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Table 1:

13CO(3-2) Observations and results.

Observed CO(3-2) quantities:
RA (J2000) 14$^{\rm h}$ 15$^{\rm m}$ 46 $~.\!\!^{\rm s}$28 $\pm$ 0 $~.\!\!^{\rm s}$03
Dec (J2000) +11$^{\circ}$ 29' 44 $~.\!\!^{\prime\prime}$0 $\pm$0 $~.\!\!^{\prime\prime}$4
Center frequency (GHz) 92.91816
Redshift (LSR)a $2.55784\pm 0.00003$
Continuum flux density (mJy)b $0.3\pm0.1$
Integrated 13CO flux (Jy kms-1)b $0.3\pm0.1$
Derived CO(3-2) quantities:
$L^\prime$(13CO (K kms-1 pc2)c ( $1.1\pm 0.3$) $\times 10^{10}$
$L^\prime$(12CO (K kms-1 pc2)c ($45.9\pm 3$) $\times 10^{10}$
$L^\prime$ratio 12CO/13CO(3-2) 40 +25-8

Notes. (a) Adopted from 12CO (Weiss et al. 2003). (b) In a beam of 6 $~.\!\!^{\prime\prime}$$1\times 5$ $~.\!\!^{\prime\prime}$4. (c) This is the lens-amplified value for a luminosity distance of DL = 21.28 Gpc (H0 =71 kms-1 Mpc-1, $\Omega_{\rm m} = 0.27$, $\Omega_{\rm vac} = 0.73$) and an angular diameter distance of $D_{\rm A} = 1.682$ Gpc; linear scale: $1'' \leftrightarrow 8152$ pc (Wright 2006).

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