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The VIMOS Ultra Deep Survey: The reversal of the star-formation rate density relation at
B. C. Lemaux, O. Cucciati, O. Le Fèvre +28
Utilizing spectroscopic observations taken for the VIMOS Ultra-Deep Survey (VUDS), new observations from Keck/DEIMOS, and publicly available observations of large samples of star-f…
Co-evolution of black hole accretion and star formation in galaxies up to z=3.5
R. Carraro, G. Rodighiero, P. Cassata +15
We study the co-evolution between the black hole accretion rate (BHAR) and the star formation rate (SFR) in different galaxy life phases: main sequence star-forming galaxies, quies…
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 VIMOS Ultra-Deep Survey: the Ly emission line morphology at
B. Ribeiro, O. Le Fèvre, A. Paulino-Afonso +20
The Lyman- (Ly) emission line has been ubiquitously used to confirm and study high redshift galaxies. We report on the line morphology as seen in the 2D spectra from the VIMO…
VALES VI: ISM enrichment in star-forming galaxies up to z0.2 using CO(1-0), CO(1-0) and CO(1-0) line luminosity ratios
H. Méndez-Hernández, E. Ibar, K. K. Knudsen +10
We present Atacama Large Millimeter/sub-millimeter Array (ALMA) observations towards 27 low-redshift () star-forming galaxies taken from the Valparaíso ALMA/APEX Line…
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…