  We present [Fe II] 1.64 {\mu}m imaging observations for jets and outflows
from young stellar objects (YSOs) over the northern part (~ 24'x45') of the
Carina Nebula, a massive star forming region. The observations were performed
with IRIS2 of Anglo-Australian Telescope and the seeing was ~1.5"+-0.5". Eleven
jet and outflow features are detected at eight different regions, and are named
as Ionized Fe Objects (IFOs). One Herbig-Haro object candidate missed in Hubble
Space Telescope H{\alpha} observations is newly identified as HHc-16, referring
our [Fe II] images. IFOs have knotty or longish shapes, and the detection rate
of IFOs against previously identified YSOs is 1.4 %, which should be treated as
a lower limit. Four IFOs show an anti-correlated peak intensities in [Fe II]
and H{\alpha}, where the ratio I([Fe II])/I(H{\alpha}) is higher for longish
IFOs than for knotty IFOs. We estimate the outflow mass loss rate from the [Fe
II] flux, using two different methods. The jet-driving objects are identified
for three IFOs (IFO-2, -4, and -7), for which we study the relations between
the outflow mass loss rate and the YSO physical parameters from the radiative
transfer model fitting. The ratios of the outflow mass loss rate over the disk
accretion rate are consistent for IFO-4 and -7 with the previously reported
values (10^-2-10^+1), while it is higher for IFO-2. This excess may be from the
underestimation of the disk accretion rate. The jet-driving objects are likely
to be low- or intermediate-mass stars. Other YSO physical parameters, such as
luminosity and age, show reasonable relations or trends.
