UV/Optical Spectroscopy of Submillimeter Galaxies

Details UV/Optical Spectroscopy of Submillimeter Galaxies UV/Optical Spectroscopy of Submillimeter Galaxies

Oct 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aspc..375..130c&link_type=abstract

From Z-Machines to ALMA: (Sub)Millimeter Spectroscopy of Galaxies ASP Conference Series, Vol. 375, proceedings of the conference

Astronomy and Astrophysics

Astronomy

Scientific paper

We summarize the astrophysical properties of the submillimeter galaxy population gleaned from our optical and near-IR spectroscopic surveys of radio-identified SCUBA galaxies. Precise redshift information allows basic evolutionary properties to be measured, but also facilitates a large range of ancilliary science, including clustering and comparisons with the inter-galactic medium, and detection of CO molecular gas. We demonstrate that the rest-frame UV offers rich astrophysical diagnostics both from individual spectra (AGN characterization and wind outflows) and from stacked spectra of SMGs in different classes (UV-bright and faint starbursts, and type 2 AGN).

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