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Laia Barrufet

University of Edinburgh · GB
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Area of research
Astronomy and Astrophysics · Instrumentation
Research interest
Research interests include Physics, Astrophysics, Galaxy, Reionization, Redshift, and Astronomy.
h-index
citations
1,263
works
19
NIH funding
primary concept
email

Recent publications

The <i>JWST</i> EXCELS survey: probing strong-line diagnostics and the chemical evolution of galaxies over cosmic time using <i>Te</i>-metallicities
Monthly Notices of the Royal Astronomical Society 2025cited by 20position: middledoi
The <i>JWST</i> EXCELS survey: an extremely metal-poor galaxy at <i>z</i> = 8.271 hosting an unusual population of massive stars
Monthly Notices of the Royal Astronomical Society 2025cited by 20position: middledoi
The <i>JWST</i> EXCELS survey: direct estimates of C, N, and O abundances in two relatively metal-rich galaxies at <i>z</i> ≃ 5
Monthly Notices of the Royal Astronomical Society 2025cited by 16position: middledoi
21 Balmer Jump Street: The Nebular Continuum at High Redshift and Implications for the Bright Galaxy Problem, UV Continuum Slopes, and Early Stellar Populations
The Open Journal of Astrophysics 2025cited by 15position: middledoi
The <i>JWST</i> EXCELS survey: too much, too young, too fast? Ultra-massive quiescent galaxies at 3 &amp;lt; z &amp;lt; 5
Monthly Notices of the Royal Astronomical Society 2024cited by 103position: middledoi
Accelerated formation of ultra-massive galaxies in the first billion years 
Nature 2024cited by 70position: middledoi
Unveiling the hidden Universe with <i>JWST</i>: the contribution of dust-obscured galaxies to the stellar mass function at <i>z</i> ~ 3 – 8
Monthly Notices of the Royal Astronomical Society 2024cited by 36position: middledoi
The NIRVANDELS survey: the stellar and gas-phase mass-metallicity relations of star-forming galaxies at z = 3.5
Monthly Notices of the Royal Astronomical Society 2024cited by 31position: middledoi
Unveiling the nature of infrared bright, optically dark galaxies with early <i>JWST</i> data
Monthly Notices of the Royal Astronomical Society 2023cited by 104position: firstdoi
The ALMA REBELS Survey: the first infrared luminosity function measurement at <i>z</i>  ∼ 7
Monthly Notices of the Royal Astronomical Society 2023cited by 35position: firstdoi
The ALMA REBELS survey: obscured star formation in massive Lyman-break galaxies at <i>z</i> <b>=</b> 4–8 revealed by the IRX–β and <i>M</i>⋆ relations
Monthly Notices of the Royal Astronomical Society 2023cited by 33position: middledoi
The ALMA REBELS Survey: discovery of a massive, highly star-forming, and morphologically complex ULIRG at <i>z</i> = 7.31
Monthly Notices of the Royal Astronomical Society 2023cited by 19position: middledoi
Reionization Era Bright Emission Line Survey: Selection and Characterization of Luminous Interstellar Medium Reservoirs in the z &gt; 6.5 Universe
The Astrophysical Journal 2022cited by 201position: middledoi
The ALMA REBELS Survey: cosmic dust temperature evolution out to <i>z</i> ∼ 7
Monthly Notices of the Royal Astronomical Society 2022cited by 120position: middledoi
The ALMA REBELS Survey: dust continuum detections at <i>z</i> &amp;gt; 6.5
Monthly Notices of the Royal Astronomical Society 2022cited by 115position: middledoi
The ALMA REBELS survey: the dust-obscured cosmic star formation rate density at redshift 7
Monthly Notices of the Royal Astronomical Society 2022cited by 96position: middledoi
The ALMA REBELS Survey. Epoch of Reionization giants: Properties of dusty galaxies at <i>z</i> ≈ 7
Monthly Notices of the Royal Astronomical Society 2022cited by 95position: middledoi
The ALMA REBELS Survey : specific star formation rates in the reionization era
CINECA IRIS Institutial research information system (University of Pisa) 2022cited by 87position: middledoi
The ALMA REBELS Survey: Average [C ii] 158 μm Sizes of Star-forming Galaxies from z ∼ 7 to z ∼ 4
The Astrophysical Journal 2022cited by 47position: middledoi

Grants

No grants ingested yet.

Frequent collaborators

Mauro Stefanon · University of Kansas6 papers (2022–2024)Yoshinobu Fudamoto · Chiba University6 papers (2022–2024)Fergus Cullen · University of Edinburgh6 papers (2023–2025)Pascal A. Oesch · University of Geneva6 papers (2022–2025)J. S. Dunlop · Royal Observatory6 papers (2023–2025)R. J. McLure · University of Edinburgh6 papers (2023–2025)Karla Z. Arellano-Córdova · The University of Texas at Austin5 papers (2024–2025)T M Stanton · University of Edinburgh5 papers (2024–2025)D.J. McLeod · University of Edinburgh5 papers (2024–2025)R. J. Bouwens · California Institute of Technology5 papers (2022–2023)Callum T. Donnan · University of Edinburgh5 papers (2024–2025)Alice E. Shapley · University of California, Los Angeles5 papers (2024–2025)Adam C. Carnall · University of Edinburgh5 papers (2024–2025)R Begley · University of Edinburgh5 papers (2024–2025)Michael W. Topping · University of Arizona4 papers (2022–2024)D. Scholte · University of Manchester4 papers (2024–2025)Hanae Inami · Université Claude Bernard Lyon 14 papers (2022–2023)Andrea Ferrara · Georgia Institute of Technology4 papers (2022–2023) · 4 papers (2022–2023)P. van der Werf · Université Claude Bernard Lyon 14 papers (2022–2023)
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