  High-precision stellar mass and radius measured directly from binaries can
effectively calibrate the stellar models. However, such a database containing
full spectral types and large range of metallicity is still not fully
established. A continuous effort of data collecting and analysis are requested
to complete the database. In this work, we provide a catalog containing 184
binaries with independent atmospheric parameters and accurate masses and radii
as the benchmark of stellar mass and radius. The catalog contains 56 new
detached binaries from LAMOST Medium-resolution spectroscopic (MRS) survey and
128 detached eclipsing binaries compiled from previous studies. We obtain the
orbital solutions of the new detached binaries with uncertainties of masses and
radii smaller than 5%. These new samples densify the distribution of
metallicity of the high-precision stellar mass library and add 9 hot stars with
Teff>8000 K. Comparisons show that these samples well agree with the PARSEC
isochrones in Teff-logg-mass-radius-luminosity space. We compare mass and
radius estimates from isochrone and SED fitting, respectively, with those from
the binary orbital solution. We find that the precision of the stellar-model
dependent mass estimates is >10% and the precision of the radius estimates
based on atmospheric parameters is >15%. These give a general view of the
uncertainty of the usual approaches to estimate stellar mass and radius.
