  The Mission Accessible Near-Earth Objects Survey (MANOS) aims to physically
characterize sub-km Near-Earth Objects (NEOs). We report first photometric
results from the survey which began in August, 2013. Photometric observations
were performed using 1 m to 4 m class telescopes around the world. We present
rotational periods and lightcurve amplitudes for 86 sub-km NEOs, though in some
cases, only lower limits are provided. Our main goal is to obtain lightcurves
for small NEOs (typically, sub-km objects) and estimate their rotational
periods, lightcurve amplitudes, and shapes. These properties are used for
statistical study to constrain overall properties of the NEO population. A weak
correlation seems to indicate that smaller objects are more spherical than the
larger ones. We also report 7 NEOs that are fully characterized (lightcurve and
visible spectra) as the most suitable candidates for a future human or robotic
mission. Viable mission targets are objects fully characterized, with a
Delta_v(NHATS) <12 km s^-1, and a rotational period P>1h. Assuming a similar
rate of object characterization as reported in this paper, approximately 1,230
NEOs need to be characterized in order to find 100 viable mission targets.
