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Table 1:

Observational results for SMMJ163555, SMMJ163541, SMMJ163556.
      RA Dec $\sigma_{\rm pos}$$^\diamond$ $I_{\rm CO}$ Flux$^\dagger$ Line width
Source Transition $z_{\rm CO}$ (J2000.0) (J2000.0) [''] [Jy km s-1] [mJy] [km s-1]
SMMJ163555 CO(2-1) $1.0313\pm0.0012$ 16 35 55.05 +66 11 50.7 $\sim$0.5 $1.2\pm0.2$ $2.6\pm0.7$ $410\pm120$
  3 mm           <1.4  
SMMJ163541 CO(3-2) $3.1824\pm0.0017$ 16 35 40.86 +66 11 44.4 $\sim$0.4 $1.0\pm0.1$ $3.3\pm0.4$ $284\pm50$
  CO(3-2) $3.1883\pm0.0006$ 16 35 41.33 +66 11 46.4 $\sim$0.8 $0.3\pm0.1$ $2.6\pm0.7$ $106\pm44$
  3 mm           <0.6  
SMMJ163556 CO(4-3) 4.035-4.082 $^{\ddagger}$       < $0.45^\star$    
  3 mm           <0.44  
$^\dagger$ For line emission this refers to the peak flux, for continuum this refers to the flux density; $^{\ddagger}$ the corresponding redshift ranged in which the CO(4-3) transition would have been detectable; $^\star$ $3\sigma$ upper limit estimated assuming a line width of 400 km s-1. $^\diamond$ $\sigma_{\rm pos}$ refers to the uncertainty on the position.

Source LaTeX | All tables | In the text

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