CaltechAUTHORS
  A Caltech Library Service

Panchromatic Study of the First Galaxies with Large ALMA Programs

Faisst, A. and Béthermin, M. and Capak, P. and Cassata, P. and LeFevre, O. and Schaerer, D. and Silverman, J. and Yan, L. (2019) Panchromatic Study of the First Galaxies with Large ALMA Programs. In: Challenges in Panchromatic Modelling with Next Generation Facilities. IAU Symposium Proceedings Series. Vol.15. No.341. Cambridge University Press , Cambridge, pp. 12-16. ISBN 9781108471473. https://resolver.caltech.edu/CaltechAUTHORS:20190813-092455553

[img] PDF - Published Version
See Usage Policy.

1221Kb
[img] PDF - Submitted Version
See Usage Policy.

1519Kb

Use this Persistent URL to link to this item: https://resolver.caltech.edu/CaltechAUTHORS:20190813-092455553

Abstract

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.


Item Type:Book Section
Related URLs:
URLURL TypeDescription
https://doi.org/10.1017/S1743921319001881DOIArticle
https://arxiv.org/abs/1901.01268arXivDiscussion Paper
ORCID:
AuthorORCID
Faisst, A.0000-0002-9382-9832
Béthermin, M.0000-0002-3915-2015
Capak, P.0000-0003-3578-6843
LeFevre, O.0000-0001-5891-2596
Schaerer, D.0000-0001-7144-7182
Silverman, J.0000-0002-0000-6977
Yan, L.0000-0003-1710-9339
Additional Information:© 2020 International Astronomical Union.
Group:Infrared Processing and Analysis Center (IPAC)
Subject Keywords:Galaxy: formation, Galaxy: evolution, galaxies: ISM, dust, extinction, ISM: evolution, ISM: kinematics and dynamics, ISM: evolution, infrared: galaxies, surveys
Series Name:IAU Symposium Proceedings Series
Issue or Number:341
Record Number:CaltechAUTHORS:20190813-092455553
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20190813-092455553
Official Citation:Faisst, A., Béthermin, M., Capak, P., Cassata, P., Le Fèvre, O., Schaerer, D., . . . Yan, L. (2019). Panchromatic study of the first galaxies with large ALMA programs. Proceedings of the International Astronomical Union, 15(S341), 12-16. doi:10.1017/S1743921319001881
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:97856
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:13 Aug 2019 18:42
Last Modified:24 Jun 2020 19:54

Repository Staff Only: item control page