Browsing by Author "De Breuck, C."

Now showing 1 - 5 of 5
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    A. survey of the cold molecular gas in gravitationally lensed star-forming galaxies at z > 2
    (2016) Aravena, M.; Spilker, J.; Bethermin, M.; Bothwell, M.; Chapman, S.; De Breuck, C.; Furstenau, R.; González López, Jorge; Greve, T.; Litke, K.; Ma, J.; Malkan, M.; Marrone, D.; Murphy, E.; Stark, A.; Strandet, M.; Vieira, J.; Weiss, A.; Welikala, N.; Wong, G.; Collier, J.
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    Rapidly growing black holes and host galaxies in the distant Universe from the Herschel Radio Galaxy Evolution Project
    (2014) Bauer, Franz Erik; Ibar, E.; Drouart, G.; De Breuck, C.; Vernet, J.; Seymour, N.; Lehnert, M.; Barthel, P.
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    SPT 0538-50: PHYSICAL CONDITIONS IN THE INTERSTELLAR MEDIUM OF A STRONGLY LENSED DUSTY STAR-FORMING GALAXY AT z=2.8
    (2013) Bothwell, M. S.; Aguirre, J. E.; Chapman, S. C.; Marrone, D. P.; Vieira, J. D.; Ashby, M. L. N.; Aravena, M.; Benson, B. A.; Bock, J. J.; Bradford, C. M.; Brodwin, M.; Carlstrom, J. E.; Crawford, T. M.; De Breuck, C.; Downes, T. P.; Fassnacht, C. D.; Gonzalez, A. H.; Greve, T. R.; Gullberg, B.; Hezaveh, Y.; Holder, G. P.; Holzapfel, W. L.; Ibar, E.; Ivison, R.; Kamenetzky, J.; Keisler, R.; Lupu, R. E.; Ma, J.; Malkan, M.; McIntyre, V.; Murphy, E. J.; Nguyen, H. T.; Reichardt, C. L.; Rosenman, M.; Spilker, J. S.; Stalder, B.; Stark, A. A.; Strandet, M.; Vernet, J.; Weiss, A.; Welikala, N.
    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 arewitnessing 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.
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    Sub-kiloparsec imaging of cool molecular gas in two strongly lensed dusty
    (2015) Spilker, J. S.; Aravena, M.; Marrone, D. P.; Bethermin, M.; Bothwell, M. S.; Carlstrom, J. E.; Chapman, S. C.; Collier, J. D.; De Breuck, C.; González López, Jorge
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    Vlt Spectroscopy of the Z=4.11 Radio Galaxy Tn J1338-1942
    (1999) De Breuck, C.; Minniti, D.