  We present optical photometric and spectroscopic studies of three supernovae
(SNe) SN 2013bz, PSN J0910+5003 and ASASSN-16ex. UV-optical photometric data of
ASASSN-16ex obtained with Swift-UVOT are also analyzed. These objects were
initially classified as 09dc-like type Ia SNe. The decline rate parameters
($\Delta m_{15}(B)_{true}$) are derived as 0.92 $\pm$ 0.04 (SN 2013bz), 0.70
$\pm$ 0.05 (PSN J0910+5003) and 0.73 $\pm$ 0.03 (ASASSN-16ex). The estimated
$B$ band absolute magnitudes at maximum: $-$19.61 $\pm$ 0.20 mag for SN 2013bz,
$-$19.44 $\pm$ 0.20 mag for PSN J0910+5003 and $-$19.78 $\pm$ 0.20 mag for
ASASSN-16ex indicate that all the three objects are relatively bright. The peak
bolometric luminosities for these objects are derived as $\log
L_\text{bol}^\text{max} =$ 43.38 $\pm$ 0.07 erg s$^{-1}$, 43.26 $\pm$ 0.07 erg
s$^{-1}$ and 43.40 $\pm$ 0.06 erg s$^{-1}$, respectively. The spectral and
velocity evolution of SN 2013bz is similar to a normal SN Ia, hence it appears
to be a luminous, normal type Ia supernova. On the other hand, the light curves
of PSN J0910+5003 and ASASSN-16ex are broad and exhibit properties similar to
09dc-like SNe Ia. Their spectroscopic evolution shows similarity with 09dc-like
SNe, strong CII lines are seen in the pre-maximum spectra of these two events.
Their photospheric velocity evolution is similar to SN 2006gz. Further, in the
UV bands, ASASSN-16ex is very blue like other 09dc-like SNe Ia.
