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Resolved Dust Emission in a Quasar at z = 3.65

  • Authors: D. L. Clements, G. Petitpas, D. Farrah, E. Hatziminaoglou, T. Babbedge, M. Rowan-Robinson, I. Pérez-Fournon, Antonio Hernán-Caballero, Nieves Castro-Rodríguez, C. Lonsdale, J. Surace, A. Franceschini, B. J. Wilkes, and H. Smith

CLEMENTS et al. 2009 The Astrophysical Journal 698 L188.

  • Provider: AAS Journals

Caption: Figure 1.

850 μm image of SDSS 160705+533558. Grayscale optical image of SDSS 160705+533558, overlaid with contours from the SMA image. Contours are in steps of 1σ starting at 2σ, i.e., at fluxes of 2.4, 3.6, etc. mJy for the 1.2 mJy noise. Note the extended emission at submillimeter wavelengths and the offset of the submillimeter emission peak from the position of the optical quasar.

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