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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
Abstract
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).
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- Copyright © International Astronomical Union 2016