There is a diversity in  the electron energy distribution in Gamma Ray
Burst  Afterglows.   The  power-law  index  of   the  electron  energy
distribution, commonly denoted  as 'p', seems to vary  between ~ 1.5 -
2.7. We present here  two cases of GRB afterglows.  GRB 041006 shows a
'hard' electron energy distribution. The multiband afterglow evolution
shows p  to be ~  1.3. GRB 060124  exhibits a curved spectrum  with an
injection break at high energy. We present the earliest ground based R
band observations for  GRB 060124 afterglow and look  for the evidence
of a jet break in its  light curve. We conclude that the optical light
curve shows  no break whereas the  X-ray light curve  shows a distinct
break  around  0.6  d.  We  attribute  this  'chromatic'  break  to  a
steepening of the electron energy spectrum at high energies.