  We present a large-scale survey of the central molecular zone (CMZ) of our
Galaxy, as well as a monitoring program of Sgr A*, with the AzTEC/Large
Millimeter Telescope (LMT) in the 1.1 mm continuum. Our 1.1 mm map covers the
main body of the CMZ over a field of $1.6 \times 1.1$ deg$^2$ with an angular
resolution of $10.5''$ and a depth of 15 mJy/beam. To account for the intensity
loss due to the background removal process, we combine this map with lower
resolution CSO/Bolocam and \textit{Planck}/HFI data to produce an effective
full intensity 1.1 mm continuum map. With this map and existing
\textit{Herschel} surveys, we have carried out a comprehensive analysis of the
spectral energy distribution (SED) of dust in the CMZ. A key component of this
analysis is the implementation of a model-based deconvolution approach,
incorporating the Point Spread Functions (PSFs) of the different instruments,
and hence recovering a significant amount of spatial information on angular
scales larger than $10.5''$. The monitoring of Sgr A* was carried out as part
of a worldwide, multi-wavelength campaign when the so-called G2 object was
undergoing the pericenter passage around the massive black hole (MBH). Our
preliminary results include 1) high-resolution maps of column density,
temperature and dust spectral index across the CMZ; 2) a 1.1~mm light curve of
Sgr A* showing an outburst of $140\%$ maximum amplitude on 9th May, 2014 but
otherwise only stochastic variations of $10\%$ and no systematic long-term
change, consistent with other observations.
