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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: [email protected] 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

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