Now showing items 1-9 of 9

    • The debris disc of solar analogue Τ Ceti : Herschel observations and dynamical simulations of the proposed multiplanet system 

      Lawler, S. M.; Di Francesco, J.; Kennedy, G. M.; Sibthorpe, B.; Booth, M.; Vandenbussche, B.; Matthews, B. C.; Holland, W. S.; Greaves, J.; Wilner, D. J.; Tuomi, Mikko; Blommaert, J. A D L; De Vries, B. L.; Dominik, C.; Fridlund, M.; Gear, W.; Heras, A. M.; Ivison, R.; Olofsson, G. (2014-11-01)
      Τ Ceti is a nearby, mature G-type star very similar to our Sun, with a massive Kuiper Belt analogue and possible multiplanet system that has been compared to our Solar system. We present Herschel Space Observatory images ...
    • GAMA/H-ATLAS: common star formation rate indicators and their dependence on galaxy physical parameters 

      Wang, L.; Norberg, P.; Gunawardhana, M. L. P.; Heinis, S.; Baldry, I. K.; Bland-Hawthorn, J.; Bourne, N.; Brough, S.; Cluver, M. E.; Cooray, A.; Cunha, E. da; Driver, S. P.; Dunne, L.; Dye, S.; Eales, S.; Grootes, M. W.; Holwerda, B. W.; Hopkins, A. M.; Ibar, E.; Ivison, R.; Lacey, C.; Lara-Lopez, M. A.; Loveday, J.; Maddox, S. J.; lowski, M. J. Micha; Oteo, I.; Owers, M. S.; Popescu, C. C.; Smith, D. J. B.; Taylor, E. N.; Tuffs, R. J.; Werf, P. van der (2016-09-11)
      We compare common star-formation rate (SFR) indicators in the local Universe in the GAMA equatorial fields (around 160 sq. deg.), using ultraviolet (UV) photometry from GALEX, far-infrared (FIR) and sub-millimetre (sub-mm) ...
    • GAMA/H-ATLAS: the ultraviolet spectral slope and obscuration in galaxies 

      Wijesinghe, D. B.; da Cunha, E.; Hopkins, A. M.; Dunne, L.; Sharp, R.; Gunawardhana, M.; Brough, S.; Sadler, E.M.; Driver, S.; Baldry, I.; Bamford, S.; Liske, J.; Loveday, J.; Norberg, P.; Peacock, J.; Popescu, C. C.; Tuffs, R.; Andrae, E.; Auld, R.; Baes, M.; Bland-Hawthorn, J.; Buttiglione, S.; Cava, A.; Cameron, E.; Conselice, C. J.; Cooray, A.; Croom, S.; Dariush, A.; DeZotti, G.; Dye, S.; Eales, S.; Frenk, C.; Fritz, J.; Hill, D.; Hopwood, R.; Ibar, E.; Ivison, R.; Jarvis, M.J.; Jones, D. H.; van Kampen, E.; Kelvin, L.; Kuijken, K.; Maddox, S. J.; Madore, B.; Michalowski, M. J.; Nichol, B.; Parkinson, H.; Pascale, E.; Pimbblet, K. A.; Pohlen, M.; Prescott, M.; Rhodighiero, G.; Robotham, A. S. G.; Rigby, E. E.; Seibert, M.; Sergeant, S.; Smith, Daniel; Temi, P.; Sutherland, W.; Taylor, E.; Thomas, D.; van der Werf, P. (2011-08)
      We use multiwavelength data from the Galaxy And Mass Assembly (GAMA) and Herschel-ATLAS (H-ATLAS) surveys to compare the relationship between various dust obscuration measures in galaxies. We explore the connections between ...
    • The Herschel ATLAS 

      Eales, S.; Dunne, L.; Clements, D.; Cooray, A.; de Zotti, G.; Dye, S.; Ivison, R.; Jarvis, M.J.; Lagache, G.; Maddox, S.; Negrello, M.; Serjeant, S.; Thompson, Mark; van Kampen, E.; Amblard, A.; Andreani, P.; Baes, M.; Beelen, A.; Bendo, G. J.; Benford, D.; Bertoldi, F.; Bock, J.; Bonfield, D.; Boselli, A.; Bridge, C.; Buat, V.; Burgarella, D.; Carlberg, R.; Cava, A.; Chanial, P.; Charlot, S.; Christopher, N.; Coles, P.; Cortese, L.; Dariush, A.; da Cunha, E.; Dalton, G.; Danese, L.; Dannerbauer, H.; Driver, S.; Dunlop, J.; Fan, L.; Farrah, D.; Frayer, D.; Frenk, C.; Geach, James; Gardner, J.; Gomez, H.; González-Nuevo, J.; González-Solares, E.; Griffin, M.; Hardcastle, M.J.; Hatziminaoglou, E.; Herranz, D.; Hughes, D.; Ibar, E.; Jeong, W.-S.; Lacey, C.; Lapi, A.; Lawrence, A.; Lee, M.; Leeuw, L.; Liske, J.; López-Caniego, M.; Müller, T.; Nandra, K.; Panuzzo, P.; Papageorgiou, A.; Patanchon, G.; Peacock, J.; Pearson, C.; Phillipps, S.; Pohlen, M.; Popescu, C.; Rawlings, S.; Rigby, E.; Rigopoulou, M.; Robotham, A.; Rodighiero, G.; Sansom, A.; Schulz, B.; Scott, D.; Smith, Daniel; Sibthorpe, B.; Smail, I.; Stevens, J.; Sutherland, W.; Takeuchi, T.; Tedds, J.; Temi, P.; Tuffs, R.; Trichas, M.; Vaccari, M.; Valtchanov, I.; van der Werf, P.; Verma, A.; Vieria, J.; Vlahakis, C.; White, G.J. (2010-05-01)
      The Herschel ATLAS is the largest open-time key project that will be carried out on the Herschel Space Observatory. It will survey 570 deg2 of the extragalactic sky, 4 times larger than all the other Herschel extragalactic ...
    • The Herschel view of the environment of the radio galaxy 4C+41.17 at z = 3.8 

      Wylezalek, D.; Vernet, J.; De Breuck, C.; Stern, D.; Galametz, A.; Seymour, N.; Jarvis, M.J.; Barthel, P.; Drouart, G.; Greve, T.R.; Haas, M.; Hatch, N.; Ivison, R.; Lehnert, M.; Meisenheimer, K.; Miley, G.; Nesvadba, N.; Rottgering, H.J.A.; Stevens, J.A. (2013-02-01)
      We present Herschel observations at 70, 160, 250, 350 and 500 μm of the environment of the radio galaxy 4C+41.17 at z = 3.792. About 65 per cent of the extracted sources are securely identified with mid-infrared sources ...
    • Herschel-ATLAS : toward a sample of similar to 1000 strongly lensed galaxies 

      Gonzalez-Nuevo, J.; Lapi, A.; Fleuren, S.; Bressan, S.; Danese, L.; De Zotti, G.; Negrello, M.; Cai, Z. -Y.; Fan, L.; Sutherland, W.; Baes, M.; Baker, A. J.; Clements, L.; Cooray, A.; Dannerbauer, H.; Dunne, L.; Dye, S.; Eales, S.; Frayer, D. T.; Harris, A. I.; Ivison, R.; Jarvis, M.J.; Michallowski, M.J.; Lopez-Caniego, M.; Rodighiero, G.; Rowlands, K.; Serjeant, S.; Scott, D.; van der Werf, P.; Auld, R.; Buttiglione, S.; Cava, A.; Dariush, A.; Fritz, J.; Hopwood, R.; Ibar, E.; Maddox, S.; Pascale, E.; Pohlen, M.; Rigby, E.; Smith, Daniel; Temi, P. (2012-04-10)
      While the selection of strongly lensed galaxies (SLGs) with 500 mu m flux density S-500 > 100 mJy has proven to be rather straightforward, for many applications it is important to analyze samples larger than the ones ...
    • Herschel-atlas galaxy counts and high-redshift luminosity functions : The formation of massive early-type galaxies 

      Lapi, A.; González-Nuevo, J.; Fan, L.; Bressan, A.; de Zotti, G.; Danese, L.; Buttiglione, S.; Negrello, M.; Hopwood, R.; Serjeant, S.; Dunne, L.; Maddox, S.; Rigby, E.; Eales, S.; Auld, R.; Dariush, A.; Dye, S.; Kaviraj, S.; Pascale, E.; Pohlen, M.; Baes, M.; Fritz, J.; Bonfield, D.G.; Jarvis, M.J.; Smith, Daniel; Cava, A.; Clements, D. L.; Dariush, A.; Hopwood, R.; Cooray, A.; Wardlow, J.; Herranz, D.; López-Caniego, M.; Ibar, E.; Ivison, R.; Michałowski, M. J.; Jarvis, M.J.; Massardi, M.; Rodighiero, G.; Temi, P.; Van Der Werf, P. (2011)
      Exploiting the Herschel Astrophysical Terahertz Large Area Survey Science Demonstration Phase survey data, we have determined the luminosity functions (LFs) at rest-frame wavelengths of 100 and 250 μm and at several redshifts ...
    • Rapid Coeval Black Hole and Host Galaxy Growth in MRCnbsp1138-262 : The Hungry Spider 

      Seymour, N.; Altieri, B.; De Breuck, C.; Barthel, P.; Coia, D.; Conversi, L.; Dannerbauer, H.; Dey, A.; Dickinson, M.; Drouart, G.; Galametz, A.; Greve, T.R.; Haas, M.; Hatch, N.; Ibar, E.; Ivison, R.; Jarvis, M.J.; Kovács, A.; Kurk, J.; Lehnert, M.; Miley, G.; Nesvadba, N.; Rawlings, J.I.; Rettura, A.; Röttgering, H.; Rocca-Volmerange, B.; Sánchez-Portal, M.; Santos, J. S.; Stern, D.; Stevens, J.; Valtchanov, I.; Vernet, J.; Wylezalek, D. (2012-08-01)
      We present a detailed study of the infrared spectral energy distribution of the high-redshift radio galaxy MRC1138-26 at z = 2.156, also known as the Spiderweb Galaxy. By combining photometry from Spitzer, Herschel and ...
    • The SCUBA Half-Degree Extragalactic Survey (SHADES) - VIII : The Nature of Faint Submillimetre Galaxies in SHADES, SWIRE and SXDF Surveys 

      Clements, D. L.; Vaccari, M.; Babbedge, T.; Oliver, S.; Rowan-Robinson, M.; Davoodi, P.; Ivison, R.; Farrah, D.; Dunlop, J.; Shupe, D.; Waddington, I.; Simpson, C.; Furusawa, H.; Serjeant, S.; Afonso-Luis, A.; Alexander, D.M.; Aretxaga, I.; Blain, A.; Borys, C.; Chapman, S.; Coppin, Kristen; Dunne, L.; Dye, S.; Eales, S. A.; Evans, T.; Fang, F.; Frayer, D.; Fox, M.; Gear, W.K.; Greve, T.R.; Halpern, M.; Hughes, D.H.; Jenness, T.; Lonsdale, C.J.; Mortier, Angela M. J.; Page, M.J.; Pope, A.; Priddey, Robert Stephen; Rawlings, S.; Savage, R.S.; Scott, D.; Scott, S.E.; Sekiguchi, K.; Smail, I.; Smith, H.E.; Stevens, Jason; Surace, J.; Takagi, T.; van Kampen, E. (2008)
      We present the optical-to-submm spectral energy distributions for 33 radio & mid-IR identified submillimetre galaxies discovered via the SHADES 850μm SCUBA imaging in the Subaru-XMM Deep Field (SXDF). Optical data for the ...