SPT 0538–50: Physical Conditions in the Interstellar Medium of a Strongly Lensed Dusty Star-forming Galaxy at z = 2.8

• Published in: The Astrophysical Journal
• Main Authors: Bothwell, M. S., Vieira, J. D., Bock, J. J., Downes, T. P.
• Format: Article in Journal/Newspaper
• Language: English
• Published: American Astronomical Society 2013
• Subjects: Hubble; South Pole; South pole
• Online Access: https://authors.library.caltech.edu/43440/; https://authors.library.caltech.edu/43440/1/0004-637X_779_1_67.pdf; https://authors.library.caltech.edu/43440/7/1309.3275v1.pdf; https://resolver.caltech.edu/CaltechAUTHORS:20140121-072415768

We present observations of SPT-S J053816–5030.8, a gravitationally lensed dusty star-forming galaxy (DSFG) at z = 2.7817 that was first discovered at millimeter wavelengths by the South Pole Telescope. SPT 0538–50 is typical of the brightest sources found by wide-field millimeter-wavelength surveys, being lensed by an intervening galaxy at moderate redshift (in this instance, at z = 0.441). We present a wide array of multi-wavelength spectroscopic and photometric data on SPT 0538–50, including data from ALMA, Herschel PACS and SPIRE, Hubble, Spitzer, the Very Large Telescope, ATCA, APEX, and the Submillimeter Array. We use high-resolution imaging from the Hubble Space Telescope to de-blend SPT 0538–50, separating DSFG emission from that of the foreground lens. Combined with a source model derived from ALMA imaging (which suggests a magnification factor of 21 ± 4), we derive the intrinsic properties of SPT 0538–50, including the stellar mass, far-IR luminosity, star formation rate, molecular gas mass, and—using molecular line fluxes—the excitation conditions within the interstellar medium. The derived physical properties argue that we are witnessing compact, merger-driven star formation in SPT 0538–50 similar to local starburst galaxies and unlike that seen in some other DSFGs at this epoch.