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  • Vaccari, M.; Marchetti, L.; Franceschini, A.; Altieri, B.; Amblard, A.; Arumugam, V.; Auld, R.; Aussel, H.; Babbedge, T.; Blain, A.; Bock, J.; Boselli, A.; Buat, V.; Burgarella, D.; Castro-Rodríguez, N.; Cava, A.; Chanial, P.; Clements, D.L.; Conley, A.; Conversi, L.; Cooray, A.; Dowell, C.D.; Dwek, E.; Dye, S.; Eales, S.; Elbaz, D.; Farrah, D.; Fox, M.; Gear, W.; Glenn, J.; González Solares, E.A.; Griffin, M.; Halpern, M.; Hatziminaoglou, E.; Huang, J.; Ibar, E.; Isaak, K.; Ivison, R.J.; Lagache, G.; Levenson, L.; Lu, N.; Madden, S.; Maffei, B.; Mainetti, G.; Mortier, A.M.J.; Nguyen, H.T.; O'Halloran, B.; Oliver, S.J.; Omont, A.; Page, M.J.; Panuzzo, P.; Papageorgiou, A.; Pearson, C.P.; Pérez-Fournon, I.; Pohlen, M.; Rawlings, J.I.; Raymond, G.; Rigopoulou, D.; Rizzo, D.; Rodighiero, G.; Roseboom, I.G.; Rowan-Robinson, M.; Sánchez Portal, M.; Schulz, B.; Scott, D.; Seymour, N.; Shupe, D.L.; Smith, A.J.; Stevens, Jason; Symeonidis, M.; Trichas, M.; Tugwell, K.E.; Valiante, E.; Valtchanov, I.; Vigroux, L.; Wang, L.; Ward, R.; Wright, G.; Xu, C.K.; Zemcov, M. (2010-07-01)
    Local luminosity functions are fundamental benchmarks for high-redshift galaxy formation and evolution studies as well as for models describing these processes. Determining the local luminosity function in the submillimeter ...
  • Nguyen, H. T.; Schulz, B.; Levenson, L.; Amblard, A.; Arumugam, V.; Aussel, H.; Babbedge, T.; Blain, A.; Bock, J.; Boselli, A.; Buat, V.; Castro-Rodriguez, N.; Cava, A.; Chanial, P.; Chapin, E.; Clements, D. L.; Conley, A.; Conversi, L.; Cooray, A.; Dowell, C. D.; Dwek, E.; Eales, S.; Elbaz, D.; Fox, M.; Franceschini, A.; Gear, W.; Glenn, J.; Griffin, M.; Halpern, M.; Hatziminaoglou, E.; Ibar, E.; Isaak, K.; Ivison, R. J.; Lagache, G.; Lu, N.; Madden, S.; Maffei, B.; Mainetti, G.; Marchetti, L.; Marsden, G.; Marshall, J.; O'Halloran, B.; Oliver, S. J.; Omont, A.; Page, M. J.; Panuzzo, P.; Papageorgiou, A.; Pearson, C. P.; Perez Fournon, I.; Pohlen, M.; Rangwala, N.; Rigopoulou, D.; Rizzo, D.; Roseboom, I. G.; Rowan-Robinson, M.; Scott, D.; Seymour, N.; Shupe, D. L.; Smith, A. J.; Stevens, Jason; Symeonidis, M.; Trichas, M.; Tugwell, K. E.; Vaccari, M.; Valtchanov, I.; Vigroux, L.; Wang, L.; Ward, R.; Wiebe, D.; Wright, G.; Xu, C. K.; Zemcov, M. (2010-07-01)
    We report on the sensitivity of SPIRE photometers on the Herschel Space Observatory. Specifically, we measure the confusion noise from observations taken during the science demonstration phase of the Herschel Multi-tiered ...
  • Schulz, B.; Pearson, C.P.; Clements, D. L.; Altieri, B.; Amblard, A.; Arumugam, V.; Auld, R.; Aussel, H.; Babbedge, T.; Blain, A.; Bock, J.; Boselli, A.; Buat, V.; Burgarella, D.; Castro-Rodríguez, N.; Cava, A.; Chanial, P.; Conley, A.; Conversi, L.; Cooray, A.; Dowell, C.D.; Dwek, E.; Eales, S.; Elbaz, D.; Fox, M.; Franceschini, A.; Gear, W.; Giovannoli, E.; Glenn, J.; Griffin, M.; Halpern, M.; Hatziminaoglou, E.; Ibar, E.; Isaak, K.; Ivison, R.J.; Lagache, G.; Levenson, L.; Lu, N.; Madden, S.; Maffei, B.; Mainetti, G.; Marchetti, L.; Marsden, G.; Mortier, A.M.J.; Nguyen, H.T.; O'Halloran, B.; Oliver, S. J.; Omont, A.; Page, M.J.; Panuzzo, P.; Papageorgiou, A.; Pérez-Fournon, I.; Pohlen, M.; Rangwala, N.; Rawlings, J.I.; Raymond, G.; Rigopoulou, D.; Rizzo, D.; Roseboom, I.G.; Rowan-Robinson, M.; Sánchez Portal, M.; Scott, D.; Seymour, N.; Shupe, D. L.; Stevens, Jason; Symeonidis, M.; Trichas, M.; Tugwell, K.E.; Vaccari, M.; Valiante, E.; Valtchanov, I.; Vigroux, L.; Wang, L.; Ward, R.; Wright, G.; Xu, C.K.; Zemcov, M. (2010-07-01)
    We present colours of sources detected with the Herschel/SPIRE instrument in deep extragalactic surveys of the Lockman Hole, Spitzer-FLS, and GOODS-N fields in three photometric bands at 250, 350 and 500 μm. We compare ...
  • Budge, G. (2008)
    A rhetoric of spectrality pervades Thomas Carlyle’s writings, in a way which is intimately related to his characteristic position of “natural supernaturalism.” This essay argues that Carlyle’s rhetorical emphasis on spectral ...
  • Phillips, Ivan (2013)
    Doctor Who is an unstable phenomenon. This is its great strength, the secret of its enduring success. Resistant to generic categories, merging futurism and nostalgia, its eponymous hero (sometimes anti-hero) is a character ...
  • Ivison, R. J.; Swinbank, A. M.; Swinyard, B.; Smail, Ian; Pearson, C. P.; Rigopoulou, D.; Polehampton, E.; Baluteau, J-P.; Barlow, M. J.; Blain, A. W.; Bock, J.; Clements, D. L.; Coppin, Kristen; Cooray, A.; Danielson, A.; Dwek, E.; Edge, A. C.; Franceschini, A.; Fulton, T.; Glenn, J.; Griffin, M.; Isaak, K.; Leeks, S.; Lim, T.; Naylor, D.; Oliver, S. J.; Page, M. J.; Perez-Fournon, I.; Rowan-Robinson, M.; Savini, G.; Scott, D.; Spencer, L.; Valtchanov, I.; Vigroux, L.; Wright, G. S. (2010)
    We present a detailed analysis of the far-IR properties of the bright, lensed, z = 2.3, SMG, SMM J2135-0102, using new observations with Herschel, SCUBA-2 and the VLA. These data allow us to constrain the galaxy's SED and ...
  • Coppin, Kristen; Geach, James; Smail, Ian; Dunne, L.; Edge, A.C.; Ivison, R. J.; Maddox, S.; Auld, R.; Baes, M.; Buttiglione, S.; Cava, A.; Clements, D. L.; Cooray, A.; Dariush, A.; De Zotti, G.; Dye, S.; Eales, S.; Fritz, J.; Hopwood, R.; Ibar, E.; Jarvis, M.J.; Michalowski, M. J.; Murphy, D. N. A.; Negrello, M.; Pascale, E.; Pohlen, M.; Rigby, E.; Rodighiero, G.; Scott, D.; Serjeant, S.; Smith, Daniel; Temi, P.; van der Werf, P. (2011-09)
    We report the detection of a significant excess in the surface density of far-infrared sources from the Herschel-Astrophysical Terahertz Large Area Survey within similar to 1Mpc of the centres of 66 optically selected ...
  • 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 ...
  • Gonzalez-Nuevo, J.; de Zotti, G.; Andreani, P.; Barton, E.; Bertoldi, F.; Birkinshaw, M.; Bonavera, L.; Buttiglione, S.; Cooke, J.; Cooray, A.; Danese, G.; Dunne, L.; Eales, S.; Fan, L.; Jarvis, M.J.; Kloeckner, H-R.; Hatziminaoglou, E.; Herranz, D.; Hughes, D.H.; Lapi, A.; Lawrence, A.; Leeuw, L.; Lopez-Caniego, M.; Massardi, M.; Mauch, T.; Michalowski, M.; Negrello, M.; Rawlings, S.; Rodighiero, G.; Samui, S.; Serjeant, S.; Vieira, J.; White, G.J.; Amblard, A.; Auld, R.; Baes, M.; Bonfield, D.; Burgarella, D.; Cava, A.; Clements, D.; Dariush, A.; Dye, S.; Frayer, D.; Fritz, J.; Ibar, E.; Ivison, R.J.; Lagache, G.; Maddox, S.; Pascale, E.; Pohlen, M.; Rigby, E.; Sibthorpe, B.; Smith, Daniel; Temi, P.; Thompson, M.A.; Valtchanov, I.; Verma, A. (2010)
    To investigate the poorly constrained sub-mm counts and spectral properties of blazars we searched for these in the Herschel-ATLAS (H-ATLAS) science demonstration phase (SDP) survey catalog.

We cross-matched 500 μm sources ...
  • Smith, Daniel; Dunne, L.; Maddox, S. J.; Eales, S.; Bonfield, D. G.; Jarvis, M.J.; Sutherland, W.; Fleuren, S.; Rigby, E. E.; Thompson, Mark; Baldry, I.K.; Bamford, S.; Buttiglione, S.; Cava, A.; Clements, D. L.; Cooray, A.; Croom, S.; Dariush, A.; de Zotti, G.; Driver, S. P.; Dunlop, J.S.; Fritz, J.; Hill, D. T.; Hopkins, A.; Hopwood, R.; Ibar, E.; Ivison, R.J.; Jones, D. H.; Kelvin, L.; Leeuw, L.; Liske, J.; Loveday, J.; Madore, B. F.; Norberg, P.; Panuzzo, P.; Pascale, E.; Pohlen, M.; Popescu, C. C.; Prescott, M.; Robotham, A.; Rodighiero, G.; Scott, D.; Seibert, M.; Sharp, R.; Temi, P.; Tuffs, R. J.; van der Werf, P.; van Kampen, E. (2011-09)
    We present a technique to identify optical counterparts of 250-mu m-selected sources from the Herschel-ATLAS survey. Of the 6621 250 mu m > 32-mJy sources in our science demonstration catalogue we find that similar to 60 ...
  • Amblard, A.; Cooray, A.; Serra, P.; Temi, P.; Barton, E.; Negrello, M.; Auld, R.; Baes, M.; Baldry, I.K.; Bamford, S.; Blain, A.W.; Bock, J.; Bonfield, D.; Burgarella, D.; Buttiglione, S.; Cameron, E.; Cava, A.; Clements, D.; Croom, S.; Dariush, A.; de Zotti, G.; Driver, S.; Dunlop, J.S.; Dunne, L.; Dye, S.; Eales, S.; Frayer, D.; Fritz, J.; Gardner, J.P.; Gonzalez-Nuevo, J.; Herranz, D.; Hill, D.; Hopkins, A.; Hughes, D.H.; Ibar, E.; Ivison, R.J.; Jarvis, M.J.; Jones, D.H.; Kelvin, L.; Lagache, G.; Leeuw, L.; Liske, J.; Lopez-Caniego, M.; Loveday, J.; Maddox, S.; Michalowski, M.; Norberg, P.; Parkinson, H.; Peacock, J.A.; Pearson, C.; Pascale, E.; Pohlen, M.; Popescu, C.; Prescott, M.; Robotham, A.; Rigby, E.; Rodighiero, G.; Samui, S.; Sansom, A.; Scott, D.; Serjeant, S.; Sharp, R.G.; Sibthorpe, B.; Smith, Daniel; Thompson, M.A.; Tuffs, R.; Valtchanov, I.; van Kampen, E.; van der Werf, P.; Verma, A.; Vieira, J.; Vlahakis, C. (2010)
    We present colour–colour diagrams of detected sources in the Herschel-ATLAS science demonstration field from 100 to 500 μm using both PACS and SPIRE. We fit isothermal modified black bodies to the spectral energy distribution ...
  • Dye, S.; Dunne, L.; Eales, S.; Smith, Daniel; Amblard, A.; Auld, R.; Baes, M.; Baldry, I.K.; Bamford, S.; Blain, A.W.; 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.S.; Frayer, D.; Fritz, J.; Gardner, J.P.; Gomez, H.L.; Gonzalez-Nuevo, J.; Herranz, D.; Hill, D.; Hopkins, A.; Ibar, E.; Ivison, R.J.; Jarvis, M.J.; Jones, D.H.; Kelvin, L.; Lagache, G.; Leeuw, L.; Liske, J.; Lopez-Caniego, M.; Loveday, J.; Maddox, S.; Michalowski, M.; Negrello, M.; Norberg, P.; Page, M.J.; Parkinson, H.; Pascale, E.; Peacock, J.A.; Pohlen, M.; Popescu, C.; Prescott, M.; Rigopoulou, D.; Robotham, A.; Rigby, E.; Rodighiero, G.; Samui, S.; Scott, D.; Serjeant, S.; Sharp, R.G.; Sibthorpe, B.; Temi, P.; Thompson, M.A.; Tuffs, R.; Valtchanov, I.; van der Werf, P.; van Kampen, E.; Verma, A. (2010)
    We have determined the luminosity function of 250 μm-selected galaxies detected in the ~14 deg2 science demonstration region of the Herschel-ATLAS project out to a redshift of z = 0.5. Our findings very clearly show that ...
  • Clements, D.; Rigby, E.; Maddox, S.; Dunne, L.; Mortier, A.M.J.; Pearson, C.; Amblard, A.; Auld, R.; Baes, M.; Bonfield, D.; Burgarella, D.; Buttiglione, S.; Cava, A.; Cooray, A.; Dariush, A.; de Zotti, G.; Dye, S.; Eales, S.; Frayer, D.; Fritz, J.; Gardner, J.P.; Gonzalez-Nuevo, J.; Herranz, D.; Ibar, E.; Ivison, R.J.; Jarvis, M.J.; Lagache, G.; Leeuw, L.; Lopez-Caniego, M.; Negrello, M.; Pascale, E.; Pohlen, M.; Rodighiero, G.; Samui, S.; Serjeant, S.; Sibthorpe, B.; Scott, D.; Smith, Daniel; Temi, P.; Thompson, M.A.; Valtchanov, I.; van der Werf, P.; Verma, A. (2010)
    Aims. The Herschel-ATLAS survey (H-ATLAS) will be the largest area survey to be undertaken by the Herschel Space Observatory. It will cover 550 sq. deg. of extragalactic sky at wavelengths of 100, 160, 250, 350 and 500 μm ...
  • Kalfountzou, E.; Stevens, J.A.; Jarvis, M.J.; Hardcastle, M.J.; Smith, Daniel; Bourne, N.; Dunne, L.; Ibar, E.; Eales, S.; Ivison, R.J.; Maddox, S.; Smith, M. W. L.; Valiante, E.; de Zotti, G. (2014-08-01)
    We have constructed a sample of radio-loud and radio-quiet quasars from the Faint Images Radio Sky at Twenty-one centimetres and the Sloan Digital Sky Survey Data Release 7, over the Herschel-ATLAS Phase 1 area (9h, 12h ...
  • Hardcastle, M.J.; Virdee, J.S.; Jarvis, M.J.; Bonfield, D.; Dunne, L.; Rawlings, S.; Stevens, J. A.; Christopher, N. M.; Heywood, I.; Mauch, Tom; Rigopoulou, D.; Verma, A.; Baldry, Ivan K.; Bamford, S. P.; Buttiglione, S.; Cava, A.; Clements, D. L.; Cooray, A.; Croom, S. M.; Dariush, A.; de Zotti, G.; Eales, S.; Fritz, J.; Hill, D. T.; Hughes, D.; Hopwood, R.; Ibar, E.; Ivison, Rob J.; Jones, D.H.; Loveday, J.; Maddox, S. J.; Michalowski, M. J.; Negrello, M.; Norberg, P.; Pohlen, M.; Prescott, M.; Rigby, E. E.; Robotham, A. S. G.; Rodighiero, G.; Scott, D.; Sharp, R.; Smith, Daniel; Temi, P.; van Kampen, E. (2010)
    We use the Herschel-Astrophysical Terahertz Large Area Survey (ATLAS) science demonstration data to investigate the star formation properties of radio-selected galaxies in the GAMA-9h field as a function of radio luminosity ...
  • Rigby, E. E.; Maddox, S. J.; Dunne, L.; Negrello, M.; Smith, Daniel; Gonzalez-Nuevo, J.; Herranz, D.; Lopez-Caniego, M.; Auld, R.; Buttiglione, S.; Baes, M.; Cava, A.; Cooray, A.; Clements, D. L.; Dariush, A.; de Zotti, G.; Dye, S.; Eales, S.; Frayer, D.; Fritz, J.; Hopwood, R.; Ibar, E.; Ivison, R.J.; Jarvis, M.J.; Panuzzo, P.; Pascale, E.; Pohlen, M.; Rodighiero, G.; Serjeant, S.; Temi, P.; Thompson, Mark (2011-08)
    The Herschel Astrophysical Terahertz LargeArea Survey (Herschel-ATLAS) is a survey of 550 deg(2) with the Herschel Space Observatory in five far-infrared and submillimetre bands. The first data for the survey, observations ...
  • 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 ...
  • Bourne, N.; Maddox, S. J.; Dunne, L.; Auld, R.; Baes, M.; Baldry, I. K.; Bonfield, D. G.; Cooray, A.; Croom, S. M.; Dariush, A.; de Zotti, G.; Driver, S. P.; Dye, S.; Eales, S.; Gomez, H.L.; Gonzalez-Nuevo, J.; Hopkins, A. M.; Ibar, E.; Jarvis, M.J.; Lapi, A.; Madore, B.; Michalowski, M. J.; Pohlen, M.; Popescu, C. C.; Rigby, E. E.; Seibert, M.; Smith, Daniel; Tuffs, R. J.; van der Werf, P.; Brough, S.; Buttiglione, S.; Cava, A.; Clements, D. L.; Conselice, C. J.; Fritz, J.; Hopwood, R.; Ivison, R. J.; Jones, D. H.; Kelvin, L. S.; Liske, J.; Loveday, J.; Norberg, P.; Robotham, A. S. G.; Rodighiero, G.; Temi, P. (2012-04)
    We use the Herschel-ATLAS survey to conduct the first large-scale statistical study of the submillimetre properties of optically selected galaxies. Using similar to 80 000 r-band selected galaxies from 126 deg2 of the GAMA ...
  • Hardcastle, M.J.; Jarvis, M.J.; Mauch, T.; Smith, Daniel; Stevens, J.A.; Ching, J. H. Y.; Croom, S. M.; Sadler, E.M.; Virdee, J.S.; Baes, M.; Baldry, Ivan K.; Brough, S.; Cooray, A.; Dariush, A.; Hopwood, R.; de Zotti, G.; Driver, S.; Robotham, A. S. G.; Dunne, L.; Maddox, S.; Dye, S.; Eales, S.; Valiante, E.; Liske, J.; Michałowski, M. J.; Rigby, E.E.; Steele, O.; Thomas, D. (2013-03)
    We have constructed a sample of radio-loud objects with optical spectroscopy from the Galaxy and Mass Assembly (GAMA) project over the Herschel Astrophysical Terahertz Large Area Survey (Herschel-ATLAS) Phase 1 fields. ...
  • Rowlands, K.; Dunne, L.; Maddox, S.; Bourne, N.; Gomez, H.L.; Kaviraj, S.; Bamford, S. P.; Brough, S.; Charlot, S.; da Cunha, E.; Driver, S. P.; Eales, S.~A.; Hopkins, A. M.; Kelvin, L.; Nichol, R.C.; Sansom, A. E.; Sharp, R.; Smith, Daniel; Temi, P.; van der Werf, P.; Baes, M.; Cava, A.; Cooray, A.; Croom, S. M.; Dariush, A.; de Zotti, G.; Dye, S.; Fritz, J.; Hopwood, R.; Ibar, E.; Ivison, R.J.; Liske, J.; Loveday, J.; Madore, B.; Norberg, P.; Popescu, C.; Rigby, E.; Robotham, A.; Rodighiero, G.; Seibert, M.; Tuffs, R. J. (2012-01)
    We present the dust properties and star formation histories of local submillimetre-selected galaxies, classified by optical morphology. Most of the galaxies are late types and very few are early types. The early-type ...

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