Browsing Faculty of Science by Author "Huang, J. -S"

Now showing items 1-7 of 7

  • AEGIS20: a radio survey of the Extended Groth Strip 

    Ivison, R. J.; Chapman, S. C.; Faber, S. M.; Smail, Ian; Biggs, A. D.; Conselice, C. J.; Wilson, G.; Salim, S.; Huang, J. -S; Wilner, S. P. (2007-05-01)
    We describe AEGIS20 - a radio survey of the Extended Groth Strip (EGS) conducted with the Very Large Array (VLA) at 1.4GHz. The resulting catalog contains 1,123 emitters and is sensitive to ultraluminous starbursts to z1 ...

  • AEGIS: Infrared Spectroscopy of An Infrared Luminous Lyman Break Galaxy at z=3.01 

    Huang, J. -S; Rigopoulou, D.; Papovich, C.; Ashby, M. L. N.; Willner, S. P.; Ivison, R.; Laird, E. S.; Webb, T.; Wilson, G.; Barmby, P.; Chapman, S.; Conselice, C.; Mcleod, B.; Shu, C. G.; Smith, H. A.; Floc'h, E. Le; Egami, E.; Willmer, C. A. N.; Fazio, G. (2007-05-01)
    We report the detection of rest--frame 6.2 and 7.7 \micron emission features arising from Polycyclic Aromatic Hydrocarbons (PAH) in the Spitzer/IRS spectrum of an infrared-luminous Lyman break galaxy at z=3.01. This is ...

  • The All-wavelength Extended Groth Strip International Survey (AEGIS) Data Sets 

    Davis, M.; Guhathakurta, P.; Konidaris, N.; Newman, J. A.; Ashby, M. L. N.; Biggs, A. D.; Barmby, P.; Bundy, K.; Chapman, S.; Coil, A. L.; Conselice, C.; Cooper, M.; Croton, D.; Eisenhardt, P.; Ellis, R.; Faber, S.; Fang, T.; Fazio, G. G.; Georgakakis, A.; Gerke, B.; Goss, W. M.; Gwyn, S.; Harker, J.; Hopkins, A.; Huang, J. -S; Ivison, R. J.; Kassin, S. A.; Kirby, E.; Koekemoer, A.; Koo, D. C.; Laird, E.; Floc'h, E. Le; Lin, L.; Lotz, J.; Marshall, P. J.; Martin, D. C.; Metevier, A.; Moustakas, L. A.; Nandra, K.; Noeske, K.; Papovich, C.; Phillips, A. C.; Rich, R. M.; Rieke, G. H.; Rigopoulou, D.; Salim, S.; Schiminovich, D.; Simard, L.; Smail, I.; Small, T. A.; Weiner, B.; Willmer, C. N. A.; Willner, S. P.; Wilson, G.; Wright, E.; Yan, R. (2007-05-01)
    In this the first of a series of Letters, we present a description of the panchromatic data sets that have been acquired in the Extended Groth Strip region of the sky. Our survey, the All-wavelength Extended Groth strip ...

  • Far-infrared characterization of an ultra-luminous starburst associated with a massively-accreting black hole at z=1.15 

    Floc'h, E. Le; Willmer, C. N. A.; Noeske, K.; Konidaris, N. P.; Laird, E. S.; Koo, D. C.; Nandra, K.; Bundy, K.; Salim, S.; Maiolino, R.; Conselice, C. J.; Lotz, J. M.; Papovich, C.; Smith, J. D.; Bai, L.; Coil, A. L.; Barmby, P.; Ashby, M. L. N.; Huang, J. -S; Blaylock, M.; Rieke, G.; Newman, J. A.; Ivison, R.; Chapman, S.; Dole, H.; Egami, E.; Elbaz, D. (2007-05-01)
    As part of the "All Wavelength Extended Groth Strip International Survey" (AEGIS), we describe the panchromatic characterization of an X-ray luminous active galactic nucleus (AGN) in a merging galaxy at z=1.15. This object ...

  • A Fully-Identified Sample of AEGIS20 Microjansky Radio Sources 

    Willner, S. P.; Ashby, M. L. N.; Barmby, P.; Chapman, S. C.; Coil, A.; Cooper, M.; Huang, J. -S; Ivison, R.; Koo, D. C. (2012-09-01)
    Infrared 3.6 to 8 micron images of the Extended Groth Strip yield plausible counterpart identifications for all but one of 510 radio sources in the AEGIS20 S(1.4 GHz) > 50 micro-Jy sample. This is the first such deep sample ...

  • Mid- to far infrared properties of star-forming galaxies and active galactic nuclei 

    Magdis, G. E.; Rigopoulou, D.; Helou, G.; Farrah, D.; Hurley, P.; Alonso-Herrero, A.; Bock, J.; Burgarella, D.; Chapman, S.; Charmandaris, V.; Cooray, A.; Dai, Y. S.; Dale, D.; Elbaz, D.; Feltre, A.; Hatziminaoglou, E.; Huang, J. -S; Morrison, G.; Oliver, S.; Page, M.; Scott, D.; Shi, Y. (2013-2013-)
    We study the mid- to far-IR properties of a 24um-selected flux-limited sample (S24 > 5mJy) of 154 intermediate redshift (~0.15), infrared luminous galaxies, drawn from the 5MUSES survey. By combining existing mid-IR ...

  • Ultra Steep Spectrum radio sources in the Lockman Hole: SERVS identifications and redshift distribution at the faintest radio fluxes 

    Afonso, J.; Bizzocchi, L.; Ibar, E.; Grossi, M.; Simpson, C.; Chapman, S.; Jarvis, M. J.; Rottgering, H.; Norris, R. P.; Dunlop, J.; Ivison, R. J.; Messias, H.; Pforr, J.; Vaccari, M.; Seymour, N.; Best, P.; González-Solares, E.; Farrah, D.; Fernandes, C. A. C.; Huang, J. -S; Lacy, M.; Maraston, C.; Marchetti, L.; Mauduit, J. -C; Oliver, S.; Rigopoulou, D.; Stanford, S. A.; Surace, J.; Zeimann, G. (2011-08-19)
    Ultra Steep Spectrum (USS) radio sources have been successfully used to select powerful radio sources at high redshifts (z>~2). Typically restricted to large-sky surveys and relatively bright radio flux densities, it has ...