  We report on the VERITAS observations of the high-frequency peaked BL Lac
object 1ES 1959+650 in the period 2007-2011. This source is detected at TeV
energies by VERITAS at 16.4 standard deviation (sigma) significance in 7.6
hours of observation in a low flux state. A multiwavelength spectral energy
distribution (SED) is constructed from contemporaneous data from VERITAS,
Fermi-LAT, RXTE PCA, and Swift UVOT. Swift XRT data is not included in the SED
due to a lack of simultaneous observations with VERITAS. In contrast to the
orphan gamma-ray flare exhibited by this source in 2002, the X-ray flux of the
source is found to vary by an order of magnitude, while other energy regimes
exhibit less variable emission. A quasi-equilibrium synchrotron self-Compton
model with an additional external radiation field is used to describe three
SEDs corresponding to the lowest, highest, and average X-ray states. The
variation in the X-ray spectrum is modeled by changing the electron injection
spectral index, with minor adjustments of the kinetic luminosity in electrons.
This scenario produces small-scale flux variability of order >~2 in the HE (E>1
MeV) and VHE (E>100 GeV) gamma-ray regimes, which is corroborated by the
Fermi-LAT, VERITAS, and Whipple 10m telescope light curves.
