Hostname: page-component-78c5997874-mlc7c Total loading time: 0 Render date: 2024-11-10T08:58:12.308Z Has data issue: false hasContentIssue false
  • English
  • Français

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
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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

References

Ando, M., Ohta, K., Iwata, I., Akiyama, M., Aoki, K., Tamura, N., et al. 2007, PASJ, 59, 717CrossRefGoogle Scholar
Bouwens, R. J., Illingworth, G. D., Franx, M., Chary, R.-R., Meurer, G. R., Conselice, C. J., Ford, H., Giavalisco, M., et al. 2009, ApJ, 705, 936CrossRefGoogle Scholar
Bouwens, R. J., Illingworth, G. D., Oesch, P. A., Trenti, M., Labbé, I., Bradley, L., Carollo, M., van Dokkum, P. G., et al. 2015, ApJ, 803, 3410.1088/0004-637X/803/1/34CrossRefGoogle Scholar
Capak, P. L., Carilli, C., Jones, G., Casey, C. M., Riechers, D., Sheth, K., Carollo, C. M., Ilbert, O., et al. 2015, Nature, 522, 455CrossRefGoogle Scholar
Dayal, P. & Ferrara, A. 2017, Physics Reports, 780, 1Google Scholar
Davidzon, I., Ilbert, O., Laigle, C., Coupon, J., McCracken, H. J., Delvecchio, I., Masters, D., Capak, P., et al. 2017, A&A, 605, A70Google Scholar
De Looze, I., Cormier, D., Lebouteiller, V., Madden, S., Baes, M., Bendo, G. J., Boquien, M., Boselli, A., et al. 2014, A&A, 568, A62Google Scholar
Faisst, A. L., Capak, P., Hsieh, B. C., Laigle, C., Salvato, M., Tasca, L., Cassata, P., Davidzon, I., et al. 2016, ApJ, 821, 12210.3847/0004-637X/821/2/122CrossRefGoogle Scholar
Faisst, A. L., Capak, P. L., Davidzon, I., Salvato, M., Laigle, C., Ilbert, O., Onodera, M., Hasinger, G., et al. 2016, ApJ, 822, 29CrossRefGoogle Scholar
Faisst, A. L., Capak, P. L., Yan, L., Pavesi, R., Riechers, D. A., Barišić, I., Cooke, K., Kartaltepe, J. S., et al. 2017, ApJ, 847, 21CrossRefGoogle Scholar
Förster Schreiber, N. M., Shapley, A. E., Erb, D. K., Genzel, R., Steidel, C. C., Bouché, N., Cresci, G., Davies, R., et al. 2011, ApJ, 731, 65CrossRefGoogle Scholar
Giacconi, R., Zirm, A., Wang, J., Rosati, P., Nonino, M., Tozzi, P., Gilli, R., Mainieri, V., et al. 2002, ApJS, 139, 369CrossRefGoogle Scholar
Hasinger, G., Capak, P., Salvato, M., Barger, A. J., Cowie, L. L., Faisst, A., Hemmati, S., Kakazu, Y., et al. 2018, ApJ, 858, 77CrossRefGoogle Scholar
Le Fèvre, O., Tasca, L. A. M., Cassata, P., Garilli, B., Le Brun, V., Maccagni, D., Pentericci, L., Thomas, R., et al. 2015, A&A, 576, A79Google Scholar
Madau, P. & Dickinson, M. 2014, ARAA, 52, 41510.1146/annurev-astro-081811-125615CrossRefGoogle Scholar
Maiolino, R., Nagao, T., Grazian, A., Cocchia, F., Marconi, A., Mannucci, F., Cimatti, A., et al. 2008, A&A, 488, 463Google Scholar
Riechers, D. A., Carilli, C. L., Capak, P. L., Scoville, N. Z., Smolčić, V., Schinnerer, E., Yun, M., Cox, P., et al. 2014, ApJ, 796, 84CrossRefGoogle Scholar
Scoville, N., Aussel, H., Brusa, M., Capak, P., Carollo, C. M., Elvis, M., Giavalisco, M., Guzzo, L., et al. 2007, ApJS, 172, 1CrossRefGoogle Scholar
Shibuya, T., Ouchi, M., Kubo, M. & Harikane, Y. 2016, ApJ, 821, 72CrossRefGoogle Scholar