245 citations · 2k across the 51 of their papers we have counts for
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The ALPINE-ALMA [CII] Survey: Obscured Star Formation Rate Density and Main Sequence of star-forming galaxies at z>4
Y. Khusanova, M. Béthermin, O. Le Fèvre +30
Star formation rate (SFR) measurements at z>4 have relied mostly on rest-frame far-ultraviolet (FUV) observations. The corrections for dust attenuation based on IRX- relation ar…
The ALPINE-ALMA [C II] survey: the luminosity function of serendipitous [C II] line emitters at
Federica Loiacono, Roberto Decarli, Carlotta Gruppioni +32
We present the first [CII] 158 m luminosity function (LF) at from a sample of serendipitous lines detected in the ALMA Large Program to INvestigate [CII] at Early time…
The ALPINE-ALMA [CII] Survey: The nature, luminosity function and star formation history of dusty galaxies up to z~6
C. Gruppioni, M. Bethermin, F. Loiacono +30
We present the detailed characterisation of a sample of 56 sources serendipitously detected in ALMA band 7, as part of the ALMA Large Program to INvestigate CII at Early Times (ALP…
The ALPINE-ALMA [CII] survey: Molecular gas budget in the Early Universe as traced by [CII]
M. Dessauges-Zavadsky, M. Ginolfi, F. Pozzi +32
The molecular gas content of normal galaxies at z>4 is poorly constrained, because the commonly used molecular gas tracers become hard to detect. We use the [CII]158um luminosity,…
The ALPINE-ALMA [CII] survey: Dust attenuation properties and obscured star formation at z~4.4-5.8
Yoshinobu Fudamoto, P. A. Oesch, A. Faisst +34
We present dust attenuation properties of spectroscopically confirmed star forming galaxies on the main sequence at a redshift of ~4.4-5.8. Our analyses are based on the far infrar…
The ALPINE-ALMA [CII] Survey: Size of Individual Star-Forming Galaxies at z=4-6 and their Extended Halo Structure
S. Fujimoto, J. D. Silverman, Matthieu Bethermin +31
We present the physical extent of [CII] 158um line-emitting gas from 46 star-forming galaxies at z=4-6 from the ALMA Large Program to INvestigate CII at Early Times (ALPINE). Using…
The ALPINE-ALMA [CII] Survey: On the nature of an extremely obscured serendipitous galaxy
Michael Romano, P. Cassata, L. Morselli +31
We report the serendipitous discovery of a bright galaxy (Gal-A) observed as part of the ALMA Large Program to INvestigate [CII] at Early times (ALPINE). While this galaxy is detec…
The ALPINE-ALMA [CII] survey. Little to no evolution in the [CII]-SFR relation over the last 13 Gyr
D. Schaerer, M. Ginolfi, M. Bethermin +34
The [CII] 158 micron line is one of the strongest IR emission lines, which has been shown to trace the star-formation rate (SFR) of galaxies in the nearby Universe and up to $z \si…
The ALPINE-ALMA [CII] survey: Small Lya-[CII] velocity offsets in main-sequence galaxies at 4.4 < z < 6
P. Cassata, L. Morselli, A. Faisst +30
The Lya line in the UV and the [CII] line in the FIR are widely used tools to identify galaxies and to obtain insights into ISM properties in the early Universe. By combining data…
The ALPINE-ALMA [CII] Survey: data processing, catalogs, and statistical source properties
M. Bethermin, Y. Fudamoto, M. Ginolfi +33
The ALPINE-ALMA large program targets the [CII] 158 m line and the far-infrared continuum in 118 spectroscopically confirmed star-forming galaxies between z=4.4 and z=5.9. It re…