In this study, we comprehensively validate the effectiveness of a molecular clump detection workflow using 13CO data from the Milky Way Image Scroll Painting (MWISP) project, covering the inner Milky Way within the longitude range 10° ≤ l ≤ 20° and a latitude strip of |b| ≤ 5:25°. The workflow, namely Facet-SS-3D-Clump, initially employs FacetClumps to identify molecular clumps. Subsequently, high-confidence clumps are obtained by cross-matching with the clumps detected by other algorithms, such as Dendrogram. Then, these high-confidence clumps are used as prior knowledge to train a semi-supervised deep clustering approach, SS-3D-Clump, which is applied to verify candidate clumps detected by FacetClumps, providing confidence levels for the molecular clumps. Finally, a catalogue comprising 18,757 molecular clumps extracted from 13CO (J = 1 - 0) emission data was obtained using the workflow. By matching with Herschel infrared dust clumps, we found that 82.3% of the dust clumps correspond to 13CO clumps, which confirmed the accuracy of the workflow. The catalogue is 90% complete above 37 K km s-1. We observe a significant deviation of the mean Galactic latitude for clumps within|b| ≤ 2° from the midplane, with b = -0.110°. In the future, Facet-SS-3D-Clump will be applied to detect 13CO clumps in the entire MWISP data.

In this study, we present a catalogue of molecular clumps extracted from 13CO (J = 1 - 0) emission data of the Milky Way Image Scroll Painting (MWISP) project. The data covers the inner MilkyWay within the longitude range 10° ≤ l ≤ 20° and the latitude strip of |b| ≤ 5:25°. The clumps extraction of workflow, namely Facet-SS-3D-Clump, consists of two parts: the identification of clumps candidates and their verification. First, Facet-SS-3D-Clump employs FacetClumps to identify clumps candidates. Subsequently, high-confidence clumps are obtained by cross-matching with the clumps detected by other algorithms, such as Dendrogram. Second, these high-confidence clumps are used as prior knowledge to train a semi-supervised deep clustering approach, SS-3D-Clump, which is applied to verify clumps candidates detected by FacetClumps, providing confidence levels for the molecular clumps. Finally, the catalogue comprising 18,757 molecular clumps was obtained using Facet-SS-3D-Clump, and the catalogue is 90% complete above 37 K km s-1. We observe a significant deviation of the mean Galactic latitude for clumps within |b| ≤ 2° from the midplane, with b = -0.110°. We found that 82.3% of the dust clumps correspond to 13CO clumps by matching with Herschel infrared dust clumps. In the future, Facet-SS-3D-Clump will be applied to detect 13CO clumps in the entire MWISP data.