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Massive and dusty Hα emitters in protocluster revealed by ALMA and JVLA

Published online by Cambridge University Press:  17 August 2016

Minju Lee  and
4C23.56 Protocluster team
Minju Lee
Affiliation:
Department of Astronomy, Graduate school of Science, The University of Tokyo, 7-3-1 Hongo, Bunkyo-ku, Tokyo 133-0033, Japan, email: minju.lee@nao.ac.jp National Astronomical Observatory of Japan, 2-21-1 Osawa, Mitaka, Tokyo 181-8588, Japan
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Abstract

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We investigate the physical properties of Hα emitters (HAEs) associated to the protocluster 4C23.56 at z ~ 2.5 using continuum observations at submm (270 GHz) and radio (3 GHz) frequencies with Atacama Large Mm/submm Array (ALMA) and K. Jansky Very Large Array (JVLA). For more details see Lee et al. (in prep).

Keywords

galaxies: evolution—galaxies: structure—galaxies: high-redshift—radio continuum: galaxies—submillimeter
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 11 , Symposium S319: Galaxies at High Redshift and Their Evolution Over Cosmic Time , August 2015 , pp. 96
Copyright
Copyright © International Astronomical Union 2016 

References

Knopp, G. P., & Chambers, K. C. 1997, ApJS, 109, 367 CrossRefGoogle Scholar
Kajisawa, M., Kodama, T., Tanaka, I., Yamada, T., & Bower, R. 2006, MNRAS, 371, 577 Google Scholar
Mayo, J. H., Vernet, J., De Breuck, C., et al. 2012, A&A, 539, A33 Google Scholar
Speagle, J. S., Steinhardt, C. L., Capak, P. L., & Silverman, J. D. 2014, ApJS, 214, 15 Google Scholar
Tanaka, I., Breuck, C. D., Kurk, J. D., et al. 2011, PASJ, 63, 415 Google Scholar