Browsing University of Hertfordshire by Author "Eales, S.A."

Now showing items 1-5 of 5

    • Accounting for the foreground contribution to the dust emission towards Kepler's supernova remnant 

      Gomez, H.L.; Dunne, L.; Ivison, R.J.; Reynoso, E.M.; Thompson, M.A.; Sibthorpe, B.; Eales, S.A.; Delaney, T.M.; Maddox, S.; Isaak, K. (2009)
      Whether or not supernovae contribute significantly to the overall dust budget is a controversial subject. Submillimetre (sub-mm) observations, sensitive to cold dust, have shown an excess at 450 and 850 μm in young remnants ...

    • First results from HerMES on the evolution of the submillimetre luminosity function 

      Eales, S.A.; Raymond, G.; Roseboom, I.G.; Altieri, B.; Amblard, A.; Arumugam, V.; Auld, R.; Aussel, H.; Babbedge, T.; Blain, A.; Bock, J.; Boselli, A.; Brisbin, D.; 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.; Elbaz, D.; Farrah, D.; Fox, M.; Franceschini, A.; Gear, W.; Glenn, J.; González Solares, E.A.; Griffin, M.; Harwit, M.; Hatziminaoglou, E.; Huang, J.; Ibar, E.; Isaak, K.; Ivison, R.J.; Lagache, G.; Levenson, L.; Lonsdale, C.J.; Lu, N.; Madden, S.; Maffei, B.; Mainetti, G.; Marchetti, L.; Morrison, G.E.; Mortier, A.M.J.; Nguyen, H.T.; O'Halloran, B.; Oliver, S.J.; Omont, A.; Owen, F.N.; Page, M.J.; Pannella, M.; Panuzzo, P.; Papageorgiou, A.; Pearson, C.P.; Pérez-Fournon, I.; Pohlen, M.; Rawlings, J.I.; Rigopoulou, D.; Rizzo, D.; Rowan-Robinson, M.; Sánchez Portal, M.; Schulz, B.; Scott, D.; Seymour, N.; Shupe, D. L.; Stevens, Jason; Strazzullo, V.; Symeonidis, M.; Trichas, M.; Tugwell, K.E.; Vaccari, M.; Valtchanov, I.; Vigroux, L.; Wang, L.; Ward, R.; Wright, G.; Xu, C.K.; Zemcov, M. (2010-07-01)
      We have carried out two extremely deep surveys with SPIRE, one of the two cameras on Herschel, at 250 μm, close to the peak of the far-infrared background. We have used the results to investigate the evolution of the ...

    • Herschel -ATLAS/GAMA : Dusty early-type galaxies and passive spirals 

      Rowlands, K.; Dunne, L.; Maddox, S.; Bourne, N.; Bamford, S. P.; Smith, Daniel; Dye, S.; Rigby, E.E.; Gomez, H.L.; Eales, S.A.; Kaviraj, S.; Dariush, A.; Hopwood, R.; Brough, S.; Hopkins, A. M.; Charlot, S.; da Cunha, E.; Driver, S. P.; Kelvin, L.; Robotham, A.; Nichol, R.C.; Sansom, A. E.; Popescu, C.C.; Sharp, R.; Temi, P.; van der Werf, P.; Baes, M.; Fritz, J.; Cava, A.; Cooray, A.; Croom, S. M.; de Zotti, G.; Rodighiero, G.; Ibar, E.; Ivison, R.J.; Norberg, P.; Liske, J.; Loveday, J.; Madore, B.; Seibert, M.; Tuffs, R. J. (2012)
      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 ...

    • The Herschel Space Observatory view of dust in M81 

      Bendo, G. J.; Wilson, C. D.; Pohlen, M.; Sauvage, M.; Auld, R.; Baes, M.; Barlow, M.J.; Bock, J. J.; Boselli, A.; Bradford, M.; Buat, V.; Castro-Rodriguez, N.; Chanial, P.; Charlot, S.; Ciesla, L.; Clements, D. L.; Cooray, A.; Cormier, D.; Cortese, L.; Davies, J.I.; Dwek, E.; Eales, S.A.; Elbaz, D.; Galametz, M.; Galliano, F.; Gear, W.K.; Glenn, J.; Gomez, H.L.; Griffin, M.; Hony, S.; Isaak, K.G.; Levenson, L. R.; Lu, N.; Madden, S.; O'Halloran, B.; Okumura, K.; Oliver, S.; Page, M. J.; Panuzzo, P.; Papageorgiou, A.; Parkin, T.J.; Perez-Fournon, I.; Rangwala, N.; Rigby, E. E.; Roussel, H.; Rykala, A.; Sacchi, N.; Schulz, B.; Schirm, M. R. P.; Smith, M. W. L.; Spinoglio, L.; Stevens, Jason; Sundar, S.; Symeonidis, M.; Trichas, M.; Vaccari, M.; Vigroux, L.; Wozniak, H.; Wright, G. S.; Zeilinger, W.W. (2010-07-01)
      We use Herschel Space Observatory data to place observational constraints on the peak and Rayleigh-Jeans slope of dust emission observed at 70–500 μm in the nearby spiral galaxy M81. We find that the ratios of wave bands ...

    • On the origin of M81 group extended dust emission 

      Davies, J.I.; Wilson, C. D.; Auld, R.; Baes, M.; Barlow, M.J.; Bendo, G. J.; Bock, J.; Boselli, A.; Bradford, M.; Buat, V.; Castro-Rodriguez, N.; Chanial, P.; Charlot, S.; Ciesla, L.; Clements, D. L.; Cooray, A.; Cormier, D.; Cortese, L.; Dwek, E.; Eales, S.A.; Elbaz, D.; Galametz, M.; Galliano, F.; Gear, W.K.; Glenn, J.; Gomez, H.L.; Griffin, M.; Hony, S.; Isaak, K.G.; Levenson, L.R.; Lu, N.; Madden, S.; O'Halloran, B.; Okumura, K.; Oliver, S.; Page, M. J.; Panuzzo, P.; Papageorgiou, A.; Parkin, T.J.; Perez-Fournon, I.; Pohlen, M.; Rangwala, N.; Rigby, E.; Roussel, H.; Rykala, A.; Sacchi, N.; Sauvage, M.; Schulz, B.; Schirm, M.R.P.; Smith, M. W. L.; Spinoglio, L.; Stevens, Jason; Srinivasan, S.; Symeonidis, M.; Trichas, M.; Vaccari, M.; Vigroux, L.; Wozniak, H.; Wright, G. S.; Zeilinger, W.W. (2010-11-01)
      Galactic cirrus emission at far-infrared wavelengths affects many extragalactic observations. Separating this emission from that associated with extragalactic objects is both important and difficult. In this paper we discuss ...