activity
20192026
most citedThe ALPINE-ALMA [CII] Survey: The nature, luminosity function and star formation history of dusty galaxies up to z~6

200 citations · 1.6k across the 36 of their papers we have counts for

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Showing 2022Show all

8 papers · 1 filter

astro-ph.GA2022★ 11 cited

The ALPINE-ALMA [CII] survey: double stellar population and AGN activity in a galaxy at

L. Barchiesi, M. Dessauges-Zavadsky, C. Vignali +16

GDS J033218.92-275302.7 (here GS-14) is a galaxy detected in [CII] as part of the ALPINE survey with unusual UV spectral features that have been interpreted as signature…

astro-ph.GA2022★ 3 cited

The ALPINE-ALMA [CII] survey: The infrared-radio correlation and AGN fraction of star-forming galaxies at z 4.4-5.9

Lu Shen, Brian C. Lemaux, Lori M. Lubin +26

We present the radio properties of 66 spectroscopically-confirmed normal star-forming galaxies (SFGs) at in the COSMOS field that were [C II] detected in the Atacama La…

astro-ph.GA2022★ 6 cited

ALPINE: A Large Survey to Understand Teenage Galaxies

A. L. Faisst, L. Yan, M. Béthermin +13

A multiwavelength study of galaxies is important to understand their formation and evolution. Only in the recent past, thanks to the Atacama Large (Sub) Millimeter Array (ALMA), we…

astro-ph.GA2022★ 13 cited

IR characteristic emission and dust properties of star-forming galaxies at 4.5 z 6.2

D. Burgarella, J. Bogdanoska, A. Nanni +31

The luminosity functions at z < 4 - 5 suggest that most galaxies have a relatively low stellar mass (logM_star = 10) and a low dust attenuation (A_FUV = 1.0). The physical properti…

astro-ph.GA2022★ 35 cited

The ALPINE-ALMA [CII] survey: dust attenuation curves at z=4.4-5.5

Mederic Boquien, Veronique Buat, Denis Burgarella +14

There is now ample evidence that dust is already present in abundance at high z. However, given the faintness of distant galaxies in the optical and the NIR, datasets are still lim…

astro-ph.GA2022★ 19 cited

The ALPINE-ALMA [CII] Survey: the population of [CII]-undetected galaxies and their role in the -SFR relation

Michael Romano, L. Morselli, P. Cassata +22

The [CII] 158m emission line represents so far one of the most profitable tools for the investigation of the high-redshift galaxies in the early Universe. Being one of the brig…