  We report the results of a multifrequency campaign targeting S5 0716+714 in
the flaring state of the source observed in 2015 January and February. The
observations have been performed using the following instruments: Fermi/Large
Area Telescope (LAT), Nuclear Spectroscopic Telescope Array, X-ray Telescope
and Ultraciolet/Optical Telescope. The elevated flux level was visible in all
frequencies and the outburst consists of five sub-flares. In this paper we
focus on the analysis of the X-ray observations both in the soft and hard
regimes for data collected with NuStar and Swift/XRT. This is the first time,
when hard X-ray observations of the source collected with NuStar are reported.
The studies reveal both low- and high-energy components clearly visible in the
energy band, with the break energy of 8 keV, which is the highest break energy
ever reported for S5 0716+714. The second part of this work is concentrated on
multifrequency observations collected during the flaring activity period. The
variability patterns recorded during the period are characterized using a
fractional variability amplitude and description of the flare profiles. The
correlation studies reveal strong and significant relation between the optical,
ultraviolet and gamma-ray observations, and no time lag is found for any of the
studied relations.
