Coadded Spectroscopic Stellar Parameters and Abundances from the LAMOST
  Low Resolution Survey
  I combine duplicate spectroscopic stellar parameter estimates in the Large
Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST) Data Release 6 Low
Resolution Spectral Survey A, F, G, and K Type stellar parameter catalog.
Combining repeat measurements results in a factor of two improvement in the
precision of the spectroscopic stellar parameter estimates. Moreover, this
trivializes the process of performing coordinate-based cross-matching with
other catalogs. Similarly, I combine duplicate stellar abundance estimates for
the Xiang et al. catalog which was produced using LAMOST Data Release 5 Low
Resolution Spectral Survey data. These data have numerous applications in
stellar, galactic, and exoplanet astronomy. The catalogs I produce are
available as machine-readable tables at https://doi.org/10.7281/T1/QISGRU .
