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Fig. 7


Far-infrared luminosity versus CO(1–0) luminosity for the three galaxies summarized in Table 4: SMM J0658 (this study), SMM J16359+6612 (Kneib et al. 2005) and SMM J2135 − 0102 (Danielson et al. 2010). Local LIRGs and ULIRGs (Yao et al. 2003; Solomon et al. 1997) and high-redshift submm galaxies (Harris et al. 2010; Ivison et al. 2011) are also shown. Because SMM J16359+6612 has not been detected in CO(1–0), the CO(3–2) line luminosity was converted using r31 = 0.6 (which appears appropriate for SMGs, see Sect. 3.2.3). SMM J0658 is the least FIR-luminous high-redshift galaxy.

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