Browsing by Author "De Zotti, G."

Now showing items 1-10 of 10

    • Blind detections of CO J=1-0 IN 11 H-ATLAS Galaxies at z=2.1-3.5 with the GBT/Zpectrometer 

      Harris, A.I.; Baker, A. J.; Frayer, D. T.; Smail, Ian; Swinbank, A.M.; Riechers, D. A.; van der Werf, P. P.; Auld, R.; Baes, M.; Bussmann, R. S.; Buttiglione, S.; Cava, A.; Clements, D. L.; Cooray, A.; Dannerbauer, H.; Dariush, A.; De Zotti, G.; Dunne, L.; Dye, S.; Eales, S.; Fritz, J.; Gonzalez-Nuevo, J.; Hopwood, R.; Ibar, E.; Ivison, R. J.; Jarvis, M.J.; Maddox, S.; Negrello, M.; Rigby, E.; Smith, Daniel; Temi, P.; Wardlow, J. (2012-06-20)
      We report measurements of the carbon monoxide ground state rotational transition ((CO)-C-12-O-16 J = 1-0) with the Zpectrometer ultrawideband spectrometer on the 100 m diameter Green Bank Telescope. The sample comprises ...

    • A comprehensive view of a strongly lensed planck-associated submillimeter galaxy 

      Fu, Hai; Jullo, E.; Cooray, A.; Bussmann, R. S.; Ivison, R. J.; Perez-Fournon, I.; Djorgovski, S.G.; Scoville, N.; Yan, L.; Riechers, D. A.; Aguirre, J.; Auld, R.; Baes, M.; Baker, A. J.; Bradford, M.; Cava, A.; Clements, D. L.; Dannerbauer, H.; Dariush, A.; De Zotti, G.; Dole, H.; Dunne, L.; Dye, S.; Eales, S.; Frayer, D.; Gavazzi, R.; Gurwell, M.; Harris, A.I.; Herranz, D.; Hopwood, R.; Hoyos, C.; Ibar, E.; Jarvis, M.J.; Kim, S.; Leeuw, L.; Lupu, R.; Maddox, S.; Martinez-Navajas, P.; Michalowski, M. J.; Negrello, M.; Omont, A.; Rosenman, M.; Scott, D.; Serjeant, S.; Smail, I.; Swinbank, A.M.; Valiante, E.; Verma, A.; Vieira, J.; Wardlow, J. L.; van der Werf, P. (2012-07-10)
      We present high-resolution maps of stars, dust, and molecular gas in a strongly lensed submillimeter galaxy (SMG) at z = 3.259. HATLAS J114637.9-001132 is selected from the Herschel-Astrophysical Terahertz Large Area Survey ...

    • A Detailed Gravitational Lens Model Based on Submillimeter Array and Keck Adaptive Optics Imaging of a Herschel-ATLAS Sub-millimeter Galaxy at z=4.243 

      S. Bussmann, R.; A. Gurwell, M.; Fu, Hai; Smith, Daniel; Dye, S.; Auld, R.; Baes, M.; J. Baker, A.; Bonfield, D.; Cava, A.; L. Clements, D.; Cooray, A.; Coppin, Kristen; Dannerbauer, H.; Dariush, A.; De Zotti, G.; Dunne, L.; Eales, S.; Fritz, J.; Hopwood, R.; Ibar, E.; J. Ivison, R.; Jarvis, M.J.; Kim, S.; L. Leeuw, L.; Maddox, S.; J. Michalowski, M.; Negrello, M.; Pascale, E.; Pohlen, M.; A. Riechers, D.; Rigby, E.; Scott, Douglas; Temi, P.; P. Van der Werf, P.; Verma, A.; Wardlow, J.; Wilner, D. (2012-09-10)
      We present high-spatial resolution imaging obtained with the Submillimeter Array (SMA) at 880 μm and the Keck Adaptive Optics (AO) system at KS-band of a gravitationally lensed sub-millimeter galaxy (SMG) at z = 4.243 ...

    • Far-infrared observations of an unbiased sample of gamma-ray burst host galaxies 

      Kohn, S.A.; Michalowski, M. J.; Bourne, N.; Baes, M.; Fritz, J.; Cooray, A.; De Looze, I.; De Zotti, G.; Dannerbauer, H.; Dunne, L.; Dye, S.; Eales, S.; Furlanetto, C.; Gonzalez-Nuevo, J.; Ibar, E.; Ivison, Rob J.; Maddox, S.J.; Scott, D.; Smith, Daniel; Smith, M.W.L.; Symeonidis, M.; Valiante, E. (2015-04-01)
      Gamma-ray bursts (GRBs) are the most energetic phenomena in the Universe; believed to result from the collapse and subsequent explosion of massive stars. Even though it has profound consequences for our understanding of ...

    • Herschel-Astrophysical Terahertz Large Area Survey: detection of a far-infrared population around galaxy clusters 

      Coppin, Kristen; Geach, James; Smail, Ian; Dunne, L.; Edge, A.C.; Ivison, R. J.; Maddox, S.; Auld, R.; Baes, M.; Buttiglione, S.; Cava, A.; Clements, D. L.; Cooray, A.; Dariush, A.; De Zotti, G.; Dye, S.; Eales, S.; Fritz, J.; Hopwood, R.; Ibar, E.; Jarvis, M.J.; Michalowski, M. J.; Murphy, D. N. A.; Negrello, M.; Pascale, E.; Pohlen, M.; Rigby, E.; Rodighiero, G.; Scott, D.; Serjeant, S.; Smith, Daniel; Temi, P.; van der Werf, P. (2011-09)
      We report the detection of a significant excess in the surface density of far-infrared sources from the Herschel-Astrophysical Terahertz Large Area Survey within similar to 1Mpc of the centres of 66 optically selected ...

    • Herschel-ATLAS : Multi-wavelength SEDs and physical properties of 250 μm selected galaxies at z <0.5 

      Smith, Daniel; Dunne, L.; Rowlands, K.; Maddox, S.J.; Bourne, N.; Dye, S.; Rigby, E.E.; Bonfield, D.G.; Jarvis, M.J.; da Cunha, E.; Eales, S.; Gomez, H.L.; Auld, R.; Dariush, A.; Pohlen, M.; Charlot, S.; Driver, S.P.; Kelvin, L.; Robotham, A.; Popescu, C.C.; Tuffs, R.J.; Andrae, E.; Dunlop, J.S.; Ivison, R.J.; Seymour, N.; Symeonidis, M.; Baes, M.; Fritz, J.; Clements, D.L.; Cooray, A.; De Zotti, G.; Buttiglione, S.; Scott, D.; Verma, A.; van der Werf, P.; Cava, A.; Hopwood, R.; Ibar, E.; Madore, B.F.; Seibert, M.; Temi, P. (2012-11-21)
      We present a pan-chromatic analysis of an unprecedented sample of 1402 250 μm selected galaxies at z < 0.5 (z-=0.24) from the Herschel-ATLAS survey. We complement our Herschel 100-500μm data with UV-K-band photometry from ...

    • Herschel-ATLAS : toward a sample of similar to 1000 strongly lensed galaxies 

      Gonzalez-Nuevo, J.; Lapi, A.; Fleuren, S.; Bressan, S.; Danese, L.; De Zotti, G.; Negrello, M.; Cai, Z. -Y.; Fan, L.; Sutherland, W.; Baes, M.; Baker, A. J.; Clements, L.; Cooray, A.; Dannerbauer, H.; Dunne, L.; Dye, S.; Eales, S.; Frayer, D. T.; Harris, A. I.; Ivison, R.; Jarvis, M.J.; Michallowski, M.J.; Lopez-Caniego, M.; Rodighiero, G.; Rowlands, K.; Serjeant, S.; Scott, D.; van der Werf, P.; Auld, R.; Buttiglione, S.; Cava, A.; Dariush, A.; Fritz, J.; Hopwood, R.; Ibar, E.; Maddox, S.; Pascale, E.; Pohlen, M.; Rigby, E.; Smith, Daniel; Temi, P. (2012-04-10)
      While the selection of strongly lensed galaxies (SLGs) with 500 mu m flux density S-500 > 100 mJy has proven to be rather straightforward, for many applications it is important to analyze samples larger than the ones ...

    • Herschel-ATLAS : VISTA VIKING near-infrared counterparts in the Phase 1 GAMA 9-h data 

      Fleuren, S.; Sutherland, W.; Dunne, L.; Smith, Daniel; Maddox, S. J.; Gonzalez-Nuevo, J.; Findlay, J.; Auld, R.; Baes, M.; Bond, N. A.; Bonfield, D. G.; Bourne, N.; Cooray, A.; Buttiglione, S.; Cava, A.; Dariush, A.; De Zotti, G.; Driver, S. P.; Dye, S.; Eales, S.; Fritz, J.; Gunawardhana, M. L. P.; Hopwood, R.; Ibar, E.; Ivison, R. J.; Jarvis, M.J.; Kelvin, L.; Lapi, A.; Liske, J.; Michalowski, M. J.; Negrello, M.; Pascale, E.; Pohlen, M.; Prescott, M.; Rigby, E. E.; Robotham, A.; Scott, D.; Temi, P.; Thompson, Mark; Valiante, E.; van der Werf, P. (2012-07)
      We identify near-infrared Ks-band counterparts to Herschel Astrophysical Terahertz Large Area Survey (H-ATLAS) submillimetre (submm) sources, using a preliminary object catalogue from the VISTA Kilo-degree Infrared Galaxy ...

    • Herschel-ATLAS/GAMA : the environmental density of far-infrared bright galaxies at z < 0.5 

      Burton, C. S.; Jarvis, M.J.; Smith, Daniel; Bonfield, D. G.; Hardcastle, M.J.; Stevens, J. A.; Bourne, N.; Baes, M.; Brough, S.; Cava, A.; Cooray, A.; Dariush, A.; De Zotti, G.; Dunne, L.; Eales, S.; Hopwood, R.; Ibar, E.; Ivison, R. J.; Liske, J.; Loveday, J.; Maddox, S. J.; Negrello, M.; Smith, M. W. L.; Valiante, E. (2013-07)
      We compare the environmental and star formation properties of far-infrared detected and non-far-infrared detected galaxies out to z similar to 0.5. Using optical spectroscopy and photometry from the Galaxy And Mass Assembly ...

    • Mining the Herschel-astrophysical terahertz large area survey : Submillimetre-selected blazars in equatorial fields 

      López-Caniego, M.; González-Nuevo, J.; Massardi, M.; Bonavera, L.; Herranz, D.; Negrello, M.; De Zotti, G.; Carrera, F. J.; Danese, L.; Fleuren, S.; Hardcastle, M.J.; Jarvis, M.J.; Klöckner, H. R.; Mauch, T.; Procopio, P.; Righini, S.; Sutherland, W.; Auld, R.; Baes, M.; Buttiglione, S.; Clark, C. J. R.; Cooray, A.; Dariush, A.; Dunne, L.; Dye, S.; Eales, S. (2013-04-11)
      The Herschel-Astrophysical Terahertz Large Area Survey (H-ATLAS) provides an unprecedented opportunity to search for blazars at sub-mm wavelengths. We cross-matched the Faint Images of the Radio Sky at Twenty-cm (FIRST) ...