Pipeline for Photometric Variability of Intermediate Mass Black hole AGN 2MASSJ094733.06+0013028 Using 1.3m DFOT Observations

Photometry, the measurement of the brightness of celestial objects, plays a crucial role in understanding the properties and dynamics of astronomical phenomena. In this study, we present photometric observations of source in 2MASSJ094733.06+0013028 obtained using the 1.3 m DFOT telescope.Our observations span multiple epochs in V band.We employed differential photometry techniques to measure the fluxes of the sources and standard stars. The resulting light curves reveal variability patterns

indicative of different types of standard stars and source. Overall, our photomet- ric investigation sheds light on the diverse population of stars and underscores the

importance of photometry in unraveling the complex nature of astrophysical phe- nomena like : stellar evolution, stellar populations, and the dynamics of source (

here it is AGN ). From there we estimated the mass of Intermediate Mass Black Hole (IMBH) present at the center of that AGN.