THE REDSHIFT DISTRIBUTION OF DUSTY STAR-FORMING GALAXIES FROM THE SPT SURVEY

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...

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Bibliographic Details
Main Authors: Strandet, M. L., Weiss, A., Vieira, J. D., de Breuck, C., Aguirre, J. E., Aravena, M., Ashby, M. L. N., Béthermin, M., Bradford, C. M., Carlstrom, J. E., Chapman, S. C., Crawford, T. M., Everett, W., Fassnacht, C. D., Furstenau, R. M., Gonzalez, A. H., Greve, T. R., Gullberg, B., Hezaveh, Y., Kamenetzky, J. R., Litke, K., Ma, J., Malkan, M., Marrone, D. P., Menten, K. M., Murphy, E. J., Nadolski, A., Rotermund, K. M., Spilker, J. S., Stark, A. A., Welikala, N.
Other Authors: Univ Arizona, Steward Observ
Language:en
Published: IOP PUBLISHING LTD 2016
Subjects:
cosmology: observations
early universe
galaxies: evolution
galaxies: high-redshift
ISM: molecules
Online Access:http://hdl.handle.net/10150/621235
http://arizona.openrepository.com/arizona/handle/10150/621235

Internet

http://hdl.handle.net/10150/621235
http://arizona.openrepository.com/arizona/handle/10150/621235

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