Browsing Physics & Atmospheric Science by Author "Aretxaga, I."

Now showing items 1-9 of 9

  • The AGN fraction of submm-selected galaxies and contributions to the submm/mm-wave extragalactic background light 

    Serjeant, S.; Negrello, M.; Pearson, C.; Mortier, A.; Austermann, J.; Aretxaga, I.; Clements, D.; Chapman, S.; Dye, S.; Dunlop, J.; Dunne, L.; Farrah, D.; Hughes, D.; Lee, H. -M; Matsuhara, H.; Ibar, E.; Im, M.; Jeong, W. -S; Kim, S.; Oyabu, S.; Takagi, T.; Wada, T.; Wilson, G.; Vaccari, M.; Yun, M. (2010-02-18)
    We present a comparison of the SCUBA Half Degree Extragalactic Survey (SHADES) at 450, 850 and 1100 microns with deep guaranteed time 15 microns AKARI FU-HYU survey data and Spitzer guaranteed time data at 3.6-24 microns ...

  • AzTEC half square degree survey of the SHADES fields - II. Identifications, redshifts, and evidence for large-scale structure 

    Michałowski, M. J.; Dunlop, J. S.; Ivison, R. J.; Cirasuolo, Michele; Caputi, K. I.; Aretxaga, I.; Arumugam, V.; Austermann, J. E.; Chapin, E. L.; Chapman, S. C.; Coppin, K. E. K.; Egami, E.; Hughes, D. H.; Ibar, E.; Mortier, A. M. J.; Schael, A. M.; Scott, K. S.; Smail, I.; Targett, T. A.; Wagg, J.; Wilson, G. W.; Xu, L.; Yun, M. (2012-05-10)
    The AzTEC 1.1 mm survey of the SCUBA HAlf Degree Extragalactic Survey (SHADES) fields is the largest (0.7 deg2) blank-field millimetre-wavelength survey undertaken to date at a resolution of ~18" and a depth of ~1 mJy. We ...

  • AzTEC Half Square Degree Survey of the SHADES Fields -- I. Maps, Catalogues, and Source Counts 

    Austermann, J. E.; Dunlop, J. S.; Perera, T. A.; Scott, K. S.; Wilson, G. W.; Aretxaga, I.; Hughes, D. H.; Almaini, O.; Chapin, E. L.; Chapman, S. C.; Cirasuolo, M.; Clements, D. L.; Coppin, K. E. K.; Dunne, L.; Dye, S.; Eales, S. A.; Egami, E.; Farrah, D.; Ferrusca, D.; Flynn, S.; Haig, D.; Halpern, M.; Ibar, E.; Ivison, R. J.; van Kampen, E.; Kang, Y.; Kim, S.; Lacey, C.; Lowenthal, J. D.; Mauskopf, P. D.; McLure, R. J.; Mortier, A. M. J.; Negrello, M.; Oliver, S.; Peacock, J. A.; Pope, A.; Rawlings, S.; Rieke, G.; Roseboom, I.; Rowan-Robinson, M.; Scott, D.; Serjeant, S.; Smail, I.; Swinbank, A. M.; Stevens, J. A.; Velazquez, M.; Wagg, J.; Yun, M. S. (2009-07-06)
    We present the first results from the largest deep extragalactic millimetre-wavelength survey undertaken to date. These results are derived from maps covering over 0.7 deg^2, made at 1.1mm, using the AzTEC continuum camera ...

  • The SCUBA HAlf Degree Extragalactic Survey (SHADES) - III. Identification of radio and mid-infrared counterparts to submillimetre galaxies 

    Ivison, R. J.; Greve, T. R.; Dunlop, J. S.; Peacock, J. A.; Egami, E.; Smail, Ian; Ibar, E.; van Kampen, E.; Aretxaga, I.; Babbedge, T.; Biggs, A. D.; Blain, A. W.; Chapman, S. C.; Clements, D. L.; Coppin, K.; Farrah, D.; Halpern, M.; Hughes, D. H.; Jarvis, M. J.; Jenness, T.; Jones, J. R.; Mortier, A. M. J.; Oliver, S.; Papovich, C.; Perez-Gonzalez, P. G.; Pope, A.; Rawlings, S.; Rieke, G. H.; Rowan-Robinson, M.; Savage, R. S.; Scott, D.; Seigar, M.; Serjeant, S.; Simpson, C.; Stevens, J. A.; Vaccari, M.; Wagg, J.; Willott, C. J. (2007-07-27)
    Determining an accurate position for a submm galaxy (SMG) is the crucial step that enables us to move from the basic properties of an SMG sample - source counts and 2-D clustering - to an assessment of their detailed, ...

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

    Dye, Simon; Eales, S. A.; Aretxaga, I.; Serjeant, S.; Dunlop, J. S.; Babbedge, T. S. R.; Chapman, S. C.; Cirasuolo, M.; Clements, D. L.; Coppin, K. E. K.; Dunne, L.; Egami, E.; Farrah, D.; Ivison, R. J.; van Kampen, E.; Pope, A.; Priddey, R.; Rieke, G. H.; Schael, A. M.; Scott, D.; Simpson, C.; Takagi, T.; Takata, T.; Vaccari, M. (2008-05)
    We present estimates of the photometric redshifts, stellar masses and star formation histories of sources in the SCUBA HAlf Degree Extragalactic Survey (SHADES). This paper describes the 60 SCUBA sources detected in the ...

  • The SCUBA HAlf Degree Extragalactic Survey (SHADES) -- II. Submillimetre maps, catalogue and number counts 

    Coppin, K.; Chapin, E. L.; Mortier, A. M. J.; Scott, S. E.; Borys, C.; Dunlop, J. S.; Halpern, M.; Hughes, D. H.; Pope, A.; Scott, D.; Serjeant, S.; Wagg, J.; Alexander, D. M.; Almaini, O.; Aretxaga, I.; Babbedge, T.; Best, P. N.; Blain, A.; Chapman, S.; Clements, D. L.; Crawford, M.; Dunne, L.; Eales, S. A.; Edge, A. C.; Farrah, D.; Gaztanaga, E.; Gear, W. K.; Granato, G. L.; Greve, T. R.; Fox, M.; Ivison, R. J.; Jarvis, M. J.; Jenness, T.; Lacey, C.; Lepage, K.; Mann, R. G.; Marsden, G.; Martinez-Sansigre, A.; Oliver, S.; Page, M. J.; Peacock, J. A.; Pearson, C. P.; Percival, W. J.; Priddey, R. S.; Rawlings, S.; Rowan-Robinson, M.; Savage, R. S.; Seigar, M.; Sekiguchi, K.; Silva, L.; Simpson, C.; Smail, I.; Stevens, J. A.; Takagi, T.; Vaccari, M.; van Kampen, E.; Willott, C. J. (2006-11-11)
    We present the maps, source catalogue and number counts of the largest, most complete and unbiased extragalactic submillimetre survey ever undertaken: the 850-micron SCUBA HAlf Degree Extragalactic Survey (SHADES). Using ...

  • The SCUBA HAlf Degree Extragalactic Survey (SHADES) -- V. Submillimetre properties of near-infrared--selected galaxies in the Subaru/XMM--Newton deep field 

    Takagi, T.; Mortier, A. M. J.; Shimasaku, K.; Coppin, K.; Pope, A.; Ivison, R. J.; Hanami, H.; Serjeant, S.; Clements, D. L.; Priddey, R. S.; Dunlop, J. S.; Takata, T.; Aretxaga, I.; Chapman, S. C.; Eales, S. A.; Farrah, D.; Granato, G. L.; Halpern, M.; Hughes, D. H.; van Kampen, E.; Scott, D.; Sekiguchi, K.; Smail, I.; Vaccari, M. (2007-09-28)
    We have studied the submillimetre (submm) properties of the following classes of near-infrared (NIR)-selected massive galaxies at high redshifts: BzK-selected star-forming galaxies (BzKs); distant red galaxies (DRGs); and ...

  • The SCUBA HAlf-Degree Extragalactic Survey (SHADES) - VIII. The Nature of Faint Submm 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, Dave; Waddington, I.; Simpson, C.; Furusawa, H.; Serjeant, S.; Afonso-Luis, A.; Alexander, D. M.; Aretxaga, I.; Blain, A.; Borys, C.; Chapman, S.; Coppin, K.; 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, A. M. J.; Page, M. J.; Pope, A.; Priddey, R. S.; Rawlings, S.; Savage, R. S.; Scott, D.; Scott, S. E.; Sekiguchi, K.; Smail, I.; Smith, H. E.; Stevens, J. A.; Surace, J.; Takagi, T.; van Kampen, E. (2008-06)
    We present the optical-to-submm spectral energy distributions for 33 radio & mid-IR identified submillimetre galaxies discovered via the SHADES 850 micron SCUBA imaging in the Subaru-XMM Deep Field (SXDF). Optical data for ...

  • The SCUBA-2 Cosmology Legacy Survey: blank-field number counts of 450um-selected galaxies and their contribution to the cosmic infrared background 

    Geach, J. E.; Chapin, E. L.; Coppin, K. E. K.; Dunlop, J. S.; Halpern, M.; Smail, Ian; van der Werf, P.; Serjeant, S.; Farrah, D.; Roseboom, I.; Targett, T.; Arumugam, V.; Asboth, V.; Blain, A.; Chrysostomou, A.; Clarke, C.; Ivison, R. J.; Jones, S. L.; Karim, A.; Mackenzie, T.; Meijerink, R.; Michalowski, M. J.; Scott, D.; Simpson, J.; Swinbank, A. M.; Alexander, D.; Almaini, O.; Aretxaga, I.; Best, P.; Chapman, S.; Clements, D. L.; Conselice, C.; Danielson, A. L. R.; Eales, S.; Edge, A. C.; Gibb, A.; Hughes, D.; Jenness, T.; Knudsen, K. K.; Lacey, C.; Marsden, G.; McMahon, R.; Oliver, S.; Page, M. J.; Peacock, J. A.; Rigopoulou, D.; Robson, E. I.; Spaans, M.; Stevens, J.; Webb, T. M. A.; Willott, C.; Wilson, C. D.; Zemcov, M. (2012-11-28)
    The first deep blank-field 450um map (1-sigma~1.3mJy) from the SCUBA-2 Cosmology Legacy Survey (S2CLS), conducted with the James Clerk Maxwell Telescope (JCMT) is presented. Our map covers 140 arcmin^2 of the COSMOS field, ...