To understand the mass distribution and co-evolution of supermassive black holes with their host galaxy, it is crucial to measure the black hole mass of AGN. Reverberation mapping is a unique tool to estimate the black hole masses in AGN. We performed spectroscopic reverberation study using long-term monitoring data with more than 100 spectra of a radio-loud quasar PKS 0736+017 to estimate the size of the broad line region (BLR) and black hole mass. The optical spectrum shows strong H$\mathrm{ \beta}$ and H$\mathrm{ \gamma}$ emission lines. We generated the light curves of 5100{ \AA} continuum flux ($f_{ 5100}$), H$\beta$, and H$\gamma$. All the light curves are found to be strongly variable with fractional variability of 69$\%$, 21$\%$, 30$\%$ for V-band, H$\beta$, and H$\gamma$ light curves, respectively. Along with the thermal contribution, non-thermal emission contributes to the estimated continuum luminosity at 5100\AA. Using different methods, e.g., CCF, { \small JAVELIN}, von-neumann, we estimated the size of the BLR, which is found to be 66.4$^{ +6.0}_{ -4.2}$ light days in the rest frame. The BLR size combined with the line width of H$\beta$ provides a black hole mass of 7.32$^{ +0.89}_{ -0.91} \times 10^{ 7}M_{ \odot}$. The source closely follows the BLR size-luminosity relation of AGN.
Categories: astro-ph.GA