tokens: and rest-frame UV spectra for each of the ALPINE galaxies are shown in Appendix B . Throughout the paper, we assume the ΛCDM cosmology with , Ω Λ = 0.70, and Ω m = 0.30. All magnitudes are given in the AB system (Oke 1974 ) and stellar masses and SFRs are normalized to a Chabrier ( 2003 ) initial mass function (IMF). 2. Spectroscopic Data and Selection 2.1. Spectroscopic Selection of ALPINE Galaxies The ALPINE survey is only possible due to a spectroscopic pre-selection of galaxies from large spectroscopic surveys on COSMOS and ECDFS. This is because the ALMA frequency bands are narrow (), and in order to observe [] emission, the redshift has to be known within a precision of . The galaxy selection is refined to optimize the efficiency of the ALMA observations by creating groups of galaxies in spectral dimensions. Our sample also includes seven galaxies that were previously observed with ALMA by Riechers et al. ( 2014 ) and Capak et al. ( 2015 ). These are HZ1 , HZ2 , HZ3 , HZ4 , HZ5 , HZ6 / LBG-1 , and HZ8 , which correspond to the ALPINE galaxies DC _ 536534 , DC _ 417567 , DC _ 683613 , DC _ 494057 , DC _ 845652 , DC _ 848185 , and DC _ 873321 , respectively. Furthermore, four galaxies from the VUDS survey ( vc _ 5101288969 , vc _ 5100822662 , and vc _ 510786441 in COSMOS and ve _ 530029038 in ECDFS) are observed twice (resulting in a total number of 122 observations). The duplicate observations are used for quality assessment. Bethermin et al. ( 2020 ) describes the combination of these observations. The rest-frame UV spectroscopic data from which the ALPINE sample is selected combine various large surveys on the COSMOS and ECDFS fields. Out of the 105 ALPINE galaxies on the COSMOS field, 84 are obtained by the large DEIMOS spectroscopic survey (Capak et al. 2004 ; Mallery et al. 2012 ; Hasinger et al. 2018 ) at the Keck telescope in Hawaii. The remaining spectra on the COSMOS field are obtained from the VIMOS Ultra Deep Survey (VUDS; Le Fèvre et al. 2015 ; Tasca et al. 2017 ) at the VLT in Chile. In total, six of the VUDS spectra are independently also observed as part of the Keck/DEIMOS survey ( vc _ 5100559223 , vc _ 5100822662 , vc _ 5101218326 , vc _ 5101244930 , vc _ 5101288969 , vc _ 510786441 ). The redshifts are consistent within , and we do not find any systematic offsets between the two observations (see also Section 2.4.1 ). Out of the 13 galaxies in the ECDFS field, 11 are obtained from spectroscopic observations with VIMOS (9) and FORS2 (2 29 29 One of these galaxies, ve _ 530029038 , has also been observed by the VUDS survey. ) at the VLT (Vanzella et al. 2007 , 2008 ; Balestra et al. 2010 ), and two come from the HST grism survey GRAPES (Malhotra et al. 2005 ; Rhoads et al. 2009 ). The spectral resolution of the different data set varies between R ∼ 100 (ECDFS/ GRAPES grism), R ∼ 180 (ECDFS/VIMOS), R ∼ 230 (COSMOS/VUDS), R ∼ 660 (ECDFS/FORS2), and R ∼ 2500 (COSMOS/DEIMOS). Biases toward dust-poor star-forming galaxies
ner_tags: O O B-Wavelength O O O O O B-Survey O O O O O O O O O O O O O B-Model I-Model O O B-Formula I-Formula I-Formula I-Formula O B-Formula I-Formula I-Formula I-Formula O O O O O O O O B-Citation I-Citation O O O O O O O O O O B-Citation I-Citation I-Citation I-Citation B-Model I-Model I-Model B-Model O O O O O O O O O B-Survey O O B-Survey I-Survey O O O O O O O O O O O O O O O B-CelestialRegion O B-CelestialRegion O O O O B-Observatory O O O O B-TextGarbage O O O O O B-TextGarbage O O O O O O O O O O O O O O O O O O O O O O O B-Observatory O O O O O O O O O O O O O O O O O O O O B-Observatory O B-Citation I-Citation I-Citation I-Citation I-Citation I-Citation O B-Citation I-Citation I-Citation I-Citation I-Citation I-Citation O O B-CelestialObject O B-CelestialObject O B-CelestialObject O B-CelestialObject O B-CelestialObject O B-CelestialObject I-CelestialObject I-CelestialObject O O B-CelestialObject O O O O O B-Survey O B-CelestialObject I-CelestialObject I-CelestialObject O B-CelestialObject I-CelestialObject I-CelestialObject O B-CelestialObject I-CelestialObject I-CelestialObject O B-CelestialObject I-CelestialObject I-CelestialObject O B-CelestialObject I-CelestialObject I-CelestialObject O B-CelestialObject I-CelestialObject I-CelestialObject O O B-CelestialObject I-CelestialObject I-CelestialObject O O O O O O O B-Survey I-Survey O B-CelestialObject I-CelestialObject I-CelestialObject O B-CelestialObject I-CelestialObject I-CelestialObject O O B-CelestialObject I-CelestialObject I-CelestialObject O B-CelestialRegion O B-CelestialObject I-CelestialObject I-CelestialObject O B-CelestialRegion O O O O O O O O O O O O O O O O O O O B-Citation I-Citation I-Citation I-Citation I-Citation I-Citation O O O O O O O O B-Wavelength O O O O O B-Survey O O O O O O O O O B-CelestialRegion O B-CelestialRegion I-CelestialRegion O O O O B-Survey O O O B-CelestialRegion I-CelestialRegion O O O O O O B-Survey O O B-Citation I-Citation I-Citation I-Citation O B-Citation I-Citation I-Citation I-Citation O B-Citation I-Citation I-Citation I-Citation O O O B-Telescope I-Telescope O B-Location O O O O O B-CelestialRegion I-CelestialRegion O O O O B-Survey I-Survey I-Survey I-Survey B-Survey B-Citation I-Citation I-Citation I-Citation I-Citation O B-Citation I-Citation I-Citation I-Citation O O O B-Telescope O B-Location O O O O O B-Survey O O O O O O O O O B-Survey I-Survey O B-CelestialObject I-CelestialObject I-CelestialObject O B-CelestialObject I-CelestialObject I-CelestialObject O B-CelestialObject I-CelestialObject I-CelestialObject O B-CelestialObject I-CelestialObject I-CelestialObject O B-CelestialObject I-CelestialObject I-CelestialObject O B-CelestialObject I-CelestialObject I-CelestialObject O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O O B-CelestialRegion I-CelestialRegion O O O O O O O B-Instrument O O B-Instrument O O O O O O O B-CelestialObject I-CelestialObject I-CelestialObject O O O O O O O B-Survey I-Survey O O O B-Telescope B-Citation I-Citation I-Citation I-Citation O B-Citation O B-Citation I-Citation I-Citation I-Citation O O O O O O B-Telescope B-Instrument O B-Survey B-Citation I-Citation I-Citation I-Citation O B-Citation I-Citation I-Citation I-Citation O O O O O O O O O O O B-Formula I-Formula I-Formula B-CelestialRegion B-Survey O B-Formula I-Formula I-Formula B-CelestialRegion B-Formula I-Formula I-Formula B-CelestialRegion B-Formula I-Formula I-Formula B-CelestialRegion O B-Formula I-Formula I-Formula B-CelestialObject O O O O O