Now showing items 1-3 of 3

    • Feedback and Feeding in the Context of Galaxy Evolution with SPICA: Direct Characterisation of Molecular Outflows and Inflows 

      González-Alfonso, Eduardo; Armus, Lee; Carrera, Francisco J.; Charmandaris, Vassilis; Efstathiou, Andreas; Egami, Eiichi E.; Fernández-Ontiveros, Juan Antonio; Fischer, Jacqueline R.; Granato, Gianluigi; Gruppioni, Carlotta; Hatziminaoglou, Evanthia; Imanishi, Masatoshi; Isobe, Naoki; Kaneda, Hidehiro; Kozieł-Wierzbowska, Dorota; Malkan, Matthew A.; Martín-Pintado, Jesús M.; Mateos, Silvia; Matsuhara, Hideo; Miniutti, Giovanni; Nakagawa, Takao; Pozzi, Francesca; Rico-Villas, F.; Rodighiero, Giulia; Roelfsema, Peter R.; Spinoglio, L.; Spoon, Henrik W.W.; Sturm, Eckhard; Van Der Tak, Floris F.S.; Vignali, Cristian; Wang, Lingyu (2017-11-10)
      A far-infrared observatory such as the SPace Infrared telescope for Cosmology and Astrophysics, with its unprecedented spectroscopic sensitivity, would unveil the role of feedback in galaxy evolution during the last ~10 ...
    • 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 ...