  We present multiband photometry of 60 spectroscopically-confirmed supernovae
(SN): 39 SN II/IIP, 19 IIn, one IIb and one that was originally classified as a
IIn but later as a Ibn. Forty-six have only optical photometry, six have only
near infrared (NIR) photometry and eight have both optical and NIR. The median
redshift of the sample is 0.016. We also present 192 optical spectra for 47 of
the 60 SN. All data are publicly available. There are 26 optical and two NIR
light curves of SN II/IIP with redshifts z > 0.01, some of which may give rise
to useful distances for cosmological applications. All photometry was obtained
between 2000 and 2011 at the Fred Lawrence Whipple Observatory (FLWO), via the
1.2m and 1.3m PAIRITEL telescopes for the optical and NIR, respectively. Each
SN was observed in a subset of the $u'UBVRIr'i'JHK_s$ bands. There are a total
of 2932 optical and 816 NIR light curve points. Optical spectra were obtained
using the FLWO 1.5m Tillinghast telescope with the FAST spectrograph and the
MMT Telescope with the Blue Channel Spectrograph. Our photometry is in
reasonable agreement with other samples from the literature. Comparison with
Pan-STARRS shows that two-thirds of our individual star sequences have
weighted-mean V offsets within $\pm$0.02 mag. In comparing our standard-system
SN light curves with common Carnegie Supernova Project objects using their
color terms, we found that roughly three-quarters have average differences
within $\pm$0.04 mag. The data from this work and the literature will provide
insight into SN II explosions, help with developing methods for photometric SN
classification, and contribute to their use as cosmological distance
indicators.
