A
Andrea Pallottini
Researcher at University of Cambridge
Publications - 109
Citations - 3327
Andrea Pallottini is an academic researcher from University of Cambridge. The author has contributed to research in topics: Galaxy & Redshift. The author has an hindex of 29, co-authored 73 publications receiving 2238 citations. Previous affiliations of Andrea Pallottini include Scuola Normale Superiore di Pisa.
Papers
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On the (cii)-sfr relation in high redshift galaxies
TL;DR: In this paper, the authors used the Vallini et al. 2013 (V13) model, based on high-resolution, radiative transfer cosmological simulations to predict the [CII] emission from the interstellar medium of a z~7 (halo mass $M_h=1.17\times10^{11}M_{\odot}$) galaxy.
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Extended ionised and clumpy gas in a normal galaxy at z=7.1 revealed by ALMA
Stefano Carniani,Roberto Maiolino,Andrea Pallottini,Livia Vallini,L. Pentericci,Andrea Ferrara,Marco Castellano,Eros Vanzella,Andrea Grazian,Simona Gallerani,Paola Santini,Jeff Wagg,Adriano Fontana +12 more
TL;DR: In this article, the authors presented new ALMA observations of the [O III] 88 mu m line and high angular resolution observations of [C II] 158 cm m line in a normal star forming galaxy at z = 7.1.
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Kiloparsec-scale gaseous clumps and star formation at z = 5–7
Stefano Carniani,Roberto Maiolino,Ricardo Amorín,Laura Pentericci,Andrea Pallottini,Andrea Ferrara,Chris J. Willott,Renske Smit,Jorryt Matthee,David Sobral,David Sobral,P. Santini,Marco Castellano,S. de Barros,S. de Barros,Adriano Fontana,Andrea Grazian,Lucia Guaita +17 more
TL;DR: In this article, the morphology of the [CII]-SFR emission in a sample of normal star-forming galaxies at 5 < z < 7 was investigated, and it was shown that the deviation from the local L[CII−SFR relation has a weak anti-correlation with the EW(Lyα).
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Zooming on the internal structure of z ≃ 6 galaxies
Andrea Pallottini,Andrea Ferrara,Simona Gallerani,Livia Vallini,Livia Vallini,Roberto Maiolino,Stefania Salvadori +6 more
TL;DR: In this paper, a zoom-in, adaptive mesh refinement, high-resolution simulation of high-redshift (z ≃ 6) galaxies with the aim of characterizing their internal properties and interstellar medium is presented.
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Simulating cosmic metal enrichment by the first galaxies
TL;DR: In this article, the authors study cosmic metal enrichment via adaptive mesh refinement hydrodynamical simulations in a (10 Mpc h-1)3 volume following the Population III (PopIII)-PopII transition and for different PopIII initial mass function (IMFs).