$TACTIC$ observations. The radio observations at 15 GHz available for six days are shown in Figure 2(f). No significant variations are observed in radio emission from the source during this period.

Spectral Analysis
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The spectral energy distribution of 1ES1218+304 during March 1, 2013 to April 15, 2013 using broad band data discussed above is shown in Figure 3. For VHE $\gamma$–rays we plot the data from the observations with $MAGIC$ and $VERITAS$ telescopes along with the 99$\%$ confidence level upper limit on integral flux obtained from $TACTIC$ in the present work. The flux points reported by $MAGIC$ group are based on the observations carried out during the period January 9-15, 2005 [@Alber06]. During six days of observations, no flux variability on timescales of days was found and the time averaged spectrum was described by a power law with $\Gamma=3.0\pm0.4$. The $VERITAS$ flux points taken from [@Accia09] correspond to observations during January-March 2007 for a total observation time of 17.4 h. The time averaged differential spectrum was described by a power law with photon index 3.08$\pm$0.34 and the integral flux above 200 GeV was 6$\%$ of the Crab Nebula flux. It is evident from the figure that the measured flux 