excess ratios listed in @flaherty07. Following the several conditions suggested in @gutermuth09 [see also @dewangan17], Class I and Class II YSOs are identified in our selected site. This color-color space gives 71 (9 Class I and 62 Class II) YSOs (see circles and triangles in Figure \[fig9\]a). Figure \[fig9\]b shows the color-magnitude plot (H$-$K/K) of point-like sources. We find the infrared-excess sources with H$-$K $>$ 1 mag. This color condition is found via the color-magnitude analysis of a nearby control field. The color-magnitude space gives 74 additional YSO candidates, which are not common with the YSOs identified using the dereddened color-color space. These two schemes yield a total of 145 YSOs in the selected site, and their positions are marked in the [*Herschel*]{} column density map (see Figure \[fig9\]c). A majority of these YSOs are distributed toward the central part of the filamentary feature observed in the [*Herschel*]{} column density map, where five dense clumps A, B, C, D, and E are investigated (see Figures \[fig2a\]b and \[fig9\]c). Furthermore, YSOs are also found toward other [*Herschel*]{} clumps (e.g., 13, 15, 17, 18, 19, and 21; see Figures \[fig2\]c and \[fig9\]c). Overlay of these selected YSOs on the [*Spitzer*]{} 8.0 $\mu$m 