VALES I: the molecular gas content in star-forming dusty H-ATLAS galaxies up to z = 0.35
We present an extragalactic survey using observations from the Atacama Large Millimeter/submillimeter Array (ALMA) to characterize galaxy populations up to z = 0.35: the Valparaíso ALMA Line Emission Survey (VALES). We use ALMA Band-3 CO(1-0) observations to study the molecular gas content in a sample of 67 dusty normal star-forming galaxies
Villanueva, V. et al.
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10
2017