2020
DOI: 10.48550/arxiv.2002.00962
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The ALPINE-ALMA [CII] Survey: data processing, catalogs, and statistical source properties

M. Bethermin,
Y. Fudamoto,
M. Ginolfi
et al.

Abstract: The ALPINE-ALMA large program targets the [CII] 158 µm line and the far-infrared continuum in 118 spectroscopically confirmed star-forming galaxies between z=4.4 and z=5.9. It represents the first large [CII] statistical sample built in this redshift range. We present details of the data processing and the construction of the catalogs. We detected 23 of our targets in the continuum. To derive accurate infrared luminosities and obscured star formation rates, we measured the conversion factor from the ALMA 158 … Show more

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Cited by 21 publications
(81 citation statements)
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“…Overview ALPINE is an ALMA large program (Project ID: 2017.1.00428.L; PI: O. Le Fèvre; see also : e.g., Le Fèvre et al 2019;Faisst et al 2019;Bethermin et al 2020), aimed at measuring [C ii] 158 µm and rest-frame FIR continuum emission from a representative sample of 118 main-sequence galaxies at 4.4 < z < 5.8. Observations were carried out between May 2018 and February 2019.…”
Section: Alpine Surveymentioning
confidence: 99%
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“…Overview ALPINE is an ALMA large program (Project ID: 2017.1.00428.L; PI: O. Le Fèvre; see also : e.g., Le Fèvre et al 2019;Faisst et al 2019;Bethermin et al 2020), aimed at measuring [C ii] 158 µm and rest-frame FIR continuum emission from a representative sample of 118 main-sequence galaxies at 4.4 < z < 5.8. Observations were carried out between May 2018 and February 2019.…”
Section: Alpine Surveymentioning
confidence: 99%
“…The details of data calibration, reduction, and [C ii] line extractions are described in Bethermin et al (2020).…”
Section: Data Productsmentioning
confidence: 99%
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“…They do, however, find a possible deviation at lower SFR. Schaerer et al (2020) also find good agreement between z ∼ 4 -6 star-forming galaxies from the APLINE-ALMA survey (Le Fèvre et al 2019;Bethermin et al 2020;Faisst et al 2020) and local galaxies. When combined with earlier measurements at z > 6, they find only a slightly steeper [C ii]-SFR relation than the local one.…”
Section: Introductionmentioning
confidence: 71%
“…The goal of this paper is to address these questions, using a unique set of observations taken by the ALMA Large Program to INvestigate C II at Early times (ALPINE) survey (Le Fèvre et al 2019;Faisst et al 2020;Bethermin et al 2020).…”
Section: Introductionmentioning
confidence: 99%