Now showing items 1-2 of 2

    • HELP: Star formation as a function of galaxy environment with Herschel 

      Duivenvoorden, S.; Oliver, Sebastian James; Buat, Véronique; Darvish, Behnam; Efstathiou, Andreas; Farrah, Duncan G.; Griffin, Matthew J.; Hurley, Peter Donald; Ibar, Edo; Jarvis, Matt J.; Papadopoulos, Andreas; Sargent, Mark T.; Scott, Douglas J.; Scudder, Jillian M.; Symeonidis, Myrto; Vaccari, Mattia; Viero, Marco P.; Wang, Lingyu (2016-10-11)
      The Herschel Extragalactic Legacy Project (HELP) brings together a vast range of data frommany astronomical observatories. Its main focus is on the Herschel data, which maps dustobscured star formation over 1300 deg2. With ...
    • Star formation rates in luminous quasars at 2 < z < 3 

      Harris, Kathryn A.; Farrah, Duncan G.; Schulz, Bernhard; Hatziminaoglou, Evanthia; Viero, Marco P.; Anderson, Nick; Béthermin, Matthieu; Chapman, Scott C.; Clements, David L.; Cooray, Asantha Roshan; Efstathiou, Andreas; Feltre, Anna; Hurley, Peter Donald; Ibar, Edo; Lacy, Mark D.; Oliver, Sebastian James; Page, Mathew J.; Pérez-Fournón, Ismaël; Petty, Sara M.; Pitchford, Lura K.; Rigopoulou, Dimitra; Scott, Douglas J.; Symeonidis, Myrto; Vieira, Joaquin D.; Wang, Lingyu (2016-02-10)
      We investigate the relation between star formation rates (M˙s) and AGN properties in optically selected type 1 quasars at 2 < z < 3 using data from Herschel and the SDSS. We find that M˙s remains approximately constant ...