Now showing items 1-11 of 11

    • ACA [CI] observations of the starburst galaxy NGC 253 

      Krips, M.; Martín, S.; Sakamoto, K.; Aalto, S.; Bisbas, T.~G.; Bolatto, A.~D.; Downes, D.; Eckart, A.; Feruglio, C.; García-Burillo, S.; Geach, J.; Greve, T.~R.; König, S.; Matsushita, S.; Neri, R.; Offner, S.; Peck, A.~B.; Viti, S.; Wagg, J. (2016-08-01)
      Context. Carbon monoxide (CO) is widely used as a tracer of the molecular gas in almost all types of environments. However, several shortcomings of CO complicate usaging it as H2 tracer, such as its optical depth effects, ...
    • A Detailed Study of Gas and Star Formation in a Highly Magnified Lyman Break Galaxy at z=3.07 

      Coppin, Kristen; Swinbank, A.M.; Neri, R.; Cox, P.; Smail, Ian; Ellis, R. S.; Geach, J.E.; Siana, B.; Teplitz, H.; Dye, S.; Kneib, J-P.; Edge, A. C.; Richard, J. (2007-08)
      We report the detection of CO(3-2) emission from a bright, gravitationally lensed Lyman Break Galaxy, LBGJ213512.73-010143 (the 'Cosmic Eye'), at z=3.07 using the Plateau de Bure Interferometer. This is only the second ...
    • The detection of a population of submillimeter-bright, strongly lensed galaxies 

      Negrello, Mattia; Hopwood, R.; de Zotti, G.; Cooray, A.; Verma, A.; Bock, J.; Frayer, D. T.; Gurwell, M.A.; Omont, A.; Neri, R.; Dannerbauer, H.; Leeuw, L. L.; Barton, E.; Cooke, J.; Kim, S.; da Cunha, E.; Rodighiero, G.; Cox, P.; Bonfield, David G.; Jarvis, M.J.; Serjeant, S.; Ivison, R.J.; Dye, S.; Aretxaga, I.; Hughes, D.H.; Ibar, E.; Bertoldi, F.; Valtchanov, I.; Eales, S.; Dunne, L.; Driver, S. P.; Auld, R.; Buttiglione, S.; Cava, A.; Grady, C.A.; Clements, D. L.; Dariush, A.; Fritz, J.; Hill, D.; Hornbeck, J.B.; Kelvin, L.; Lagache, G.; Lopez-Caniego, M.; Gonzalez-Nuevo, J.; Maddox, S.; Pascale, E.; Pohlen, M.; Rigby, E. E.; Robotham, A.; Simpson, C.; Smith, Daniel; Temi, P.; Thompson, Mark; Woodgate, B.E.; York, D.G.; Aguirre, J.E.; Beelen, A.; Blain, A.; Baker, A.J.; Birkinshaw, M.; Blundell, R.; Bradford, C.M.; Burgarella, D.; Danese, L.; Dunlop, J. S.; Fleuren, S.; Glenn, J.; Harris, A.I.; Kamenetzky, J.; Lupu, R. E.; Maddalena, R. J.; Madore, B. F.; Maloney, P. R.; Matsuhara, H.; Michaowski, M. J.; Murphy, E. J.; Naylor, B.J.; Nguyen, H.; Popescu, C.; Rawlings, S.; Rigopoulou, D.; Scott, D.; Scott, K.S.; Seibert, M.; Smail, I.; Tuffs, R. J.; Vieira, J. D.; van der Werf, P. P.; Zmuidzinas, J. (2010)
      Gravitational lensing is a powerful astrophysical and cosmological probe and is particularly valuable at submillimeter wavelengths for the study of the statistical and individual properties of dusty star-forming galaxies. ...
    • Discovery of a multiply lensed submillimeter galaxy in early HerMES Herschel/SPIRE data 

      Conley, A.; Cooray, A.; Vieira, J.; Solares, E.A.G.; Kim, S.; Aguirre, J.E.; Amblard, A.; Auld, R.; Baker, A.J.; Beelen, A.; Blain, A.W.; Blundell, R.; Bock, J.; Bradford, C.M.; Bridge, C.; Brisbin, D.; Burgarella, D.; Carpenter, J.M.; Chanial, P.; Chapin, E.; Christopher, N.; Clements, D.; Cox, P.; Djorgovski, S.G.; Dowell, C.D.; Eales, S.; Earle, L.; Ellsworth-Bowers, T.P.; Farrah, D.; Franceschini, A.; Frayer, D.; Fu, H.; Gavazzi, R.; Glenn, J.; Griffin, M.; Gurwell, M.A.; Halpern, M.; Ibar, E.; Ivison, R.J.; Jarvis, M.J.; Kamenetzky, J.; Krips, M.; Levenson, L.; Lupu, R.; Mahabal, A.; Maloney, P.D.; Maraston, C.; Marchetti, L.; Marsden, G.; Matsuhara, H.; Mortier, A.M.J.; Murphy, E.; Naylor, B.J.; Neri, R.; Nguyen, H.T.; Oliver, S.; Omont, A.; Page, M.J.; Papageorgiou, A.; Pearson, C.; Perez-Fournon, I.; Pohlen, M.; Rangwala, N.; Rawlings, J.I.; Raymond, G.; Riechers, D.; Rodighiero, G.; Roseboom, I.G.; Rowan-Robinson, M.; Schulz, B.; Scott, D.; Scott, K.; Serra, P.; Seymour, N.; Shupe, D.; Smith, A.J.; Symeonidis, M.; Tugwell, K.E.; Vaccari, M.; Valiante, E.; Valtchanov, I.; Verma, A.; Viero, M.P.; Vigroux, L.; Wang, L.; Wiebe, D.; Wright, G.; Xu, C.K.; Zeimann, G.; Zemcov, M.; Zmuidzinas, J. (2011)
      We report the discovery of a bright (f (250 μm)>400 mJy), multiply lensed submillimeter galaxy HERMES J105751.1+573027 in Herschel/SPIRE Science Demonstration Phase data from the HerMES project. Interferometric 880 μm ...
    • Fueling the central engine of radio galaxies: I. The molecular/dusty disk of 4C 31.04 

      Garcia-Burillo, S.; Combes, F.; Neri, R.; Fuente, A.; Usero, A.; Leon, S.; Lim, J. (2007)
    • Intense star formation within resolved compact regions in a galaxy at z = 2.3 

      Swinbank, A.M.; Smail, I.; Longmore, S.; Harris, A.I.; Baker, A.J.; De Breuck, C.; Richard, J.; Edge, A.C.; Ivison, R.J.; Blundell, R.; Coppin, Kristen; Cox, P.; Gurwell, M.; Hainline, L.J.; Krips, M.; Lundgren, A.; Neri, R.; Siana, B.; Siringo, G.; Stark, D.P.; Wilner, D.; Younger, J.D. (2010-04-01)
      Massive galaxies in the early Universe have been shown to be forming stars at surprisingly high rates. Prominent examples are dust-obscured galaxies which are luminous when observed at sub-millimetre wavelengths and which ...
    • Large-scale molecular shocks in galaxies: the SiO interferometer map of IC 342 

      Usero, A.; Garcia-Burillo, S.; Martin-Pintado, J.; Fuente, A.; Neri, R. (2006)
    • Modeling of the Hermes submillimeter source lensed by a dark matter dominated foreground group of galaxies 

      Gavazzi, R.; Cooray, A.; Conley, A.; Aguirre, J. E.; Amblard, A.; Auld, R.; Beelen, A.; Blain, A.; Blundell, R.; Bock, J.; Bradford, C. M.; Bridge, C.; Brisbin, D.; Burgarella, D.; Chanial, P.; Chapin, E.; Christopher, N.; Clements, D. L.; Cox, P.; Djorgovski, S. G.; Dowell, C. D.; Eales, S.; Earle, L.; Ellsworth-Bowers, T. P.; Farrah, D.; Franceschini, A.; Fu, H.; Glenn, J.; Solares, E. A. Gonzalez; Griffin, M.; Gurwell, M. A.; Halpern, M.; Ibar, E.; Ivison, R. J.; Jarvis, M.J.; Kamenetzky, J.; Kim, S.; Krips, M.; Levenson, L.; Lupu, R.; Mahabal, A.; Maloney, P. D.; Maraston, C.; Marchetti, L.; Marsden, G.; Matsuhara, H.; Mortier, A. M. J.; Murphy, E.; Naylor, B. J.; Neri, R.; Nguyen, H. T.; Oliver, S. J.; Omont, A.; Page, M. J.; Papageorgiou, A.; Pearson, C. P.; Perez-Fournon, I.; Pohlen, M.; Rangwala, N.; Rawlings, J. I.; Raymond, G.; Riechers, D.; Rodighiero, G.; Roseboom, I. G.; Rowan-Robinson, M.; Schulz, B.; Scott, Douglas; Scott, K. S.; Serra, P.; Seymour, N.; Shupe, D. L.; Smith, A. J.; Symeonidis, M.; Tugwell, K. E.; Vaccari, M.; Valiante, E.; Valtchanov, I.; Verma, A.; Vieira, J. D.; Vigroux, L.; Wang, L.; Wardlow, J.; Wiebe, D.; Wright, G.; Xu, C. K.; Zeimann, G.; Zemcov, M.; Zmuidzinas, J. (2011-09-10)
      We present the results of a gravitational lensing analysis of the bright z(s) = 2.957 submillimeter galaxy (SMG) HERMES found in the Herschel/SPIRE science demonstration phase data from the Herschel Multi-tiered Extragalactic ...
    • Molecular Gas in Submillimetre-Faint, Star-Forming Ultraluminous Galaxies at z>1 

      M. Casey, C.; C. Chapman, S.; Neri, R.; Bertoldi, F.; Smail, I.; Coppin, Kristen; R. Greve, T.; S. Bothwell, M.; J. Beswick, R.; W. Blain, A.; Cox, P.; Genzel, R.; W. B. Muxlow, T.; Omont, A.; M. Swinbank, A. (2011)
      [abridged] We present interferometric CO observations of twelve z~2 submillimetre-faint, star-forming radio galaxies (SFRGs) which are thought to be ultraluminous infrared galaxies (ULIRGs) possibly dominated by warmer ...
    • Observation of H2O in a strongly lensed Herschel-ATLAS source at z=2.3 

      Omont, A.; Neri, R.; Cox, P.; Lupu, R.; Guelin, M.; van der Werf, P.; Weiss, A.; Ivison, R.J.; Negrello, M.; Leeuw, L.; Lehnert, M.D.; Smail, I.; Verma, A.; Baker, A.J.; Beelen, A.; Aguirre, J.E.; Baes, M.; Bertoldi, F.; Clements, D.; Cooray, A.; Coppin, Kristen; Dannerbauer, H.; de Zotti, G.; Dye, S.; Fiolet, N.; Frayer, D.; Gavazzi, R.; Hughes, D.H.; Jarvis, M.J.; Krips, M.; Michalowski, M.; Murphy, E.; Riechers, D.; Serjeant, S.; Swinbank, A.M.; Temi, P.; Vaccari, M.; Vieira, J.; Auld, R.; Buttiglione, B.; Cava, A.; Dariush, A.; Dunne, L.; Eales, S.; Fritz, J.; Gomez, H.L.; Ibar, E.; Maddox, S.; Pascale, E.; Pohlen, M.; Rigby, E.; Smith, Daniel; Bock, J.; Bradford, C.M.; Glenn, J.; Scott, K.S.; Zmuidzinas, J. (2011)
      The Herschel survey, H-ATLAS, with its large areal coverage, has recently discovered a number of bright, strongly lensed high-z submillimeter galaxies. The strong magnification makes it possible to study molecular species ...
    • On the chemistry and distribution of HOC+ in M 82: More evidence for extensive PDRs 

      Fuente, A.; Garcia-Burillo, S.; Usero, A.; Gerin, M.; Neri, R.; Faure, A.; Le Bourlot, J.; Gonzalez-Garcia, M.; Rizzo, J.R.; Alonson-Albi, T.; Tennyson, J. (2008)