DSpace Repository

Browsing by Author "Calanog, J. A."

Browsing by Author "Calanog, J. A."

Sort by: Order: Results:

  • Herschel-ATLAS: A Binary HyLIRG Pinpointing a Cluster of Starbursting Protoellipticals 
    Ivison, R. J.; Swinbank, A. M.; Smail, Ian; Harris, A. I.; Bussmann, R. S.; Cooray, A.; Cox, P.; Fu, H.; Kovács, A.; Krips, M.; Narayanan, D.; Negrello, M.; Neri, R.; Peñarrubia, J.; Richard, J.; Riechers, D. A.; Rowlands, K.; Staguhn, J. G.; Targett, T. A.; Amber, S.; Baker, A. J.; Bourne, N.; Bertoldi, F.; Bremer, M.; Calanog, J. A.; Clements, D. L.; Dannerbauer, H.; Dariush, A.; De Zotti, G.; Dunne, L.; Eales, S. A.; Farrah, D.; Fleuren, S.; Franceschini, A.; Geach, J. E.; George, R. D.; Helly, J. C.; Hopwood, R.; Ibar, E.; Jarvis, M. J.; Kneib, J. -P; Maddox, S.; Omont, A.; Scott, D.; Serjeant, S.; Smith, M. W. L.; Thompson, M. A.; Valiante, E.; Valtchanov, I.; Vieira, J.; van der Werf, P. (2013)
    Panchromatic observations of the best candidate hyperluminous infrared galaxies from the widest Herschel extragalactic imaging survey have led to the discovery of at least four intrinsically luminous z = 2.41 galaxies ...
  • The rapid assembly of an elliptical galaxy of 400 billion solar masses at a redshift of 2.3 
    Fu, Hai; Cooray, Asantha; Feruglio, C.; Ivison, R. J.; Riechers, D. A.; Gurwell, M.; Bussmann, R. S.; Harris, A. I.; Altieri, B.; Aussel, H.; Baker, A. J.; Bock, J.; Boylan-Kolchin, M.; Bridge, C.; Calanog, J. A.; Casey, C. M.; Cava, A.; Chapman, S. C.; Clements, D. L.; Conley, A.; Cox, P.; Farrah, D.; Frayer, D.; Hopwood, R.; Jia, J.; Magdis, G.; Marsden, G.; Martínez-Navajas, P.; Negrello, M.; Neri, R.; Oliver, S. J.; Omont, A.; Page, M. J.; Pérez-Fournon, I.; Schulz, B.; Scott, D.; Smith, A.; Vaccari, M.; Valtchanov, I.; Vieira, J. D.; Viero, M.; Wang, L.; Wardlow, J. L.; Zemcov, M. (2013)
    Stellar archaeology shows that massive elliptical galaxies formed rapidly about ten billion years ago with star-formation rates of above several hundred solar masses per year. Their progenitors are probably the submillimetre ...

Search DSpace

Browse

My Account