Possible TeV Gamma-Ray Binary Origin of HESS J1828–099

The High Energy Stereoscopic System (H.E.S.S.) observatory has carried a deep survey of the Galactic plane, in course which existence significant number ($\sim$ 78) TeV $\gamma$-ray sources was confirmed, many remain unidentified. HESS J1828-099 is point-like (Gaussian stand. dev. $<$ 0.07$^{\circ}$) unidentified source among 17 confirmed H.E.S.S. Plane Survey (HGPS) catalog. This also unique because it does not seem to have any apparent association with object detected at other wavelengths. We investigate nature and multi-wavelength observational data. A high mass X-Ray binary (HMXB) - comprising pulsar XTE J1829-098 companion Be star been observed earlier X-ray infrared bands, 14$'$ away from J1828-099. With 12 years $\textit{Fermi}$-LAT data, we explore possibility 4FGL J1830.2-1005 being GeV counterpart Within RXTE confidence region, steep spectrum ($\alpha_{radio}$ = 0.746 $\pm$ 0.284), plausible data existing radio frequency surveys. In this letter, probe for first time using whether J1828-099, HMXB system common origin. Our study indicates that might be source.