Browsing by Title

Now showing items 9858-9877 of 24055

    • 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 ...

    • A Herschel*-ATLAS study of dusty spheroids : Probing the minor-merger process in the local Universe 

      Kaviraj, S.; Rowlands, K.; Alpaslan, M.; Dunne, L.; Ting, Y. S.; Bureau, M.; Shabala, S.; Lintott, C.J.; Smith, Daniel; Agius, N.; Auld, R.; Baes, M.; Bourne, N.; Cava, A.; Clements, D. L.; Cooray, A.; Dariush, A.; de Zotti, G.; Driver, S. P.; Eales, S.; Hopwood, R.; Hoyos, C.; Ibar, E.; Maddox, S.; Michalowski, M. J.; Sansom, A. E.; Smith, M.; Valiante, E. (2013-10)
      We use multiwavelength (0.12-500 μm) photometry from Herschel-ATLAS, WISE, UKIDSS, SDSS and GALEX to study 23 nearby spheroidal galaxies with prominent dust lanes (DLSGs). DLSGs are considered to be remnants of recent minor ...

    • Herschel-Astrophysical Terahertz Large Area Survey: detection of a far-infrared population around galaxy clusters 

      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 ...

    • Herschel-ATLAS : Counterparts from the ultraviolet-near-infrared in the science demonstration phase catalogue 

      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 ...

    • Herschel-ATLAS : Multi-wavelength SEDs and physical properties of 250 μm selected galaxies at z <0.5 

      Smith, Daniel; Dunne, L.; Rowlands, K.; Maddox, S.J.; Bourne, N.; Dye, S.; Rigby, E.E.; Bonfield, D.G.; Jarvis, M.J.; da Cunha, E.; Eales, S.; Gomez, H.L.; Auld, R.; Dariush, A.; Pohlen, M.; Charlot, S.; Driver, S.P.; Kelvin, L.; Robotham, A.; Popescu, C.C.; Tuffs, R.J.; Andrae, E.; Dunlop, J.S.; Ivison, R.J.; Seymour, N.; Symeonidis, M.; Baes, M.; Fritz, J.; Clements, D.L.; Cooray, A.; De Zotti, G.; Buttiglione, S.; Scott, D.; Verma, A.; van der Werf, P.; Cava, A.; Hopwood, R.; Ibar, E.; Madore, B.F.; Seibert, M.; Temi, P. (2012-11-21)
      We present a pan-chromatic analysis of an unprecedented sample of 1402 250 μm selected galaxies at z < 0.5 (z-=0.24) from the Herschel-ATLAS survey. We complement our Herschel 100-500μm data with UV-K-band photometry from ...

    • Herschel-ATLAS : statistical properties of Galactic cirrus in the GAMA-9 Hour Science Demonstration Phase Field 

      Bracco, A.; Cooray, A.; Veneziani, M.; Amblard, A.; Serra, P.; Wardlow, J.; Thompson, Mark; White, G.; Auld, R.; Baes, M.; Bertoldi, F.; Buttiglione, S.; Cava, A.; Clements, D.; Dariush, A.; de Zotti, G.; Dunne, L.; Dye, S.; Eales, S.; Fritz, J.; Gomez, H.; Hopwood, R.; Ibar, E.; Ivison, R.J.; Jarvis, M.J.; Lagache, G.; Lee, M.G.; Leeuw, L.; Maddox, S.; Michalowski, M.; Pearson, C.; Pohlen, M.; Rigby, E.; Rodighiero, G.; Smith, Daniel; Temi, P.; Vaccari, M.; van der Werf, P. (2011)
      We study the spectral energy distribution (SED) and the power spectrum of Galactic cirrus emission observed in the 14 deg2 Science Demonstration Phase field of the Herschel-ATLAS using Herschel and IRAS data from 100 to ...

    • Herschel-ATLAS : the far-infrared properties and star-formation rates of broad absorption line quasi-stellar objects 

      Cao Orjales, J.M.; Stevens, J. A.; Jarvis, M.J.; Smith, Daniel; Hardcastle, M.J.; Auld, R.; Baes, M.; Cava, A.; Clements, D. L.; Cooray, A.; Coppin, Kristen; Dariush, A.; de Zotti, G.; Dunne, L.; Dye, S.; Eales, S.; Hopwood, R.; Hoyos, C.; Ibar, E.; Ivison, R. J.; Maddox, S.; Page, M.J.; Valiante, E. (2012-12-01)
      We have used data from the Herschel Astrophysical Terahertz Large-Area Survey (H-ATLAS) at 250, 350 and 500 μm to determine the far-infrared (FIR) properties of 50 broad absorption line quasars (BAL QSOs)

    • 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 : VISTA VIKING near-infrared counterparts in the Phase 1 GAMA 9-h data 

      Fleuren, S.; Sutherland, W.; Dunne, L.; Smith, Daniel; Maddox, S. J.; Gonzalez-Nuevo, J.; Findlay, J.; Auld, R.; Baes, M.; Bond, N. A.; Bonfield, D. G.; Bourne, N.; Cooray, A.; Buttiglione, S.; Cava, A.; Dariush, A.; De Zotti, G.; Driver, S. P.; Dye, S.; Eales, S.; Fritz, J.; Gunawardhana, M. L. P.; Hopwood, R.; Ibar, E.; Ivison, R. J.; Jarvis, M.J.; Kelvin, L.; Lapi, A.; Liske, J.; Michalowski, M. J.; Negrello, M.; Pascale, E.; Pohlen, M.; Prescott, M.; Rigby, E. E.; Robotham, A.; Scott, D.; Temi, P.; Thompson, Mark; Valiante, E.; van der Werf, P. (2012-07)
      We identify near-infrared Ks-band counterparts to Herschel Astrophysical Terahertz Large Area Survey (H-ATLAS) submillimetre (submm) sources, using a preliminary object catalogue from the VISTA Kilo-degree Infrared Galaxy ...

    • The Herschel-ATLAS Data Release 1 Paper II : Multi-wavelength counterparts to submillimetre sources 

      Bourne, N.; Dunne, L.; Maddox, S. J.; Dye, S.; Furlanetto, C.; Hoyos, C.; Smith, D. J. B.; Eales, S.; Smith, M. W. L.; Valiante, E.; Alpaslan, M.; Andrae, E.; Baldry, I. K.; Cluver, M. E.; Cooray, A.; Driver, S. P.; Dunlop, J. S.; Grootes, M. W.; Ivison, R. J.; Jarrett, T. H.; Liske, J.; Madore, B. F.; Popescu, C. C.; Robotham, A. G.; Rowlands, K.; Seibert, M.; Thompson, M. A.; Tuffs, R. J.; Viaene, S.; Wright, A. H. (2016-10-21)
      This paper is the second in a pair of articles presenting data release 1 (DR1) of the Herschel Astrophysical Terahertz Large Area Survey (H-ATLAS), the largest single open-time key project carried out with the Herschel ...

    • The Herschel-ATLAS Data Release 2, Paper I. Submillimeter and Far-infrared Images of the South and North Galactic Poles : The Largest Herschel Survey of the Extragalactic Sky 

      Smith, Matthew W. L.; Ibar, Edo; Maddox, Steve J.; Valiante, Elisabetta; Dunne, Loretta; Eales, Stephen; Dye, Simon; Furlanetto, Christina; Bourne, Nathan; Cigan, Phil; Ivison, Rob J.; Gomez, Haley; Smith, Daniel J. B.; Viaene, Sébastien (2017-12-21)
      We present the largest submillimeter images that have been made of the extragalactic sky. The Herschel Astrophysical Terahertz Large Area Survey (H-ATLAS) is a survey of 660 deg$^2$ with the PACS and SPIRE cameras in five ...

    • 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 ...

    • Herschel-ATLAS/GAMA : Spatial clustering of low-redshift submm galaxies 

      Smith, Daniel; Maddox, S.; Dunne, L.; Rigby, E.; Bamford, S.; Jarvis, M.J.; Bonfield, D.G.; Hill, D.; Hopkins, A.M.; Sharp, R.; Valtchanov, I.; Peacock, J.A.; Michałowski, M. J.; van der Werf, P.; Auld, R.; Dunlop, J.S.; Parkinson, H.; Norberg, P.; Eales, S.; Pascale, E.; Pohlen, M.; Baes, M.; Fritz, J.; Scott, D.; Robotham, A.; Driver, S.; Kelvin, L.; Ibar, E.; Ivison, R.J.; Loveday, J.; Baldry, I.K.; Prescott, M.; Cameron, E.; Croom, S.; Buttiglione, S.; de Zotti, G.; Cava, A.; Cooray, A.; Dariush, A.; Rodighiero, G.; Temi, P.; Serjeant, S.; Popescu, C.C.; Tuffs, R. J.; van Kampen, E.; Liske, J. (2012-11-11)
      We have measured the clustering properties of low-redshift (z <0.3) submm galaxies detected at 250 μm in the Herschel-ATLAS science demonstration phase field. We selected a sample for which we have high-quality spectroscopic ...

    • Herschel-ATLAS/GAMA : the environmental density of far-infrared bright galaxies at z < 0.5 

      Burton, C. S.; Jarvis, M.J.; Smith, Daniel; Bonfield, D. G.; Hardcastle, M.J.; Stevens, J. A.; Bourne, N.; Baes, M.; Brough, S.; Cava, A.; Cooray, A.; Dariush, A.; De Zotti, G.; Dunne, L.; Eales, S.; Hopwood, R.; Ibar, E.; Ivison, R. J.; Liske, J.; Loveday, J.; Maddox, S. J.; Negrello, M.; Smith, M. W. L.; Valiante, E. (2013-07)
      We compare the environmental and star formation properties of far-infrared detected and non-far-infrared detected galaxies out to z similar to 0.5. Using optical spectroscopy and photometry from the Galaxy And Mass Assembly ...

    • Herschel-ATLAS/GAMA: A difference between star formation rates in strong-line and weak-line radio galaxies 

      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. ...

    • Herschel-ATLAS/GAMA: What determines the far-infrared properties of radio galaxies? 

      Virdee, J.S.; Hardcastle, M.J.; Rawlings, S.; Rigopoulou, D.; Mauch, T.; Jarvis, M.J.; Verma, A.; Smith, Daniel; Heywood, I.; White, S. V.; Baes, M.; Cooray, A.; de Zotti, G.; Eales, S.; Michalowski, M. J.; Bourne, N.; Dariush, A.; Dunne, L.; Hopwood, R.; Ibar, E.; Maddox, S.; Smith, M. W. L.; Valiante, E. (2013-06)
      We perform a stacking analysis of Herschel Astrophysical Terahertz Large Area Survey (H-ATLAS) data in order to obtain isothermal dust temperatures and rest-frame luminosities at 250 mu m (L-250), for a well-defined sample ...

    • Herschel-ATLAS: Blazars in the science demonstration phase field 

      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 ...

    • Herschel-ATLAS: Dust temperature and redshift distribution of SPIRE and PACS detected sources using submillimetre colours 

      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 ...

    • Herschel-ATLAS: Evolution of the 250 µm luminosity function out to z = 0.5 

      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 ...

    • Herschel-ATLAS: Extragalactic number counts from 250 to 500 microns 

      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 ...