We report J, H, and K photometry of 86 stars in 40 fields in the North
ern Hemisphere. The fields are smaller than or comparable to a 4' x 4'
held of view and are roughly uniformly distributed over the sky, maki
ng them suitable for a homogeneous broadband calibration network for n
ear-infrared panoramic detectors. K magnitudes range from 8.5 to 14 an
d J-K colors, from -0.2 to 1.2. The photometry is derived from a total
of 3899 reduced images; each star has been measured, on average, 26.0
times per filter on 5.5 nights. Typical errors on the photometry are
similar to 0.012 mag.