All Tables

• Table 1: Integrated flux densities of the lines observed in the SWS02 and LWS01 modes. Numbers in parentheses are the errors of the last significant digit.
• Table 2: Integrated flux densities (in units of 10^-18 W cm^-2), widths and peak velocities (in  km s^-1) of the lines observed in the LWS04 mode. Numbers in parentheses are the errors of the last significant digit.
• Table 3: Detailed results of the fits to the dust emission in two sources with two independent gray bodies (see text).
• Table 4: Total flux (FIR) and temperature (T) of the warm (w) and cold (c) components needed to fit the spectra with two independent gray bodies.