Observing Cold Gas in Submillimeter Galaxies: Detection of CO (1→0) Emission in SMM J13120+4242 with the Green Bank Telescope

Abstract

We report the first detection of CO (1→0) emission from a submillimeter-selected galaxy, using the Green Bank Telescope. We identify the line in the spectrum of SMM J13120+4242 as a broad emission feature at z = 3.408, with ΔV_(FWHM) = 1040 ± 190 km s^(-1). If the observed CO (1→0) line profile arises from a single object and not several merging objects, then the CO (4 → 3)/CO (1 → 0) brightness temperature ratio of ~0.26 suggests n(H_2) > (3-10) × 10^2 cm^(-3) and the presence of subthermally excited gas. The integrated line flux implies a cold molecular gas mass M(H_2) = 1.6 × 10^(11) M_☉, comparable to the dynamical mass estimate and 4 times larger than the H_2 mass predicted from the CO (4→3) line, assuming a brightness temperature ratio of 1.0. While our observations confirm that this submillimeter galaxy is massive and gas-rich, they also suggest that extrapolating gas masses from J_(upper) ≥ 3 transitions of CO leads to considerable uncertainties. We also report an upper limit to the mass of cold molecular gas in a second submillimeter galaxy, SMM J09431+4700, of M(H_2) ≲ 4 × 10^(10) M_☉.