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.; 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.; Romano, M.; Scoville, N.; Scoville, N.; Toft, S.; Toft, S.; Vallini, L.; 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.; 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.; Romano M.; Scoville N.; Scoville N.; Toft S.; Toft S.; Vallini L.; Vallini L.; Vergani D.; Zamorani G.; Zucca E.. - In: THE ASTROPHYSICAL JOURNAL. - ISSN 0004-637X. - ELETTRONICO. - 247:(2020), pp. 61.0-61.0. [10.3847/1538-4365/ab7ccd]