Massive and dusty Hα emitters in protocluster revealed by ALMA and JVLA
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).
- Publication:
-
Galaxies at High Redshift and Their Evolution Over Cosmic Time
- Pub Date:
- 2016
- DOI:
- 10.1017/S1743921315010236
- Bibcode:
- 2016IAUS..319...96L
- Keywords:
-
- galaxies: evolution-galaxies: structure-galaxies: high-redshift-radio continuum: galaxies-submillimeter