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20192026
most citedThe ALPINE-ALMA [CII] Survey: data processing, catalogs, and statistical source properties

245 citations · 2.5k across the 214 of their papers we have counts for

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Showing 2022Show all

6 papers · 1 filter

astro-ph.GA2022★ 20 cited

Massive galaxy formation caught in action at z~5 with JWST

Shuowen Jin, Nikolaj B. Sillassen, Georgios E. Magdis +13

We report the discovery of a compact group of galaxies, CGG-z5, at z~5.2 in the EGS field covered by the JWST/CEERS survey. CGG-z5 was selected as the highest overdensity of galaxi…

astro-ph.GA2022★ 193 cited

COSMOS2020: The Galaxy Stellar Mass Function: the assembly and star formation cessation of galaxies at

J. R. Weaver, I. Davidzon, S. Toft +30

How galaxies form, assemble, and cease their star-formation is a central question within the modern landscape of galaxy evolution studies. These processes are indelibly imprinted o…

astro-ph.GA2022★ 26 cited

COSMOS2020: UV selected galaxies at

O. B. Kauffmann, O. Ilbert, J. R. Weaver +16

This paper presents a new search for galaxies using the COSMOS2020 photometric catalogues. Finding galaxies at the reionization epoch through deep imaging surveys remain…

astro-ph.GA2022★ 29 cited

COSMOS2020: Manifold Learning to Estimate Physical Parameters in Large Galaxy Surveys

I. Davidzon, K. Jegatheesan, O. Ilbert +16

We present a novel method to estimate galaxy physical properties from spectral energy distributions (SEDs), alternate to template fitting techniques and based on self-organizing ma…

astro-ph.GA2022★ 60 cited

Dynamical characterization of galaxies up to

F. Rizzo, M. Kohandel, A. Pallottini +4

The characterization of the dynamical state of galaxies up to z~7 is crucial for constraining the mechanisms driving the mass assembly in the early Universe. However, it is unclear…

astro-ph.GA2022★ 93 cited

COSMOS2020: The cosmic evolution of the stellar-to-halo mass relation for central and satellite galaxies up to z~5

M. Shuntov, H. J. McCracken, R. Gavazzi +13

We use the COSMOS2020 catalogue to measure the stellar-to-halo mass relation (SHMR) divided by central and satellite galaxies from to . Starting from accurate phot…