08-01T14:10:55.618275Z

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Unavailable: canonical work link unavailable.

Observation 33195da9-8837-463b-934b-850ad63e35ef · outbound

This paper cites Equilibrium States of Galactic Atmospheres II: Interpretation and Implications.

Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity Equilibrium States of Galactic Atmospheres II: Interpretation and Implications

Reference 91

Resolution: unresolved; no resolver link, observed 2026-08-01T14:10:55.667186Z

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Unavailable: canonical work link unavailable.

Observation 2b873ec4-0531-4a8e-8714-275ec5907bd1 · outbound

This paper cites , keywords =.

Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity , keywords =

Reference 92

Resolution: unresolved; no resolver link, observed 2026-08-01T14:10:55.809750Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7f3db280-b1fe-4ac7-89c0-62c1436bf405 · outbound

This paper cites The Ultraviolet Slopes of Early Universe Galaxies: The Impact of Bursty Star Formation, Dust, and Nebular Continuum Emission.

Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity The Ultraviolet Slopes of Early Universe Galaxies: The Impact of Bursty Star Formation, Dust, and Nebular Continuum Emission

Reference 93

Resolution: unresolved; no resolver link, observed 2026-08-01T14:10:55.867145Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 82308d31-79da-4987-9da9-41a8ba4797ae · outbound

This paper cites The Open Journal of Astrophysics , keywords =.

Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity The Open Journal of Astrophysics , keywords =

Reference 94

Resolution: unresolved; no resolver link, observed 2026-08-01T14:10:55.940803Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0df825e8-4ad5-410e-878a-72472aa73aef · outbound

This paper cites The Formation of the First Star in the Universe.

Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity The Formation of the First Star in the Universe

Reference 95

Resolution: unresolved; no resolver link, observed 2026-08-01T14:10:56.012910Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a4abef17-3449-4624-94fe-b0de23c956b1 · outbound

This paper cites On the Origin of the High Star-Formation Efficiency in Massive Galaxies at Cosmic Dawn.

Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity On the Origin of the High Star-Formation Efficiency in Massive Galaxies at Cosmic Dawn

Reference 96

Resolution: unresolved; no resolver link, observed 2026-08-01T14:10:56.250345Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 92afde5d-e7f7-4e1c-bdcd-ab77ea5df4a4 · outbound

This paper cites arXiv e-prints , keywords =.

Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity arXiv e-prints , keywords =

Reference 98

Resolution: unresolved; no resolver link, observed 2026-08-01T14:10:56.382628Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 3c3ee7ea-4f9c-418c-9831-24fd046caa9e · outbound

This paper cites SPICE: the connection between cosmic reionisation and stellar feedback in the first galaxies.

Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity SPICE: the connection between cosmic reionisation and stellar feedback in the first galaxies

Reference 99

Resolution: unresolved; no resolver link, observed 2026-08-01T14:10:56.430350Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a1db14a0-9a7a-4940-ae73-486490882e8d · outbound

This paper cites Stress Testing $\Lambda$CDM with High-redshift Galaxy Candidates.

Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity Stress Testing $\Lambda$CDM with High-redshift Galaxy Candidates

Reference 100

Resolution: unresolved; no resolver link, observed 2026-08-01T14:10:56.448838Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c38ebe4e-570d-4c9a-a62f-31e69e347b9c · outbound

This paper cites The Formation of the First Stars. I. The Primordial Star Forming Cloud.

Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity The Formation of the First Stars. I. The Primordial Star Forming Cloud

Reference 101

Resolution: unresolved; no resolver link, observed 2026-08-01T14:10:56.453444Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 9683789c-6924-45ac-b62b-71b03c319a2d · outbound

This paper cites Redshift-dependent galaxy formation efficiency at $z=5-13$ in the FirstLight simulations.

Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity Redshift-dependent galaxy formation efficiency at $z=5-13$ in the FirstLight simulations

Reference 102

Resolution: unresolved; no resolver link, observed 2026-08-01T14:10:56.458259Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 857079f4-b17f-4fb1-8f6e-a4d5f2d31702 · outbound

This paper cites Variations of the stellar initial mass function in the progenitors of massive early-type galaxies and in extreme starburst environments.

Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity Variations of the stellar initial mass function in the progenitors of massive early-type galaxies and in extreme starburst environments

Reference 103

Resolution: unresolved; no resolver link, observed 2026-08-01T14:10:56.463022Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 930961ad-20a6-448c-b529-0c42294ed371 · outbound

This paper cites A Simple Model for the Absorption of Starlight by Dust in Galaxies.

Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity A Simple Model for the Absorption of Starlight by Dust in Galaxies

Reference 104

Resolution: unresolved; no resolver link, observed 2026-08-01T14:10:56.467182Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e41cc9ec-632d-4cce-9a4c-04ca670273f3 · outbound

This paper cites Feedback-Free Star Formation in Clusters within a Galaxy Simulated at High Resolution in Cosmic Dawn.

Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity Feedback-Free Star Formation in Clusters within a Galaxy Simulated at High Resolution in Cosmic Dawn

Reference 105

Resolution: metadata mismatch; local_arxiv, observed 2026-08-01T14:14:42.554555Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

Observation f9d6a4df-3d47-4d22-83a1-8030e9ea957b · outbound

This paper cites Impact of the cosmic background radiation on the initial mass function of metal-poor stars.

Bright Galaxies at Cosmic Dawn: A Cloud-Scale Star Formation Model Unifying Variable SFE, IMFs, and Stochasticity Impact of the cosmic background radiation on the initial mass function of metal-poor stars

Reference 106

Resolution: unresolved; no resolver link, observed 2026-08-01T14:10:56.476111Z

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