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The search for life in the universe is currently focused on Earth-analogplanets. However, we should be prepared to find a diversity of terrestrialexoplanets not only in terms of host star but also in terms of surfaceenvironment. Simulated high-resolution spectra of habitable planets covering awide parameter space are essential in training retrieval tools, optimizingobserving strategies, and interpreting upcoming observations. Ground-basedextremely large telescopes like ELT, GMT, and TMT; and future space-basedmission concepts like Origins, HabEx, and LUVOIR are designed to have thecapability of characterizing a variety of potentially habitable worlds. Some ofthese telescopes will use high precision radial velocity techniques to obtainthe required high-resolution spectra ($R\approx100,000$) needed to characterizepotentially habitable exoplanets.  Here we present a database of high-resolution (0.01 cm$^{-1}$) reflection andemission spectra for simulated exoplanets with a wide range of surfaces,receiving similar irradiation as Earth around 12 different host stars from F0to K7.  Depending on surface type and host star, we show differences in spectralfeature strength as well as overall reflectance, emission, and star to planetcontrast ratio of terrestrial planets in the Habitable zone of their hoststars. Accounting for the wavelength-dependent interaction of the stellar fluxand the surface will help identify the best targets for upcoming spectralobservations in the visible and infrared.  All of our spectra and model profiles are available online.

High-resolution Spectra for a Wide Range of Habitable Zone Planets around Sun-like Stars