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In the interstellar medium, the amide-type molecules play an important rolein the formation of the prebiotic molecules in the hot molecular cores orhigh-mass star formation regions. The complex amide-related molecule cyanamide(NH$_{2}$CN) is known as one of the rare interstellar molecule which has playeda major role in the formation of urea (NH$_{2}$CONH$_{2}$). In this article, wepresented the detection of the emission lines of cyanamide (NH$_{2}$CN) towardsthe hot molecular core G10.47+0.03 between the frequency range 158.49$-$160.11GHz using the Atacama Large Millimeter/submillimeter Array (ALMA)interferometric radio telescope. The estimated column density of the emissionlines of NH$_{2}$CN using the rotational diagram model was $N$(NH$_{2}$CN) =(6.60$\pm$0.1)$\times$10$^{15}$ cm$^{-2}$ with rotational temperature($T_{rot}$) = 201.2$\pm$3.3 K. The fractional abundance of NH$_{2}$CN withrespect to H$_{2}$ towards G10.47+0.03 was $f$(NH$_{2}$CN) =5.076$\times$10$^{-8}$. Additionally, we estimated the NH$_{2}$CN/NH$_{2}$CHOabundance ratio towards the G10.47+0.03 was 0.170, which was nearly similarwith NH$_{2}$CN/NH$_{2}$CHO abundance ratio towards IRAS 16293$-$2422 B and SgrB2 (M). We found that the observed abundance of NH$_{2}$CN with respect toH$_{2}$ towards G10.47+0.03 fairly agrees with the theoretical value predictedby Garrod (2013). We also discussed the possible formation and destructionpathways of NH$_{2}$CN.

Detection of interstellar cyanamide (NH$_{2}$CN) towards the hot molecular core G10.47+0.03