Browsing University of Hertfordshire by Author "Dye, S."

Now showing items 41-60 of 73

    • 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 ...

    • Herschel-ATLAS: first data release of the Science Demonstration Phase source catalogues 

      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 ...

    • Herschel-ATLAS: properties of dusty massive galaxies at low and high redshifts 

      Rowlands, K.; Dunne, L.; Dye, S.; Aragón-Salamanca, A.; Maddox, S.; da Cunha, E.; Smith, Daniel; Bourne, N.; Eales, S.; Gomez, H.L.; Smail, I.; Alpaslan, M.; Clark, C.J.R.; Driver, S.; Ibar, E.; Ivison, Rob J.; Robotham, A.; Smith, M.W.L.; Valiante, E. (2014-06-21)
      We present a comparison of the physical properties of a rest-frame 250-μm-selected sample of massive, dusty galaxies from 0 < z < 5.3. Our sample comprises 29 high-redshift submillimetre galaxies (SMGs) from the literature ...

    • Herschel-ATLAS: Revealing dust build-up and decline across gas, dust and stellar mass selected samples: I. Scaling relations 

      Vis, P. De; Dunne, L.; Maddox, S.; Gomez, H. L.; Clark, C. J. R.; Bauer, A. E.; Viaene, S.; Schofield, S. P.; Baes, M.; Baker, A. J.; Bourne, N.; Driver, S. P.; Dye, S.; Eales, S. A.; Furlanetto, C.; Ivison, R. J.; Robotham, A. S. G.; Rowlands, K.; Smith, D. J. B.; Smith, M. W. L.; Valiante, E.; Wright, A. H. (2017-02-01)
      We present a study of the dust, stars and atomic gas (HI) in an HI-selected sample of local galaxies (z 80 per cent), low stellar mass sources that appear to be in the earliest stages of their evolution. We compare this ...

    • Herschel-ATLAS: The angular correlation function of submillimetre galaxies at high and low redshift 

      Maddox, S.; Dunne, L.; Rigby, E.; Eales, S.; Cooray, A.; Scott, D.; Peacock, J.A.; Negrello, M.; Smith, Daniel; Benford, D.; Amblard, A.; Auld, R.; Baes, M.; Bonfield, D.; Burgarella, D.; Buttiglione, S.; Cava, A.; Clements, D.; Dariush, A.; de Zotti, G.; Dye, S.; Frayer, D.; Fritz, J.; Gonzalez-Nuevo, J.; Herranz, D.; Ibar, E.; Ivison, R.J.; Jarvis, M.J.; Lagache, G.; Leeuw, L.; Lopez-Caniego, M.; Pascale, E.; Pohlen, M.; Rodighiero, G.; Samui, S.; Serjeant, S.; Temi, P.; Thompson, M.A.; Verma, A. (2010)
      We present measurements of the angular correlation function of galaxies selected from the first field of the H-ATLAS survey. Careful removal of the background from galactic cirrus is essential, and currently dominates the ...

    • Herschel-ATLAS: The dust energy balance in the edge-on spiral galaxy UGC 4754 

      Baes, M.; Fritz, J.; Gadotti, D.A.; Smith, Daniel; Dunne, L.; da Cunha, E.; Amblard, A.; Auld, R.; Bendo, G.; Bonfield, D.; Burgarella, D.; Buttiglione, S.; Cava, A.; Clements, D.; Cooray, A.; Dariush, A.; de Zotti, G.; Dye, S.; Eales, S.; Frayer, D.; Gonzalez-Nuevo, J.; Herranz, D.; Ibar, E.; Ivison, R.J.; Lagache, G.; Leeuw, L.; Lopez-Caniego, M.; Jarvis, M.J.; Maddox, S.; Negrello, M.; Michalowski, M.; Pascale, E.; Pohlen, M.; Rigby, E.; Rodighiero, G.; Samui, S.; Serjeant, S.; Temi, P.; Thompson, M.A.; van der Werf, P.; Verma, A.; Vlahakis, C. (2010)
      We use Herschel PACS and SPIRE observations of the edge-on spiral galaxy UGC 4754, taken as part of the H-ATLAS SDP observations, to investigate the dust energy balance in this galaxy. We build detailed SKIRT radiative ...

    • Herschel-ATLAS: the far-infrared-radio correlation at z <0.5 

      Jarvis, M.J.; Smith, Daniel; Bonfield, David G.; Hardcastle, M.J.; Falder, J. T.; Stevens, Jason; Ivison, R.J.; Auld, R.; Baes, M.; Baldry, I.K.; Bamford, S. P.; Bourne, N.; Buttiglione, S.; Cava, A.; Cooray, A.; Dariush, A.; de Zotti, G.; Dunlop, J. S.; Dunne, L.; Dye, S.; Eales, S.; Fritz, J.; Hill, D. T.; Hopwood, R.; Hughes, D.H.; Ibar, E.; Jones, D. H.; Kelvin, L.; Lawrence, A.; Leeuw, L.; Loveday, J.; Maddox, S. J.; Michalowski, M. J.; Negrello, M.; Norberg, P.; Pohlen, M.; Prescott, M.; Rigby, E. E.; Robotham, A.; Rodighiero, G.; Scott, D.; Sharp, R.; Temi, P.; Thompson, Mark; van der Werf, P.; van Kampen, E.; Vlahakis, C.; White, G. (2010)
      We use data from the Herschel-ATLAS to investigate the evolution of the far-infrared–radio correlation over the redshift range 0 < z < 0.5. Using the total far-infrared luminosity of all >5σ sources in the Herschel-ATLAS ...

    • Herschel-ATLAS: the link between accretion luminosity and star formation in quasar host galaxies 

      Bonfield, D. G.; Jarvis, M.J.; Hardcastle, M.J.; Cooray, A.; Hatziminaoglou, E.; Ivison, R. J.; Page, M. J.; Stevens, J. A.; de Zotti, G.; Auld, R.; Baes, M.; Buttiglione, S.; Cava, A.; Dariush, A.; Dunlop, J. S.; Dunne, L.; Dye, S.; Eales, S.; Fritz, J.; Hopwood, R.; Ibar, E.; Maddox, S. J.; Michalowski, M. J.; Pascale, E.; Pohlen, M.; Rigby, E. E.; Rodighiero, G.; Serjeant, S.; Smith, Daniel; Temi, P.; van der Werf, P. (2011-09)
      We use the science demonstration field data of the Herschel Astrophysical Terahertz Large Area Survey to study how star formation, traced by the far-infrared Herschel data, is related to both the accretion luminosity and ...

    • Lens magnification by CL0024+1654 in the and band 

      Dye, S.; Taylor, A.N.; Greve, T.R.; Rognvaldsson, O.E.; van Kampen, E.; Jakobsson, P.; Sigmundsson, V.S.; Gudmundsson, E.H.; Hjorth, J. (2002)

    • A Magnified View of Circumnuclear Star Formation and Feedback around an Active Galactic Nucleus at z = 2.6 

      Geach, J. E.; Ivison, R. J.; Dye, S.; Oteo, I. (2018-10-10)
      We present Atacama Large Millimeter/submillimeter Array observations of an intrinsically radio-bright (L 1.4 GHz = (1.7 ± 0.1) ×10 25 W Hz -1) and infrared luminous (L IR ≈ 10 13 L o) galaxy at z = 2.6. The infrared-to-radio ...

    • Measurements of CO Redshifts with Z-Spec for Lensed Submillimeter Galaxies Discovered in the H-ATLAS Survey 

      Lupu, R. E.; Scott, K.S.; Aguirre, J.E.; Aretxaga, I.; Auld, R.; Barton, E.; Beelen, A.; Bertoldi, F.; Bock, J.J.; Bonfield, D.; Bradford, C.M.; Buttiglione, S.; Cava, A.; Clements, D. L.; Cooke, J.; Cooray, A.; Dannerbauer, H.; Dariush, A.; de Zotti, G.; Dunne, L.; Dye, S.; Eales, S.; Frayer, D.; Fritz, J.; Glenn, J.; Hughes, D.H.; Ibar, E.; Ivison, Rob J.; Jarvis, M.J.; Kamenetzky, J.; Kim, S.; Lagache, G.; Leeuw, L.; Maddox, S.; Maloney, P. R.; Matsuhara, H.; Murphy, E. J.; Naylor, B.J.; Negrello, M.; Nguyen, H.; Omont, A.; Pascale, E.; Pohlen, M.; Rigby, E.; Rodighiero, G.; Serjeant, S.; Smith, Daniel; Temi, P.; Thompson, M.; Valtchanov, I.; Verma, A.; Vieira, J. D.; Zmuidzinas, J. (2012-10-01)
      We present new observations from Z-Spec, a broadband 185-305 GHz spectrometer, of five submillimeter bright lensed sources selected from the Herschel-Astrophysical Terahertz Large Area Survey science demonstration phase ...

    • Mid-infrared spectroscopy of candidate AGN-dominated submillimeter galaxies 

      Coppin, Kristen; Pope, A.; Menendez-Delmestre, K.; Alexander, D. M.; Dunlop, J. S.; Egami, E.; Gabor, J.; Ibar, Edo; Ivison, R. J.; Austermann, J. E.; Blain, A. W.; Chapman, S. C.; Clements, D. L.; Dunne, L.; Dye, S.; Farrah, D.; Hughes, D. H.; Mortier, A. M. J.; Page, M. J.; Rowan-Robinson, M.; Scott, D.; Simpson, C.; Smail, Ian; Swinbank, A. M.; Vaccari, M.; Yun, M. S. (2010)
      Spitzer spectroscopy has revealed that ~80% of submm galaxies (SMGs) are starburst (SB) dominated in the mid-infrared. Here we focus on the remaining ~20% that show signs of harboring powerful active galactic nuclei (AGN). ...

    • Mining the Herschel-astrophysical terahertz large area survey : Submillimetre-selected blazars in equatorial fields 

      López-Caniego, M.; González-Nuevo, J.; Massardi, M.; Bonavera, L.; Herranz, D.; Negrello, M.; De Zotti, G.; Carrera, F. J.; Danese, L.; Fleuren, S.; Hardcastle, M.J.; Jarvis, M.J.; Klöckner, H. R.; Mauch, T.; Procopio, P.; Righini, S.; Sutherland, W.; Auld, R.; Baes, M.; Buttiglione, S.; Clark, C. J. R.; Cooray, A.; Dariush, A.; Dunne, L.; Dye, S.; Eales, S. (2013-04-11)
      The Herschel-Astrophysical Terahertz Large Area Survey (H-ATLAS) provides an unprecedented opportunity to search for blazars at sub-mm wavelengths. We cross-matched the Faint Images of the Radio Sky at Twenty-cm (FIRST) ...

    • [NII] fine-structure emission at 122 and 205um in a galaxy at z=2.6: a globally dense star-forming interstellar medium 

      Doherty, M. J.; Geach, J. E.; Ivison, R. J.; Dye, S. (2020-12-23)
      We present new observations with the Atacama Large Millimeter/sub-millimeter Array of the 122um and 205um fine-structure line emission of singly-ionised nitrogen in a strongly lensed starburst galaxy at z=2.6. The 122/205um ...

    • Observation of H2O in a strongly lensed Herschel-ATLAS source at z=2.3 

      Omont, A.; Neri, R.; Cox, P.; Lupu, R.; Guelin, M.; van der Werf, P.; Weiss, A.; Ivison, R.J.; Negrello, M.; Leeuw, L.; Lehnert, M.D.; Smail, I.; Verma, A.; Baker, A.J.; Beelen, A.; Aguirre, J.E.; Baes, M.; Bertoldi, F.; Clements, D.; Cooray, A.; Coppin, Kristen; Dannerbauer, H.; de Zotti, G.; Dye, S.; Fiolet, N.; Frayer, D.; Gavazzi, R.; Hughes, D.H.; Jarvis, M.J.; Krips, M.; Michalowski, M.; Murphy, E.; Riechers, D.; Serjeant, S.; Swinbank, A.M.; Temi, P.; Vaccari, M.; Vieira, J.; Auld, R.; Buttiglione, B.; Cava, A.; Dariush, A.; Dunne, L.; Eales, S.; Fritz, J.; Gomez, H.L.; Ibar, E.; Maddox, S.; Pascale, E.; Pohlen, M.; Rigby, E.; Smith, Daniel; Bock, J.; Bradford, C.M.; Glenn, J.; Scott, K.S.; Zmuidzinas, J. (2011)
      The Herschel survey, H-ATLAS, with its large areal coverage, has recently discovered a number of bright, strongly lensed high-z submillimeter galaxies. The strong magnification makes it possible to study molecular species ...

    • Physical conditions of the interstellar medium of high-redshift, strongly lensed submillimetre galaxies from the Herschel-ATLAS 

      Valtchanov, I.; Virdee, J.; Ivison, R.J.; Swinyard, B.; van der Werf, P.; Rigopoulou, D.; da Cunha, E.; Lupu, R.; Benford, D. J.; Riechers, D.; Smail, Ian; Jarvis, M.J.; Pearson, C.; Gomez, H.; Hopwood, R.; Altieri, B.; Birkinshaw, M.; Coia, D.; Conversi, L.; Cooray, A.; de Zotti, G.; Dunne, L.; Frayer, D.; Leeuw, L.; Marston, A.; Negrello, M.; Portal, M. Sanchez; Scott, D.; Thompson, M.A.; Vaccari, M.; Baes, M.; Clements, D.; Michalowski, M. J.; Dannerbauer, H.; Serjeant, S.; Auld, R.; Buttiglione, S.; Cava, A.; Dariush, A.; Dye, S.; Eales, S.; Fritz, J.; Ibar, E.; Maddox, S.; Pascale, E.; Pohlen, M.; Rigby, E.; Rodighiero, G.; Smith, Daniel; Temi, P.; Carpenter, J.; Bolatto, A.; Gurwell, M.; Vieira, J. D. (2011-08-01)
      We present Herschel-Spectral and Photometric Imaging Receiver (SPIRE) Fourier transform spectrometer (FTS) and radio follow-up observations of two Herschel-Astrophysical Terahertz Large Area Survey (H-ATLAS)-detected ...

    • Polarized thermal emission from dust in a galaxy at redshift 2.6 

      Geach, Jim; Lopez Rodriguez, Enrique; Doherty, M.J.; Chen, Jianhang; Ivison, R. J.; Bendo, G.J.; Dye, S.; Coppin, Kristen (2023-09-06)
      Magnetic fields are fundamental to the evolution of galaxies, playing a key role in the astrophysics of the interstellar medium and star formation. Large-scale ordered magnetic fields have been mapped in the Milky Way and ...

    • The SCUBA Half Degree Extragalactic Survey (SHADES) - IX : the environment, mass and redshift dependence of star formation 

      Serjeant, S.; Dye, S.; Mortier, A.; Peacock, J.; Egami, E.; Cirasuolo, M.; Rieke, G.; Borys, C.; Chapman, S.; Clements, D.; Coppin, Kristen; Dunlop, J.; Eales, S.; Farrah, D.; Halpern, M.; Mauskopf, P.; Pope, A.; Rowan-Robinson, M.; Scott, D.; Smail, I.; Vaccari, M. (2008-06-01)
      We present a comparison between the SCUBA (Submillimetre Common User Bolometer Array) Half Degree Extragalactic Survey (SHADES) at 450 and 850 μm in the Lockman Hole East with a deep Spitzer Space Telescope survey at 3.6-24 ...

    • The SCUBA HAlf Degree Extragalactic Survey (SHADES) - VII. Optical/IR photometry and stellar masses of sub-millimeter galaxies 

      Dye, S.; Eales, S.; Aretxaga, I.; Serjeant, S.; Dunlop, J.S.; Babbedge, T.; Chapman, S.; Cirasuolo, M.; Clements, D.; Coppin, Kristen; Dunne, L.; Egami, E.; Farrah, D.; Ivison, R.J.; van Kampen, E.; Pope, A.; Priddey, R.; Rieke, G.; Schael, A.M.; Scott, D.; Simpson, C.; Takagi, T.; Takata, T.; Vaccari, M. (2008)