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published · living versions
W_x23wpc43·v1 · currentpublished
How bursty star formation shapes spectral diversity at high redshifts: breaking degeneracies in early galaxy formation
with Charlotte A. Mason, Daniel P. Stark, Mengtao Tang, Julian B. Muñoz +2
1 version

Preprints & journals

27 papers in the corpus · 2020–2026
SPURS: An Ultra-deep View Inside the Compact, Nitrogen-Enriched Nuclei of Little Red Dots2609.11094v1 · Mengtao Tang, Daniel P. Stark, Charlotte A. Mason et al.2026 · 0 citationsarXiv
SPURS: Massive Stars, Dense Gas, and Lyα\alpha Escape in GN-z11 at z=10.6z = 10.62608.12699v3 · Zuyi Chen, Daniel P. Stark, Charlotte A. Mason et al.2026 · 0 citationsarXiv
Chemical signatures from the first stars embedded in metal-poor gas in galaxies at cosmic dawn2606.13078v1 · Clara L. Pollock, Kasper E. Heintz, Elka Rusta et al.2026 · 0 citationsarXiv
NEFERTITI: Linking early galaxy formation to the assembly of the Milky Way2605.00990v1 · Ioanna Koutsouridou, Stefania Salvadori, 'Asa Sk'ulad'ottir et al.2026 · 0 citationsarXiv
SPURS: Bursty Star Formation in an Extremely Luminous Weak Emission Line Galaxy at z=9.3z=9.32604.21516v1 · Zuyi Chen, Daniel P. Stark, Charlotte A. Mason et al.2026 · 1 citationarXiv
BEACON: JWST NIRCam Pure-parallel Imaging Survey. III. Constraints on the UV LF and the Clustering of z~7-14 Galaxies2604.17963v2 · Kimi C. Kreilgaard, Charlotte A. Mason, Takahiro Morishita et al.2026 · 0 citationsarXiv
The Pristine HeII Emitter near GN-z11: Constraining the Mass Distribution of the First Stars2603.20363v2 · Elka Rusta, Stefania Salvadori, Roberto Maiolino et al.2026 · 1 citationarXiv
BEACON: JWST NIRCam Pure-parallel Imaging Survey. II. Physical Properties of z=7−14z=7-14 Galaxies2601.02861v1 · Yechi Zhang, Takahiro Morishita, Kimi C. Kreilgaard et al.2026 · 0 citationsarXiv
Neutral hydrogen in and around galaxies during the Epoch of Reionization2510.01315v1 · V. Gelli, C. Mason, A. Pallottini et al.2025 · 0 citationsarXiv
The JWST Spectroscopic Properties of Galaxies at z=9−14z=9-142507.08245v3 · Mengtao Tang, Daniel P. Stark, Charlotte A. Mason et al.2025 · 17 citationsarXiv
Metal-polluted Population III galaxies and How to Find Them2506.17400v2 · Elka Rusta, Stefania Salvadori, Viola Gelli et al.2025 · 11 citationsarXiv
Temporarily quiescent galaxies at cosmic dawn: probing bursty star formation2501.16418v1 · Viola Gelli, Andrea Pallottini, Stefania Salvadori et al.2025 · 18 citationsarXiv
BEACON: JWST NIRCam Pure-parallel Imaging Survey. I. Survey Design and Initial Results2412.04211v2 · Takahiro Morishita, Charlotte A. Mason, Kimi C. Kreilgaard et al.2024 · 25 citationsarXiv
Linking high-z and low-z: Are We Observing the Progenitors of the Milky Way with JWST?2407.06255v2 · Elka Rusta, Stefania Salvadori, Viola Gelli et al.2024 · 5 citationsarXiv
The impact of mass-dependent stochasticity at cosmic dawn2405.13108v3 · Viola Gelli, Charlotte Mason, Christopher C. Hayward2024 · 63 citationsarXiv
Gas-phase metallicity gradients in galaxies at z∼6−8z \sim 6-82403.03977v2 · G. Venturi, S. Carniani, E. Parlanti et al.2024 · 56 citationsA&A 691, A19 (2024)
Can supernovae quench star formation in high-zz galaxies?2310.03065v1 · Viola Gelli, Stefania Salvadori, Andrea Ferrara et al.2023 · 18 citationsarXiv
Quiescent low-mass galaxies observed by JWST in the Epoch of Reionization2303.13574v2 · Viola Gelli, Stefania Salvadori, Andrea Ferrara et al.2023 · 37 citationsarXiv
PISN-explorer: hunting the descendants of very massive first stars2301.03604v1 · D. S. Aguado (UNIFI), S. Salvadori (UNIFI), A. Sk'ulad'ottir (UNIFI) et al.2023 · 19 citationsarXiv
A survey of high-zz galaxies: SERRA simulations2201.02636v2 · A. Pallottini, A. Ferrara, S. Gallerani et al.2022 · 102 citationsarXiv
Dwarf satellites of high-z Lyman Break Galaxies: a free lunch for JWST2105.05252v1 · Viola Gelli, Stefania Salvadori, Andrea Ferrara et al.2021 · 14 citationsarXiv
The stellar populations of high-redshift dwarf galaxies2009.03912v1 · V. Gelli, S. Salvadori, A. Pallottini et al.2020 · 26 citationsarXiv
Career total: 35 works. 27 are in this corpus.

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