THE REDSHIFT DISTRIBUTION OF DUSTY STAR-FORMING GALAXIES FROM THE SPT SURVEY
We use the Atacama Large Millimeter/submillimeter Array (ALMA) in Cycle 1 to determine spectroscopic redshifts of high-redshift dusty star-forming galaxies (DSFGs) selected by their 1.4 mm continuum emission in the South Pole Telescope (SPT) survey. We present ALMA 3 mm spectral scans between 84 and...
Main Authors: | , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , |
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Language: | en |
Published: |
IOP PUBLISHING LTD
2016
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Online Access: | http://hdl.handle.net/10150/621235 http://arizona.openrepository.com/arizona/handle/10150/621235 |