The description above assumes that the source signal comes only from the
(so-called) signal sideband. This is of course not true for
continuum radiation. If we neglect spectral index effects,
one can derive the proper calibration of a continuum source
from the description above. Tcal should be multiplied by
| (15) |
Similarly for spectral line observations, if you are interested
in the image band, Tcal should be multiplied by
| (16) |