Now showing items 1-3 of 3

    • Galaxy evolution studies with the SPace IR telescope for cosmology and astrophysics (SPICA): The power of IR spectroscopy 

      Spinoglio, L.; Alonso-Herrero, Almudena; Armus, Lee; Baes, Maarten; Bernard-Salas, Jeronimo; Bianchi, Simone; Bocchio, Marco; Bolatto, Alberto D.; Bradford, Charles Matt; Braine, Jonathan; Carrera, Francisco J.; Ciesla, Laure; Clements, David L.; Dannerbauer, Helmut; Doi, Yasuo; Efstathiou, Andreas; Egami, Eiichi E.; Fernández-Ontiveros, Juan Antonio; Ferrara, Andrea; Fischer, Jacqueline R.; Franceschini, Alberto; Gallerani, Simona; Giard, Martin; González-Alfonso, Eduardo; Gruppioni, Carlotta; Guillard, Pierre; Hatziminaoglou, Evanthia; Imanishi, Masatoshi; Ishihara, D.; Isobe, N.; Kaneda, H.; Kawada, M.; Kohno, K.; Kwon, J.; Madden, S.; Malkan, M.A.; Marassi, S.; Matsuhara, H.; Matsuura, M.; Miniutti, G.; Nagamine, K.; Nagao, T.; Roelfsema, P.; Sakon, I.; Santini, P.; Schaerer, D.; Schneider, R.; Scott, Douglas J.; Serjeant, Stephen B.G.; Shibai, H.; Smith, J.-D.T.; Sobacchi, E.; Sturm, E.; Suzuki, T.; Vallini, L.; Van Der Tak, Floris F.S.; Vignali, Cristian; Yamada, T.; Wada, T.; Wang, Lingyu (2017-11-16)
      IR spectroscopy in the range 12–230 μm with the SPace IR telescope for Cosmology and Astrophysics (SPICA) will reveal the physical processes governing the formation and evolution of galaxies and black holes through cosmic ...
    • Tracing the Evolution of Dust Obscured Star Formation and Accretion Back to the Reionisation Epoch with SPICA 

      Gruppioni, Carlotta; Ciesla, Laure; Hatziminaoglou, Evanthia; Pozzi, Francesca; Rodighiero, Giulia; Santini, Paola; Armus, Lee; Baes, Maarten; Braine, Jonathan; Charmandaris, Vassilis; Clements, David L.; Christopher, Natalie M.; Dannerbauer, Helmut; Efstathiou, Andreas; Egami, Eiichi E.; Fernández-Ontiveros, Juan Antonio; Fontanot, Fabio; Franceschini, Alberto; González-Alfonso, Eduardo; Griffin, Matthew J.; Kaneda, Hidehiro; Marchetti, L.; Monaco, Pierluigi; Nakagawa, Takao; Onaka, Takashi; Papadopoulos, Andreas; Pearson, C.; Pérez-Fournón, Ismaël; Pérez-González, Pablo G.; Roelfsema, Peter R.; Scott, Douglas J.; Serjeant, Stephen B.G.; Spinoglio, L. (2017-11-16)
      Our current knowledge of star formation and accretion luminosity at high redshift (z > 3–4), as well as the possible connections between them, relies mostly on observations in the rest-frame ultraviolet, which are strongly ...
    • Unbiased Large Spectroscopic Surveys of Galaxies Selected by SPICA Using Dust Bands 

      Kaneda, Hidehiro; Ishihara, Daisuke; Oyabu, Shinki; Yamagishi, Mitsuyoshi; Wada, Takehiko; Armus, Lee; Baes, Maarten; Charmandaris, Vassilis; Czerny, Bozena; Efstathiou, Andreas; Fernández-Ontiveros, Juan Antonio; Ferrara, Andrea; González-Alfonso, Eduardo; Griffin, Matthew J.; Gruppioni, Carlotta; Hatziminaoglou, Evanthia; Imanishi, Masatoshi; Kohno, Kotaro; Kwon, Jungmi; Nakagawa, Takao; Onaka, Takashi; Pozzi, Francesca; Scott, Douglas J.; Smith, John David T.; Spinoglio, L.; Suzuki, Toyoaki; Van Der Tak, Floris F.S.; Vaccari, Mattia; Vignali, Cristian; Wang, Lingyu (2017-01-01)
      The mid-infrared range contains many spectral features associated with large molecules and dust grains such as polycyclic aromatic hydrocarbons and silicates. These are usually very strong compared to fine-structure gas ...