Tracing black hole accretion with SED decomposition and IR lines: from local galaxies to the high-z Universe ανά Gruppioni, C, Berta, S, Spinoglio, L, Pereira-Santaella, M, Pozzi, F, Andreani, P, Bonato, M, De Zotti, G, Malkan, M, Negrello, M, Vallini, L, Vignali, C

Herschel-ATLAS*: far-infrared properties of radio-loud and radio-quiet quasars ανά Kalfountzou, E, Stevens, J, Jarvis, M, Hardcastle, M, Smith, D, Bourne, N, Dunne, L, Ibar, E, Eales, S, Ivison, R, Maddox, S, Smith, M, Valiante, E, de Zotti, G

The temperature dependence of the far-infrared-radio correlation in the Herschel-ATLAS ανά Smith, D, Jarvis, M, Hardcastle, M, Vaccari, M, Bourne, N, Dunne, L, Ibar, E, Maddox, N, Prescott, M, Vlahakis, C, Eales, S, Maddox, S, Smith, M, Valiante, E, de Zotti, G

The star formation rates of QSOs ανά Symeonidis, M, Maddox, N, Jarvis, MJ, Michalowski, MJ, Andreani, P, Clements, DL, De Zotti, G, Duivenvoorden, S, Gonzalez-Nuevo, J, Ibar, E, Ivison, RJ, Leeuw, L, Page, MJ, Shirley, R, Smith, MWL, Vaccari, M

Stacked average far-infrared spectrum of dusty star-forming galaxies from the Herschel /SPIRE Fourier Transform Spectrometer ανά Wilson, D, Cooray, A, Nayyeri, H, Bonato, M, Bradford, CM, Clements, DL, De Zotti, G, Díaz-Santos, T, Farrah, D, Magdis, G, Michałowski, MJ, Pearson, C, Rigopoulou, D, Valtchanov, I, Wang, L, Wardlow, J

Isothermal dust models of Herschel-ATLAS star galaxies ανά Smith, D, Hardcastle, M, Jarvis, M, Maddox, S, Dunne, L, Bonfield, D, Eales, S, Serjeant, S, Thompson, M, Baes, M, Clements, D, Cooray, A, De Zotti, G, Gonzalez-Nuevo, J, van der Werf, P, Virdee, J, Bourne, N, Dariush, A, Hopwood, R, Ibar, E, Valiante, E

Herschel-ATLAS: the link between accretion luminosity and star formation in quasar host galaxies★ ανά Bonfield, D, Jarvis, M, Jarvis, M, Hardcastle, M, Hardcastle, M, Cooray, A, Cooray, A, Hatziminaoglou, E, Hatziminaoglou, E, Ivison, R, Ivison, R, Page, M, Page, M, Stevens, J, Stevens, J, de Zotti, G, de Zotti, G, Auld, R, Auld, R, Baes, M, Baes, M, Buttiglione, S, Buttiglione, S, Cava, A, Cava, A, Dariush, A, Dariush, A, Dunlop, J, Dunlop, J, Dunne, L, Dunne, L, Dye, S, Dye, S, Eales, S, Eales, S, Fritz, J, Fritz, J, Hopwood, R, Hopwood, R, Ibar, E, Ibar, E, Maddox, S, Maddox, S, Michałowski, M, Michałowski, M, Pascale, E, Pascale, E, Pohlen, M, Pohlen, M

Herschel-ATLAS: counterparts from the ultraviolet-near-infrared in the science demonstration phase catalogue ανά Smith, D, Dunne, L, Maddox, S, Eales, S, Bonfield, D, Jarvis, M, Sutherland, W, Fleuren, S, Rigby, E, Thompson, M, Baldry, I, Bamford, S, Buttiglione, S, Cava, A, Clements, D, Cooray, A, Croom, S, Dariush, A, de Zotti, G, Driver, S, Dunlop, J, Fritz, J, Hill, D, Hopkins, A, Hopwood, R

Herschel-ATLAS: Evolution of the 250 mu m luminosity function out to z = 0.5 ανά Dye, S, Dunne, L, Eales, S, Smith, D, Amblard, A, Auld, R, Baes, M, Baldry, I, Bamford, S, Blain, A, Bonfield, D, Bremer, M, Burgarella, D, Buttiglione, S, Cameron, E, Cava, A, Clements, D, Cooray, A, Croom, S, Dariush, A, de Zotti, G, Driver, S, Dunlop, J, Frayer, D, Fritz, J

Herschel-ATLAS*: Evolution of the 250 μm luminosity function out to z = 0.5 ανά Dye, S, Dunne, L, Eales, S, Smith, D, Amblard, A, Auld, R, Baes, M, Baldry, I, Bamford, S, Blain, A, Bonfield, D, Bremer, M, Burgarella, D, Buttiglione, S, Cameron, E, Cava, A, Clements, D, Cooray, A, Croom, S, Dariush, A, De Zotti, G, Driver, S, Dunlop, J, Frayer, D, Fritz, J

The new galaxy evolution paradigm revealed by the Herschel surveys ανά Eales, S, Smith, D, Bourne, N, Loveday, J, Rowlands, K, Werf, P, Driver, S, Dunne, L, Dye, S, Furlanetto, C, Ivison, R, Maddox, S, Robotham, A, Smith, M, Taylor, E, Valiante, E, Wright, A, Cigan, P, De Zotti, G, Jarvis, M, Marchetti, L, Michałowski, M, Phillipps, S, Viaene, S, Vlahakis, C

Herschel-ATLAS/GAMA: a difference between star formation rates in strong-line and weak-line radio galaxies ανά Hardcastle, M, Ching, J, Virdee, J, Jarvis, M, Croom, S, Sadler, E, Mauch, T, Smith, D, Stevens, J, Baes, M, Baldry, I, Brough, S, Cooray, A, Dariush, A, De Zotti, G, Driver, S, Dunne, L, Dye, S, Eales, S, Hopwood, R, Liske, J, Maddox, S, Michalowski, M, Rigby, E, Robotham, A

-IRAC IDENTIFICATION OF -ATLAS SPIRE SOURCES ανά Kim, S, Wardlow, J, Cooray, A, Fleuren, S, Sutherland, W, Khostovan, A, Auld, R, Baes, M, Bussmann, R, Buttiglione, S, Cava, A, Clements, D, Dariush, A, De Zotti, G, Dunne, L, Dye, S, Eales, S, Fritz, J, Hopwood, R, Ibar, E, Ivison, R, Jarvis, M, Maddox, S, Michałowski, M, Pascale, E

Which haloes host Herschel-ATLAS galaxies in the local Universe? ανά Guo, Q, Cole, S, Lacey, C, Baugh, C, Frenk, C, Norberg, P, Auld, R, Baldry, I, Bamford, S, Bourne, N, Buttiglione, E, Cava, A, Cooray, A, Croom, S, Dariush, A, De Zotti, G, Driver, S, Dunne, L, Dye, S, Eales, S, Fritz, J, Hopkins, A, Hopwood, R, Ibar, E, Ivison, R

THE INFRARED PROPERTIES OF SOURCES MATCHED IN THE WISE ALL-SKY AND HERSCHEL ATLAS SURVEYS ανά Bond, N, Benford, D, Gardner, J, Amblard, A, Fleuren, S, Blain, A, Dunne, L, Smith, D, Maddox, S, Hoyos, C, Baes, M, Bonfield, D, Bourne, N, Bridge, C, Buttiglione, S, Cava, A, Clements, D, Cooray, A, Dariush, A, de Zotti, G, Driver, S, Dye, S, Eales, S, Eisenhardt, P, Hopwood, R

Herschel -ATLAS: rapid evolution of dust in galaxies over the last 5 billion years ανά Dunne, L, Gomez, H, da Cunha, E, Charlot, S, Dye, S, Eales, S, Maddox, S, Rowlands, K, Smith, D, Auld, R, Baes, M, Bonfield, D, Bourne, N, Buttiglione, S, Cava, A, Clements, D, Coppin, K, Cooray, A, Dariush, A, de Zotti, G, Driver, S, Fritz, J, Geach, J, Hopwood, R, Ibar, E

Herschel★-ATLAS/GAMA: a census of dust in optically selected galaxies from stacking at submillimetre wavelengths ανά Bourne, N, Maddox, S, Dunne, L, Auld, R, Baes, M, Baldry, I, Bonfield, D, Cooray, A, Croom, S, Dariush, A, de Zotti, G, Driver, S, Dye, S, Eales, S, Gomez, H, González-Nuevo, J, Hopkins, A, Ibar, E, Jarvis, M, Lapi, A, Madore, B, Michałowski, M, Pohlen, M, Popescu, C, Rigby, E

Herschel-Astrophysical Terahertz Large Area Survey: detection of a far-infrared population around galaxy clusters★ ανά Coppin, K, Geach, J, Smail, I, Dunne, L, Edge, A, Ivison, R, Maddox, S, Auld, R, Baes, M, Buttiglione, S, Cava, A, Clements, D, Cooray, A, Dariush, A, De Zotti, G, Dye, S, Eales, S, Fritz, J, Hopwood, R, Ibar, E, Jarvis, M, Michałowski, M, Murphy, D, Negrello, M, Pascale, E

H-ATLAS: PACS imaging for the Science Demonstration Phase ανά Ibar, E, Ivison, R, Cava, A, Rodighiero, G, Buttiglione, S, Temi, P, Frayer, D, Fritz, J, Leeuw, L, Baes, M, Rigby, E, Verma, A, Serjeant, S, Mueller, T, Auld, R, Dariush, A, Dunne, L, Eales, S, Maddox, S, Panuzzo, P, Pascale, E, Pohlen, M, Smith, D, de Zotti, G, Vaccari, M

Herschel-ATLAS: the far-infrared-radio correlation at z < 0.5★ ανά Jarvis, M, Smith, D, Bonfield, D, Hardcastle, M, Falder, J, Stevens, J, Ivison, R, Auld, R, Baes, M, Baldry, I, Bamford, S, Bourne, N, Buttiglione, S, Cava, A, Cooray, A, Dariush, A, De Zotti, G, Dunlop, J, Dunne, L, Dye, S, Eales, S, Fritz, J, Hill, D, Hopwood, R, Hughes, D