The alpine-alma [cii] survey : multiwavelength ancillary data and basic physical measurements

Faisst, A. L.; Schaerer, D.; Schaerer, D.; Lemaux, B. C.; Oesch, P. A.; Fudamoto, Y.; Cassata, P.; Cassata, P.; Bethermin, M.; Capak, P. L.; Capak, P. L.; Capak, P. L.; Fevre, O. L.; Silverman, J. D.; Silverman, J. D.; Yan, L.; Ginolfi, M.; Koekemoer, A. M.; Morselli, L.; Morselli, L.; Amorin, R.; Amorin, R.; Bardelli, S.; Boquien, M.; Brammer, G.; Cimatti, A.; Dessauges-Zavadsky, M.; Fujimoto, S.; Fujimoto, S.; Gruppioni, C.; Hathi, N. P.; Hemmati, S.; Ibar, E.; Jones, G. C.; Jones, G. C.; Khusanova, Y.; Khusanova, Y.; Loiacono, F.; Loiacono, F.; Pozzi, F.; Talia, M.; Talia, M.; Tasca, L. A. M.; Riechers, D. A.; Riechers, D. A.; Riechers, D. A.; Rodighiero, G.; Rodighiero, G.; Romano, M.; Scoville, N.; Scoville, N.; Toft, S.; Toft, S.; Vallini, L.; Vergani, D.; Zamorani, G.; Zucca, E.

doi:10.3847/1538-4365/ab7ccd

We present the ancillary data and basic physical measurements for the galaxies in the ALMA Large Program to Investigate C+ at Early Times (ALPINE) survey-the first large multiwavelength survey that aims at characterizing the gas and dust properties of 118 main-sequence galaxies at redshifts 4.4?3.5σ) and the surrounding far-infrared continuum in conjunction with a wealth of optical and near-infrared data. We outline in detail the spectroscopic data and selection of the galaxies as well as the ground- A nd space-based imaging products. In addition, we provide several basic measurements including stellar masses, star formation rates (SFR), rest-frame ultra-violet (UV) luminosities, UV continuum slopes (β), and absorption line redshifts, as well as Hα?emission derived from Spitzer colors. We find that the ALPINE sample is representative of the 4?

The alpine-alma [cii] survey : multiwavelength ancillary data and basic physical measurements

Faisst A. L.;Schaerer D.;Schaerer D.;Lemaux B. C.;Oesch P. A.;Fudamoto Y.;Cassata P.;Cassata P.;Bethermin M.;Capak P. L.;Capak P. L.;Capak P. L.;Fevre O. L.;Silverman J. D.;Silverman J. D.;Yan L.;Ginolfi M.;Koekemoer A. M.;Morselli L.;Morselli L.;Amorin R.;Amorin R.;Bardelli S.;Boquien M.;Brammer G.;Cimatti A.;Dessauges-Zavadsky M.;Fujimoto S.;Fujimoto S.;Gruppioni C.;Hathi N. P.;Hemmati S.;Ibar E.;Jones G. C.;Jones G. C.;Khusanova Y.;Khusanova Y.;Loiacono F.;Loiacono F.;Pozzi F.;Talia M.;Talia M.;Tasca L. A. M.;Riechers D. A.;Riechers D. A.;Riechers D. A.;Rodighiero G.;Rodighiero G.;Romano M.;Scoville N.;Scoville N.;Toft S.;Toft S.;Vallini L.;Vergani D.;Zamorani G.;Zucca E.

2020

Abstract

We present the ancillary data and basic physical measurements for the galaxies in the ALMA Large Program to Investigate C+ at Early Times (ALPINE) survey-the first large multiwavelength survey that aims at characterizing the gas and dust properties of 118 main-sequence galaxies at redshifts 4.4?3.5σ) and the surrounding far-infrared continuum in conjunction with a wealth of optical and near-infrared data. We outline in detail the spectroscopic data and selection of the galaxies as well as the ground- A nd space-based imaging products. In addition, we provide several basic measurements including stellar masses, star formation rates (SFR), rest-frame ultra-violet (UV) luminosities, UV continuum slopes (β), and absorption line redshifts, as well as Hα?emission derived from Spitzer colors. We find that the ALPINE sample is representative of the 4?

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	Anno di pubblicazione
	
				2020
			
	Settore Scientifico Disciplinare (validi fino a 24/06/2024)
	
				Settore FIS/05 - Astronomia e Astrofisica
			
	Titolo Rivista
	
				ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES
			
	DOI
	
				https://dx.doi.org/10.3847/1538-4365/ab7ccd
			
	Parole chiave
	
				Galaxy evolution; Galactic and extragalactic astronomy; Interstellar medium; Star formation; Galaxy photometry; Stellar masses; Interstellar
medium wind; Galaxy winds; Galaxy processes; Stellar winds; Far infrared astronomy
			
	Progetti che finanziano la ricerca
	
	Finanziamento
	
									Horizon 2020
								
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				1.1 Articolo in rivista

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