Following photodissociation at 248 nm of gaseous methyl formate (HC(O)OCH 3 , 0.73 Torr) and Ar (0.14 Torr), temporally resolved vibration−rotational emission spectra of highly internally excited CO (ν ≤ 11, J ≤ 27) in the 1850−2250 cm −1 region were recorded with a step-scan Fourier-transform spectrometer. The vibration−rotational distribution of CO is almost Boltzmann, with a nascent average rotational energy (E R 0 ) of 3 ± 1 kJ mol −1 and a vibrational energy (E V 0 ) of 76 ± 9 kJ mol −1 . With 3 Torr of Ar added to the system, the average vibrational energy was decreased to E V 0 = 61 ± 7 kJ mol −1 . We observed no distinct evidence of a bimodal rotational distribution for ν = 1 and 2, as reported previously [Lombardi et al., J. Phys. Chem. A 2016, 129, 5155], as evidence of a roaming mechanism. The vibrational distribution with a temperature of ∼13000 ± 1000 K, however, agrees satisfactorily with trajectory calculations of these authors, who took into account conical intersections from the S 1 state. Highly internally excited CH 3 OH that is expected to be produced from a roaming mechanism was unobserved. Following photodissociation at 193 nm of gaseous HC(O)OCH 3 (0.42 Torr) and Ar (0.09 Torr), vibration− rotational emission spectra of CO (ν ≤ 4, J ≤ 38) and CO 2 (with two components of varied internal distributions) were observed, indicating that new channels are open. Quantum-chemical calculations, computed at varied levels of theory, on the ground electronic potential-energy schemes provide a possible explanation for some of our observations. At 193 nm, the CO 2 was produced from secondary dissociation of the products HC(O)O and CH 3 OCO, and CO was produced primarily from secondary dissociation of the product HCO produced on the S 1 surface or the decomposition to CH 3 OH + CO on the S 0 surface.