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Panchromatic study of the first galaxies with large ALMA programs

Published online by Cambridge University Press:  10 June 2020

A. Faisst Open the ORCID record for A. Faisst [Opens in a new window] ,
M. Béthermin ,
P. Capak ,
P. Cassata ,
O. Le Fèvre ,
D. Schaerer ,
J. Silverman ,
L. Yan  and
the ALPINE team
A. Faisst
Affiliation:
IPAC, California Institute of Technology, 1200 East California Boulevard, Pasadena, CA91125, USA email: afaisst@ipac.caltech.edu
M. Béthermin
Affiliation:
Laboratoire d’Astrophysique de Marseille UMR 7326, 13388, Marseille, France
P. Capak
Affiliation:
IPAC, California Institute of Technology, 1200 East California Boulevard, Pasadena, CA91125, USA email: afaisst@ipac.caltech.edu
P. Cassata
Affiliation:
University of Padova, Department of Physics and Astronomy Vicolo Osservatorio 3, 35122, Padova, Italy
O. Le Fèvre
Affiliation:
Laboratoire d’Astrophysique de Marseille UMR 7326, 13388, Marseille, France
D. Schaerer
Affiliation:
Observatoire de Genève, Université de Genève 51 Ch. des Maillettes, 1290 Versoix, Switzerland
J. Silverman
Affiliation:
Kavli Institute for the Physics and Mathematics of the Universe, The University of TokyoKashiwa, Chiba 277-8583, Japan
L. Yan
Affiliation:
IPAC, California Institute of Technology, 1200 East California Boulevard, Pasadena, CA91125, USA email: afaisst@ipac.caltech.edu Caltech Optical Observatories, Cahill Center for Astronomy and Astrophysics 1200 East California Boulevard, Pasadena, CA91125, USA
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Abstract

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Thanks to deep optical to near-IR imaging and spectroscopy, significant progress is made in characterizing the rest-frame UV to optical properties of galaxies in the early universe (z > 4. Surveys with Hubble, Spitzer, and ground-based facilities (Keck, Subaru, and VLT) provide spectroscopic and photometric redshifts, measurements of the spatial structure, stellar masses, and optical emission lines for large samples of galaxies. Recently, the Atacama Large (Sub) Millimeter Array (ALMA) has become a major player in pushing studies of high redshift galaxies to far-infrared wavelengths, hence making panchromatic surveys over many orders of frequencies possible. While past studies focused mostly on bright sub-millimeter galaxies, the sensitivity of ALMA now enables surveys like ALPINE, which focuses on measuring the gas and dust properties of a large sample of normal main-sequence galaxies at z > 4. Combining observations across different wavelengths into a single, panchromatic picture of galaxy formation and evolution is currently and in the future an important focus of the astronomical community.

Keywords

Galaxy: formationGalaxy: evolutiongalaxies: ISMdustextinctionISM: evolutionISM: kinematics and dynamicsISM: evolutioninfrared: galaxiessurveys
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 15 , Symposium S341: Challenges in Panchromatic Modelling with Next Generation Facilities , November 2019 , pp. 12 - 16
Copyright
© International Astronomical Union 2020

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