Now showing items 1-3 of 3

  • 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 ...
  • 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 ...